Differences between revisions 287 and 324 (spanning 37 versions)
⇤ ← Revision 287 as of 2021-11-22 13:28:08 →
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  * Meeting time: 14:00-15:00 JST/KST on every Thursday   * Meeting time: 13:00-13:30 JST/KST on every Monday
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=== 20211122 (Mon.) ===
=== 20220228 (Mon.) ===
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    * Investigation about 120Hz glitches
    * Segments for Open data
    * Progress of DQR
    * Site commissioning
    * Report from LVK DAC telecon
  * Minutes
    * Investigation about 120Hz glitches
    * Segments for Open data
      * Have the provision of information been finished from DET?
      * Yuzurihara finished the review of DQ segments of open data [[https://wiki.ligo.org/LOSC/O3aBulkDataReview|review page]]
    * Progress of DQR
      * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=18966|test of igwn-alert (new LVAlert) is on-going]]
    * Site commissioning
      * X-arm cavity was locked with GR laser frequency in air (a few minutes) ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=18921|klog#18921]])
        * We can see the continuous flash on GigE camera at TMSX.
        * Error signal of Green PDH is K1:ALS-X_PDH_MIXER_DAQ_OUT_DQ
      * Y-arm laser was also reach Y-end (PD and camera) ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=18952|klog#18952]])
        * ETMY damping is the next step for detecting reflected light at ETMY.
    * Report from LVK DAC telecon
      * In order to integrate KAGRA's data for low-latency searches, we need reliable DQ flags.
        * Well known auxiliary (witness) sensors
        * Well known coupling mechanism
        * Suitable threshold in statistically
        * See also [[https://wiki.ligo.org/DetChar/DataQuality/HowToCreateDQFlag|LIGO Wiki]] about DQ flags.

=== 20211115 (Mon.) ===
  * Agenda
    * O3GK Glitch investigation
    * Segment information for open data
    * Progress of DQR
    * Site commissioning
  * Minutes
    * O3GK Glitch investigation => Skipped.
    * Segment information for open data
      * Data reproduction with correct segments were finished.
      * We need to check about error estimation of 4kHz downsampled data. => TY
      * Data will be release at the same time with O3GK paper.
    * Progress of DQR
      * LValert was update as python3 in LIGO.
      * We also need to move new version for O4.
      * Software test will be conducted on k1det0,1 => HY
    * Site commissioning
      * PSL room is now in working mode for future works.
        * PMC, PLL, IMC signals are affected by sound noise.
      * Glitches on MC OpLevs were decreased by wind shields.
        * [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/summary/day/20211101/detchar/mce_yaw/|before]] -> [[https://gwdet.icrr.u-tokyo.ac.jp/~controls/summary/day/20211103/detchar/mce_yaw/|after]]
        * Noise floor level was also improved. ([[https://klog.icrr.u-tokyo.ac.jp/osl/?r=18756|klog#18756]])
        * Alignment jump by seismic disturbance in high frequency (1Hz~) still remains.
          * We need to take care about K1:VIS-MC{I,E,O}_TM_WIT_{P,Y} and K1:IMC-IMMT1_TARNS_QPDA1_DC_{PIT,YAW}_OUT
        * Plot range should be changed on SummaryPages. => SO
-----
=== 20211108 (Mon.) ===
  * Agenda
    * O3GK Glitch investigation
    * Segment information for open data
    * Progress of DQR

  * Minutes (Yuzurihara)
    * O3GK Glitch investigation (Kihyun)
     * Kihyun checked the omega-scan at the time of glitch. [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=13383|slide (see the last three slides)]]
     * There is no glitches in these channels at the same time of the glitch.
    * Segment information for open data (Uchikata)
     * They checked which data segments were used for GRB analysis. The correct DQ segment was used for GRB analysis.
     * For some reason, the wrong segment information was used for open data.
     * The reproduction of open data is on-going. The data set needs the review again.
    * Progress of DQR (Yuzurihara)
     * Recently the new feature to archive the parallel process was added in [[https://o4-dqr.docs.ligo.org/o4-dqr-configuration/#how-to-specify-directory-of-a-task|TaskManager]].
     * Yuzurihara is testing this feature to apply KAGRA data.

=== 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		     * LVK meeting March 2022 [[https://wiki.ligo.org/LSC/Meeting/LVKMeetingMarch2022|wiki]]
    * 120Hz glitches
    * DQ flags for O4
    * progress of DQR
    * lock loss study of GreenX
Line 362: Line 19:
=== 20210628 (Mon.) === === 20220221 (Mon.) ===
Line 364: Line 21:
    * O3GK paper
    * white paper
    * O4 commissioning & preparation		     * 120Hz glitches
    * DQ flags for O4
    * progress of DQR
Line 368: Line 26:
    * 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.		     * 120Hz glitches
      * No updates
    * DQ flags for O4
      * No updates
    * progress of DQR
      * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=19847|klog#19847]]
    * Proposal new tool to see past data by NDS (Darkhan)
Line 444: Line 35:

