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=== 20201111 (Thu.) === * Agenda * C20 offline h(t) * [[KAGRA/Subgroups/DET/DataRlease|O4 data release schedule]] * f2f/KIW7 * Minutes * C20 offline h(t) * Comment from DAC meeting: * Burst group can be provide GW event trigger list (schedule is not decided yet.) * Detail DQ info. around GRB events is very useful. * Data transfer on DET server * * Omicron trigger generation for C20 h(t) * * O4 data release schedule === 20201103 (Thu.) === * Agenda * C20 offline h(t) * O4 data release schedule * Minutes * C20 offline h(t) * Data should be copied to Kamioka server. * Glitch trigger search by Omicron * After data copy, it will be resumed. * hveto needs GW trigger search * We can demonstrate with omicron trigger of h(t). * After GW search triggers are available it will be resumed. * Data transfer to KISTI * discuss with DAS people on the next KGWG meeting * O4 data release schedule * Dead line: December .. * Please fill the requested time to link below. * http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/DET/DataRlease === 20201022 (Thu.) === * Agenda * Segment of O3GK * Documentation about O3GK info. * SummaryPage for O4 installation * Minutes === 20201008 (Thu.) === * Agenda * Planned power outage * hveto bug * Minutes * Planned power outage * All jobs on k1det must be stopped until 10/13 morning. * hveto bug * Code reading is in progress by Chihiro. * There is no response from LIGO people. * Analysis of Apr 8th - 21st data is on going. * Segment update * Discussion with Robert is resumed. * Upload method is 'pull' from LIGO side. * They already know the path to the segment files and types of segment file. * Remains tasks are schedule and segment name on DQSEGDB. |
=== 20211108 (Mon.) === * Agenda * O3GK Glitch investigation * Segment information for open data * Progress of DQR * Minutes * O3GK Glitch investigation * (Kihyun) checked the omega-scan of three channels * The last three pages [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=13383|slide]] * Segment information for open data * (Uchikata) checked which data segments were used for GRB analysis. * The correct data segments was used for analysis. But, for some reason, the time of the wrong segment was transmitted to gwosc group. * The open data set will be re-produced by Uchikata-san and Narikawa-san. After that, the data set will be reviewed. * Progress of DQR * (Yuzurihara) === 20211101 (Mon.) === * Agenda * O3GK noise budget paper [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=13405|JGW-P2113405-v1]] * 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 ----- === 20210401 (Thu.) === * Agenda * Progress of hveto analysis * DetChar cluster * lvalert * SummaryPages * RRT for O4 * Minutes |
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* 22:00 (JST/KST) tonight, LVK operation workshop will be held. === 20201001 (Thu.) === * Agenda * Planned power outage (10/14) * Minutes * Planned power outage (10/14) * k1det will be stopped until 10/13 morning. * They will come back online after 10/15. === 20200924 (Thu.) === * Agenda * Segment update * hveto problem * Minutes * Segment update * All 9 segment info. were fixed. * They had already copied to Kashiwa and Kamioka. * They should be copied also KISTI. * TY will contact to Robert again. * After then, segments will be uploaded to DQSEGDB. * hveto problem * Problem is cased by hveto * Some trigger files are sent to LDAS. * Investigation on LDAS is ongoing. * Conf. file on Kamioka should be share to KISTI. === 20200911 (Thu.) === |
* 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.) === |
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* Duty cycle evaluation during O3GK * Lock loss study * O3GK DetChar talk in LVK meeting * Minuets |
* O4 preparation * Minutes |
