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| * Meeting time: 14:00-15:00 JST/KST on every Thursday * Meeting room: Zoom |
* Meeting time: 11:00-11:30 JST/KST on every Wednesday * Meeting room: Zoom3 |
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| === 20211101 (Mon.) === * Agenda * hveto, O3GK glitches * Info. for open data * Progress of DQR * Minutes * Info. for open data * We should refer segments on [[https://segments-web.ligo.org|DQSEGDB]] * For GW searches: K1-SCIENCE_MODE, DET_FOR_GRB200415A * We need to check [1270965983, 1270976372) and [1270976435, 1270976783). === 20211025 (Mon.) === * Agenda * Omicron glitches (40?, 120Hz) * DQR [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=13381|slide]] * Minutes * Omicron glitches * ALS channels has some coincidence. * Cavity and suspensions are shared GR and IR lasers. * It's not identified the cause (GR laser or suspensions) yet from current results. * Chamber ACC at EXC has also same glitches. * hveto cannot detect coincidence on EYC and other ACC channels. * These channels also checked by Omega-scan once => Kihyun. === 20211011 (Mon.) === * Agenda * site commissioning * omicron/hveto analysis * DQR * Minutes * site commissioning * MC OpLev glitches ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=18518|klog#18518]]) * PLL resonance ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=18466|klog#18466]]) * IX MN glitches vanished(?) ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17876|klog#17876]]) * === 20210927 (Mon.) === * Agenda * hveto analysis * O4 commissioning * progress of DQR [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=13326|slide]] * Minutes * hveto * glitch rate was computed for O3GK paper [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=13311|JGW-D2113311]] * Clustering (with 0.1s window) was performed on gwpy function * O4 commissioning * Commissioning is now pending and suspension health check is ongoing. === 20210906 (Mon.) === * Agenda * hveto analysis * O4 commissioning * JPS meeting * Minutes * O4 commissioning * Turn on the clustering option of Omicron ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=18070|k-log#18070]]) * periodic glitches are happening in ITMX ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17876|klog#17876]]) * These glitches seems to be correlated to IXV temperature ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17912|#17912]]) * To find the source of ITMX glitches, there is a investigation ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17980|#17980]]) * Update of summary page : Added ITMX signals for glitch pipeline ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=18112|k-log#18112]]) * Implementation of GAS DC control for ITMX ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=18153|k-log#18153]]) === 20210830 (Mon.) === * Agenda * hveto analysis * O4 commissioning * O4 readiness * Minutes * hveto analysis * veto segment list will be shared. => Kihyun * O4 commissioning * PLL noise ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=18014|klog#18014]]) * periodic glitches are happening in ITMX ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17876|klog#17876]]) * These glitches seems to be correlated to IXV temperature ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17912|#17912]]) * To find the source of ITMX glitches, there is a investigation ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17980|#17980]]) * MCi and MCo pitch strange behavior ([[https://klog.icrr.u-tokyo.ac.jp/osl/index.php?r=18027|k-log#18027]]) * Glitch investigation by Omicron * If there are many sources of glitches, information about small change in glitch rate is helpful to noise hunting. * ITMX PS should be added on SummaryPages => Oshino * And also we should set 0.1s clustering option as the first test for Omicron process. * In pyomicron, 0.1s clustering is default settings and pyomicron is available in igwn. * O4 readiness * #15 [Cont'd] State Vector Definition * Responsible: '''T. Yamamoto -> T. Yamamoto''' * #16 + #20 Segment production with short latency * Responsible: '''K. Kokeyama -> S. Oshino, T. Yamamoto''' * #17 [Cont'd ] Status web pages (summary pages, [[https://monitor.ligo.org/gwstatus|gw status]], [[https://ldas-jobs.ligo.caltech.edu/~gwistat/gwistat/gwistat_p.html|gw istat]]) * Responsible: '''S. Oshino -> S. Oshino''' * #18 [Cont'd] DQ event validation * Responsible: '''C. Kozakai -> K. Ueno, T. Yamamoto''' * #19 [Cont'd] GraceDB * Responsible: '''H. Tagoshi -> H. Tegoshi(?)''' * #21 [New] Data Category (at least CAT1) production * Responsible: '''N. Uchikata(?)''' * #22 [New] RRT contribution * Responsible: '''H. Yuzurihara''' * Taks list of DetChar * We need to set concrete task list for authorship issue. (within 1 month?) => Yamamoto * Time line of each tasks also should be decided => Yamamoto & each responsible person * After creating the draft version of task list and time line, they will be shared on DET telecon. === 20210823 (Mon.) === * Agenda * hveto analysis * O4 commissioning & preparation * f2f meeting * Minutes * hveto analysis * O3GK 2 weeks data was analyzed with new configuration. * Blip, LF burst were found in many times. * All vetoed segments will be shared soon. * O4 commissioning * IMC commissioning is on-going * beam shape of transmitted beam at MCE is not clear circle. It looks like ellipse. * Now Kenta Tanaka and I are investigating the cause. If the cause is happening outside of mode cleaner, we can do something to remove the cause. * From the last week investigate, we are doubting it is ghost beam. [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17930|k-log]] [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17903|k-log]] [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17883|k-log]] * VIS commissioning * VIS team is working the implementation of dumping filter, which is called local dumpling. Now they are discussing about the evaluation of the requirement value for dumpling. * Many glitches in the feedback signal were observed. [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17974|k-log]] * f2f meeting * Status talk of DAC/DET (28th Sat. 9:00~?) * => Yamamoto * Contribution talks * Pastavi development (poster) => Yuzurihara * Gaussianity search (poster) => Morisue === 20210816 (Mon.) === * Agenda * hveto analysis * O4 commissioning * KAGRA readiness * f2f meeting * Minutes * hveto analysis * various clustering * ([[https://gwdet.icrr.u-tokyo.ac.jp/~controls/hveto/manual/2020-04-15cl0.1/|0.1]], [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/hveto/manual/2020-04-15cl0.2/|0.2]], [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/hveto/manual/2020-04-15cl0.3/|0.3]], [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/hveto/manual/2020-04-15cl0.4/|0.4]], [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/hveto/manual/2020-04-15cl0.5/|0.5]], [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/hveto/manual/2020-04-15cl0.6/|0.6]], [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/hveto/manual/2020-04-15cl0.7/|0.7]], [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/hveto/manual/2020-04-15cl0.8/|0.8]], [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/hveto/manual/2020-04-15cl0.9/|0.9]], [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/hveto/manual/2020-04-15cl1.0/|1.0]]) * old results * ([[https://gwdet.icrr.u-tokyo.ac.jp/~controls/hveto/manual/2020-04-15_cl0_1v2/|0.1]], [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/hveto/manual/2020-04-15_cl0_2/|0.2]]) * O4 commissioning * FNC instability ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17748|klog#17748]], [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17865|klog#17865]]) * We are not investigating the cause of instability of Michelson fringes of FNC (green laser) * Fiber coupling at PSL room is the most reasonable candidate. * We need to investigate temperature environment around green laser more detailed. * MN Photo sensor noise ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17876|klog#17876]]) * It doesn't seem to be not a real ground motion because upper stage isn't shaked. * We doubt the electrical noise now. * O4 readiness * O4 readiness * #15 [Cont'd] State Vector Definition * Responsible: '''T. Yamamoto -> T. Yamamoto''' * #16 + #20 Segment production with short latency * Responsible: '''K. Kokeyama -> S. Oshino, T. Yamamoto''' * #17 [Cont'd ] Status web pages (summary pages, [[https://monitor.ligo.org/gwstatus|gw status]], [[https://ldas-jobs.ligo.caltech.edu/~gwistat/gwistat/gwistat_p.html|gw istat]]) * Responsible: '''S. Oshino -> S. Oshino''' * #18 [Cont'd] DQ event validation * Responsible: '''C. Kozakai -> K. Ueno, T. Yamamoto''' * #19 [Cont'd] GraceDB * Responsible: '''H. Tagoshi -> H. Tegoshi(?)''' * #21 [New] Data Category (at least CAT1) production * Responsible: '''!!!!!''' * #22 [New] RRT contribution * Responsible: '''H. Yuzurihara''' === 20210802 (Mon.) === * Agenda: * hveto analysis * O4 commissioning and preparation * Hardware injection plan during O4 * KAGRA O4 readiness * Proposal of O3GK DetChar paper [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=13149|slide]] * Minutes: * hveto analysis * clustering test * Round winer doesn't change by clustering option. * Some kind of clustering is necessary but best parameter is not clear yet. * Kihyun will share the event time of clustered events. * We should check each event by spectrogram, Omega-scan, etc. * hveto with clustering will be also performed for 2 weeks day. * O4 commissioning * Omega-scan on Kashiwa has some error now. And * Hardware injection plan during O4 * KAGRA CAL group is now gathering the plan of HWI during observations. * In LIGO case, in order to do HWI during obs., they need special and reasonable reasons. * KAGRA CAL also plan to adopt same procedures of the HWI management as LIGO. * If you have any HWI plan related to DET activities pls. share in DET telecons once. * We would like to discuss that the requested plans should be conducted during ER or obs. * O4 readiness * #15 [Cont'd] State Vector Definition * Responsible: '''T. Yamamoto -> T. Yamamoto''' * #16 + #20 Segment production with short latency * Responsible: '''K. Kokeyama -> S. Oshino, T. Yamamoto''' * #17 [Cont'd ] Status web pages (summary pages, [[https://monitor.ligo.org/gwstatus|gw status]], [[https://ldas-jobs.ligo.caltech.edu/~gwistat/gwistat/gwistat_p.html|gw istat]]) * Responsible: '''S. Oshino -> S. Oshino''' * #18 [Cont'd] DQ event validation * Responsible: '''C. Kozakai -> T. Yamamoto''' * #19 [Cont'd] GraceDB * Responsible: '''H. Tagoshi -> H. Tegoshi(?)''' * #21 [New] Data Category (at least CAT1) production * Responsible: '''!!!!!''' * #22 [New] RRT contribution * Responsible: '''H. Yuzurihara''' === 20210726 (Mon.) === * Agenda: * hveto analysis * O4 commissioning * O4 readiness * Minutes: * hveto analysis * Analyses with various clustering parameter are in progress. Kihyun will report in next telecon. * O4 commissioning * no updates * SummaryPages * lvalert * DET cluster * O4 readiness * It is preferable that the same person does not become multiple responsible person * As WP2021, DET tasks which is taken into account an effort follows readiness issues. * #15 [Cont'd] State Vector Definition * Responsible: '''T. Yamamoto -> T. Yamamoto''' * #16 + #20 Segment production with short latency * Responsible: '''K. Kokeyama -> S. Oshino, T. Yamamoto''' * #17 [Cont'd ] Status web pages (summary pages, [[https://monitor.ligo.org/gwstatus|gw status]], [[https://ldas-jobs.ligo.caltech.edu/~gwistat/gwistat/gwistat_p.html|gw istat]]) * Responsible: '''S. Oshino -> S. Oshino''' * #18 [Cont'd] DQ event validation * Responsible: '''C. Kozakai -> !!!!!''' * #19 [Cont'd] GraceDB * Responsible: '''H. Tagoshi -> H. Tegoshi(?)''' * #21 [New] Data Category (at least CAT1) production * Responsible: '''!!!!!''' * #22 [New] RRT contribution * Responsible: '''H. Yuzurihara''' === 20210719 (Mon.) === * Agenda: * hveto analysis * O4 commissioning * O4 readiness * Minutes * O4 commissioning * IMC-XARM commissioning * FNC control saturation [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17464|klog17464]] * MC Oplev glitches and 120Hz line still exist (K1:VIS-MC{I,E,O}_TM_WIT_{P,Y}) * Unstational noise excess on Green laser above 100Hz still exists (K1:ALS- * O4 readiness * #15 [Cont'd] State Vector Definition * Responsible: '''T. Yamamoto -> T. Yamamoto(?)''' * #16 + #20 Segment production with short latency * Responsible: '''K. Kokeyama -> S. Oshino, T. Yamamoto''' * #17 [Cont'd ] Status web pages (summary pages, [[https://monitor.ligo.org/gwstatus|gw status]], [[https://ldas-jobs.ligo.caltech.edu/~gwistat/gwistat/gwistat_p.html|gw istat]]) * Responsible: '''S. Oshino -> S. Oshino(?)''' * #18 [Cont'd] DQ event validation * Responsible: '''C. Kozakai -> ''' * #19 [Cont'd] GraceDB * Responsible: '''H. Tagoshi -> H. Tegoshi(?)''' * #21 [New] Data Category (at least CAT1) production * Responsible: * #22 [New] RRT contribution * Responsible: '''H. Yuzurihara(?)''' === 20210705 (Mon.) === * Agenda: * O3GK paper * white paper * O4 commissioning * Minutes: * O3GK paper * Hveto was rerun with various parameters. * But there is no improvement in the veto efficiency. * white paper * Final version was released. * There was no additional comments from LV * [[https://git.ligo.org/operations/operations-white-paper-2021|LIGO Git]] * O4 commissioning * no report ----- === 20210628 (Mon.) === * Agenda * O3GK paper * white paper * O4 commissioning & preparation * Minutes * O3GK paper * Uchikata-san and Narikawa-san got a consistent results with Kozakai-san's one. * hveto was performed with 0.1 duration. * There is no efficient channel/sensor for glitch veto. * Some parameters comes from LIGO's one. * So we need to find better parameters for KAGRA's data. * We also need prepare the more efficient sensors for O4 observing run * Kihyun is also performing the crosscheck. (1 or 2 weeks later he can report.) * white paper * [[https://git.ligo.org/operations/operations-white-paper-2021|Draft on LIGO Git]] * TY will be added a description about CAGMon until LVK DET call. * WP will be fixed at Ops call on 6/30 (?) * O4 commissioning & preparation * IMC commissioning * [Ongoing] Glitches on OpLev * Because of too many glitches, it's difficult to investigate one by one. * K1:VIS-MC{I,E,O}_TM_WIT_{P,Y} (MC Oplevs) * [Fixed] PLL noise coming from broken circuit [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17188|klog17188]] * [Ongoing] PLL also has glitches (maybe) due to electrostatic discharge. [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17239|klog17239]] * K1:ALS-{X,Y}_BEAT_ERR_OUT_DQ (error signal) * K1:ALS-{X,Y}_PLL_SLOW_DAQ_OUT_DQ (feedback signal) * [Ongoing] non-stational correlation between IMC/PLL and Microphone * K1:CAL-CS_PROC_IMC_FREQUENCY_DQ (calibrated frequency noise) * K1:IMC-SERVO_SLOW_DAQ_OUT_DQ (feedback signal of IMC) * K1:ALS-{X,Y}_PLL_SLOW_DAQ_OUT_DQ (feedback signal of PLL) * [Ongoing] station correlation between PMC and Microphone * Investigation about significance of coherence is ongoing. ----- === 20210621 (Mon.) === * Agenda * O3GK paper * O4 whitepaper * O4 commissioning & preparation * Minutes * O4 white paper * The 1st version of the draft was submitted on June 17th. * [[https://git.ligo.org/operations/operations-white-paper-2021|LIGO Git]] * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12985|JGW-T-2112985]] * Final deadline is June 30th. * We can still do the miner fix. * O4 commissioning & preparation * IMC Commissioning * Omicron trigger searches for MC Oplevs were resumed ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=17150|klog#17150]]). * K1:VIS-MC{I,E,O}_TM_WIT_{P,Y} (oplev signals) * K1:VIS-IMMT{1,2}_TM_WIT_{P,Y} (as a reference of circuit noise) * SummaryPages * Glitch trigger tabs are added. * Loudest glitches can be seen on Pastavi (only internal ICRR network) === 20210614 (Mon.) === * Agenda * O3GK paper * O4 whitepaper * O4 commissioning & preparation * Minutes * O3GK paper * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=13009|plot]] * O4 white paper * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12985|draft]] * It's better to include PEM plans in commissions support section if exits. * O4 commissioning & preparation * IMC Commissioning * We have now four frequency noise signal (IMC, PMC, PLL-X, PLL-Y) * K1:CAL-CS_PROC_IMC_FREQUENCY_DQ (calibrated IMC as MHz) * K1:PSL-PMC_PZT_HV_MON_OUT_DQ (calibrated PMC as Volt at PZT amp.) * K1:ALS-X_PLL_SLOW_DAQ_OUT_DQ (calibrated Green-X as Volt at PZT) * K1:ALS-X_PLL_SLOW_DAQ_OUT_DQ (calibrated Green-Y as Volt at PZT) * PMC (always) and others (sometimes) have correlation with microphone signal * K1:PEM-MIC_PSL_TABLE_PSL1_Z_OUT_DQ (calibrated as Pascal) * OpLev signals have some glitches and are investigated now. * K1:VIS-MC{I,E,O}_TM_WIT_{P,Y} * Real SUS motion?, electrical glitches?, scattered light? etc. * SummaryPages * Updated PSL, PEM tabs. * PLL signals are available. ----- === 20210607 (Mon.) === * Agenda * O3GK paper * O4 whitepaper * O4 commissioning & preparation * Minutes * O3GK paper * Preparing some plots about histgram and glitch rate of both KAGRA and GEO * O4 whitepaper * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12985|draft]] * O4 commissioning & preparation * CAGMon development * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12986|slide]] * Found correlation between wind power and BNS ranges * OMMT1 doesn't (maybe) have Oplev. It's better to confirm what kind of sensors were coneected. * BNS range channel has ~2min latency. It may become better results by considering the latency in BNS range calculation. * IMC commissioning * Noise investigation ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=16928|klog]]) * Correlation between IMC and MIC sometimes increase in spite of no change in microphone spectra. * Coupling coefficients may be changed in time. * Cross check of hveto