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== References == === References ===
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 * [[KAGRA/Subgroups/MIF/OpticalCharacterization|Summary of Optical Characterization]]
 * Commissioning (IOO): Evaluation meeting [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12491|JGW-G2112491]]
 * MIF Schedule Estimate for bKAGRA Phase 2 [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=7079|JGW-T1707079]]
 * Definitions for the X arm commissioning [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=8343|JGW-T1808343]]
 * Definitions for the DRMI commissioning [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=9573|JGW-T1909573]]

=== Priority legend ===
 * [A] High priority and/or easy to do
 * [B] Medium priority and/or preferable to do
 * [C] Low priority and/or can skip if too hard
 * [d] Destructive. Might not be able to go back.
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 * [A] Tune f1, f2, f3 frequencies to IMC FSR.
 * [B,d] Replace all the in-vac steering mirrors and pick-off mirrors to proper ones [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12592|JGW-T2112592]]
  * [C,d] Also POP and POS in-vac and in-air dichroic mirrors if necessary.
  * In the process of finalizing the specs
 * [B,d] Replace all the beam splitters in in-air optical tables to non-polarizing beam splitters [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12956|JGW-D2112956]]
  * This is necessary to estimate the polarization content of the interferometer correctly (without too much confusion)
  * BSs arrived at Mozumi on June 30
 * [B,d] Install polarization optics to backward POP or POS, and TRY and TRY.
  * This is necessary to estimate the arm cavity round-trip loss correctly [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=11633|JGW-T2011633]]
  * Items not yet purchased
 * [A] Check actuation efficiencies of IMC mirrors, frequency actuation efficiencies of PSL.
 * [B,d] Install picomotor+PZT steering mirrors for POP green and POS green.
  * Ordered on June 29
 * [B] Install coil driver switch for ETMs (and ITMs?).
  * High power for lock acquisition, low power for low noise mode.
  * High power for ETMX and low power for ETMY is also possible, but anyway we need a switch to turn off the driver.
 * [C,d] Install picomotors to center the beam on oplev QPDs and ASC QPDs.
  * Already PZT mirrors installed for some ASC QPDs?
 * [C] Inject a fake RF signal to PDA1 to reproduce the spurious coupling around the REFL table and ALS racks
   * klogs 10958,10959, 11014, 11315, 12382, 12392,
   * Perhaps illuminating PDA1 by intensity modulated light maybe interesting.
   * Insert Baluns as necessary. [[https://dcc.ligo.org/LIGO-E1200148/public|LIGO-E1200148]]
   * Do other things also.
 * [C] Check ground issues of RF PDs and RF QPDs.
 * [B] Assemble optical table covers
  * IMC REFL: arrived, not assembled
  * TRX and TRY: ordered
  * AS: arrived, not assembled
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 * [A] Measure the finesse at room temperature and at cryogenic temperatures, for both 1064 nm and 532 nm.
 * [B] Measure the round-trip loss by taking into account the effect of birefringence correctly.
   * Measure the beam spot position dependence.
 * [A] Measure the amount of POP/POS p-pol when the arm is locked and unlocked.
 * [A] Measure the mode-matching for both 1064 nm and 532 nm.
 * [B,d] Tune the Gouy phase separation between two QPDs at REFL/AS/TRX.
   * Make sure all the signals are in in-phase.
 * [A] Measure the alignment sensing matrix at REFL/AS/TRX, for ITM and ETM.
   * Try closing ASC loops.
   * Check TRX IR QPDs.
 * [A] Measure modulation depths for f1, f2 and f3.
 * [A] Check ITM and ETM actuation efficiencies.
 * [B] Make a power budget of each ISC detection port.
 * [B] Refining the automation -- mainly for the successive full ifo initial alignment.
 * [B] Leave a record on the demod phases -- for repeating the Schnup asymmetry measurement.
 * [B] Establish IR/Green co-alignment procedure -- for full ifo initial alignment.
 * [B] Could we check out the common mode servo board at this point?
 * [A] Check new fiber noise cancellation system for ALS.
 * [B] Goal of ALS: RMS of 1.7 Hz (CARM width)
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 * Same as Xarm.
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 * [A] Check BS actuation efficiency.
 * [A] Check out the LSC optical gain. Should be easy enough to doublecheck.
 * [A] Measure, again, the contrast defect.
 * [C] Measure the mode content of AS beam using OMC.
 * [B] Record typical Mich length noise.
 * [B] Close the ASC loops -- mainly for the purpose of the initial alignment automation.
 * [B] Refine the automation.
 * [C] Check why the alignment procedure of Xarm->Yarm->PRMI is not good and we took Xarm->PRMI->Yarm. [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12594|JGW-T2112594]]
  * Check beam spot positions on mirrors?
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== FPMI == == Power recycling cavity ==
 * [B] Measure PRY length and PRX length.
  * Previous methods give inconsistent results and also not compatible with Schnupp asymmetry measurements.
 * [C,d] Tune IMC length to PRC length (and re-tune sideband frequencies).
 * [A] Check actuation efficiency of PR mirrors.
 * [A] Measure PRC Gouy phase.
 * [A] Close the ASC loops.
 * [B] Refine the automation.
 * [A] Check out the power build up in the carrier-locked and side-band locked conditions (PRMI)
 * [C] Correlation measurement of p/s-pol sloshing (https://klog.icrr.u-tokyo.ac.jp/osl/?r=9333) against angular fluctuations or whatever.
 * [B] Identification of any drifty suspensions as the carrier is locked -- to support the coming full lock operation.
 * [B] Tune up the triggers and filter shapes for fast lock acquisition.
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== PRFPMI == == Signal recycling cavity ==
 * [A] Check actuation efficiency of SR mirrors.
 * [A] Measure SRC Gouy phase.
 * [B] Automation?