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* Investigating strange behavior of hveto * On KISTI cluster, it works well. * Cross check of Chihiro's result and Kihyun's one is ongoing. * Round winner channel changes day by day. (Is it consistent with past results?) * K1:ASC-AS*** is not maintained well. * Both Safe and Unsafe channel list should be used as same ones. * Duty cycle evaluation during O3GK * 54% duty factor (2 weeks average) * BNS range, 500kpc (2 weeks average, cal mistakes is already revised.) * Only last a few days, BPC lines are enabled. * Lock loss study * BLRMS has some time delay. * LOCKED segments should be used ins * O3GK DetChar talk in LVK meeting * topics * Achievement of KAGRA readiness * Progress of concrete analysis * BNS ranges, duty factor as the overview. => Yamamoto, Kozakai === 20200903 (Thu.) === * Agenda * trigger generation * hveto analysis * Minutes * trigger generation * Analysis is finished. * Two channels have some problem. * The version problem of gwpy occurs on KISTI. * Latest channel list should be shared on GitHub. * hveto analysis * Omicron triggers should be shared with LIGO people. (Kamioka -> LIGO) => Kozakai-san will contact to Alex. * hveto works well on KISTI. => Kihyun will continue to analysis. === 20200827 (Thu.) === * Agenda * Segment Update * KAGRA data analysis * GEO data analysis * Minutes * Segment Update * Broken frames period are removed from new science segments (K1-GRD_SCIENCE_MODE_AND_DAQ_STATUS_OK) * Broken frames period as provided a new segments definition (K1-DAQ_STATUS_BAD) * They are store in detchar@m31:Segments/ * Obsolete segments are still generated (???). * KAGRA data analysis * Some PEM sensors are added to the channel list for omicron analysis. => (until next week.) * When is the location of each sensor fixed? => At least around Feb. (also for PORTABLE) * Disk full problem and script errors are occur KISTI * hveto problem occurs (Apr 15. UTC) * GEO data analysis === 20200806 (Thu.) === * Agenda * f2f meeting * progress of O3GK * Minutes * f2f meeting * We have parallel session. (need to prepare two talks for Experiment and Data analysis.) * Experiment -> Yamamoto, Data Analysis -> Kozakai? Kihyun also considers an oral or a poster session. * progress of O3GK * Reconsidering Safe/Unsafe channels is on going. * We need to re-analyze for some channels and some segments by Omicron. * Cross check of KAGRA data analysis can be done by Kihyun. * GEO data transfer to KISTI cluster is almost done. * Kihyun can continue to analyze the GEO data. * We need to do cross check of the results of GEO data analysis. === 20200730 (Thu.) === * Agenda * Safe/Unsafe channel ([[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=11854|slide]]) === 20200723 (Thu.) === * Cancelled === 20200702 (Thu.) === * Agenda * Safe/Unsafe channel * Omicron troubles * GEO data analysis === 20200625 (Thu.) === * Agenda * Broken frames * O3GK * trigger generation * hveto * CAGMon * Minutes * Broken frames * Totally 26 broken frames. (Science: 4, Locked: 4, Unlocked: 18) * TY will remove 32-second long data which is in broken frames from science mode segments by manually. * After then, the segment script will be updated for taking into account broken frames. * O3GK * trigger generation * Some runtime error occurs on the Kamioka server. * Trigger generation test is started with KAGRA data on the KISTI server. * GEO data transfer to the KISTI server is not finished yet. * hveto * Test with short time data is ongoing * CAGMon * Analysis with Apr. observation data is already started. * Used Channel list is same as YuzuSummary's one. * Safe/Unsefe channel list is also required --> will be discussed next week. === 20200618 (Thu.) === * Agenda * LVK operations white paper * task list * introduction of ICA * Current progress of CAGMON === 20200610 (Thu.) === * Agenda * DAQ error during O3GK ([[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=11751|JGW-G2011751]]) * KAGRA data analysis (Omicron/hveto) * GEO