results. * Kihyun's (KISTI) and Chihiro's (Kamioka) results were confirmed as consistent each other. * For O4 observing run, Kashiwa environment is also important for increasing machine power. * Requirement of machine power should be estimated soon (but it's strongly depends on the situation of O4 joining) * We plan to use 100-200 aux. channels and it's very helpful to analyze them at the same time for each pipeline. * lvalert * no report * SummaryPage * no report * DetChar cluster * no report ----- === 20210531 (Mon.) === * Agenda * O3GK paper * O4 readiness * O4 commissioning & preparation * Minutes * O3GK paper * Comparison with Uchikata-san's and GEO people's results is ongoing. * Kihyun is performing validation check of his results => He will report in next or 2 weeks later telecon. * O4 readiness * #15 [Cont'd] State Vector Definition * Responsible: '''T. Yamamoto -> T. Yamamoto(?)''' * #16 + #20 Segment production with short latency * Responsible: '''K. Kokeyama -> ''' * #17 [Cont'd ] Status web pages (summary pages, [[https://monitor.ligo.org/gwstatus|gw status]], [[https://ldas-jobs.ligo.caltech.edu/~gwistat/gwistat/gwistat_p.html|gw istat]]) * Responsible: '''S. Oshino -> S. Oshino(?)''' * #18 [Cont'd] DQ event validation * Responsible: '''C. Kozakai -> ''' * #19 [Cont'd] GraceDB * Responsible: '''H. Tagoshi -> H. Tegoshi(?)''' * #21 [New] Data Category (at least CAT1) production * Responsible: * #22 [New] RRT contribution * Responsible: '''H. Yuzurihara(?)''' * white paper 2021 * No progress in draft. * Task list will be based on O4 readiness. * If there is another task plan, please let TY know (maybe CAGMon, ICA, pastavi development etc.). * O4 commissioning & preparation * LVAlert * no report * SummaryPages update * no report * DET cluster * no report * CAGMon development * no report ----- === 20210524 (Mon.) === * Agenda * O3GK paper * O4 commissioning & preparation * O4 readiness * Minutes * O3GK paper * Discussion with GEO people is ongoing * O4 commissioning & preparation * MC circuit noise hunting * Current spectrum is too clean 1/f noise. * Frequency noise should shows 1/f spectrum. * But we haven't checked it's a real frequency noise (circuit noise etc.). * Nakano-kun said current spectrum is consistent with past measurements. * sound correlation * Investigating sound correlation with three microphones. [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12937|slide]] * lvalert test * no report * DET cluster * no report * SummaryPages * added for some IMC signals and it work well. * White paper 2021 * [[https://git.ligo.org/operations/operations-white-paper-2021|2021]] * [[https://git.ligo.org/operations/operations-white-paper-2020|2020]] === 20210517 (Mon.) === * Agenda * KAGRA O4 readiness * LVK white paper 2021 * O3GK paper * IMC commissioning * Minutes * KAGRA O4 readiness * #15 [Cont'd] State Vector Definition * Responsible: '''T. Yamamoto -> ''' * #16 [Cont'd] DQSEGDB capability * Responsible: '''K. Kokeyama -> ''' * #17 [Cont'd ] Status web pages (summary pages, [[https://monitor.ligo.org/gwstatus|gw status]], [[https://ldas-jobs.ligo.caltech.edu/~gwistat/gwistat/gwistat_p.html|gw istat]]) * Responsible: '''S. Oshino -> ''' * #18 [Cont'd] DQ event validation * Responsible: '''C. Kozakai -> ''' * #19 [Cont'd] GraceDB * Responsible: '''H. Tagoshi -> ''' * #20 [New] Segment production (merged with #16?) * Responsible: * #21 [New] Data Category (at least CAT1) production * Responsible: * #22 [New] RRT contribution * LVK white paper * Responsible: * What TY thought * All activities which are submitted as 2021 DET effort should be described on this documents. * It will be based on white paper 2020 and KAGRA O4 readiness. * Should clarify who will do each item (though personal name itself is not described on this documents). * Should show the rough timeline for R&D tasks. * O3GK paper * We need to continue to discuss with GEO people about GEO data analysis. * IMC Commissioning * Current IMC control signals on DGS are contaminated by circuit noise. * Important thing is that contamination is occurred only on DGS signals or also on real analog signals * Important channels * K1:IMC-SERVO_{MIXER,FAST,SLOW}_DAQ_OUT_DQ * K1:IMC-SERVO_NPRO_TEMP_BIAS_OUT_DQ * => These channels will be added to SummaryPages * O4 preparation * CAGMon development * no report * lvalert test * no report * DET cluster * no report === 20210510 (Mon.) === * Agenda * KIW * O3GK paper * IMC Commissioning * O4 preparation * Minutes * KIW {{{ - Status of KAGRA DET (20 min) => T. Yamamoto - Status of LIGO Detchar (20 min) - Status of Virgo Detchar (20 min) - Contributed Talk 1 - one slot from KAGRA (15 min) => H. Yuzurihara - Contributed Talk 2 - CAGMon tools (15 min) - Contributed Talk 3 - KISTI's data transfer and computing (15 min) }}} * O3GK paper * hveto process for GEO600 was done. * IMC Commissioning * [PMC] Acoustic coherence (20-200Hz) * [IMC] Oscillation? (13-15MHz) * O4 preparation * SummaryPages * no report * lvalert * no report * DET cluster * no report === 20210426 (Mon.) === * Agenda * O3GK analysis * O4 preparation * IMC Commissioning * Minutes * O3GK analysis * Omicron analysis of GEO was finished. * Checking results is ongoing. * We need to convert segment information on DQSEGDB to xml format. * After checking omicron results, hveto analysis can be started. * CAG Mon development * CAG Mon was able to detect some correlation in O3GK data * Prioritize is not done yet. * prioritize can be decided by correlation coefficient value or total duration of correlation appearing * We need more time to develop CAGMon (before we move to review process.). * IMC Commissioning * Microphone self noise is evaluating now. * They will be installed in PSL room * Paper writing person(s) from DET * TY takes over from Kozakai-san. * summary of lvalert test for LVK DET telecon ----- === 20210419 (Mon.) === * Agenda * O3GK analysis * O4 preparation (LV alert, SummaryPages, CAGMon) * PMC/IMC noise hunting * Minutes * O3GK analysis * GEO data analysis is started. * Channel list is prepared by GEO people. * PMC/IMC noise hunting * Sound noise * Frequency noise has coherence with microphone signal. * Sound noise affected to DARM sensitivity during O3GK. * Noise source and injection injection route should be investigated. * Electrical noise(?) * Accelerometer channel has coherence with frequency noise when PEM sensor turned OFF. * Circuit noise level is small, but some electrical coherence may exist. === 20210408 (Thu.) === * Agenda * O3GK analysis * SummaryPage * LV alert [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12760|slide]] * NDS2 * IMC Commissioning * Minutes * O3GK analysis * hveto re-analysis for a part of data was done. * round winner is same * significant is slightly difference, (using same conf. triggers, version, etc) * Next step is to check consistency of veto segment * GEO data * Analysis itself will be performed by KAGRA people * Understanding results will be performed by GEO (+KAGRA) people |
----- === 20241009 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': O4b will now end 9 June 2025. * [[https://observing.docs.ligo.org/plan/|Run plan(9/15 updated)]] [[https://wiki.ligo.org/Operations/Agenda240919|operation (09/19)]] * Scheduled conference * JGRG33 @Kindai University: 2024/12/02(Mon)~2024/12/6(Fri) [[https://sites.google.com/view/jgrg33|web]] * KAGRA site report [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0160/L2416034/001/KAGRAReport_20240909.pdf|09/09]] * Next meeting: October 16 * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * lock loss study in the commissioning (YamaT, Yuzurihara) [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/misc/html/lockloss_o4b_break.html|web]] * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * provide the CAT1 veto-definer file for IPC glitch (Uchikata) * Minutes * Recovery work after Kashiwa cluster maintenance, such as cache file and segment production. (Uchikata) [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=31182|klog]] ----- === 20241002 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': O4b will now end 9 June 2025. * [[https://observing.docs.ligo.org/plan/|Run plan(9/15 updated)]] [[https://wiki.ligo.org/Operations/Agenda240919|operation (09/19)]] * Scheduled conference * JGRG33 @Kindai University: 2024/12/02(Mon)~2024/12/6(Fri) [[https://sites.google.com/view/jgrg33|web]] * KAGRA site report [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0160/L2416034/001/KAGRAReport_20240909.pdf|09/09]] * Next meeting: October 9 * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * lock loss study in the commissioning (YamaT, Yuzurihara) [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/misc/html/lockloss_o4b_break.html|web]] * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * provide the CAT1 veto-definer file for IPC glitch (Uchikata) * Minutes * Upgrade DetChar computers (YamaT) * Due to Kachiwa maitanance, nds2 is working partially. * lock loss study in the commissioning (YamaT, Yuzurihara) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=31068|lockloss investigation: 2024/09/11 16:45:56 JST]] * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=31135|Shutdown the Pastavi server for power outage]] * Characterization of relationship between Omicron triggers and inspiral range during O4a (Ishikawa) [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0160/G2416062/001/report241001.pdf|slide]] * Line investigation (Takahiro.S.Yamamoto) [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=16063|slide]] * Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down. * Recovery work after Kashiwa cluster maintenance, such as cache file and segment production. (Uchikata) * Update of the condor in Kashiwa cluster to version 23.0.14 * This version looks fine for stochastic search (Chia-Hsuan) ----- === 20240911 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': O4b will now end 9 June 2025. * [[https://observing.docs.ligo.org/plan/|Run plan(8/27 updated)]] [[https://wiki.ligo.org/Operations/Agenda240829|operation (08/29)]] * Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down. * LIGO Detector Characterization in the first half of the fourth Observing run [[https://arxiv.org/abs/2409.02831|arxiv]] * Scheduled conference * JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.[[https://www.jps.or.jp/activities/meetings/annual/annual-index.php|web]] * LVK meeting @Barcelona, Spain: Registration is now open. Sept 23 – 26. [[https://lvkmeeting2024.ifae.es/|web]] * block schedule for the meeting is now ready * JGRG33 @Kindai University: 2024/12/02(Mon)~2024/12/6(Fri) [[https://www-tap.scphys.kyoto-u.ac.jp/jgrg/|web]] * KAGRA site report [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0160/L2416022/001/KAGRAReport_20240829.pdf|09/02]] * Next meeting: October 2. We will skip the meeting on September 18 and 25. * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * provide the CAT1 veto-definer file for IPC glitch (Uchikata) * Minutes * lock loss study in the commissioning (YamaT, Yuzurihara) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=30987|Segment for lockloss of LSC_LOCK guardian]] * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=30997|lockloss investigation: 2024/09/05 14:50:00 JST]] * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=31032|lockloss investigation: 2024/09/09 10:36:18 JST]] * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=31045|Helper guardian for lockloss check]] * lock loss investigation tool was developed. The web page will be automatically updated: [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/misc/html/lockloss_o4b_break.html|web]] * cache file at Kashiwa cluster (Uchikata) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=31051|Cache file genetation at kmst2]] * The cache file included duplicated frame files. By changing the execution timing, this issue was solved. * Segment reproduction (Uchikata, Narikawa, YamaT, Yuzu) * There was a missing period at the Kamioka cluster. While generating the segment at the Kashiwa cluster, we noticed that it's important to use the consistent version of gwpy and python-ligo-xml to upload the segment for DQSEGDB. We found a suitable conda environment at the Kaashiwa cluster. The segment file generated in the Kashiwa cluster looks consistent with the one generated in the Kamioka cluster. The next step is to ask Robert to include the updated segments on DQSEGDB. * Line investigation (Takahiro.S.Yamamoto) * The script was developed to merge the spreading line noise into one line noise. Although the test script is working well, it requires more time to mature. ----- === 20240904 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': O4b will now end 9 June 2025. * [[https://observing.docs.ligo.org/plan/|Run plan(8/27 updated)]] [[https://wiki.ligo.org/Operations/Agenda240718|operation (07/18)]] * Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down. * Scheduled conference * JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.[[https://www.jps.or.jp/activities/meetings/annual/annual-index.php|web]] * LVK meeting @Barcelona, Spain: Registration is now open. Sept 23 – 26. [[https://lvkmeeting2024.ifae.es/|web]] * block schedule for the meeting is now ready * JGRG33 @Kindai University: 2024/12/02(Mon)~2024/12/6(Fri) [[https://www-tap.scphys.kyoto-u.ac.jp/jgrg/|web]] * KAGRA site report [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0160/L2416022/001/KAGRAReport_20240829.pdf|09/02]] * Next meeting: September 11. We will skip the meeting on September 18 and 25. * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * provide the CAT1 veto-definer file for IPC glitch (Uchikata) * Minutes * KAGRA student workshop (Yuzurihara) * During the KAGRA student workshop (2024/08/27-29), we visualized the KAGRA data around the trigger time of high chi^2 statistics by using the time-frequency map [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=30968|klog]] [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=16024|JGWdoc]] * scattered light affects the high SNR? --> Chi^2 can mitigate the effect of the scattered light * What about the effect on parameter estimation? --> I'm not sure. The effect can be evaluated by analyzing the data injected with scatter light noise. * Providing segment information on the scattered light noise might be helpful. The difficulty is in identifying the time that occurs when the scattered light is present. * Chia-Jui-san mentioned the method using the Omicron triggers and Q-transform. * (Narikawa) The other trigger list of high SNR was used? --> Not yet, due to the time constraints * Update contents of summary page (Oshino) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=30969|klog]] * Related to segment files (Uchikata, Narikawa) * There was a missing period at the Kamioka cluster. While generating the segment at the Kashiwa cluster, we noticed that it's important to use the consistent version of gwpy and python-ligo-xml to upload the segment for DQSEGDB. We found a suitable conda environment at the Kaashiwa cluster. The segment file generated in the Kashiwa cluster looks consistent with the one generated in the Kamioka cluster. * The automatic generation of the cache file sometimes fails at the Kashiwa cluster. We doubt the cause is the cluster setting. We are discussing how to avoid the failure of cache file generations. * pyCBC trigger list for O4a data (Narikawa and Uchikata) * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15681|slide]] * He injected the BNS signal into the data using Bilby and showed the reconstruction result. * The duration of the BNS template (fmin=30Hz) is 250s. * Line investigation (Takahiro S Yamamoto) * He implemented the code to generate the normalized spectrum. By eyeball check, the result looks consistent with the results by YamaT-san. * The next step is to fit the line peak using Gaussian or Lorenzian distribution and characterize the line width and stability of the frequency. * Clustering might be necessary to merge the broad line noise into one line. * [[https://git.ligo.org/yamamoto2/line_identification_for_kagra|Working repo(internal)]] ----- === 20240807 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': O4b will now end 9 June 2025. * [[https://observing.docs.ligo.org/plan/|Run plan(7/18 updated)]] [[https://wiki.ligo.org/Operations/Agenda240718|operation (07/18)]] * Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down. * Request to reduce batch job during 8/27-30 for the Student Workshop (See [kagra 06769]) * Scheduled conference * KAGRA f2f meeting: 2024/08/21(Wed)~23(Fri) @Tokyo City University [[https://dac.icrr.u-tokyo.ac.jp/KAGRA/KSC/f2f/2024August|web]] * Satellite meeting for noise reduction of KAGRA: 2024/08/24 9:00~12:00 [[https://dac.icrr.u-tokyo.ac.jp/KAGRA/KSC/f2f/2024August#Day4%3A%20August%2024%20(Saturday)%20JST%209%3A00-12%3A00|web]] * JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.[[https://www.jps.or.jp/activities/meetings/annual/annual-index.php|web]] * LVK meeting @Barcelona, Spain: Registration is now open. Sept 23 – 26. [[https://lvkmeeting2024.ifae.es/|web]] * JGRG33 @Kindai University: 2024/12/02(Mon)~2024/12/6(Fri) [[https://www-tap.scphys.kyoto-u.ac.jp/jgrg/|web]] * KAGRA site report [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0159/L2415918/001/KAGRAReport_20240729.pdf|07/29]] * Next meeting is September 4 * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * provide the CAT1 veto-definer file for IPC glitch (Uchikata) * Minutes * pyCBC trigger list for O4a data (Narikawa and Uchikata) * Although they updated the way of clustering, the basic feature didn't change. [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15876|slide]] * The usage manual for veto definer was prepared by Uchikata-san [[https://dac.icrr.u-tokyo.ac.jp/KAGRA/DAWG/Detchar/Veto%20Definer%20File%20(VDF)|usage manual for veto definer]] * Hveto analysis * The comparison between Omicron 2.4 and 3.2 was done ----- === 20240731 (Wed.) === * Wide presentation of PhD thesis * Date: Wednesday, July 31 at 11:00 JST/KST or 2:00 UTC. (20~30 min. for the presentation. 