== Dual Recycled Michelson ==
 * [A] Measure power recycling gains for carrier and sidebands, with and without SRC.
 * [B] Measure length sensing matrix.
   * Both for 1f and 3f signals.
   * Optimize the modulation depths if necessary for sufficient signal-to-noise ratio for 3f signals.
 * [B] Measure power at each ISC detection port when DRMI is locked.
 * [B,d] Tune the Gouy phase separation between two QPDs at POP.
 * [B] Measure the alignment sensing matrix at REFL/POP/AS.
  * Try closing ASC loops.
  * Most notably the f1-f2 WFSs at AS (RF QPD is already installed)
 * [C] Examine the mode-hop criteria (https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12213)
   * Which mirror affects most and how much angular motions are tolerable?
   * Is the SRC Gouy phase large enough?
 * [B] Refine automation.
 * [B] Make a noise budget for MICH/PRCL/SRCL.

== Fabry-Perot Michelson ==
 * [B] Measure length sensing matrix.
 * [B] Measure power at each ISC detection port when FPMI is locked.
 * [B] Measure the alignment sensing matrix at REFL/POP/AS/TRX/TRY.
  * Try closing ASC loops.
  * Test out the radiation pressure basis actuation scheme (SOFT/HARD)
 * [A] Do some noise hunting at low frequencies and VIS commissioning with FPMI
  * Perhaps interesting to lock OMC to check out the freq/int noise couplings (down to ~10 Hz) to AS port.
  * Also, rf phase and amp noises.
 * [B] Measure the contrast defect, compare it with Michelson.
 * [C] Measure the mode content of AS beam using OMC, compare it with Michelson.
 * [B] OMC ASC commissioning?
 * [C] Repeat the same measurements as described in
  * klogs 10958,10959, 11014, 11315, 12382, 12392,
  * to make sure whether the problem still persists or not.


== Power Recycled Fabry-Perot Michelson ==
 * [B] Measure length sensing matrix.
 * [B] Measure power recycling gains for carrier and sidebands.
 * [B] Measure power at each ISC detection port when PRFPMI is locked.
 * [B] Measure the alignment sensing matrix at REFL/POP/AS/TRX/TRY.
  * Try closing ASC loops.
 * [B] Refine automation.
  * Review/refine the O3GK lock acquisition process.
 * [B] Measure frequency/intensity noise coupling, down to ~10 Hz.
 * [B] Measure MICH/PRCL to DARM coupling.