data analysis (Omicron/CAGMon) * Minutes * DAQ error during O3GK * Ueno-san found file reading error with following frames. {{{ K-K1_C-1270444416-32.gwf 2020-04-09 14:13:18 (JST) K-K1_C-1270570496-32.gwf 2020-04-11 01:14:38 (JST) K-K1_C-1270577376-32.gwf 2020-04-11 03:09:18 (JST) K-K1_C-1270680672-32.gwf 2020-04-12 07:50:54 (JST) K-K1_C-1271033536-32.gwf 2020-04-16 09:51:58 (JST) K-K1_C-1271174912-32.gwf 2020-04-18 01:08:14 (JST) K-K1_C-1271226144-32.gwf 2020-04-18 15:22:06 (JST) K-K1_C-1271440736-32.gwf 2020-04-21 02:58:38 (JST) }}} * KAGRA data analysis * Omicron search around GRB was finished. * Whole 2-weeks analysis is now being performed. * It's better to remove some channels from unsafe channel list. * We should test hveto with some channel lists. === 20200604 (Thu.) === * Agenda * LVK white paper * O3GK analysis * Minutes * LVK white paper * Operations white paper {{{ 2. Observatory Operations 3. Detector Commissioning 4. Calibration 5. Detector Characterization 6. Computing and software }}} * Observational Science white paper {{{ 1.1 Burst 1.2 CBC 1.3 CW 1.4 Stochastic 2 Burst 3 CBC 4 CW 5 Stochastic 6 Burst+CBC+DetChar Joint Activity Plans 7 Burst+CBC Joint Activity Plans 8 Burst+Stochastic Joint Activity Plans 9 Stochastic+CBC 10 Stochastic+Detchar }}} === 20200521 (Thu.) === * Agenda * Talk plans for JPS meeting * PTEP paper * O3GK analysis * Minutes * Talk plans for JPS meeting * TY will give a DET summary talk. * Deadline 4th June. * PTEP paper * Writing draft was finished. * After checking the whole, draft will be submitted to CPC. * O3GK analysis * Segment information is being reprovided as Science, Locked , Unlock, and OMC Overflow. * Omicron triggers will be regenerated with new segment information. * hveto will be applied after generating Omicron triggers with new segment and configurations. * O3GK data is available on the KISTI cluster. * Bug fix is required for using CAGMon. === LVK 20200518/19 (Mon./Tue.) === * [[https://wiki.ligo.org/DetChar/Telecon20200518|Agenda]] === 20200514 (Thu.) === * Agenda * PTEP paper * Regenerate segment information * Regenerate omicron triggers * SummaryPage stability * Activities on KISTI * Minutes === 20200507 (Thu.) === * O3GK DetChar analysis * KAGRA DQ flags/segments * Glitch searches * Burst trigger veto * GEO DQ flags/segments * Minutes * KAGRA DQ flags/segments * Reproducing OMC overflow segments * Overflow segments are provided as separately from Science mode * 'SegmentList_locked_UTC_***.txt' is expired. * Reproduced segments information should be uploaded to DQSEGDB * Glitch searches * Omicron configuration should be reoconsidered * Triggers will be regenerated with new configurations * Discussion of configuration (chunk-size, intervals...) is ongoing. * Burst trigger veto * All cWB triggers are not vetoed by hveto * cWB has some problems(?) * Omicron parameter should be considered again. * GEO DQ flags/segments * GEO people are now providing new frames including both the strain signal and important auxiliary channels. * GEO frames will be transferred form CIT to Kashiwa (and Kashiwa to KISTI?) * Omicron can be used on KISTI cluster * We need the information about the amount of data. * CAGMon results will be also available in near future. === 20200423 (Thu.) === * Irregular meeting / Agenda: * 17:00-, zoom 2 https://zoom.us/j/6676627462 * Participants: Kozakai, Ochino, Kokeyama ==== Minutes ==== * How to manage a DQ check for event alerts * Shall we make a proper data quality report for each event? => after collecting information we will make a report and put on JGW doc * Does ligo have the template to be sent to segdb? => to be checked * For now, we make a dedicated wiki page * list a specific check list: For GRB200415A, check resG condition, check if OMC PD A was overflow or not * Share Detchar info with CAL, BURST, DMG * How to organize RRT for the next obs === 20200416 (Thu.) === * Agenda: * Run status * DQ Shift * KISTI activities === 20200402 (Thu.) === * Agenda: * File server status * SummaryPage * Omicron trigger generation * Segment Information * KISTI results capability * Observing run * GlitchPlot for burst analysis * DetChar DQ shift * Update for O4 plan === 20200326 (Thu.) === * Agenda: * Commissioning situation * Commissioning test will be continued until Mar. 31st * During Apr. 1st to 7th, engineering run will be performed. * After Apr. 7th, we have a two weeks observing run (only KAGRA) * If LIGO, and Virgo will come back to observing run, we will aim to join O3. * SummaryPage (RAID trouble) * File server has a disk problem. * RAID system is now being rebuilt. (It will be finished today's evening.) * GlitchPlot for Burst evnet triggers * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=11571|JGW-G2011571]] * DetChar pipelines on KISTI * Code update of CAGMon * === 20200312 (Thu.) === * Agenda: * Current status of site (commissioning) activities * Commissioning break was started from 10th Mar. It continues until 24th Mar. * Joinning O3 should be discussed on JRPC meeting on 26th Mar.(?). * Update of DQ state vector * Science mode during 25th Feb. - 10th Mar. didn't include SDF flags. * I updated to contain the SDF flags as the one of the condition of the Science mode. * Automation plan of GlitchPlot for GW event alert * We plan to move GlitchPlot from ICRR cluster to Kamioka computers. * Requirement: * Disk: 100MB/event * CPU: ??? * Data transfer to KISTI * ER on Dec. data was transferred. * Many tools is already available on KISTI cluster. * Announce about LVK session * We plan to have DetChar telecons instead of LVK meeting. * TY circulate concrete date and time on ML after deciding. === 20200305 (Thu.) === * Agenda: * Observing run status * Binary range is ~400kpc (Best is 500kpc.) * Trigger rate check * Quite difference Trigger rate between the strain signal and the error signal. * Glitch plot with Burst triggers. * SummaryPage troubles * Some process (LSC.ini) was frequently stopped. * RRT tools * Shinkai-san suggested us it's better to prepare the dedicated workstation and mail address. * RRT tools from medm interface is available at Kamioka site * LValert can be receive alert from GraceDB. * Event information is not enough (no mass parameter). * Tagoshi-san tested on Kashiwa server. === 20200227 (Thu.) === * Agenda: * SummaryPage trouble * Configuration file errors -> fixed and checking now (Oshino-san) * Past two day's pages will be regenerated. * RRT * Short-time SummaryPage generator tool on MEDM. * lvalert may be already available for KAGRA. * We can receive RRT call by setting 'GCN PRELIM SENT'. * DQ shift * This taks should be assigned for collaborator shift. * TY will discuss this issue with Miyoki-san. === 20200130 (Thu.) === * Agenda: * KAGRA Readiness * RRT shift * PEM DQ flags === 20200116 (Thu.) === * Agenda: * Minimum goal of KAGRA readiness issue * State Vector definition * goal: send {{{K1:DET-DQ_STATE_VECTOR}}} * status: Done. * DQSEGDB capability * goal: send OBSERVATION segment * status: 95% Automation should be done. (will be done by Robert) * Web page preparation * goal: publish SummaryPage * status: Done. * DQ event validation * under discussion Probably we cannot provide so many veto segments.<<BR>> So at least one (hopefully a few) simple segments will be provided and uploaded.<<BR>> (e.g. Omicron triggered segments, Earthquake segments, etc.) * GraceDB issue * under discussion Full(?) access to GraceDB is opened for KAGRA people.