10~15 min. for the question.) * Presenter: Kihyun Jung * Thesis title: Classification and Analysis of KAGRA Glitch * Thesis manuscript: https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15866 ----- === 20240724 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': O4b will now end 9 June 2025. * [[https://observing.docs.ligo.org/plan/|Run plan(7/18 updated)]] [[https://wiki.ligo.org/Operations/Agenda240718|operation (07/18)]] * Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down. * Scheduled conference * KAGRA f2f meeting: 2024/08/21(Wed)~23(Fri) @Tokyo City University [[https://dac.icrr.u-tokyo.ac.jp/KAGRA/KSC/f2f/2024August|web]] * JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.[[https://www.jps.or.jp/activities/meetings/annual/annual-index.php|web]] * LVK meeting @Barcelona, Spain: Registration is now open. Sept 23 – 26. [[https://lvkmeeting2024.ifae.es/|web]] * JGRG33 @Kindai University: 2024/12/02(Mon)~2024/12/6(Fri) [[https://www-tap.scphys.kyoto-u.ac.jp/jgrg/|web]] * KAGRA site report [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0158/L2415897/002/KAGRAReport_20240716.pdf|07/16]] * Next meeting is 08/07(Wed). Next week, we will have Wide presentation of PhD thesis by Kihyun. * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * provide the CAT1 veto-definer file for IPC glitch (Uchikata) * Minutes * Add cooler ondotori page (Oshino) [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=30353|klog]] * [[https://git.ligo.org/computing/helpdesk/-/issues/6176#note_1061004|KAGRA segment file production stopped on 28 June 2024]] * The cause was the stop of cache file at Kamioka computer due to the expire of gps time package. * To return to an automated setup, would it be possible to have the incomplete files created in one directory and only moved to their final location after the whole day's segments are finalized? * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=30519|Reduce the cadence of segment production at Kamioka site]] * On this Friday, we shut down the Kamioka computers due to a planned power outage. * pyCBC trigger list for O4a data (Narikawa and Uchikata) * They are updating the way to cluster the triggers. * veto definer (Uchikata) * When we make veto definer, we need the segment updated in DQSEGDB. But, currently, the necessary segment was not uploaded on DQSEDB. We will ask Robert to include them soon. * Uchikata-san will summarize the procedure at the DAC wiki. * Line identification (Takahiro S. Yamamoto) * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15909|slide]] * By using Fscan, the line noise in O1 data was investigated. [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15768|Fscan]] * The goal is to obtain the line frequency and the typical width. * Investigating the stability of line noise is important. It will be the first task. * Stochastic search (Chia-Hsuan) * The line list computed from the data with a shorter duration might be important. Currently, we use the line list of 0.001 mHz resolution. The unification between the stochastic analysis and the detchar analysis is necessary. * Parameter estimation analysis with KAGRA O4a data (Kobayashi) * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15905|slide]] ----- === 20240717 (Wed.) === * canceled ----- === 20240710 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': O4b will now end 9 June 2025. * [[https://observing.docs.ligo.org/plan/|Run plan(6/17 updated)]] * Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down. * Future meeting * JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.[[https://www.jps.or.jp/activities/meetings/annual/annual-index.php|web]] * KAGRA f2f meeting: 2024/08/21(Wed)~23(Fri) @Tokyo City University [[https://dac.icrr.u-tokyo.ac.jp/KAGRA/KSC/f2f/2024August|web]] * LVK meeting @Barcelona, Spain: Registration is now open. Sept 23 – 26. https://lvkmeeting2024.ifae.es/ * KAGRA site report [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0158/L2415869/001/KAGRAReport_20240702.pdf|07/02]] * Recovery from the Noto Earthquake Disaster * Next meeting is 07/24(Wed). * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * provide the CAT1 veto-definer file for IPC glitch (Uchikata) * Minutes * Comparison of Hveto results according to Omicron HPF(Kihyun Jung) [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=30318|klog#30318]] * (Yamat) The Summary page needs to be updated. It is now a bottleneck for updating the detchar tools in IGWN conda environment. * CBC trigger list for O4a (Uchikata, Narikawa) * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15876|slide]] * Check the details for large chi^2 /SNR triggers. * Generate the lists automatically and upload it to the daily summary page. * Extend the analysis to the CBC search. * We may need to gate the IPC error segments for the search. * O4a event rate by pyCBC search (Narikawa, Uchikata) * If configuration is same as Omicron, we can compare the results. * How does pycbc treat the time-clustering? --> clustered triggers within 10 seconds. * How the clustering length is decided? In Omicron case, the 0.1 clustering length is decided empirically. * Hveto analysis (Kiyun) * Kiyun agreed with the wide presentation for KAGRA collaborators, which will be an alternative presentation in the f2f meeting. * Deep clean(Shu-Wei Yeh) * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15878|slide]] * They checked the response on the strain at the hardware injection. For these data, they didn't apply the deep clean. * Stochastic search (Chia-Hsuan) * Yuzurihara shared the procedure to submit the application of the account on the kmst cluster. * Detchar member (Uchikata+) will prepare the veto definer for IPC glitches instead of segment file. ----- === 20240703 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': O4b will now end 9 June 2025. * [[https://observing.docs.ligo.org/plan/|Run plan(6/17 updated)]] * Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down. * Future meeting * JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.[[https://www.jps.or.jp/activities/meetings/annual/annual-index.php|web]] * KAGRA f2f meeting: 2024/08/21(Wed)~23(Fri) @Tokyo City University [[https://dac.icrr.u-tokyo.ac.jp/KAGRA/KSC/f2f/2024August|web]] * LVK meeting @Barcelona, Spain: Registration is now open. Sept 23 – 26. https://lvkmeeting2024.ifae.es/ * Announcements from Operations (Sawada) * KAGRA site report [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0158/L2415847/001/KAGRAReport_20240618.pdf|06/18]] * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * provide the CAT1 veto-definer file for IPC glitch (Uchikata) * Minutes * Bruco configuration for MICH (yamaT) [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=30133|klog#30133]] * Bruco server was replaced to new system * Inconsistence of number of triggers between Omicron versions [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=30101|klog#30101]] * On LIGO summary page, the old Omicron(>v4.0) seems to run for Hveto analysis. * For Hveto at different computers (Kamioka, Kashiwa, KISTI), we should use the Omicron with the consistent versions. * pyCBC trigger list for O4a data (Narikawa and Uchikata) * They generated the triggers for O4a data. There were no daily fluctuations in the triggers. * The comparison between the O4a triggers and triggers computed by the simulated Gaussian noise is underway. The Gaussian data doesn't include the line noise. * Report of updating the DeepClean results using training and cleaning times that avoid IPC glitches (Shu-Wei Yeh) [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15868|slide]] * Subtraction of the 60 Hz line noise and noise monitored by the microphone is underway. * They showed some improvement by excluding the data of IPC glitches. * (yamaT) How did you confirm the current-voltage monitor can track the line drift? The coherence might not be the evidence for a narrow frequency bin. * (yamaT) Acoustic injection test many times, they investigated the coupling functions between sound and DARM. ----- === 20240626 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': O4b will now end 9 June 2025. * [[https://observing.docs.ligo.org/plan/|Run plan(6/17 updated)]] * Power outage of ICRR Kashiwa campus on 2024/09/28 9:00~18:00 JST. The system-B cluster and Pastevi server will be down. * Conference * JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.[[https://www.jps.or.jp/activities/meetings/annual/annual-index.php|web]] * KAGRA f2f meeting: 2024/08/21(Wed)~23(Fri) @Tokyo City University * Announcements from Operations (Sawada) * KAGRA site report [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0158/L2415847/001/KAGRAReport_20240618.pdf|06/18]] * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * Minutes * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=30013|Usage manual was updated for the latest Omicron (v4.1)]] * We compared the number of triggers between different Omicron versions (v4.1 and v3.1) in root/hds5/xml formats. * Based on the reply from the developer, the Omicron (v3.1) had the bug. The developer recommends using the latest Omicron for the analysis. * Yuzurihara updated [[https://dac.icrr.u-tokyo.ac.jp/KAGRA/DAWG/Detchar/Omicron|usage manual]] for v4.1 using the hdf5 format. * Update for gates found in stochastic search (Chia-Hsuan) * The gating with 3.5 s tme window was applied in pygwb when the large transient (IPC glitch) occurred. To mitigate the length losing by gating, it's better to usr the veto-definer. * Uchikata-san have an experience on the veto-definer. She will try to prepare it. * Currently they analyzed O4a data (L1, H1, K1) on CIT. But, the L1 and H1 data are stored in system-B(kmst2). * Trigger generation for O4a data by pycbc (Narikawa) * They showed the result of comparing the O4a triggers with the triggers computed by Gaussian noise (~5days). The discussion is underway. * Hveto analysis (Syifa) * Analysis-flag change: https://hveto.readthedocs.io/_/downloads/en/stable/pdf/ * Glitch investigation (Chia-Jui) * They explained how to apply the whitening: (1) estimate the ASD from the data of (tc-58)~(tc-2), (2) apply the whitening by using the estimated ASD * Based on their request, we shared the list of aux. channel which was used in O4a Hveto analysis in Summary page. [[https://github.com/gw-detchar/tools/blob/master/Hveto/etc/k1-hveto-daily-o4.ini|git]] ----- === 20240619 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': O4b will now end 9 June 2025. * [[https://observing.docs.ligo.org/plan/|Run plan(6/17 updated)]] * Power outage of ICRR Kashiwa campus on 2024/09/28 9:00~18:00 JST. The system-B cluster and Pastevi server will be down. * Conference * JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.[[https://www.jps.or.jp/activities/meetings/annual/annual-index.php|web]] * KAGRA f2f meeting: 2024/08/21(Wed)~23(Fri) @Tokyo City University * Announcements from Operations (Sawada) * KAGRA site report [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0158/L2415835/001/KAGRAReport_20240607.pdf|06/07]] * new commissioning leader: Takafumi Ushiba * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * Minutes * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28986|O4a summary page]] * This task is finished. The summary page is available [[https://www.icrr.u-tokyo.ac.jp/~uchikata/Detchar/O4aSumm/gps/1368975618-1371337218/|here]]. * The data set for the inspiral range is also available on system-B. * pyCBC trigger list for O4a data (Narikawa and Uchikata) * They are working on comparing the effect by changing the segment durations of 256s and 128s. * In the future, we will connect the trigger results with the summary page. * Currently they produced the triggers by using the template of 1.4-1.4Msun. * Glitch classification * They showed the summaries of the glitch classification. * The glitches located in the upper right on Q-transform might be related to the lockloss. ----- === 20240612 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': We plan to commence O4b at 1500 UTC (2400 JST) on '''10 April 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda240321|internal discussion]], [[https://observing.docs.ligo.org/plan/|public announcements]] * [[https://observing.docs.ligo.org/plan/|Run plan(5/23 updated)]] * Power outage of ICRR Kashiwa campus on 2024/09/28 9:00~18:00 JST. The system-B cluster and Pastevi server will be down. * Conference * JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.[[https://www.jps.or.jp/activities/meetings/annual/annual-index.php|web]] * KAGRA f2f meeting: 2024/08/21(Wed)~23(Fri) @Tokyo City University * Announcements from Operations (Sawada) * KAGRA site report [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0158/L2415835/001/KAGRAReport_20240607.pdf|06/07]] * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * Minutes * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * Computed the inspiral range from the strain channel with gwpy. Basically they used only the data in the science mode. * The histogram of the inspiral range changed. We can see the peak on the histogram. * pyCBC trigger list for O4a data (Narikawa and Uchikata) * They computed the triggers by using pycbc package from the strain data and packed in the xml. * The analyzed data include the IPC glitches. But, the chi-square could mitigated the glitch effect. * (Yuzu) Did you find the interesting or new triggers? --> no. Data seems stable. * (YamaT) Can you compare the trigger histogram with the one from Gaussian noise data? --> not yet. It's possible by replacing the input data with the generated Gaussian noise. * Glitch classification (Hsu Shih-Hong) * They took the average of the Q-spectrograms for each class. The obvious common features were not observed. * They tried to extract the common features on the Q-spectrograms. * It's important to take into account of the whitening effect. The whitening in gwpy could make the sharp glitch wider. ----- === 20240605 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': We plan to commence O4b at 1500 UTC (2400 JST) on '''10 April 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda240321|internal discussion]], [[https://observing.docs.ligo.org/plan/|public announcements]] * [[https://observing.docs.ligo.org/plan/|Run plan(5/23 updated)]] * Next 10yr Task Force Meeting: 2024/06/07 17:00JST, see [kagra 06570] * Power outage of ICRR Kashiwa campus on 2024/09/28 9:00~18:00 JST. The system-B cluster and Pastevi server will be down. * JPS registration: 2024/5/21~6/5 [[https://www.jps.or.jp/activities/meetings/annual/annual-index.php|web]] * Does anyone have a presentation related to DetChar activity? * Announcements from Operations (Sawada) * KAGRA site report [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0158/L2415802/001/KAGRAReport_20240522.pdf|05/22]] * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * isotropic stochastic search result (Chia-Hsuan) * Minutes * In next JPS meeting(Sep.), YamaT plan to talk the detchat topics related to the web service (https://gwdet.icrr.u-tokyo.ac.jp/~controls/misc/html/). * Issue of monopolizing the CPU resources of system-B cluster. (this might be the third time in my memory) * Yuzurihara contacted the administrators to set some threshold or update the cluster settings so that the job submission system will manage the jobs submitted by many users effectively. Still no response from the administrators. * isotropic stochastic search result (Chia-Hsuan) [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15825|slide]] * They analyzed the O4a KAGRA data with other detectors by using the pygwb pipiline, at CIT cluster. * They found the strange peak on the gating length. They shared the list of the gated time. The comparison between the list and the time of IPC glitches will be done soon. * They reported the coherence between KAGRA and LIGO (Livingston and Hanford). About the coherence of 960 and 961 Hz, yamaT pointed out that it came from the timing system. We use the same timing system between KAGRA and LIGO. See also [[https://alog.ligo-la.caltech.edu/aLOG/index.php?callRep=71308|alog]]. * AI for detchar: Collect the information of the remaining frequencies with coherence * (YamaT) How did you integrate the data for narrow-line analysis? --> all of the science mode * How was the gate process applied? * What is the good frequency band for the analysis? --> (YamaT) Comments from the calibration side: use 30~1000Hz. * Glitch classification (Chia-Jui) [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15824|slide]] * They reported the glitches detected in O4a data can be classified into several classes by using unsupervised classification. * Q-transform plots are available [[https://git.ligo.org/agoodmanjerry/k1-o4a-glitches/-/tree/main/O4a-no-ipc/K1/q_spectrogram_4s_snr_g10?ref_type=heads|git]]. * Yama-T commented on slack that the glitch effect might be widen by the whitening process. * O4a summary page (Uchikata) * We have decided to compute the inspiral range without the gwsumm. The computation is on-going. ----- === 20240529 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': We plan to commence O4b at 1500 UTC (2400 JST) on '''10 April 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda240321|internal discussion]], [[https://observing.docs.ligo.org/plan/|public announcements]] * [[https://observing.docs.ligo.org/plan/|Run plan(5/23 updated)]] * Next 10yr Task Force Meeting: 2024/06/07 17:00JST, see [kagra 06570] * Power outage of ICRR Kashiwa campus on 2024/09/28 9:00~18:00 JST. The system-B cluster and Pastevi server will be down. * Renewal of the account on KAGRA Main Data System: deadline 2024/05/31 * JPS registration: 2024/5/21~6/5 [[https://www.jps.or.jp/activities/meetings/annual/annual-index.php|web]] * Does anyone have a presentation related to DetChar activity? * KAGRA site report [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0158/L2415802/001/KAGRAReport_20240522.pdf|05/22]] * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * Minutes * Glitch analysis (Ishikawa) * The Omicron analysis for non-stationary noise around 360 Hz is on-going. * There might the 5-minutes fluctuation on the inspiral range. The analysis for other data will be done next. * Glitch analysis (Chia-Jui) * The Omicron analysis for the science mode excluding the IPC glitch is on-going. * (Guo Chin Liu) Do you have a flag to indicate the glitch time? --> Omicron provide the time of the glitch. * (Guo Chin Liu) What is the ratio in the science mode? * He found several characteristic types of glitches in KAGRA O4a data. For details, see [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15808|slide]]. * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=29675|klog]] * Hveto analysis (Syifa) * Hveto analysis with high pass filter is on-going. * Dedicated O4a summary page (Uchikata) * She found that the cache file for O4a data has the issue of overlapping or missing. She updated the cache file. [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=29592|Modification of cache files at system B]] * (Sawada) Matlab on the LDAS cluster will stop on the next maintenance day. If you want to use the Matlab on LDAS cluster, please contact with Sawada-san. ----- === 20240515 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': We plan to commence O4b at 1500 UTC (2400 JST) on '''10 April 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda240321|internal discussion]], [[https://observing.docs.ligo.org/plan/|public announcements]] * KAGRA detchar liaison to CBC group * Nami Uchikata as the new liaison between the CBC group and the KAGRA Detchar group. * KAGRA site report * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * Minutes * Update contents of summary page (Oshino) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=29496|4.5 Hz peak of IMC]] * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=29439|Modified IMC page on SummaryPage]] * Hveto (Shifa) * By changing cutoff frequency of 8 or 12Hz, they checked the Hveto results and found the artificial glitches around 10Hz. * When they apply the HPF with 6 Hz or 4 Hz, the artificial glitches around 10Hz disappeared. * (YamaT) Do you know the design of HPF (butterworth?)