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== 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
  * K1:CAL-CS_PROC_C00_STRAIN_DBL_DQ

 * Low latency data channels
  * K1:DCS-CALIB_STRAIN_C10 16384
  * K1:DCS-CALIB_STATE_VECTOR_C10 16
  * K1:DET-DQ_STATE_VECTOR 16

 * lock flag
  * '''LSC_LOCK_STATE_N = 1000'''

 * data quality vector
  * the definition of DQV in full data : [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/DET/DataQuality#Engineering_Run_with_FPMI_from_17th_to_23rd_Dec. | definition]]
  * the definition of DQV in ll_merged data is same as full data.

 * CBC lock segments

  || '''#''' || '''start GPS''' || '''stop GPS''' || '''duration''' ||
  || 1 || xxxx || xxxx || xxxx ||

== Off line analysis(yuzurihara) ==

=== Check point ===

/* '''(done)''' */

 * Check the available locked data
  * Summarize the data length

 * Estimate power spectrum density
  * Summarize information in pdf

 * Generate lock list and segment list

 * Generate template bank
  * How many waveforms we need?

 * Search signals by matched filter and chi^2

 * Summary the output of search
  * histogram of SNR
  * glitch list(GPS, JST, mass, ISCO frequency, duration)

=== Output of search ===

 * Summary of locked data

 * Averaged PSD

  * 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
  * If data is Gaussian, <snr>=1.

 * Time series of detection statistics
  * 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 ==

 * 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)]]

 * [[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/DAWG/CBC/ER2 | CBC search in ER2]]

Engineering Run December 2019

  • JST: Dec. 17, 2019, 17:00 -- Dec. 24, 2019, 9:00
  • GPS:

  • 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
    • K1:CAL-CS_PROC_C00_STRAIN_DBL_DQ
  • Low latency data channels
    • K1:DCS-CALIB_STRAIN_C10 16384
    • K1:DCS-CALIB_STATE_VECTOR_C10 16
    • K1:DET-DQ_STATE_VECTOR 16
  • lock flag
    • LSC_LOCK_STATE_N = 1000

  • data quality vector
    • the definition of DQV in full data : definition

    • the definition of DQV in ll_merged data is same as full data.
  • CBC lock segments
    • #

      start GPS

      stop GPS

      duration

      1

      xxxx

      xxxx

      xxxx

Off line analysis(yuzurihara)

Check point

  • Check the available locked data
    • Summarize the data length
  • Estimate power spectrum density
    • Summarize information in pdf
  • Generate lock list and segment list
  • Generate template bank
    • How many waveforms we need?
  • Search signals by matched filter and chi^2
  • Summary the output of search
    • histogram of SNR
    • glitch list(GPS, JST, mass, ISCO frequency, duration)

  • Summary of locked data
  • Averaged PSD
    • 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
    • If data is Gaussian, <snr>=1.

  • Time series of detection statistics
    • 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

  • Plots

KAGRA/DAWG/CBC/ER-Dec-2019 (last edited 2020-01-08 12:59:52 by HirotakaYuzurihara)