<<BR>> Developing/importing GraceDB API tools is better to be done with DET and DAWG. === 20200109 (Thu.) === * Agenda: * KAGRA readiness issue * State Vector definition * SV is provided on the real-time IFO control model. * SV is contained in both raw frames and low-latency frames. * SV definition is summarized on [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/DET/DataQuality|Wiki]] and kept as latest information. * Finally it should be summarized as a tech-report. * DQSEGDB capability * Segment files are provided on the Kamioka and Kashiwa servers. * Files will be shared with LV by rsync+ssh method. * Accessing gwdet.icrr.u-tokyo.ac.jp from LIGO's DQSEGDB was already successfully. * Web page preparation * SummaryPage is opened also for remote site people. * Contents are being closed to LIGO's SummaryPage contents. * TY and Alex are now updating some softwares on k1sum0. So SummaryPage may become unstable next couple of days. * DetChar/DQ event validataion * We are now planning to provide DQ flags indicating earthquake, loud seismotion, etc. (See Kozakai-san's slide) * These information are shared with LV via DQSEGDB. * Low-Latency tools and GraceDB issues * Some tools used as low-latency ones in LIGO (Omicron, hveto etc.) are available. * We are waiting for the update of GraceDB authentication by LIGO. * Offline DQ [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=11176}|Slides]] * E-run analysis (washimi) [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=11177|Slide]] === 20191121 (Tue.) === * Agenda: * Offline Web tool at Kashiwa * Tools stability * Joint meeting wit Busrt search group === 20191107 (Tue.) === * Agenda: * Offline Web tool at Kashiwa * GlitchPlot [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10935|summary slides]] * Tools stability * [[https://www.icrr.u-tokyo.ac.jp/~washimi/KAGRA/PEM/PEMmap/|PEM MAP]], [[https://www.icrr.u-tokyo.ac.jp/~washimi/KAGRA/PEM/KamioKaminari/|KamioKaminari]], [[https://www.icrr.u-tokyo.ac.jp/~washimi/KAGRA/SEM/|Slow Environment Monitors ]] === 20191031 (Tue.) === * Agenda: * Tools stability * Activities on Kashiwa cluster * Talk on f2f meeting === 20191024 (Tue.) === * Agenda: * Tools stability * KGWG activities * PTEP PWT * Minutes: * https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10903 === 20191010 (Tue.) === * Agenda: * SummaryPage update * DetChar data server at Kamioka * Data transfer to KISTI (If someone knows the situation) === 20190905 (Tue.) === * Agenda: * SummaryPage updates * Minutes * https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10785 === 20190827 (Thu.) === * SummaryPageMeeting20190827 === 20190801 (Thu.) === * Agenda: * Each pipeline status (Omicron, Fscan, Glitch plot…) * Purpose/Goal of the next engineering run === 20190725 (Thu.) === * Agenda * Engineering run results from data analysis * DetChar tool automation plan * update of PEM map [[https://github.com/gw-pem/kagra-pem/issues/159|detail]] === 20190723 (Tue.) === * SummaryPageMeeting20190723 === 20190711 (Thu.) === * Agenda * F2F talk(s) === 20190704 (Thu.) === * Agenda * Kashiwa cluster ([[attachment:DET_Kashiwa_Memo.txt|attachment]]) * Engineering run on Jul. 13th. ([[KAGRA/Subgroups/DET/RUN|link]]) * Data Category flags for BURST. ([[KAGRA/Subgroups/DET/DataQuality|link]], [[https://github.com/gw-detchar/DQConvert|generation script]]) * YuzuSummary ([[https://www.icrr.u-tokyo.ac.jp/~yuzu/bKAGRA_summary/html/GlitchPlot/20190702/1246085661.0_K1:IMC-CAV_TRANS_OUT_DQ.html|sample]]) === 20190613 (Thu.) === * Agenda * Database issue * See [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/DET/Meeting/LVK0612|LVK Joint meeting]] * Progresses of Engineering Run analysis * [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/DET/RUN|RUN Summary]] * What else * Announcement * TY requested DMG group to create the detchar account on the Kashiwa server. * Data transfer cannot be done due to much amount of data size. So we are now trying to reduce data size. * TY plan to discuss with Kanda-san on next Tue. and Wed. how to transfer the DetChar information. * Mervyn from Fukuoka Univ. plans to come to Kamioka from 25th to 28th Jun. === LVK 20190611/0612 (Tue/Wed) === [[KAGRA/Subgroups/DET/Meeting/LVK0612|Agenda]] === 20190606 (Thu.) === * Agenda * Urgent task for ER with X-arm cavity * Omicron update (Yamamoto) ... Done. * DQ Vector update (Yamamoto). * Glitch visualization (Kozakai) * SummaryPage update (Yokozawa) * Segment file update (Oshino) * Fscan update (Oshino, Yamamoto) === 20190530 (Thu.) === * Agenda * [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/DET/Task/O3|Task list for O3 run and Engineering Run on 8th Jun]] * [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/DET/DataQuality|Data Quality Flags]] * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10289|Glitch plot]] === 20190523 (Thu.) === * Agenda * Task list for Engineering Run on 8th Jun. * Trigger based plotting tool [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10253|ckozakai]] === 20190516 (Thu.) === * Agenda * Comment of JRPC meeting and PAB review. * * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=xxxx|Minutes]] === 20190509 (Thu.) === * Skipped due to the PAB review. === 20190502 (Thu.) === * Skipped due to the Japanese holiday. === 20190425 (Thu.) === * Agenda * SDF preparation * DQ flags for data analysis * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10147|Minutes]] === 20190418 === * Skipped due to the F2F meeting === 20190411 (Thu.) === * Agenda * SDF flags preparation [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=9228|slide]] * Fscan on SummaryPage * DetChar computers * Tool development [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10044}|slide]] === 20190404 (Thu.) === * Agenda * IMC run (3/29-3/31, 4/3-4/4) * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10024|yamat]] * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10029|ckozakai]] * Progress of Kamioka works * hveto * There are some bugs on the latest version of hveto. * Old version of hveto was installed in k1sumX and will be installed in k1det0. * Fscan * Automation of the Scan is already succeeded. * We found a bug in our cache generation system and start to fix this bug. === 20190328 (Thu.) === * Agenda * Progress of Kamioka works * Fscan run on test computer by manually. * For automating and integrating to SummaryPage, we need to generate Segment file in automatically. * We need to consider how to pick up line information and list up it from FScan results. * Automation of hveto on KISTI is succeeded with PMC error signal and PEM channels. * We start to install hveto on hveto@k1sumX. === 20190322 (Fri.) === * --(Zoom3)-- -> Zoom2 (https://zoom.us/j/6676627462) * Agenda * f2f talk * 1 slot (Status talk -> T. Yamamoto) * DAC satellite [?] * Task list in next week * Sharing the current situation of SummaryPage * Preparing k1det0/1 * Managing SDF for VIS * Installing LIGO's tools and KGWG's tools * Task list of engineering run * Providing glitch information: (t, f, SNR) * Providing line information: (f, df, Amplitude, noise source) * Preparing the information server * hveto and glitch identification (Pil-Jong & Kokeyama) * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=9984|PMC important channel list]] * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=9258|Glitch analysis presented in JPS]] === 20190314 === * Skipped due to the JPS meeting === 20190307 === * Agenda * Task list of engineering run on May * Tools and results from KGWG * Summary Page isseus * f2f talk === 20190228 === * Meeting room * Zoom3 (https://zoom.us/j/5045179604) * Agenda * Magnetic coupling proposal with LV (Jishnu) * Enhancement of SummaryPage * Data sharing between Kamioka, Kashiwa, and KISTI * Young-Min's trip * Slide * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=9903|yamat]] |
* 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. === Past meeting === * [[KAGRA/Subgroups/DET/Meeting/2020|2020]] * [[KAGRA/Subgroups/DET/Meeting/2019|2019]] |
Meetings
- Meeting time: 14:00-15:00 JST/KST on every Thursday
- Meeting room: Zoom
Contents
-
Meetings
-
Agenda & Minutes
- 20211108 (Mon.)