? * (Uchikata) Minimum frequency of Hveto should be larger than the cutoff frequency of high pass filter in Omicron. * (YamaT) It might make the ripple. * (Yuzu) You can analysis the Omicron triggers with the higher cut-off frequency. * Glitch analysis (Ishikawa) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=29454|klog#29454]] [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15785|slide]] * (Chia-Jui) How do you set-up the Omicron configuration files? --> Same as commonly used one. * (Chia-Jui) What was the typical SNR of 300-500Hz? --> SNR 6~10? He didn't have a clear answer. He will check it. * Glitch analysis (Chir-Jui) * Omicron analysis without high pass filter was done. * In page 7, there were gaps due to the exceed of threshold of glitch rate. At that time, Omicron failed due to the error. * We confirmed the goal of the Detchar activity is to contribute the sensitivity or noise hunting of KAGRA. ----- === 20240508 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': We plan to commence O4b at 1500 UTC (2400 JST) on '''10 April 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda240321|internal discussion]], [[https://observing.docs.ligo.org/plan/|public announcements]] * Introduction of new comer * KAGRA site report * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * Minutes * Omicron triggers at System B (Uchikata) [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=29328|klog]] * Update contents of summary page (Oshino) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=29408|Add shindo plots on SummaryPage]] * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=29387|Update navigation bar on SummaryPage]] * line identification by fscan for kagra (Takahiro.S.Yamamoto) [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15768|slide+supplement]] * What is the frequency resolution? * Segment duration of 1800 s is a typycal value in continuous wave search? --> yes * Is is posible to real-time monitoring of 60 Hz? * What is the advantage to used fscan? * The result for O4a data is available on the [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/fscan/summ/fscans_2023_05_31_09_00_00_JST/K1_CAL-CS_PROC_DARM_STRAIN_DBL_DQ/fscanK1_CAL-CS_PROC_DARM_STRAIN_DBL_DQ_K1_1369526418_1369612818.html|web]]. Due to computational costs, we didn't use aux. channels. * Hveto analysis (Kyujin, Kihyun, Syifa) * By adding the high pass filter, the artificial glitches appeared, although there is no such glitches in Uchikata-san's results. * Omicron on K1 O4a Data (Chia-Jui) [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15769|slide]] * They proposed the way to identify the IPC glitches. --> The way to identify the IPC glitches was already established. * They found three classes of glitches in KAGRA data. * Dedicated summaru page for O4a KAGRA (Uchikata) * When we compute the inspiral range by reading the data from NDS server, ----- === 20240424 (Wed.) === * Agenda * Announcement * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': We plan to commence O4b at 1500 UTC (2400 JST) on '''10 April 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda240321|internal discussion]], [[https://observing.docs.ligo.org/plan/|public announcements]] * Introduction of new comer * KAGRA site report * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * cache file for O3GK and O4a * pyCBC trigger list for O4a data (Narikawa and Uchikata) * Minutes * Meeting on Next week will be canceled. Next meeting is 8 May. * Report of KIW and open data workshop#7 (Yuzurihara) * Computer cluster at Kamioka (Oshino) * We purchased the rack. In future, we move the computer in the rack. * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * Confirmation of the result is on-going. * The scale of histogram was changed. The apperance looks consistent with the dedicated summary page and the YamaT-san's [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/misc/html/binaryRanges_o4a.html|result]]. * TODO: Inspiral range should be computed from the strain channel, not using the RANGE channel. That Range channel is used for the prompt report. * Hveto (Kyujin, Kihyun, Syifa) * The analysis result was explained in the meeting. * The high pass filter with 10 Hz or 15 Hz was applied for the Omicron analysis. The frequency range for Omicron should be tuned at the same time to mitigate the artificial noise in the Omicron triggers. * whale-like shape disappered in the histogram of Omicron triggers when we remove the segment of IPC glitch from the analysis. * Is there any suggestion to the interferometer experts? For example, which channels seems problematic. * Glitch investigation (Ishikawa) * Studying the Omicron pipeline and applying to the KAGRA's O4a data [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15747|Progress report]] * Line investigation (Samurai) * Reading Fscan paper for past observation run (S6, O1, O2). The report will be done in the future meeting. ----- === 20240410 (Wed.) === * Agenda * Announcement * KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 [[https://indico.phys.sinica.edu.tw/event/92/|web]] * Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 [[https://indico.phys.sinica.edu.tw/event/92/page/220-gravitational-wave-open-data-workshop|web]], [[https://gwosc.org/odw/odw2024/|Info. from GWOSC]] * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': We plan to commence O4b at 1500 UTC (2400 JST) on '''10 April 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda240321|internal discussion]], [[https://observing.docs.ligo.org/plan/|public announcements]] * Introduction of new comer * KAGRA site report * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * pyCBC trigger list for O4a data (Narikawa and Uchikata) * Minutes * pyCBC trigger list for O4a data (Narikawa and Uchikata) * Use segment information of SCIENCE MODE + IPC glitch ==> ongoing * ongoing * Change data length 4096s -> 64s. Apply the high pass filter before splitting the data. ==> done * Estimate common PSD and use it for the analysis ==> done * Is it possible to output the trigger list in xml format? * https://gwpy.github.io/docs/latest/table/io/#ligo-lw-xml ----- === 20240403 (Wed.) === * Agenda * Announcement * KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 [[https://indico.phys.sinica.edu.tw/event/92/|web]] * Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 [[https://indico.phys.sinica.edu.tw/event/92/page/220-gravitational-wave-open-data-workshop|web]], [[https://gwosc.org/odw/odw2024/|Info. from GWOSC]] * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4b''': We plan to commence O4b at 1500 UTC (2400 JST) on '''10 April 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda240321|internal discussion]], [[https://observing.docs.ligo.org/plan/|public announcements]] * Update of DQSEGDB server [[https://git.ligo.org/computing/helpdesk/-/issues/5672|help ticket]] * KAGRA site report * Budget request * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * pyCBC trigger list for O4a data (Narikawa and Uchikata) * Minutes * Upgrade DetChar computers (YamaT) * waiting the update of workstation machines. I will take a few monthes. * DQR update (Yuzurihara) * no update. * Update contents of summary page (Oshino) * no update * Hveto (Kyujin) * Trouble on KISTI cluster. * pyCBC trigger list for O4a data (Narikawa and Uchikata) * Use segment information of SCIENCE MODE + IPC glitch * Change data length 4096s -> 64s. Apply the high pass filter before splitting the data. * Estimate common PSD and use it for the analysis * Is it possible to output the trigger list in xml format? ----- === 20240326 (Wed.) === * Agenda * Announcement * KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 [[https://indico.phys.sinica.edu.tw/event/92/|web]] * Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 [[https://indico.phys.sinica.edu.tw/event/92/page/220-gravitational-wave-open-data-workshop|web]], [[https://gwosc.org/odw/odw2024/|Info. from GWOSC]] * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''ER16''': It will nominally start at 1500 UTC (2400 JST) on '''20 Mar 2024''', and last for 2 weeks. * '''O4b''': We plan to commence O4b at 1500 UTC (2400 JST) on '''3 April 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda240321|internal discussion]], [[https://observing.docs.ligo.org/plan/|public announcements]] * KAGRA site report * Budget request * Progress reports * Upgrade DetChar computers (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * pyCBC trigger list for O4a data (Narikawa and Uchikata) * Minutes * Budget request * New computers for replacing too old servers (k1det0, 1): 500k-yen x2 * HDD for new systems: 10k-yen x10-20 * Progress reports * Upgrade DetChar computers (YamaT) * Testing DetChar softwares can be started after the update of CDS workstations is completed. * Test of CDS workstation needs more time (hopefully by end of April) * DQR update (Yuzurihara) * No update * Update contents of summary page (Oshino) * No update * Related to segment files (Uchikata, Narikawa) * No update * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) * [[https://www.icrr.u-tokyo.ac.jp/~uchikata/Detchar/O4aSumm/gps/1368975618-1371337218/range/]] * SummaryPages process was executed on Kashiwa System-B. * Results were copied to the personal region of ICRR's Web server. * Finally this page will be opened only for LVK folks(?) on gwdet. * pyCBC trigger list for O4a data (Narikawa and Uchikata) * No update ----- === 20240306 (Wed.) === * Agenda * Announcement * KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 [[https://indico.phys.sinica.edu.tw/event/92/|web]] * Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 [[https://indico.phys.sinica.edu.tw/event/92/page/220-gravitational-wave-open-data-workshop|web]], [[https://gwosc.org/odw/odw2024/|Info. from GWOSC]] * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''ER16''': It will nominally start at 1500 UTC (2400 JST) on '''20 Mar 2024''', and last for 2 weeks. * '''O4b''': We plan to commence O4b at 1500 UTC (2400 JST) on '''3 April 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda231214#Agenda|internal short announcements (reminders)]], [[https://observing.docs.ligo.org/plan/|public announcements]] * LVK meeting on March 11-14 at Louisiana State University [[https://www.lsu.edu/physics/lvkmeeting/|web]] * There is no fee for online participants * Update of member list for DetChar mailing list * KAGRA site report * Task list for the authorship 2024 * Progress reports * O4a summary page(Uchikata) * After several attempts, the job was finished without errors. Another small problems, ----- === 20240228 (Wed.) === * Agenda * Announcement * KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 [[https://indico.phys.sinica.edu.tw/event/92/|web]] * Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 [[https://indico.phys.sinica.edu.tw/event/92/page/220-gravitational-wave-open-data-workshop|web]], [[https://gwosc.org/odw/odw2024/|Info. from GWOSC]] * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''ER16''': It will nominally start at 1500 UTC (2400 JST) on '''20 Mar 2024''', and last for 2 weeks. * '''O4b''': We plan to commence O4b at 1500 UTC (2400 JST) on '''3 April 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda231214#Agenda|internal short announcements (reminders)]], [[https://observing.docs.ligo.org/plan/|public announcements]] * LVK meeting on March 11-14 at Louisiana State University [[https://www.lsu.edu/physics/lvkmeeting/|web]] * Early Registration is open until February 1 * There is no fee for online participants * Update of member list for DetChar mailing list * KAGRA site report * Task list for the authorship 2024 * Progress reports * Minutes * Task list for the authorship 2024 (not fixed yet) {{{ 1. Commissioning support : serving data monitoring tools for site commissioners. This task focuses on the support of the IFO lock trial and/or noise hunting based on the request from the interferometer commissioners. Support of analyses to measured data (e.g. noise projection to the DARM with measured noise and TFs) is also contained in this task. Specialized tasks for each subgroup should be applied for in the respective group task. 2. Production and validation of Online Data Quality State Vector (for O4b/O5 preparation. This task focusing on providing the online DetChar products such as the online DQSV and managing various reliable online flags. Developing real-time and guardian codes for providing such flags should be contained in this task. 3. Production and validation of Segment information for O4b/O5 preparation. This task focusing on providing low-latency/offline segments. Providing segment itself, evaluation of efficient channels to make segments, evaluating benefit of segments on GW searches and cooperation with CIT staffs to update segment contents on DQSEGDB are contained in this task. 4. Construction of DQR (Data Quality Report) and igwn-alert framework for O4b/O5 RRT activities. This task focusing on providing contents from KAGRA to DQR web pages which is merged with LIGO, Virgo and KAGRA. 5. Support of Data Analysis group to set Data Category criteria for O4b/O5 joint observing run. This task focusing on the support of the GW-search activities based on the each WG of DAC. Providing data category for the pipelines of each GW sources, providing veto segments and other noise information such as identified spectral lines are also contained in this task. 6. Managing DET computers and their environments. This task contains the computer environment construction for providing the DetChar products in the cadence of online/low-latency/offline. Managing dedicated servers for sharing DetChar products among LVK is also contained in this task. ===== - Noise hunting in KAGRA commissioning. Obsolescent Noise *hunting* without IFO (hardware) experts is unrealistic. In this meaning, the most of noise *hunting* can be covered in "Commissioning support”. If the tasks are related to the noise *finding* for the purpose of providing veto segment, they can be covered in “Support of Data Analysis”. }}} * hveto analysis is contained in 1. in the case that there is some communication with onsite commissioners via klog etc. * It's also potentially contained in 5. in the case of providing veto-ed segments, correlated channels etc. * Providing Run SummaryPage is contained in 5. * Exact sentence as "Making Run Summary" should be added the description in 5. |
| Line 605: | Line 807: |
