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| * Meeting time: 14:00-15:00 JST/KST on every Thursday * Meeting room: Zoom3 (https://zoom.us/j/5045179604) |
* Meeting time: 13:00-13:30 JST/KST on every Monday * Meeting room: Zoom |
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| === 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. |
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| === 20220228 (Mon.) === * Agenda * announcement * RRT plan during O4 [[https://dcc.ligo.org/G2200220|slide]] * LVK meeting March 2022 [[https://wiki.ligo.org/LSC/Meeting/LVKMeetingMarch2022|wiki]] [[https://cgca.uwm.edu/events/2021lvk|web]] * 120Hz glitches investigation during O3GK * unify conda environment in Kamioka detchar computers, k1sum[01] and k1det[012] (YamaT) * DQ flags for O4 * progress of DQR * lock loss study of GreenX |
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| === 20210204 (Thu.) === | ----- === 20220228 (Mon.) === |
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| * Progress of O3GK paper * O3 data replay * O4 requirement |
* 120Hz glitches * DQ flags for O4 * progress of DQR * lock loss study of GreenX * Minutes (Yuzurihara) * accouncement * LVK meeting March 2022 [[https://wiki.ligo.org/LSC/Meeting/LVKMeetingMarch2022|wiki]] [[https://cgca.uwm.edu/events/2021lvk|web]] * registration is available * Wed, 17 March 2021: * Plenary Session #1 (09:00-10:30 US/CDT) (=3/16 23:00 JST) * Paper Presentation Session #1 * Plenary Session #2 (16:00-17:30 US/CDT) (=3/17 6:00 JST) * Thu, 18 March 2021: * Plenary Session #3 (09:00-10:30 US/CDT) (=3/17 23:00 JST) * Paper Presentation Session #2 * Plenary Session #4 (16:00-17:30 US/CDT) (=3/18 6:00 JST) * Pastavi server will be unavailable tonight * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=19913|klog#19913]] * 120Hz glitches * no update * DQ flags for O4 * no update * progress of DQR * igwn-alert is running more than 9days and receiving the MDC alert * next step is to connect the MDC alert with the launch TaskManager. * remained task is to develop InspiralRange [[https://git.ligo.org/detchar/dqrtasks/-/issues/8|issue]] * lock loss study of GreenX * [[https://klog.icrr.u-tokyo.ac.jp/osl/?r=19906|klog#19906]] * From the Hveto result, the channel (K1:IMC-SERVO_MIXER_DAQ_OUT_DQ) was the most coincident channel with the lock loss of GreenX. * unify the detchar computing environment (YamaT) * scattered codes and applications (Omicron, summary page, ) over Kamioka computers are troubling. * we plan to unify the environment by using igwn conda * detail will be reported in next meeting * (Darkhan) conda environment on k1ctr*. someone accidentally update someone's conda environment. administrator should prepare the conda environment? * (YamaT) k1ctr* share the environment. this activity is not related to k1ctr* but k1sum[01], k1det[012]. we should separate the user environment and the environment for the DET tools * (Darkhan) should avoid accidental mistake. ----- === 20220221 (Mon.) === * Agenda * 120Hz glitches * DQ flags for O4 * progress of DQR |
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| * 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. |
* 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) |
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| === 20210128 (Thu.) === | === 20220207 (Mon.) === |
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| * Report from Burst search * Binary range evaluation with C20 offline h(t) * Progress of O3GK paper |
* 120Hz glitches * Report from [[https://wiki.ligo.org/DetChar/JanFeb2022DetCharF2F|LIGO Detchar F2F Meeting]] * DQ flags for O4 * progress of DQR |
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| * 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 * |
* 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]] |
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| ----- === 20220131 (Mon.) === * Agenda * 120Hz glitches * Report from DQR hackathon * DQ flags for O4 * Master thesis (Morisue-san) |
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| === 20210121 (Thu.) === | ----- === 20220117 (Mon.) === |
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| * Announcement * LVK DetChar call will be held (Jan. 25 19:00 JST, KST) * Progress of O3GK paper * CAGMon results * O3 Data replay |
* 120Hz glitches * ITMX glitches * DQR progress * DQ flags for O4 |
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| * 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. |
* 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 * 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. |
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=== 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. |
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| * [[KAGRA/Subgroups/DET/Meeting/2021|2021]] |
Meetings
- Meeting time: 13:00-13:30 JST/KST on every Monday
- Meeting room: Zoom
Contents
Agenda & Minutes
20220228 (Mon.)
- Agenda
20220228 (Mon.)
- Agenda
- 120Hz glitches
- DQ flags for O4
- progress of DQR
- lock loss study of GreenX
- Minutes (Yuzurihara)
- accouncement
LVK meeting March 2022 wiki web
- registration is available
- Wed, 17 March 2021:
- Plenary Session #1 (09:00-10:30 US/CDT) (=3/16 23:00 JST)
- Paper Presentation Session #1
- Plenary Session #2 (16:00-17:30 US/CDT) (=3/17 6:00 JST)
- Thu, 18 March 2021:
- Plenary Session #3 (09:00-10:30 US/CDT) (=3/17 23:00 JST)
- Paper Presentation Session #2
- Plenary Session #4 (16:00-17:30 US/CDT) (=3/18 6:00 JST)
- Pastavi server will be unavailable tonight
- 120Hz glitches
- no update
- DQ flags for O4
- no update
- progress of DQR
- igwn-alert is running more than 9days and receiving the MDC alert
next step is to connect the MDC alert with the launch TaskManager.
remained task is to develop InspiralRange issue
- lock loss study of GreenX
- From the Hveto result, the channel (K1:IMC-SERVO_MIXER_DAQ_OUT_DQ) was the most coincident channel with the lock loss of GreenX.
- unify the detchar computing environment (YamaT)
- scattered codes and applications (Omicron, summary page, ) over Kamioka computers are troubling.
- we plan to unify the environment by using igwn conda
- detail will be reported in next meeting
- (Darkhan) conda environment on k1ctr*. someone accidentally update someone's conda environment. administrator should prepare the conda environment?
- (YamaT) k1ctr* share the environment. this activity is not related to k1ctr* but k1sum[01], k1det[012]. we should separate the user environment and the environment for the DET tools
- (Darkhan) should avoid accidental mistake.
- accouncement
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)
- 120Hz glitches
20220207 (Mon.)
- Agenda
- 120Hz glitches
Report from LIGO Detchar F2F Meeting
- DQ flags for O4
- progress of DQR
- Minutes
- 120Hz glitches
- No updates
- DQ flags for O4
- (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
- 120Hz glitches
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
- 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.
- 120Hz glitches