== Resonant Sideband Extraction ==
 * [B] Measure length sensing matrix.
 * [B] Measure power recycling gains for carrier and sidebands.
 * [B] Measure the cavity pole.
 * [B] Measure power at each ISC detection port when PRFPMI is locked.
 * [B] Measure the alignment sensing matrix at REFL/POP/AS/TRX/TRY.
  * Try closing ASC loops.
 * [B] Measure MICH/PRCL/SRCL to DARM coupling.

O4 Commissioning Task List

This is a list of things to do for each commissioning stage for O4.

Each stage include ASC.

References

Priority legend

  • [A] High priority and/or easy to do
  • [B] Medium priority and/or preferable to do
  • [C] Low priority and/or can skip if too hard
  • [d] Destructive. Might not be able to go back.

Preparations

  • [A] Tune f1, f2, f3 frequencies to IMC FSR.
  • [B,d] Replace all the in-vac steering mirrors and pick-off mirrors to proper ones JGW-T2112592

    • [C,d] Also POP and POS in-vac and in-air dichroic mirrors if necessary.
    • In the process of finalizing the specs
  • [B,d] Replace all the beam splitters in in-air optical tables to non-polarizing beam splitters JGW-D2112956

    • This is necessary to estimate the polarization content of the interferometer correctly (without too much confusion)
    • BSs arrived at Mozumi on June 30
  • [B,d] Install polarization optics to backward POP or POS, and TRY and TRY.
    • This is necessary to estimate the arm cavity round-trip loss correctly JGW-T2011633

    • Items not yet purchased
  • [A] Check actuation efficiencies of IMC mirrors, frequency actuation efficiencies of PSL.
  • [B,d] Install picomotor+PZT steering mirrors for POP green and POS green.
    • Ordered on June 29
  • [B] Install coil driver switch for ETMs (and ITMs?).
    • High power for lock acquisition, low power for low noise mode.
    • High power for ETMX and low power for ETMY is also possible, but anyway we need a switch to turn off the driver.
  • [C,d] Install picomotors to center the beam on oplev QPDs and ASC QPDs.
    • Already PZT mirrors installed for some ASC QPDs?
  • [C] Inject a fake RF signal to PDA1 to reproduce the spurious coupling around the REFL table and ALS racks
    • klogs 10958,10959, 11014, 11315, 12382, 12392,
    • Perhaps illuminating PDA1 by intensity modulated light maybe interesting.
    • Insert Baluns as necessary. LIGO-E1200148

    • Do other things also.
  • [C] Check ground issues of RF PDs and RF QPDs.
  • [B] Assemble optical table covers
    • IMC REFL: arrived, not assembled
    • TRX and TRY: ordered
    • AS: arrived, not assembled

Xarm

  • [A] Measure the finesse at room temperature and at cryogenic temperatures, for both 1064 nm and 532 nm.
  • [B] Measure the round-trip loss by taking into account the effect of birefringence correctly.
    • Measure the beam spot position dependence.
  • [A] Measure the amount of POP/POS p-pol when the arm is locked and unlocked.
  • [A] Measure the mode-matching for both 1064 nm and 532 nm.
  • [B,d] Tune the Gouy phase separation between two QPDs at REFL/AS/TRX.
    • Make sure all the signals are in in-phase.
  • [A] Measure the alignment sensing matrix at REFL/AS/TRX, for ITM and ETM.
    • Try closing ASC loops.
    • Check TRX IR QPDs.
  • [A] Measure modulation depths for f1, f2 and f3.
  • [A] Check ITM and ETM actuation efficiencies.
  • [B] Make a power budget of each ISC detection port.
  • [B] Refining the automation -- mainly for the successive full ifo initial alignment.
  • [B] Leave a record on the demod phases -- for repeating the Schnup asymmetry measurement.
  • [B] Establish IR/Green co-alignment procedure -- for full ifo initial alignment.
  • [B] Could we check out the common mode servo board at this point?
  • [A] Check new fiber noise cancellation system for ALS.
  • [B] Goal of ALS: RMS of 1.7 Hz (CARM width)

Yarm

  • Same as Xarm.

