= Engineering Run 2 (JST 2019/7/13) = <> * JST: Jul. 13, 2019, --(12:00)-- 12:37 - 18:00 JST * GPS: --(1247022018)-- 1247024238 - 1247043618 == Data related == * KAGRA full data * m31:/data/full : Full KAGRA data * Low latency data * m31:/data/ll_merged/ : Low latency data packed in 4096 seconds * hydra:/data/ll_merged/ : Low latency data packed in 4096 seconds * hydra: /data/ll-sharing/shm/llhoft/ : Low latency data (1 second) dumped from shared memory (retained only for 8192 seconds) * channel name * From [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/DET/RUN#ER_with_MICH_on_Jul._13 | ER2 (DetChar)]] * K1:CAL-CS_PROC_MICH_DISPLACEMENT_DQ (We used this channel.) * K1:CAL-CS_PROC_IMC_FREQUENCY_DQ * Low latency data channels * K1:DCS-CALIB_STRAIN_C10 16384 * K1:DCS-CALIB_STATE_VECTOR_C10 16 * K1:CAL-CS_PROC_IMC_FREQUENCY_DQ 16384 * lock flag * K1:GRD-LSC_LOCK_STATE_N = 157 * data quality vector * [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/DET/DataQuality#Online_Data_Quality_Vector | definition]] * We cbc group should check the second bit is 1. * CBC lock segments * We checked lock flag of each data and collected the locked data. We considered lock segments by file units for convenience. If compared with [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/DET/RUN#ER_with_MICH_on_Jul._13 | lock segment(DetChar)]], this lock segment is small slightly. || '''#''' || '''start GPS''' || '''stop GPS''' || '''duration''' || || 1 || 1247024288 || 1247043616 || 19328 || == Off line analysis == === Check point === * Check the available locked data '''(done)''' * Summarize the data length '''(done)''' * Estimate power spectrum density '''(done)''' * Summarize information in pdf '''(done)''' * Generate lock list and segment list '''(done)''' * Generate template bank '''(skipped)''' * How many waveforms we need? '''(skipped)''' * Search signals by matched filter and chi^2 '''(done)''' * Summary the output of search '''(done)''' * histogram of SNR '''(done)''' * glitch list(GPS, JST, mass, ISCO frequency, duration) '''(done)''' === Output of search === * Summary of locked data [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/DAWG/CBC/ER2#Data_related | CBC locked segment]] * Averaged PSD [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10448 | JGWdoc]] * Power spectrum density (PSD) is averaged over 1 sec chunks by taking median. * Calculation time to search for signals * Read 500 sec data : < 1 min * Estimate PSD : 2~3 min. * matched filter+chi^2 with single waveform (not bank) : < 1 min * Histogram of detection statistics [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10448 | JGWdoc]] * If data is Gaussian, =1. * Time series of detection statistics [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10448 | JGWdoc]] * waveform : 1.4 - 1.4 Msun * Beginning and ending 50 sec data were removed from the result. * We uploaded the 3 kinds of time series results which were maximized over rho(matched filter), chi square, rhohat(detection statistics) during 1 second window. We added time series of rho and chi square, because time series of rhohat don't contain the information of the glitch. * File names are * "cbc_max_rho_ER2.txt" (this data indicates the time when data contains high power) * "cbc_max_chi2_ER2.txt" (this data indicates the time when data contains high power in specific frequency band) * "cbc_max_rhohat_ER2.txt" (this data indicates the time when data "might" contains gravitational wave signal) == Online analysis == * Online matched filtering * July 13, 17:08 - 18:00 JST * Using low latency data files (1 sec) dumped from shared memory * About 1 minutes deley * CH: K1:DCS-CALIB_STRAIN_C10 * Template: (30,30)Msun, no spin, Waveform: IMRPhenomD * Used pre-computed PSD * Plots == Link == * [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/DAWG/CBC/ER1 | CBC search in ER1]] * [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/DET/RUN#ER_with_MICH_on_Jul._13 | ER2 (DetChar)]]