| ----- === 20210401 (Thu.) === * Agenda * Progress of hveto analysis * DetChar cluster * lvalert * SummaryPages * RRT for O4 * Minutes * Announcement * New slot of DET meeting. * => Pending because TY cannot know free time slot yet. (7 doodle poll is running...). * hveto * Omicron test analysis is successful. * hveto doesn't run on m31 yet. * We need to KISTI environment. * lvalert * Waiting response from LV people. * We need realistic json format of GW alert. * Only for the purpose of launching pipelines, dummy format is also used. * SummaryPages * The 1st version of VIS tab is already available (Only Type-A and guardians). * Importing PSL tab from LIGO is already done. * But there is many difference of channel name convention. ----- === 20210325 (Thu.) === * Agenda * Progress of hveto analysis * GEO data analysis * SummaryPage construction * lvalert test * PMC/IMC commissioning * Meeting time in the next FY * Minutes * Progress of hveto analysis * Consistency check still remains and it is solved yet. * GEO data analysis * Basic takeover is finished. * Uchikata-san and Narikawa-san can start to use Omicron and hveto. * But some error occurs on hveto@m31. * We should fixed environmental problem. * SummaryPage construction * The 1st version is already constructed on test directory. * We can apply it for product environment because current SummaryPage is not valid. * lvalert test * lvalert itself works well. * Next step is receiving alert. * We need to ask LIGO people about alert format etc. * PMC/IMC commissioning * Due to a lot of troubles, we haven't achieved IMC locked yet. * We may start some kind of commissioning from Mid or Late of April. * Meeting time in the next FY * TY will circulate doodle poll. === 20210317 (Thu.) === * O3GK paper * hveto cross-check * Checking Omicron parameter remains. * Required re-run for whole two weeks. * veto segment production * Merging short segments is not required. * GEO data analysis * It can be done by someone form Tagoshi-san's group. * O4 preparation * Kamioka cluster * It's pending due to the recovery work of power outage. * Takeover about Omicron, hveto, GlitchPlot * Takeover itself is done. * TY is finding candidate person of each pipelines toward O4. * Omega-scan test * Installing on Kashiwa * lvalert test * It's works well on k1det1 * SummaryPage update * The 1st version of VIS page is constructed. * It's being checked by Miyo-kun. * IMC commissioning * It is not locked yet because of some troubles. === 20210225 (Thu.) === * Agenda * Progress of O3GK paper * O4 preparation * Minutes * Progress of O3GK paper * Chihiro re-analysis with proper science segment for omicron triggers. * A part of Kihyun's analysis is done. * Cross-check can be done. But not start yet. * DetChar cluster in Kamioka * http://klog.icrr.u-tokyo.ac.jp/osl/?r=16082 * OS installation for master node was done. * Omega-scan test * Installation for Kashiwa cluster was done. * Error is occurred on gwdatafind. * SummaryPages * LVAlert ----- === 20210218 (Thu.) === * Agenda * Progress of O3GK paper * O3 data replay * O4 preparation * Minutes * Progress of O3GK paper * hveto conf is same * segment is used as latest same science segments * definition of cutting end of segments is difference. * Channel list is used as on github's one. * Next step -> unifying cutting definition. * Kihyun will re-run omicron with new segment cutting definition * We need to merge veto segment from a lot of short ones to continuous one. * O3 data replay * Main purpose of O3 data replay is performing end-2-end test of low-latency pipelines (CAL, DET, DAS, etc). * LV will use real O3 data. * KAGRA provides simulated data (~80Mpc for BNS) because of too poor sensitivity of O3GK data. * We may need to inject GWs on software with consistency with LV's real events. * Frame work of software injection is already available. * SummaryPage * Updating VIS page. * It will be closed to LIGO's one. * LVAlert * k1det1 can be used for test. * Need personal account because we use personal DCC account for accessing GraceDB. * Ask LV people how to get common account on next LVK DET meeting. ----- === 20210204 (Thu.) === * Agenda * Progress of O3GK paper * O3 data replay * O4 requirement * Minutes * Progress of O3GK paper * Omicron trigger transfer: Kamioka -> KISTI, it is postponed. * Young-Min asked KISTI administrator. * GW-search triggers have not been served yet. * O3 data replay * K1:OPS-SIM_GAUSS1_IN1 (simulated error signal) * K1:OPS-SIM_GAUSS1_OUT (simulated h(t) ) * gaussian noise as floor level * Some spectral lines (cal lines, violin mode, power lines) * Simulated glitches. * K1:OPS-SIM_GAUSS3_OUT (simulated auxiliary channel) * O4 requirement * DQ state vector (Yamamoto) * Providing on real-time model. * Data Quality Report (Yuzurihara) * First step is to use lvalert in order to receive GW alert from GraceDB. * Transient Event validation (Kozakai) * Basic idea is omicron+hveto (same as O3GK) * Takeover should be done from Kozakai-san. * Category veto (Yamamoto) * At least CAT1 should be provided. * We need to convert to veto-definer file format. * Spectral lines investigation (Yokozawa) * Listing of VIS-derived peak frequencies. ----- === 20210128 (Thu.) === * Agenda * Report from Burst search * Binary range evaluation with C20 offline h(t) * Progress of O3GK paper * Minutes * Report from Burst search * * Binary range evaluation with C20 offline h(t) * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12499|slide]] * Multi-taper and Welch show similar results * Bayesline result is slightly different from results by other two methods. * Estimated values are enough for O3GK (search) paper. * LVK review of this work is necessary for publishing results. * Progress of O3GK paper * === 20210121 (Thu.) === * Agenda * Announcement * LVK DetChar call will be held (Jan. 25 19:00 JST, KST) * Progress of O3GK paper * CAGMon results * O3 Data replay * Minutes * Progress of O3GK paper * Some difference between Kihyun's and Chihiro's results. * hveto setting should be tuned on conf file and re-run again. * GW search results will be provided 1-2 months later (?). * CAGMon results * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12481|slide]] * O3 data replay * LV requested the simulated data instead of O3GK data as KAGRA's data. * Auxiliary channels which has realistic coherence, coincidence etc are not available. * All multi-channel analyses cannot work well in such situation. * We need more discussion how do we join O3 data replay. === 20210107 (Thu.) === * Agenda * Progress of O3GK analysis * O4 preparation * Minutes * Progress of O3GK analysis * Analysis itself was finished. * Results by Chihiro and Kihyun are now comparing. * => Some conf. is still difference. * At least after finishing paper work, omicron triggers should be shared on Kashiwa cluster for remote site people. * O4 preparation * Model update will be finished soon. * => After model update, suspension commissioning will be started. * SummaryPages seems to be stopped. * => Because of the channel name update by VIS model changes. * => Current situation of real-time model is slightly complicated. ITMY: Old model, others: new model etc. * => After finishing CRY measurements, all suspension models are unified. |
* Progress reports * Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT) * start consideration about the system upgrade to new Debian system. * DET tools depend on the CDS tools and CDS tools are well managed on apt-repository. * Only a part of CDS tools can be available on Anaconda now. * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Combine DET computer resources into one DET cluster at Kamioka site * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) [[https://ldas-jobs.ligo.caltech.edu/~detchar/summary/O4a/|O4a (LV)]] * pyCBC trigger list for O4a data (Narikawa and Uchikata) [[https://ldas-jobs.ligo-wa.caltech.edu/~detchar/summary/day/20240108/detchar/pycbc_live_medium/| O4a (H1)]] * 4000s data analysis is ongoing. * Processed time is a few hours * Used template is changed from BBH to BNS. * Trigger behavior is changed by used templates. * Generated triggers are in the text format. * If LIGO's XML (LW XML?) is available, it may be very easy to make various plots on SummaryPages. ----- === 20240221 (Wed.) === * Agenda * Announcement * KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 [[https://indico.phys.sinica.edu.tw/event/92/|web]] * Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 [[https://indico.phys.sinica.edu.tw/event/92/page/220-gravitational-wave-open-data-workshop|web]] * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''ER16''': It will nominally start at 1500 UTC (2400 JST) on '''20 Mar 2024''', and last for 2 weeks. * '''O4b''': We plan to commence O4b at 1500 UTC (2400 JST) on '''3 April 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda231214#Agenda|internal short announcements (reminders)]], [[https://observing.docs.ligo.org/plan/|public announcements]] * LVK meeting on March 11-14 at Louisiana State University [[https://www.lsu.edu/physics/lvkmeeting/|web]] * Early Registration is open until February 1 * There is no fee for online participants * Update of member list for DetChar mailing list * KAGRA site report (Yuzurihara) * Commissioning support + tasks related to O4a * O4a for KAGRA : 2023/05/25 0:00 JST (=2023/05/24 15:00UTC) ~ 2023/06/21 8:00 JST * Event validation (YamaT) * Online data quality state vector (YamaT) * Tool to evaluate Gaussianity (Yamamura) * Scattered light noise (Yamamura) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28584|Investigation of scattered light noise in O4a]] [[https://dac.icrr.u-tokyo.ac.jp/KAGRA/DAWG/Detchar/klog/klog28584|plots]] * Pastavi update (Yuzurihara) * Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa) * Classification of glitch noise (Shikano, Oshino) * IPC glitch * line noise study (Samurai) * Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Combine DET computer resources into one DET cluster at Kamioka site * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) [[https://ldas-jobs.ligo.caltech.edu/~detchar/summary/O4a/|O4a (LV)]] * pyCBC trigger list for O4a data (Narikawa) * Minutes ----- === 20240214 (Wed.) === * Agenda * Announcement * KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 [[https://indico.phys.sinica.edu.tw/event/92/|web]] * Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 [[https://indico.phys.sinica.edu.tw/event/92/page/220-gravitational-wave-open-data-workshop|web]] * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''ER16''': It will nominally start on '''13 Mar 2024''', and last for 2 weeks. (Note that ER16 will begin in the middle of the next LVK meeting at LSU, 11-14 March.) * '''O4b''': We plan to commence O4b at 1600 UTC (2500 JST) on '''27 Mar 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda231214#Agenda|internal short announcements (reminders)]], [[https://observing.docs.ligo.org/plan/|public announcements]] * White paper and task list for 2024 [[https://git.ligo.org/operations/operations-white-paper-2023|git repo]] * LVK meeting on March 11-14 at Louisiana State University [[https://www.lsu.edu/physics/lvkmeeting/|web]] * Early Registration is open until February 1 * There is no fee for online participants * Update of member list for DetChar mailing list * KAGRA site report (Yuzurihara) * Commissioning support + tasks related to O4a * O4a for KAGRA : 2023/05/25 0:00 JST (=2023/05/24 15:00UTC) ~ 2023/06/21 8:00 JST * Event validation (YamaT) * Online data quality state vector (YamaT) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28555|Sanity check of DAC saturation bit provided by a new model]] * Tool to evaluate Gaussianity (Yamamura) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28568|Investigation of scattered light noise in O4a]] * Scattered light noise (Yamamura) * Pastavi update (Yuzurihara) * Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa) * Classification of glitch noise (Shikano, Oshino) * IPC glitch * line noise study (Samurai) * Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Combine DET computer resources into one DET cluster at Kamioka site * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) [[https://ldas-jobs.ligo.caltech.edu/~detchar/summary/O4a/|O4a (LV)]] * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28538|O4a summary page]] * pyCBC trigger list for O4a data (Narikawa) * Minutes * Online data quality state vector (YamaT) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28555|Sanity check of DAC saturation bit provided by a new model]] * We need same test for ETMY model. * Scattered light noise (Yamamura) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28568|Investigation of scattered light noise in O4a]] * (oshino) why the double bounce occurred? * (yamaT) it's better to check both the feedback and error signal (OUT_DQ and IN1_DQ). * (oshino) PD signal might be helpful in the investigation. In POP_FORWARD, the scattered light was seen in the past. * Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa) * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15527|KAGRA O4a hveto results (0524 ~ 0606)]] [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15632|KAGRA O4a hveto results (0607 ~ 0619)]] * hveto shows the many triggers on the time the scattered light noise appeared * (yamaT) IPC glitch was taken care in this analysis? It's better to use SCIENCE segment + IPC glitch segment. * It is interesting to compare the glitch rate and the analysis result with and without IPC glitch segments. * Yuzurihara shared that segment with Kihyun. * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) [[https://ldas-jobs.ligo.caltech.edu/~detchar/summary/O4a/|O4a (LV)]] * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28538|O4a summary page]] * pyCBC trigger list for O4a data (Narikawa) * (yamaT) can we include the trigger information by pycbc, in the summary page? ----- === 20240207 (Wed.) === * Agenda * Announcement * KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 [[https://indico.phys.sinica.edu.tw/event/92/|web]] * Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 [[https://indico.phys.sinica.edu.tw/event/92/page/220-gravitational-wave-open-data-workshop|web]] * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''ER16''': It will nominally start on '''13 Mar 2024''', and last for 2 weeks. (Note that ER16 will begin in the middle of the next LVK meeting at LSU, 11-14 March.) * '''O4b''': We plan to commence O4b at 1600 UTC (2500 JST) on '''27 Mar 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda231214#Agenda|internal short announcements (reminders)]], [[https://observing.docs.ligo.org/plan/|public announcements]] * White paper and task list for 2024 [[https://git.ligo.org/operations/operations-white-paper-2023|git repo]] * LVK meeting on March 11-14 at Louisiana State University [[https://www.lsu.edu/physics/lvkmeeting/|web]] * Early Registration is open until February 1 * There is no fee for online participants * Update of member list for DetChar mailing list * KAGRA site report (Yuzurihara) * Commissioning support + tasks related to O4a * O4a for KAGRA : 2023/05/25 0:00 JST (=2023/05/24 15:00UTC) ~ 2023/06/21 8:00 JST * Event validation (YamaT) * Online data quality state vector (YamaT) * Tool to evaluate Gaussianity (Yamamura) * Scattered light noise (Yamamura) * Pastavi update (Yuzurihara) * Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa) * Classification of glitch noise (Shikano, Oshino) * IPC glitch * line noise study (Samurai) * Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Combine DET computer resources into one DET cluster at Kamioka site * Related to segment files (Uchikata, Narikawa) * Provide the dedicated summary page for O4a of KAGRA (Uchikata) [[https://ldas-jobs.ligo.caltech.edu/~detchar/summary/O4a/|O4a (LV)]] * Minutes * Online data quality state vector (YamaT) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28498|model update of k1detdq0]] This is bug fix of production of online data quality state vector related to DAC saturation. * The hardware test will be done this week an next week. * Tool to evaluate Gaussianity (Yamamura) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28519|Relaunch of GauCh]] * The codes were uploaded at [[https://git.ligo.org/yamamura/gauch|git repo]]. The preparation of brief documentation is ongoing. * Classification of glitch noise (Shikano, Oshino) * They restarted this project. The report will be done soon. * Provide the dedicated summary page for O4a of KAGRA (Uchikata) [[https://ldas-jobs.ligo.caltech.edu/~detchar/summary/O4a/|O4a (LV)]] * They tested the conda environment and configuration files for the production of the summary page. Except for the specific short time, they can generated the O4a summary page including duty cycle and inspiral range. * Generation of trigger list by pycbc (Narikawa) * Code test is ongoing by using the short 4096s data of O4a. The timeseries of chi square looks strange. They plan to apply the high pass filter, instead of window function. * (yamat) How do you decide clustering length? * (Narikawa) By software injection, we can evaluate how the SNR spreads and determine the clustering length. ----- === 20240131 (Wed.) === * Agenda * Announcement * KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 [[https://indico.phys.sinica.edu.tw/event/92/|web]] * Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 [[https://indico.phys.sinica.edu.tw/event/92/page/220-gravitational-wave-open-data-workshop|web]] * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''ER16''': It will nominally start on '''13 Mar 2024''', and last for 2 weeks. (Note that ER16 will begin in the middle of the next LVK meeting at LSU, 11-14 March.) * '''O4b''': We plan to commence O4b at 1600 UTC (2500 JST) on '''27 Mar 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda231214#Agenda|internal short announcements (reminders)]], [[https://observing.docs.ligo.org/plan/|public announcements]] * White paper and task list for 2024 [[https://git.ligo.org/operations/operations-white-paper-2023|git repo]] * LVK meeting on March 11-14 at Louisiana State University [[https://www.lsu.edu/physics/lvkmeeting/|web]] * Early Registration is open until February 1 * There is no fee for online participants * Update of member list for DetChar mailing list * LVK MoA survey summary [[https://dcc.ligo.org/G2400189|LIGO DCC]] * KAGRA site report (Yuzurihara) * Commissioning support + tasks related to O4a * O4a for KAGRA : 2023/05/25 0:00 JST (=2023/05/24 15:00UTC) ~ 2023/06/21 8:00 JST * Event validation (YamaT) * Tool to evaluate Gaussianity (Yamamura) * Scattered light noise (Yamamura) * Pastavi update (Yuzurihara) * Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa) * Classification of glitch noise (Shikano, Oshino) * IPC glitch * line noise study (Samurai) * Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * Combine DET computer resources into one DET cluster at Kamioka site * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) [[https://ldas-jobs.ligo.caltech.edu/~detchar/summary/O4a/|O4a (LV)]] * Minutes * Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28392|O4a hveto results]] * line noise study (Samurai) * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15613|slide]] * Is it possible to set the initial parameter in advance, such as prominence and height? * In future, it is better to extend the fft length to be longer for fine frequency resolution. * Update contents of summary page (Oshino) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28397|Update configuration file on SummaryPage]] * Related to segment files (Uchikata, Narikawa) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28399|Glitch rate for O4a]] * provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) [[https://ldas-jobs.ligo.caltech.edu/~detchar/summary/O4a/|O4a (LV)]] * The attempt to generate summary page is on system-B. For reading data, NDS2 server is helpful. ----- === 20240124 (Wed.) === * Agenda * Announcement * KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 * Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 [[https://gwosc.org/workshops/|web]] * LIGO-Virgo-KAGRA detchar joint meeting * tileslot: onthly, 23:00 JST (14:00 UTC) or 6:00 JST (21 UTC) * Last meeting on Nov. 15 23:00 JST (14:00 UTC) [[https://wiki.ligo.org/DetChar/Telecon20231115|wiki]] * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4a''': It will end at 1600 UTC on '''16 Jan 2024'''. LLO will end O4a observing early, at 1400 UTC. * '''ER16''': It will nominally start on '''13 Mar 2024''', and last for 2 weeks. (Note that ER16 will begin in the middle of the next LVK meeting at LSU, 11-14 March.) * '''O4b''': We plan to commence O4b at 1600 UTC (2500 JST) on '''27 Mar 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda231214#Agenda|internal short announcements (reminders)]], [[https://observing.docs.ligo.org/plan/|public announcements]] * Information of O4a [[https://dac.icrr.u-tokyo.ac.jp/KAGRA/Observations/O4a|wiki]] page * White paper and task list for 2024 [[https://git.ligo.org/operations/operations-white-paper-2023|git repo]] * LVK meeting on March 11-14 at Louisiana State University * Update of member list for DetChar mailing list * KAGRA site report (Yuzurihara) * Commissioning support + tasks related to O4a * O4a for KAGRA : 2023/05/25 0:00 JST (=2023/05/24 15:00UTC) ~ 2023/06/21 8:00 JST * Event validation (YamaT) * Tool to evaluate Gaussianity (Yamamura) * Scattered light noise (Yamamura) * Pastavi update (Yuzurihara) * Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa) * Classification of glitch noise (Shikano, Oshino) * IPC glitch * line noise study (Samurai) * Peak identifications [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/misc/html/knownlines_o4a.html|web]] * Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * run Omicron at Kamioka site and refresh the Omicron plots on summary page during O4a period * Combine DET computer resources into one DET cluster at Kamioka site * Script to generate segment files (Uchikata, Narikawa) * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA? [[https://ldas-jobs.ligo.caltech.edu/~detchar/summary/O3a/|O3a (LV)]] * Minutes * Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28392|O4a hveto results]] * Update contents of summary page (Oshino) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28390|Modified configuration file on SummaryPage]] ----- === 20240117 (Wed.) === * Agenda * Announcement * KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 * Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 [[https://gwosc.org/workshops/|web]] * LIGO-Virgo-KAGRA detchar joint meeting * tileslot: onthly, 23:00 JST (14:00 UTC) or 6:00 JST (21 UTC) * Last meeting on Nov. 15 23:00 JST (14:00 UTC) [[https://wiki.ligo.org/DetChar/Telecon20231115|wiki]] * O4a/preO4b(not call it as postO4a)/ER16/O4b schedule: * '''O4a''': It will end at 1600 UTC on '''16 Jan 2024'''. LLO will end O4a observing early, at 1400 UTC. * '''ER16''': It will nominally start on '''13 Mar 2024''', and last for 2 weeks. (Note that ER16 will begin in the middle of the next LVK meeting at LSU, 11-14 March.) * '''O4b''': We plan to commence O4b at 1600 UTC (2500 JST) on '''27 Mar 2024'''. * Ref.[[https://wiki.ligo.org/Operations/Agenda231214#Agenda|internal short announcements (reminders)]], [[https://observing.docs.ligo.org/plan/|public announcements]] * Information of O4a [[https://dac.icrr.u-tokyo.ac.jp/KAGRA/Observations/O4a|wiki]] page * White paper and task list for 2024 [[https://git.ligo.org/operations/operations-white-paper-2023|git repo]] * LVK meeting on March 11-14 at Louisiana State University * KAGRA site report (Yuzurihara) * Commissioning support + tasks related to O4a * O4a for KAGRA : 2023/05/25 0:00 JST (=2023/05/24 15:00UTC) ~ 2023/06/21 8:00 JST * Event validation (YamaT) * Tool to evaluate Gaussianity (Yamamura) * Scattered light noise (Yamamura) * Pastavi update (Yuzurihara) * Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa) * Classification of glitch noise (Shikano, Oshino) * IPC glitch * line noise study (Samurai) * Peak identifications [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/misc/html/knownlines_o4a.html|web]] * Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT) * DQR update (Yuzurihara) * Update contents of summary page (Oshino) * run Omicron at Kamioka site and refresh the Omicron plots on summary page during O4a period * Combine DET computer resources into one DET cluster at Kamioka site * Script to generate segment files (Uchikata, Narikawa) * Related to segment files (Uchikata, Narikawa) * provide the dedicated summary page for O4a of KAGRA? [[https://ldas-jobs.ligo.caltech.edu/~detchar/summary/O3a/|O3a (LV)]] * Minutes * Tool to evaluate Gaussianity (Yamamura) * Gauch recently looks not running. There is no html page linked from summary page. We will check the details later. * DQR update (Yuzurihara) * I asked the remote help to Derek. I'm submitteing the application for the ICRR computer account. * IPC glitch * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28025|Summary of recent segment for IPC glitch (2023/11~12)]] * Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28194|2023-05-24 ~ 06-07 O4a hveto results]] * The analysis for the remained date will be * Update contents of summary page (Oshino) * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28057|Modified configuration files of SummaryPage]] * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=28247|Modified configuration file on SummaryPage]] ----- |
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| * [[KAGRA/Subgroups/DET/Meeting/2023|2023]] * [[KAGRA/Subgroups/DET/Meeting/2022|2022]] * [[KAGRA/Subgroups/DET/Meeting/2021|2021]] |
Meetings
- Meeting time: 11:00-11:30 JST/KST on every Wednesday
- Meeting room: Zoom3
Contents
-
Meetings
-
Agenda & Minutes
- 20241009 (Wed.)
- 20241002 (Wed.)
- 20240911 (Wed.)
- 20240904 (Wed.)
- 20240807 (Wed.)
- 20240731 (Wed.)
- 20240724 (Wed.)
- 20240717 (Wed.)
- 20240710 (Wed.)
- 20240703 (Wed.)
- 20240626 (Wed.)
- 20240619 (Wed.)
- 20240612 (Wed.)
- 20240605 (Wed.)
- 20240529 (Wed.)
- 20240515 (Wed.)
- 20240508 (Wed.)
- 20240424 (Wed.)
- 20240410 (Wed.)
- 20240403 (Wed.)
- 20240326 (Wed.)
- 20240306 (Wed.)
- 20240228 (Wed.)
- 20240221 (Wed.)
- 20240214 (Wed.)
- 20240207 (Wed.)
- 20240131 (Wed.)
- 20240124 (Wed.)
- 20240117 (Wed.)
- Past meeting
-
Agenda & Minutes
Agenda & Minutes
20241009 (Wed.)
- Agenda
- Announcement
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
lock loss study in the commissioning (YamaT, Yuzurihara) web
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- provide the CAT1 veto-definer file for IPC glitch (Uchikata)
- Minutes
Recovery work after Kashiwa cluster maintenance, such as cache file and segment production. (Uchikata) klog
20241002 (Wed.)
- Agenda
- Announcement
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
lock loss study in the commissioning (YamaT, Yuzurihara) web
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- provide the CAT1 veto-definer file for IPC glitch (Uchikata)
- Minutes
Upgrade DetChar computers (YamaT)
- Due to Kachiwa maitanance, nds2 is working partially.
- lock loss study in the commissioning (YamaT, Yuzurihara)
Characterization of relationship between Omicron triggers and inspiral range during O4a (Ishikawa) slide
Line investigation (Takahiro.S.Yamamoto) slide
- Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down.
- Recovery work after Kashiwa cluster maintenance, such as cache file and segment production. (Uchikata)
- Update of the condor in Kashiwa cluster to version 23.0.14
- This version looks fine for stochastic search (Chia-Hsuan)
20240911 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: O4b will now end 9 June 2025.
- Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down.
LIGO Detector Characterization in the first half of the fourth Observing run arxiv
- Scheduled conference
KAGRA site report 09/02
- Next meeting: October 2. We will skip the meeting on September 18 and 25.
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- provide the CAT1 veto-definer file for IPC glitch (Uchikata)
- Announcement
- Minutes
- lock loss study in the commissioning (YamaT, Yuzurihara)
lock loss investigation tool was developed. The web page will be automatically updated: web
- cache file at Kashiwa cluster (Uchikata)
- The cache file included duplicated frame files. By changing the execution timing, this issue was solved.
- Segment reproduction (Uchikata, Narikawa, YamaT, Yuzu)
- There was a missing period at the Kamioka cluster. While generating the segment at the Kashiwa cluster, we noticed that it's important to use the consistent version of gwpy and python-ligo-xml to upload the segment for DQSEGDB. We found a suitable conda environment at the Kaashiwa cluster. The segment file generated in the Kashiwa cluster looks consistent with the one generated in the Kamioka cluster. The next step is to ask Robert to include the updated segments on DQSEGDB.
- Line investigation (Takahiro.S.Yamamoto)
- The script was developed to merge the spreading line noise into one line noise. Although the test script is working well, it requires more time to mature.
- lock loss study in the commissioning (YamaT, Yuzurihara)
20240904 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: O4b will now end 9 June 2025.
- Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down.
- Scheduled conference
KAGRA site report 09/02
- Next meeting: September 11. We will skip the meeting on September 18 and 25.
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- provide the CAT1 veto-definer file for IPC glitch (Uchikata)
- Announcement
- Minutes
- KAGRA student workshop (Yuzurihara)
During the KAGRA student workshop (2024/08/27-29), we visualized the KAGRA data around the trigger time of high chi^2 statistics by using the time-frequency map klog JGWdoc
scattered light affects the high SNR? --> Chi^2 can mitigate the effect of the scattered light
What about the effect on parameter estimation? --> I'm not sure. The effect can be evaluated by analyzing the data injected with scatter light noise.
- Providing segment information on the scattered light noise might be helpful. The difficulty is in identifying the time that occurs when the scattered light is present.
- Chia-Jui-san mentioned the method using the Omicron triggers and Q-transform.
(Narikawa) The other trigger list of high SNR was used? --> Not yet, due to the time constraints
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- There was a missing period at the Kamioka cluster. While generating the segment at the Kashiwa cluster, we noticed that it's important to use the consistent version of gwpy and python-ligo-xml to upload the segment for DQSEGDB. We found a suitable conda environment at the Kaashiwa cluster. The segment file generated in the Kashiwa cluster looks consistent with the one generated in the Kamioka cluster.
- The automatic generation of the cache file sometimes fails at the Kashiwa cluster. We doubt the cause is the cluster setting. We are discussing how to avoid the failure of cache file generations.
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- He injected the BNS signal into the data using Bilby and showed the reconstruction result.
- The duration of the BNS template (fmin=30Hz) is 250s.
- Line investigation (Takahiro S Yamamoto)
- He implemented the code to generate the normalized spectrum. By eyeball check, the result looks consistent with the results by YamaT-san.
- The next step is to fit the line peak using Gaussian or Lorenzian distribution and characterize the line width and stability of the frequency.
- Clustering might be necessary to merge the broad line noise into one line.
- KAGRA student workshop (Yuzurihara)
20240807 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: O4b will now end 9 June 2025.
- Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down.
- Request to reduce batch job during 8/27-30 for the Student Workshop (See [kagra 06769])
- Scheduled conference
KAGRA f2f meeting: 2024/08/21(Wed)~23(Fri) @Tokyo City University web
Satellite meeting for noise reduction of KAGRA: 2024/08/24 9:00~12:00 web
JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.web
LVK meeting @Barcelona, Spain: Registration is now open. Sept 23 – 26. web
JGRG33 @Kindai University: 2024/12/02(Mon)~2024/12/6(Fri) web
KAGRA site report 07/29
- Next meeting is September 4
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- provide the CAT1 veto-definer file for IPC glitch (Uchikata)
- Announcement
- Minutes
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
Although they updated the way of clustering, the basic feature didn't change. slide
The usage manual for veto definer was prepared by Uchikata-san usage manual for veto definer
- Hveto analysis
- The comparison between Omicron 2.4 and 3.2 was done
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
20240731 (Wed.)
- Wide presentation of PhD thesis
- Date: Wednesday, July 31 at 11:00 JST/KST or 2:00 UTC. (20~30 min. for the presentation. 10~15 min. for the question.)
- Presenter: Kihyun Jung
- Thesis title: Classification and Analysis of KAGRA Glitch
Thesis manuscript: https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=15866
20240724 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: O4b will now end 9 June 2025.
- Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down.
- Scheduled conference
KAGRA site report 07/16
- Next meeting is 08/07(Wed). Next week, we will have Wide presentation of PhD thesis by Kihyun.
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- provide the CAT1 veto-definer file for IPC glitch (Uchikata)
- Announcement
- Minutes
Add cooler ondotori page (Oshino) klog
KAGRA segment file production stopped on 28 June 2024
- The cause was the stop of cache file at Kamioka computer due to the expire of gps time package.
- To return to an automated setup, would it be possible to have the incomplete files created in one directory and only moved to their final location after the whole day's segments are finalized?
- On this Friday, we shut down the Kamioka computers due to a planned power outage.
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- They are updating the way to cluster the triggers.
- veto definer (Uchikata)
- When we make veto definer, we need the segment updated in DQSEGDB. But, currently, the necessary segment was not uploaded on DQSEDB. We will ask Robert to include them soon.
- Uchikata-san will summarize the procedure at the DAC wiki.
- Line identification (Takahiro S. Yamamoto)
- Stochastic search (Chia-Hsuan)
- The line list computed from the data with a shorter duration might be important. Currently, we use the line list of 0.001 mHz resolution. The unification between the stochastic analysis and the detchar analysis is necessary.
- Parameter estimation analysis with KAGRA O4a data (Kobayashi)
20240717 (Wed.)
- canceled
20240710 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: O4b will now end 9 June 2025.
- Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down.
- Future meeting
JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.web
KAGRA f2f meeting: 2024/08/21(Wed)~23(Fri) @Tokyo City University web
LVK meeting @Barcelona, Spain: Registration is now open. Sept 23 – 26. https://lvkmeeting2024.ifae.es/
KAGRA site report 07/02
- Recovery from the Noto Earthquake Disaster
- Next meeting is 07/24(Wed).
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- provide the CAT1 veto-definer file for IPC glitch (Uchikata)
- Announcement
- Minutes
Comparison of Hveto results according to Omicron HPF(Kihyun Jung) klog#30318
- (Yamat) The Summary page needs to be updated. It is now a bottleneck for updating the detchar tools in IGWN conda environment.
- CBC trigger list for O4a (Uchikata, Narikawa)
- Check the details for large chi^2 /SNR triggers.
- Generate the lists automatically and upload it to the daily summary page.
- Extend the analysis to the CBC search.
- We may need to gate the IPC error segments for the search.
- O4a event rate by pyCBC search (Narikawa, Uchikata)
- If configuration is same as Omicron, we can compare the results.
How does pycbc treat the time-clustering? --> clustered triggers within 10 seconds.
- How the clustering length is decided? In Omicron case, the 0.1 clustering length is decided empirically.
- Hveto analysis (Kiyun)
- Kiyun agreed with the wide presentation for KAGRA collaborators, which will be an alternative presentation in the f2f meeting.
- Deep clean(Shu-Wei Yeh)
- They checked the response on the strain at the hardware injection. For these data, they didn't apply the deep clean.
- Stochastic search (Chia-Hsuan)
- Yuzurihara shared the procedure to submit the application of the account on the kmst cluster.
- Detchar member (Uchikata+) will prepare the veto definer for IPC glitches instead of segment file.
20240703 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: O4b will now end 9 June 2025.