=== 20210607 (Mon.) ===		 === 20220207 (Mon.) ===
Line 447: Line 37:
    * 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
     * 120Hz glitches
    * Report from [[https://wiki.ligo.org/DetChar/JanFeb2022DetCharF2F|LIGO Detchar F2F Meeting]]
    * DQ flags for O4
    * progress of DQR
  * Minutes
    * 120Hz glitches
      * No updates
    * DQ flags for O4
      * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=13851|slide]]
      * (Yuzurihara) read BLRMS data and made the several plots with 1% and 99% percentile.
      * When KAGRA will be locked as observation mode?
       * hopefully after july, there will be lock trial for two monthes(?)
      * When you set the 1% criteria, always you throw away the 1% data?
       * We might need to consider the better procedure to care that point.
    * progress of DQR
      * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=19671|klog#19671]]
Line 479: Line 55:
=== 20210531 (Mon.) === === 20220131 (Mon.) ===
Line 481: Line 57:
    * 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		     * 120Hz glitches
    * Report from DQR hackathon
    * DQ flags for O4
    * Master thesis (Morisue-san)
Line 518: Line 63:
=== 20210524 (Mon.) === === 20220117 (Mon.) ===
Line 520: Line 65:
    * 120Hz glitches
    * ITMX glitches
    * DQR progress
    * DQ flags for O4
  * Minutes
    * 120Hz glitches
      * No updates
      * Next step is coincidence search with signals around ETMY including local control sensors.
    * ITMX glitches
      * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=19212|klog#19212]]
      * K1:VIS-ITMX_F3_LVDTINF_GAS_{IN1,OUT} have glitches.
      * It seems to occur around AA chassis. (AA and cable replacement didn't help to improve situation).
      * We will try to find glitches on other channels on the same ADC board.
      * This channel should be added to Omicron search on SummaryPages.
    * DQR progress
      * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=13721|JGW-G2213721]]
    * DQ flags for O4
      * No updates
Line 521: Line 84:
    * 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		       * Threshold used for computing a glitch rate was changed as SNR=6.5.
      * It's a same criterion with LIGO, and Virgo.
      * Both GEO and KAGRA's results are now computed and draft was also updated.
Line 644: Line 89:
=== 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
    * 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.
Line 899: Line 90:
  * [[KAGRA/Subgroups/DET/Meeting/2021|2021]]

Meetings

  • Meeting time: 13:00-13:30 JST/KST on every Monday
  • Meeting room: Zoom

Contents

  1. Meetings
    1. Agenda & Minutes
      1. 20220228 (Mon.)
      2. 20220221 (Mon.)
      3. 20220207 (Mon.)
      4. 20220131 (Mon.)
      5. 20220117 (Mon.)
      6. Past meeting

Agenda & Minutes

20220228 (Mon.)

  • Agenda

    • LVK meeting March 2022 wiki

    • 120Hz glitches
    • DQ flags for O4
    • progress of DQR
    • lock loss study of GreenX

20220221 (Mon.)

  • Agenda
    • 120Hz glitches
    • DQ flags for O4
    • progress of DQR
  • Minutes
    • 120Hz glitches
      • No updates
    • DQ flags for O4
      • No updates
    • progress of DQR
    • Proposal new tool to see past data by NDS (Darkhan)

20220207 (Mon.)

  • Agenda
  • Minutes
    • 120Hz glitches
      • No updates
    • DQ flags for O4

      • slide

      • (Yuzurihara) read BLRMS data and made the several plots with 1% and 99% percentile.
      • When KAGRA will be locked as observation mode?
        • hopefully after july, there will be lock trial for two monthes(?)
      • When you set the 1% criteria, always you throw away the 1% data?
        • We might need to consider the better procedure to care that point.
    • progress of DQR

20220131 (Mon.)

  • Agenda
    • 120Hz glitches
    • Report from DQR hackathon
    • DQ flags for O4
    • Master thesis (Morisue-san)

20220117 (Mon.)

  • Agenda
    • 120Hz glitches
    • ITMX glitches
    • DQR progress
    • DQ flags for O4
  • Minutes
    • 120Hz glitches
      • No updates
      • Next step is coincidence search with signals around ETMY including local control sensors.
    • ITMX glitches

      • klog#19212

      • K1:VIS-ITMX_F3_LVDTINF_GAS_{IN1,OUT} have glitches.
      • It seems to occur around AA chassis. (AA and cable replacement didn't help to improve situation).
      • We will try to find glitches on other channels on the same ADC board.

      • This channel should be added to Omicron search on SummaryPages.

    • DQR progress
    • DQ flags for O4
      • No updates
    • O3GK paper
      • Threshold used for computing a glitch rate was changed as SNR=6.5.
      • It's a same criterion with LIGO, and Virgo.
      • Both GEO and KAGRA's results are now computed and draft was also updated.

Past meeting

KAGRA/Subgroups/DET/Meeting (last edited 2024-11-01 12:16:19 by HirotakaYuzurihara)