- 20211101 (Mon.)
- 20211025 (Mon.)
- 20211011 (Mon.)
- 20210927 (Mon.)
- 20210906 (Mon.)
- 20210830 (Mon.)
- 20210823 (Mon.)
- 20210816 (Mon.)
- 20210802 (Mon.)
- 20210726 (Mon.)
- 20210719 (Mon.)
- 20210705 (Mon.)
- 20210628 (Mon.)
- 20210621 (Mon.)
- 20210614 (Mon.)
- 20210607 (Mon.)
- 20210531 (Mon.)
- 20210524 (Mon.)
- 20210517 (Mon.)
- 20210510 (Mon.)
- 20210426 (Mon.)
- 20210419 (Mon.)
- 20210408 (Thu.)
- 20210401 (Thu.)
- 20210325 (Thu.)
- 20210317 (Thu.)
- 20210225 (Thu.)
- 20210218 (Thu.)
- 20210204 (Thu.)
- 20210128 (Thu.)
- 20210121 (Thu.)
- 20210107 (Thu.)
- Past meeting
-
Agenda & Minutes
Agenda & Minutes
20211108 (Mon.)
- Agenda
- O3GK Glitch investigation
- Segment information for open data
- Progress of DQR
- Minutes
- O3GK Glitch investigation
- (Kihyun) checked the omega-scan of three channels
The last three pages slide
- Segment information for open data
- (Uchikata) checked which data segments were used for GRB analysis.
- The correct data segments was used for analysis. But, for some reason, the time of the wrong segment was transmitted to gwosc group.
- The open data set will be re-produced by Uchikata-san and Narikawa-san. After that, the data set will be reviewed.
- Progress of DQR
- (Yuzurihara)
- O3GK Glitch investigation
20211101 (Mon.)
- Agenda
O3GK noise budget paper JGW-P2113405-v1
- hveto, O3GK glitches
- Info. for open data
- Progress of DQR
- Minutes
- Info. for open data
We should refer segments on DQSEGDB
- For GW searches: K1-SCIENCE_MODE, DET_FOR_GRB200415A
- We need to check [1270965983, 1270976372) and [1270976435, 1270976783).
- Info. for open data
20211025 (Mon.)
- Agenda
- Omicron glitches (40?, 120Hz)
DQR 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.
- ALS channels has some coincidence.
- Omicron glitches
20211011 (Mon.)
- Agenda
- site commissioning
- omicron/hveto analysis
- DQR
- Minutes
- site commissioning
MC OpLev glitches (klog#18518)
PLL resonance (klog#18466)
IX MN glitches vanished(?) (klog#17876)
- site commissioning
20210927 (Mon.)
- Agenda
- hveto analysis
- O4 commissioning
progress of DQR slide
- Minutes
- hveto
glitch rate was computed for O3GK paper JGW-D2113311
- Clustering (with 0.1s window) was performed on gwpy function
- O4 commissioning
- Commissioning is now pending and suspension health check is ongoing.
- hveto
20210906 (Mon.)
- Agenda
- hveto analysis
- O4 commissioning
- JPS meeting
- Minutes
- O4 commissioning
Turn on the clustering option of Omicron (k-log#18070)
periodic glitches are happening in ITMX (klog#17876)
These glitches seems to be correlated to IXV temperature (#17912)
To find the source of ITMX glitches, there is a investigation (#17980)
Update of summary page : Added ITMX signals for glitch pipeline (k-log#18112)
Implementation of GAS DC control for ITMX (k-log#18153)
- O4 commissioning
20210830 (Mon.)
- Agenda
- hveto analysis
- O4 commissioning
- O4 readiness
- Minutes
- hveto analysis
veto segment list will be shared. => Kihyun
- O4 commissioning
PLL noise (klog#18014)
periodic glitches are happening in ITMX (klog#17876)
MCi and MCo pitch strange behavior (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, gw status, 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
- #15 [Cont'd] State Vector Definition
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.