- Power outage of ICRR Kashiwa campus on 2024/09/28(Sat) 9:00~18:00 JST. The system-B cluster and Pastevi server will be down.
- Future meeting
JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.web
KAGRA f2f meeting: 2024/08/21(Wed)~23(Fri) @Tokyo City University web
LVK meeting @Barcelona, Spain: Registration is now open. Sept 23 – 26. https://lvkmeeting2024.ifae.es/
- Announcements from Operations (Sawada)
KAGRA site report 06/18
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- provide the CAT1 veto-definer file for IPC glitch (Uchikata)
- Announcement
- Minutes
Bruco configuration for MICH (yamaT) klog#30133
- Bruco server was replaced to new system
Inconsistence of number of triggers between Omicron versions klog#30101
On LIGO summary page, the old Omicron(>v4.0) seems to run for Hveto analysis.
- For Hveto at different computers (Kamioka, Kashiwa, KISTI), we should use the Omicron with the consistent versions.
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- They generated the triggers for O4a data. There were no daily fluctuations in the triggers.
- The comparison between the O4a triggers and triggers computed by the simulated Gaussian noise is underway. The Gaussian data doesn't include the line noise.
Report of updating the DeepClean results using training and cleaning times that avoid IPC glitches (Shu-Wei Yeh) slide
- Subtraction of the 60 Hz line noise and noise monitored by the microphone is underway.
- They showed some improvement by excluding the data of IPC glitches.
- (yamaT) How did you confirm the current-voltage monitor can track the line drift? The coherence might not be the evidence for a narrow frequency bin.
- (yamaT) Acoustic injection test many times, they investigated the coupling functions between sound and DARM.
20240626 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: O4b will now end 9 June 2025.
- Power outage of ICRR Kashiwa campus on 2024/09/28 9:00~18:00 JST. The system-B cluster and Pastevi server will be down.
- Conference
JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.web
- KAGRA f2f meeting: 2024/08/21(Wed)~23(Fri) @Tokyo City University
- Announcements from Operations (Sawada)
KAGRA site report 06/18
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- Announcement
- Minutes
Usage manual was updated for the latest Omicron (v4.1)
- We compared the number of triggers between different Omicron versions (v4.1 and v3.1) in root/hds5/xml formats.
- Based on the reply from the developer, the Omicron (v3.1) had the bug. The developer recommends using the latest Omicron for the analysis.
Yuzurihara updated usage manual for v4.1 using the hdf5 format.
- Update for gates found in stochastic search (Chia-Hsuan)
- The gating with 3.5 s tme window was applied in pygwb when the large transient (IPC glitch) occurred. To mitigate the length losing by gating, it's better to usr the veto-definer.
- Uchikata-san have an experience on the veto-definer. She will try to prepare it.
- Currently they analyzed O4a data (L1, H1, K1) on CIT. But, the L1 and H1 data are stored in system-B(kmst2).
- Trigger generation for O4a data by pycbc (Narikawa)
- They showed the result of comparing the O4a triggers with the triggers computed by Gaussian noise (~5days). The discussion is underway.
- Hveto analysis (Syifa)
Analysis-flag change: https://hveto.readthedocs.io/_/downloads/en/stable/pdf/
- Glitch investigation (Chia-Jui)
- They explained how to apply the whitening: (1) estimate the ASD from the data of (tc-58)~(tc-2), (2) apply the whitening by using the estimated ASD
Based on their request, we shared the list of aux. channel which was used in O4a Hveto analysis in Summary page. git
20240619 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: O4b will now end 9 June 2025.
- Power outage of ICRR Kashiwa campus on 2024/09/28 9:00~18:00 JST. The system-B cluster and Pastevi server will be down.
- Conference
JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.web
- KAGRA f2f meeting: 2024/08/21(Wed)~23(Fri) @Tokyo City University
- Announcements from Operations (Sawada)
KAGRA site report 06/07
- new commissioning leader: Takafumi Ushiba
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- Announcement
- Minutes
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
This task is finished. The summary page is available here.
- The data set for the inspiral range is also available on system-B.
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- They are working on comparing the effect by changing the segment durations of 256s and 128s.
- In the future, we will connect the trigger results with the summary page.
- Currently they produced the triggers by using the template of 1.4-1.4Msun.
- Glitch classification
- They showed the summaries of the glitch classification.
- The glitches located in the upper right on Q-transform might be related to the lockloss.
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
20240612 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: We plan to commence O4b at 1500 UTC (2400 JST) on 10 April 2024.
- Power outage of ICRR Kashiwa campus on 2024/09/28 9:00~18:00 JST. The system-B cluster and Pastevi server will be down.
- Conference
JPS: 2024/09/16(Mon)~09/19 @Hokkaidou univ.web
- KAGRA f2f meeting: 2024/08/21(Wed)~23(Fri) @Tokyo City University
- Announcements from Operations (Sawada)
KAGRA site report 06/07
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- Announcement
- Minutes
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
- Computed the inspiral range from the strain channel with gwpy. Basically they used only the data in the science mode.
- The histogram of the inspiral range changed. We can see the peak on the histogram.
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- They computed the triggers by using pycbc package from the strain data and packed in the xml.
- The analyzed data include the IPC glitches. But, the chi-square could mitigated the glitch effect.
(Yuzu) Did you find the interesting or new triggers? --> no. Data seems stable.
(YamaT) Can you compare the trigger histogram with the one from Gaussian noise data? --> not yet. It's possible by replacing the input data with the generated Gaussian noise.
- Glitch classification (Hsu Shih-Hong)
- They took the average of the Q-spectrograms for each class. The obvious common features were not observed.
- They tried to extract the common features on the Q-spectrograms.
- It's important to take into account of the whitening effect. The whitening in gwpy could make the sharp glitch wider.
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
20240605 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: We plan to commence O4b at 1500 UTC (2400 JST) on 10 April 2024.
- Next 10yr Task Force Meeting: 2024/06/07 17:00JST, see [kagra 06570]
- Power outage of ICRR Kashiwa campus on 2024/09/28 9:00~18:00 JST. The system-B cluster and Pastevi server will be down.
JPS registration: 2024/5/21~6/5 web
Does anyone have a presentation related to DetChar activity?
- Announcements from Operations (Sawada)
KAGRA site report 05/22
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- isotropic stochastic search result (Chia-Hsuan)
- Announcement
- Minutes
In next JPS meeting(Sep.), YamaT plan to talk the detchat topics related to the web service (https://gwdet.icrr.u-tokyo.ac.jp/~controls/misc/html/).
- Issue of monopolizing the CPU resources of system-B cluster. (this might be the third time in my memory)
- Yuzurihara contacted the administrators to set some threshold or update the cluster settings so that the job submission system will manage the jobs submitted by many users effectively. Still no response from the administrators.
isotropic stochastic search result (Chia-Hsuan) slide
- They analyzed the O4a KAGRA data with other detectors by using the pygwb pipiline, at CIT cluster.
- They found the strange peak on the gating length. They shared the list of the gated time. The comparison between the list and the time of IPC glitches will be done soon.
They reported the coherence between KAGRA and LIGO (Livingston and Hanford). About the coherence of 960 and 961 Hz, yamaT pointed out that it came from the timing system. We use the same timing system between KAGRA and LIGO. See also alog.
- AI for detchar: Collect the information of the remaining frequencies with coherence
(YamaT) How did you integrate the data for narrow-line analysis? --> all of the science mode
- How was the gate process applied?
What is the good frequency band for the analysis? --> (YamaT) Comments from the calibration side: use 30~1000Hz.
Glitch classification (Chia-Jui) slide
- They reported the glitches detected in O4a data can be classified into several classes by using unsupervised classification.
Q-transform plots are available git.
- Yama-T commented on slack that the glitch effect might be widen by the whitening process.
- O4a summary page (Uchikata)
- We have decided to compute the inspiral range without the gwsumm. The computation is on-going.
20240529 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: We plan to commence O4b at 1500 UTC (2400 JST) on 10 April 2024.
- Next 10yr Task Force Meeting: 2024/06/07 17:00JST, see [kagra 06570]
- Power outage of ICRR Kashiwa campus on 2024/09/28 9:00~18:00 JST. The system-B cluster and Pastevi server will be down.
- Renewal of the account on KAGRA Main Data System: deadline 2024/05/31
JPS registration: 2024/5/21~6/5 web
Does anyone have a presentation related to DetChar activity?
KAGRA site report 05/22
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- Announcement
- Minutes
- Glitch analysis (Ishikawa)
- The Omicron analysis for non-stationary noise around 360 Hz is on-going.
- There might the 5-minutes fluctuation on the inspiral range. The analysis for other data will be done next.
- Glitch analysis (Chia-Jui)
- The Omicron analysis for the science mode excluding the IPC glitch is on-going.
(Guo Chin Liu) Do you have a flag to indicate the glitch time? --> Omicron provide the time of the glitch.
- (Guo Chin Liu) What is the ratio in the science mode?
He found several characteristic types of glitches in KAGRA O4a data. For details, see slide.
- Hveto analysis (Syifa)
- Hveto analysis with high pass filter is on-going.
- Dedicated O4a summary page (Uchikata)
She found that the cache file for O4a data has the issue of overlapping or missing. She updated the cache file. Modification of cache files at system B
- (Sawada) Matlab on the LDAS cluster will stop on the next maintenance day. If you want to use the Matlab on LDAS cluster, please contact with Sawada-san.
- Glitch analysis (Ishikawa)
20240515 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: We plan to commence O4b at 1500 UTC (2400 JST) on 10 April 2024.
- KAGRA detchar liaison to CBC group
- Nami Uchikata as the new liaison between the CBC group and the KAGRA Detchar group.
- KAGRA site report
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- Announcement
- Minutes
- Update contents of summary page (Oshino)
- Hveto (Shifa)
- By changing cutoff frequency of 8 or 12Hz, they checked the Hveto results and found the artificial glitches around 10Hz.
- When they apply the HPF with 6 Hz or 4 Hz, the artificial glitches around 10Hz disappeared.
- (YamaT) Do you know the design of HPF (butterworth?)?
- (Uchikata) Minimum frequency of Hveto should be larger than the cutoff frequency of high pass filter in Omicron.
- (YamaT) It might make the ripple.
- (Yuzu) You can analysis the Omicron triggers with the higher cut-off frequency.
- Glitch analysis (Ishikawa)
(Chia-Jui) How do you set-up the Omicron configuration files? --> Same as commonly used one.
(Chia-Jui) What was the typical SNR of 300-500Hz? --> SNR 6~10? He didn't have a clear answer. He will check it.
- Glitch analysis (Chir-Jui)
- Omicron analysis without high pass filter was done.
- In page 7, there were gaps due to the exceed of threshold of glitch rate. At that time, Omicron failed due to the error.
- We confirmed the goal of the Detchar activity is to contribute the sensitivity or noise hunting of KAGRA.
20240508 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: We plan to commence O4b at 1500 UTC (2400 JST) on 10 April 2024.
- Introduction of new comer
- KAGRA site report
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- Announcement
- Minutes
Omicron triggers at System B (Uchikata) klog
- Update contents of summary page (Oshino)
line identification by fscan for kagra (Takahiro.S.Yamamoto) slide+supplement
- What is the frequency resolution?
Segment duration of 1800 s is a typycal value in continuous wave search? --> yes
- Is is posible to real-time monitoring of 60 Hz?
- What is the advantage to used fscan?
The result for O4a data is available on the web. Due to computational costs, we didn't use aux. channels.
- Hveto analysis (Kyujin, Kihyun, Syifa)
- By adding the high pass filter, the artificial glitches appeared, although there is no such glitches in Uchikata-san's results.
Omicron on K1 O4a Data (Chia-Jui) slide
They proposed the way to identify the IPC glitches. --> The way to identify the IPC glitches was already established.
- They found three classes of glitches in KAGRA data.
- Dedicated summaru page for O4a KAGRA (Uchikata)
- When we compute the inspiral range by reading the data from NDS server,
20240424 (Wed.)
- Agenda
- Announcement
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: We plan to commence O4b at 1500 UTC (2400 JST) on 10 April 2024.
- Introduction of new comer
- KAGRA site report
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
- cache file for O3GK and O4a
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- Announcement
- Minutes
- Meeting on Next week will be canceled. Next meeting is 8 May.
- Report of KIW and open data workshop#7 (Yuzurihara)
- Computer cluster at Kamioka (Oshino)
- We purchased the rack. In future, we move the computer in the rack.
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
- Confirmation of the result is on-going.
The scale of histogram was changed. The apperance looks consistent with the dedicated summary page and the YamaT-san's result.
- TODO: Inspiral range should be computed from the strain channel, not using the RANGE channel. That Range channel is used for the prompt report.
- Hveto (Kyujin, Kihyun, Syifa)
- The analysis result was explained in the meeting.
- The high pass filter with 10 Hz or 15 Hz was applied for the Omicron analysis. The frequency range for Omicron should be tuned at the same time to mitigate the artificial noise in the Omicron triggers.
- whale-like shape disappered in the histogram of Omicron triggers when we remove the segment of IPC glitch from the analysis.
- Is there any suggestion to the interferometer experts? For example, which channels seems problematic.
- Glitch investigation (Ishikawa)
Studying the Omicron pipeline and applying to the KAGRA's O4a data Progress report
- Line investigation (Samurai)
- Reading Fscan paper for past observation run (S6, O1, O2). The report will be done in the future meeting.
20240410 (Wed.)
- Agenda
- Announcement
KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 web
Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 web, Info. from GWOSC
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: We plan to commence O4b at 1500 UTC (2400 JST) on 10 April 2024.
- Introduction of new comer
- KAGRA site report
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- Announcement
- Minutes
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
Use segment information of SCIENCE MODE + IPC glitch ==> ongoing
- ongoing
Change data length 4096s -> 64s. Apply the high pass filter before splitting the data. ==> done
Estimate common PSD and use it for the analysis ==> done
- Is it possible to output the trigger list in xml format?
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
20240403 (Wed.)
- Agenda
- Announcement
KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 web
Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 web, Info. from GWOSC
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4b: We plan to commence O4b at 1500 UTC (2400 JST) on 10 April 2024.
Update of DQSEGDB server help ticket
- KAGRA site report
- Budget request
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- Announcement
- Minutes
Upgrade DetChar computers (YamaT)
- waiting the update of workstation machines. I will take a few monthes.
- DQR update (Yuzurihara)
- no update.
- Update contents of summary page (Oshino)
- no update
- Hveto (Kyujin)
- Trouble on KISTI cluster.
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- Use segment information of SCIENCE MODE + IPC glitch
Change data length 4096s -> 64s. Apply the high pass filter before splitting the data.
- Estimate common PSD and use it for the analysis
- Is it possible to output the trigger list in xml format?
20240326 (Wed.)
- Agenda
- Announcement
KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 web
Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 web, Info. from GWOSC
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
ER16: It will nominally start at 1500 UTC (2400 JST) on 20 Mar 2024, and last for 2 weeks.
O4b: We plan to commence O4b at 1500 UTC (2400 JST) on 3 April 2024.
- KAGRA site report
- Budget request
- Progress reports
Upgrade DetChar computers (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- Announcement
- Minutes
- Budget request
- New computers for replacing too old servers (k1det0, 1): 500k-yen x2
- HDD for new systems: 10k-yen x10-20
- Progress reports
Upgrade DetChar computers (YamaT)
Testing DetChar softwares can be started after the update of CDS workstations is completed.
- Test of CDS workstation needs more time (hopefully by end of April)
- DQR update (Yuzurihara)
- No update
- Update contents of summary page (Oshino)
- No update
- Related to segment files (Uchikata, Narikawa)
- No update
- provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa)
https://www.icrr.u-tokyo.ac.jp/~uchikata/Detchar/O4aSumm/gps/1368975618-1371337218/range/
SummaryPages process was executed on Kashiwa System-B.
- Results were copied to the personal region of ICRR's Web server.
- Finally this page will be opened only for LVK folks(?) on gwdet.
- pyCBC trigger list for O4a data (Narikawa and Uchikata)
- No update
- Budget request
20240306 (Wed.)
- Agenda
- Announcement
KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 web
Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 web, Info. from GWOSC
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
ER16: It will nominally start at 1500 UTC (2400 JST) on 20 Mar 2024, and last for 2 weeks.
O4b: We plan to commence O4b at 1500 UTC (2400 JST) on 3 April 2024.
Ref.internal short announcements (reminders), public announcements
LVK meeting on March 11-14 at Louisiana State University web
- There is no fee for online participants
Update of member list for DetChar mailing list
- KAGRA site report
- Task list for the authorship 2024
- Progress reports
- O4a summary page(Uchikata)
- After several attempts, the job was finished without errors. Another small problems,
- O4a summary page(Uchikata)
- Announcement
20240228 (Wed.)
- Agenda
- Announcement
KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 web
Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 web, Info. from GWOSC
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
ER16: It will nominally start at 1500 UTC (2400 JST) on 20 Mar 2024, and last for 2 weeks.
O4b: We plan to commence O4b at 1500 UTC (2400 JST) on 3 April 2024.
Ref.internal short announcements (reminders), public announcements
LVK meeting on March 11-14 at Louisiana State University web
- Early Registration is open until February 1
- There is no fee for online participants
Update of member list for DetChar mailing list
- KAGRA site report
- Task list for the authorship 2024
- Progress reports
- Announcement
- Minutes
- Task list for the authorship 2024 (not fixed yet)
1. Commissioning support : serving data monitoring tools for site commissioners. This task focuses on the support of the IFO lock trial and/or noise hunting based on the request from the interferometer commissioners. Support of analyses to measured data (e.g. noise projection to the DARM with measured noise and TFs) is also contained in this task. Specialized tasks for each subgroup should be applied for in the respective group task. 2. Production and validation of Online Data Quality State Vector (for O4b/O5 preparation. This task focusing on providing the online DetChar products such as the online DQSV and managing various reliable online flags. Developing real-time and guardian codes for providing such flags should be contained in this task. 3. Production and validation of Segment information for O4b/O5 preparation. This task focusing on providing low-latency/offline segments. Providing segment itself, evaluation of efficient channels to make segments, evaluating benefit of segments on GW searches and cooperation with CIT staffs to update segment contents on DQSEGDB are contained in this task. 4. Construction of DQR (Data Quality Report) and igwn-alert framework for O4b/O5 RRT activities. This task focusing on providing contents from KAGRA to DQR web pages which is merged with LIGO, Virgo and KAGRA. 5. Support of Data Analysis group to set Data Category criteria for O4b/O5 joint observing run. This task focusing on the support of the GW-search activities based on the each WG of DAC. Providing data category for the pipelines of each GW sources, providing veto segments and other noise information such as identified spectral lines are also contained in this task. 6. Managing DET computers and their environments. This task contains the computer environment construction for providing the DetChar products in the cadence of online/low-latency/offline. Managing dedicated servers for sharing DetChar products among LVK is also contained in this task. ===== - Noise hunting in KAGRA commissioning. Obsolescent Noise *hunting* without IFO (hardware) experts is unrealistic. In this meaning, the most of noise *hunting* can be covered in "Commissioning support”. If the tasks are related to the noise *finding* for the purpose of providing veto segment, they can be covered in “Support of Data Analysis”.- hveto analysis is contained in 1. in the case that there is some communication with onsite commissioners via klog etc.
- It's also potentially contained in 5. in the case of providing veto-ed segments, correlated channels etc.
Providing Run SummaryPage is contained in 5.
- Exact sentence as "Making Run Summary" should be added the description in 5.
- hveto analysis is contained in 1. in the case that there is some communication with onsite commissioners via klog etc.
- Progress reports
- Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT)
- start consideration about the system upgrade to new Debian system.
- DET tools depend on the CDS tools and CDS tools are well managed on apt-repository.
- Only a part of CDS tools can be available on Anaconda now.
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Combine DET computer resources into one DET cluster at Kamioka site
- Related to segment files (Uchikata, Narikawa)
provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) O4a (LV)
pyCBC trigger list for O4a data (Narikawa and Uchikata) O4a (H1)
- 4000s data analysis is ongoing.
- Processed time is a few hours
- Used template is changed from BBH to BNS.
- Trigger behavior is changed by used templates.
- Generated triggers are in the text format.
If LIGO's XML (LW XML?) is available, it may be very easy to make various plots on SummaryPages.
- 4000s data analysis is ongoing.
- Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT)
- Task list for the authorship 2024 (not fixed yet)
20240221 (Wed.)
- Agenda
- Announcement
KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 web
Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 web
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
ER16: It will nominally start at 1500 UTC (2400 JST) on 20 Mar 2024, and last for 2 weeks.
O4b: We plan to commence O4b at 1500 UTC (2400 JST) on 3 April 2024.
Ref.internal short announcements (reminders), public announcements
LVK meeting on March 11-14 at Louisiana State University web
- Early Registration is open until February 1
- There is no fee for online participants
Update of member list for DetChar mailing list
- KAGRA site report (Yuzurihara)
- Commissioning support + tasks related to O4a
- O4a for KAGRA : 2023/05/25 0:00 JST (=2023/05/24 15:00UTC) ~ 2023/06/21 8:00 JST
- Event validation (YamaT)
- Online data quality state vector (YamaT)
- Tool to evaluate Gaussianity (Yamamura)
- Scattered light noise (Yamamura)
- Pastavi update (Yuzurihara)
- Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa)
- Classification of glitch noise (Shikano, Oshino)
- IPC glitch
- line noise study (Samurai)
- Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Combine DET computer resources into one DET cluster at Kamioka site
- Related to segment files (Uchikata, Narikawa)
provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) O4a (LV)
- pyCBC trigger list for O4a data (Narikawa)
- Announcement
- Minutes
20240214 (Wed.)
- Agenda
- Announcement
KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 web
Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 web
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
ER16: It will nominally start on 13 Mar 2024, and last for 2 weeks. (Note that ER16 will begin in the middle of the next LVK meeting at LSU, 11-14 March.)
O4b: We plan to commence O4b at 1600 UTC (2500 JST) on 27 Mar 2024.
Ref.internal short announcements (reminders), public announcements
White paper and task list for 2024 git repo
LVK meeting on March 11-14 at Louisiana State University web
- Early Registration is open until February 1
- There is no fee for online participants
Update of member list for DetChar mailing list
- KAGRA site report (Yuzurihara)
- Commissioning support + tasks related to O4a
- O4a for KAGRA : 2023/05/25 0:00 JST (=2023/05/24 15:00UTC) ~ 2023/06/21 8:00 JST
- Event validation (YamaT)
- Online data quality state vector (YamaT)
- Tool to evaluate Gaussianity (Yamamura)
- Scattered light noise (Yamamura)
- Pastavi update (Yuzurihara)
- Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa)
- Classification of glitch noise (Shikano, Oshino)
- IPC glitch
- line noise study (Samurai)
- Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Combine DET computer resources into one DET cluster at Kamioka site
- Related to segment files (Uchikata, Narikawa)
provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) O4a (LV)
- pyCBC trigger list for O4a data (Narikawa)
- Announcement
- Minutes
- Online data quality state vector (YamaT)
- We need same test for ETMY model.
- Scattered light noise (Yamamura)
- (oshino) why the double bounce occurred?
- (yamaT) it's better to check both the feedback and error signal (OUT_DQ and IN1_DQ).
- (oshino) PD signal might be helpful in the investigation. In POP_FORWARD, the scattered light was seen in the past.
- Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa)
KAGRA O4a hveto results (0524 ~ 0606) KAGRA O4a hveto results (0607 ~ 0619)
- hveto shows the many triggers on the time the scattered light noise appeared
- (yamaT) IPC glitch was taken care in this analysis? It's better to use SCIENCE segment + IPC glitch segment.
- It is interesting to compare the glitch rate and the analysis result with and without IPC glitch segments.
- Yuzurihara shared that segment with Kihyun.
provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) O4a (LV)
- pyCBC trigger list for O4a data (Narikawa)
- (yamaT) can we include the trigger information by pycbc, in the summary page?
- Online data quality state vector (YamaT)
20240207 (Wed.)
- Agenda
- Announcement
KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 web
Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 web
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
ER16: It will nominally start on 13 Mar 2024, and last for 2 weeks. (Note that ER16 will begin in the middle of the next LVK meeting at LSU, 11-14 March.)
O4b: We plan to commence O4b at 1600 UTC (2500 JST) on 27 Mar 2024.
Ref.internal short announcements (reminders), public announcements
White paper and task list for 2024 git repo
LVK meeting on March 11-14 at Louisiana State University web
- Early Registration is open until February 1
- There is no fee for online participants
Update of member list for DetChar mailing list
- KAGRA site report (Yuzurihara)
- Commissioning support + tasks related to O4a
- O4a for KAGRA : 2023/05/25 0:00 JST (=2023/05/24 15:00UTC) ~ 2023/06/21 8:00 JST
- Event validation (YamaT)
- Online data quality state vector (YamaT)
- Tool to evaluate Gaussianity (Yamamura)
- Scattered light noise (Yamamura)
- Pastavi update (Yuzurihara)
- Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa)
- Classification of glitch noise (Shikano, Oshino)
- IPC glitch
- line noise study (Samurai)
- Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Combine DET computer resources into one DET cluster at Kamioka site
- Related to segment files (Uchikata, Narikawa)
Provide the dedicated summary page for O4a of KAGRA (Uchikata) O4a (LV)
- Announcement
- Minutes
- Online data quality state vector (YamaT)
model update of k1detdq0 This is bug fix of production of online data quality state vector related to DAC saturation.
- The hardware test will be done this week an next week.
- Tool to evaluate Gaussianity (Yamamura)
The codes were uploaded at git repo. The preparation of brief documentation is ongoing.
- Classification of glitch noise (Shikano, Oshino)
- They restarted this project. The report will be done soon.
Provide the dedicated summary page for O4a of KAGRA (Uchikata) O4a (LV)
- They tested the conda environment and configuration files for the production of the summary page. Except for the specific short time, they can generated the O4a summary page including duty cycle and inspiral range.
- Generation of trigger list by pycbc (Narikawa)
- Code test is ongoing by using the short 4096s data of O4a. The timeseries of chi square looks strange. They plan to apply the high pass filter, instead of window function.
- (yamat) How do you decide clustering length?
- (Narikawa) By software injection, we can evaluate how the SNR spreads and determine the clustering length.
- Online data quality state vector (YamaT)
20240131 (Wed.)
- Agenda
- Announcement
KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17 web
Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 web
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
ER16: It will nominally start on 13 Mar 2024, and last for 2 weeks. (Note that ER16 will begin in the middle of the next LVK meeting at LSU, 11-14 March.)
O4b: We plan to commence O4b at 1600 UTC (2500 JST) on 27 Mar 2024.
Ref.internal short announcements (reminders), public announcements
White paper and task list for 2024 git repo
LVK meeting on March 11-14 at Louisiana State University web
- Early Registration is open until February 1
- There is no fee for online participants
Update of member list for DetChar mailing list
LVK MoA survey summary LIGO DCC
- KAGRA site report (Yuzurihara)
- Commissioning support + tasks related to O4a
- O4a for KAGRA : 2023/05/25 0:00 JST (=2023/05/24 15:00UTC) ~ 2023/06/21 8:00 JST
- Event validation (YamaT)
- Tool to evaluate Gaussianity (Yamamura)
- Scattered light noise (Yamamura)
- Pastavi update (Yuzurihara)
- Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa)
- Classification of glitch noise (Shikano, Oshino)
- IPC glitch
- line noise study (Samurai)
- Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- Combine DET computer resources into one DET cluster at Kamioka site
- Related to segment files (Uchikata, Narikawa)
provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) O4a (LV)
- Announcement
- Minutes
- Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa)
- line noise study (Samurai)
- Is it possible to set the initial parameter in advance, such as prominence and height?
- In future, it is better to extend the fft length to be longer for fine frequency resolution.
- Update contents of summary page (Oshino)
- Related to segment files (Uchikata, Narikawa)
provide the dedicated summary page for O4a of KAGRA (Uchikata and Narikawa) O4a (LV)
- The attempt to generate summary page is on system-B. For reading data, NDS2 server is helpful.
20240124 (Wed.)
- Agenda
- Announcement
- KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17
Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 web
- LIGO-Virgo-KAGRA detchar joint meeting
- tileslot: onthly, 23:00 JST (14:00 UTC) or 6:00 JST (21 UTC)
Last meeting on Nov. 15 23:00 JST (14:00 UTC) wiki
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4a: It will end at 1600 UTC on 16 Jan 2024. LLO will end O4a observing early, at 1400 UTC.
ER16: It will nominally start on 13 Mar 2024, and last for 2 weeks. (Note that ER16 will begin in the middle of the next LVK meeting at LSU, 11-14 March.)
O4b: We plan to commence O4b at 1600 UTC (2500 JST) on 27 Mar 2024.
Ref.internal short announcements (reminders), public announcements
Information of O4a wiki page
White paper and task list for 2024 git repo
- LVK meeting on March 11-14 at Louisiana State University
Update of member list for DetChar mailing list
- KAGRA site report (Yuzurihara)
- Commissioning support + tasks related to O4a
- O4a for KAGRA : 2023/05/25 0:00 JST (=2023/05/24 15:00UTC) ~ 2023/06/21 8:00 JST
- Event validation (YamaT)
- Tool to evaluate Gaussianity (Yamamura)
- Scattered light noise (Yamamura)
- Pastavi update (Yuzurihara)
- Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa)
- Classification of glitch noise (Shikano, Oshino)
- IPC glitch
- line noise study (Samurai)
Peak identifications web
- Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- run Omicron at Kamioka site and refresh the Omicron plots on summary page during O4a period
- Combine DET computer resources into one DET cluster at Kamioka site
- Script to generate segment files (Uchikata, Narikawa)
- Related to segment files (Uchikata, Narikawa)
provide the dedicated summary page for O4a of KAGRA? O3a (LV)
- Announcement
- Minutes
- Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa)
- Update contents of summary page (Oshino)
20240117 (Wed.)
- Agenda
- Announcement
- KAGRA international workshop (KIW11)@Taiwan: 2023/04/16-17
Gravitaional wave open data workshop (GWODW7)@Taiwan: 2023/04/18-20 web
- LIGO-Virgo-KAGRA detchar joint meeting
- tileslot: onthly, 23:00 JST (14:00 UTC) or 6:00 JST (21 UTC)
Last meeting on Nov. 15 23:00 JST (14:00 UTC) wiki
- O4a/preO4b(not call it as postO4a)/ER16/O4b schedule:
O4a: It will end at 1600 UTC on 16 Jan 2024. LLO will end O4a observing early, at 1400 UTC.
ER16: It will nominally start on 13 Mar 2024, and last for 2 weeks. (Note that ER16 will begin in the middle of the next LVK meeting at LSU, 11-14 March.)
O4b: We plan to commence O4b at 1600 UTC (2500 JST) on 27 Mar 2024.
Ref.internal short announcements (reminders), public announcements
Information of O4a wiki page
White paper and task list for 2024 git repo
- LVK meeting on March 11-14 at Louisiana State University
- KAGRA site report (Yuzurihara)
- Commissioning support + tasks related to O4a
- O4a for KAGRA : 2023/05/25 0:00 JST (=2023/05/24 15:00UTC) ~ 2023/06/21 8:00 JST
- Event validation (YamaT)
- Tool to evaluate Gaussianity (Yamamura)
- Scattered light noise (Yamamura)
- Pastavi update (Yuzurihara)
- Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa)
- Classification of glitch noise (Shikano, Oshino)
- IPC glitch
- line noise study (Samurai)
Peak identifications web
- Unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT)
- DQR update (Yuzurihara)
- Update contents of summary page (Oshino)
- run Omicron at Kamioka site and refresh the Omicron plots on summary page during O4a period
- Combine DET computer resources into one DET cluster at Kamioka site
- Script to generate segment files (Uchikata, Narikawa)
- Related to segment files (Uchikata, Narikawa)
provide the dedicated summary page for O4a of KAGRA? O3a (LV)
- Announcement
- Minutes
- Tool to evaluate Gaussianity (Yamamura)
- Gauch recently looks not running. There is no html page linked from summary page. We will check the details later.
- DQR update (Yuzurihara)
- I asked the remote help to Derek. I'm submitteing the application for the ICRR computer account.
- IPC glitch
- Noise hunting by machine learning and Hveto (Kyujin, Kihyun, Syifa)
- The analysis for the remained date will be
- Update contents of summary page (Oshino)
- Tool to evaluate Gaussianity (Yamamura)