- hveto analysis
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. k-log k-log 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. k-log
- IMC commissioning is on-going
- f2f meeting
- Status talk of DAC/DET (28th Sat. 9:00~?)
=> Yamamoto
- Contribution talks
Pastavi development (poster) => Yuzurihara
Gaussianity search (poster) => Morisue
- Status talk of DAC/DET (28th Sat. 9:00~?)
- hveto analysis
20210816 (Mon.)
- Agenda
- hveto analysis
- O4 commissioning
- KAGRA readiness
- f2f meeting
- Minutes
- hveto analysis
- O4 commissioning
FNC instability (klog#17748, 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 (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, gw status, 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
- #15 [Cont'd] State Vector Definition
20210802 (Mon.)
- Agenda:
- 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.
- clustering test
- 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, gw status, 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
- #15 [Cont'd] State Vector Definition
- hveto analysis
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
- lvalert
- DET cluster
- no updates
- 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, gw status, 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
- hveto analysis
20210719 (Mon.)
- Agenda:
- hveto analysis
- O4 commissioning
- O4 readiness
- Minutes
- O4 commissioning
- IMC-XARM commissioning
FNC control saturation 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-
- IMC-XARM commissioning
- 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, gw status, 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(?)
- #15 [Cont'd] State Vector Definition
- O4 commissioning
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
- O4 commissioning
- no report
- O3GK paper
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
- 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 klog17188
[Ongoing] PLL also has glitches (maybe) due to electrostatic discharge. 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.
- IMC commissioning
- O3GK paper
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.
- 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 (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)
- Glitch trigger tabs are added.
- Loudest glitches can be seen on Pastavi (only internal ICRR network)
- IMC Commissioning
- O4 white paper
20210614 (Mon.)
- Agenda
- O3GK paper
- O4 whitepaper
O4 commissioning & preparation
- Minutes
- O3GK paper
- O4 white paper
- 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.
- We have now four frequency noise signal (IMC, PMC, PLL-X, PLL-Y)
- Updated PSL, PEM tabs.
- PLL signals are available.
- Updated PSL, PEM tabs.
- IMC Commissioning
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
O4 commissioning & preparation
- CAGMon development
- 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 (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
- no report
DetChar cluster
- no report
- CAGMon development
- O3GK paper
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, gw status, 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(?)
- #15 [Cont'd] State Vector Definition
- 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
- LVAlert
- O3GK paper
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.
- Current spectrum is too clean 1/f noise.
- sound correlation
Investigating sound correlation with three microphones. slide
- lvalert test
- no report
- DET cluster
- no report
- added for some IMC signals and it work well.
- MC circuit noise hunting
- White paper 2021
- O3GK paper
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, gw status, 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
- #15 [Cont'd] State Vector Definition
- 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
- CAGMon development
- KAGRA O4 readiness
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
- no report
- lvalert
- no report
- DET cluster
- no report
- KIW
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
- O3GK analysis
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.
- Sound noise
- O3GK analysis
20210408 (Thu.)
- Agenda
- O3GK analysis
LV alert 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
- hveto re-analysis for a part of data was done.
- O3GK analysis
20210401 (Thu.)
- Agenda
- Progress of hveto analysis
DetChar cluster
- lvalert
- 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.
- 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.
- New slot of DET meeting.
- Announcement
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.
- Progress of hveto analysis
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.
- hveto cross-check
- 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.
- Kamioka cluster
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
- OS installation for master node was done.
- Omega-scan test
- Installation for Kashiwa cluster was done.
- Error is occurred on gwdatafind.
- LVAlert
- Progress of O3GK paper
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.
- 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.
- Progress of O3GK paper
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.
- DQ state vector (Yamamoto)
- Progress of O3GK paper
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)
- 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
- Report from Burst search
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
- Announcement
- 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
- 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.
- Progress of O3GK paper
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.
- Model update will be finished soon.
- Progress of O3GK analysis