Michelson

  • [A] Check BS actuation efficiency.
  • [A] Check out the LSC optical gain. Should be easy enough to doublecheck.
  • [A] Measure, again, the contrast defect.
  • [C] Measure the mode content of AS beam using OMC.
  • [B] Record typical Mich length noise.
  • [B] Close the ASC loops -- mainly for the purpose of the initial alignment automation.
  • [B] Refine the automation.
  • [C] Check why the alignment procedure of Xarm->Yarm->PRMI is not good and we took Xarm->PRMI->Yarm. JGW-T2112594

    • Check beam spot positions on mirrors?

Power recycling cavity

  • [B] Measure PRY length and PRX length.
    • Previous methods give inconsistent results and also not compatible with Schnupp asymmetry measurements.
  • [C,d] Tune IMC length to PRC length (and re-tune sideband frequencies).
  • [A] Check actuation efficiency of PR mirrors.
  • [A] Measure PRC Gouy phase.
  • [A] Close the ASC loops.
  • [B] Refine the automation.
  • [A] Check out the power build up in the carrier-locked and side-band locked conditions (PRMI)
  • [C] Correlation measurement of p/s-pol sloshing (https://klog.icrr.u-tokyo.ac.jp/osl/?r=9333) against angular fluctuations or whatever.

  • [B] Identification of any drifty suspensions as the carrier is locked -- to support the coming full lock operation.
  • [B] Tune up the triggers and filter shapes for fast lock acquisition.

Signal recycling cavity

  • [A] Check actuation efficiency of SR mirrors.
  • [A] Measure SRC Gouy phase.
  • [B] Automation?

Dual Recycled Michelson

  • [A] Measure power recycling gains for carrier and sidebands, with and without SRC.
  • [B] Measure length sensing matrix.
    • Both for 1f and 3f signals.
    • Optimize the modulation depths if necessary for sufficient signal-to-noise ratio for 3f signals.
  • [B] Measure power at each ISC detection port when DRMI is locked.
  • [B,d] Tune the Gouy phase separation between two QPDs at POP.
  • [B] Measure the alignment sensing matrix at REFL/POP/AS.
    • Try closing ASC loops.
    • Most notably the f1-f2 WFSs at AS (RF QPD is already installed)
  • [C] Examine the mode-hop criteria (https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12213)

    • Which mirror affects most and how much angular motions are tolerable?
    • Is the SRC Gouy phase large enough?
  • [B] Refine automation.
  • [B] Make a noise budget for MICH/PRCL/SRCL.

Fabry-Perot Michelson

  • [B] Measure length sensing matrix.
  • [B] Measure power at each ISC detection port when FPMI is locked.
  • [B] Measure the alignment sensing matrix at REFL/POP/AS/TRX/TRY.
    • Try closing ASC loops.
    • Test out the radiation pressure basis actuation scheme (SOFT/HARD)
  • [A] Do some noise hunting at low frequencies and VIS commissioning with FPMI
    • Perhaps interesting to lock OMC to check out the freq/int noise couplings (down to ~10 Hz) to AS port.
    • Also, rf phase and amp noises.
  • [B] Measure the contrast defect, compare it with Michelson.
  • [C] Measure the mode content of AS beam using OMC, compare it with Michelson.
  • [B] OMC ASC commissioning?
  • [C] Repeat the same measurements as described in
    • klogs 10958,10959, 11014, 11315, 12382, 12392,
    • to make sure whether the problem still persists or not.

Power Recycled Fabry-Perot Michelson

  • [B] Measure length sensing matrix.
  • [B] Measure power recycling gains for carrier and sidebands.
  • [B] Measure power at each ISC detection port when PRFPMI is locked.
  • [B] Measure the alignment sensing matrix at REFL/POP/AS/TRX/TRY.
    • Try closing ASC loops.
  • [B] Refine automation.
    • Review/refine the O3GK lock acquisition process.
  • [B] Measure frequency/intensity noise coupling, down to ~10 Hz.
  • [B] Measure MICH/PRCL to DARM coupling.

Resonant Sideband Extraction

  • [B] Measure length sensing matrix.
  • [B] Measure power recycling gains for carrier and sidebands.
  • [B] Measure the cavity pole.
  • [B] Measure power at each ISC detection port when PRFPMI is locked.
  • [B] Measure the alignment sensing matrix at REFL/POP/AS/TRX/TRY.
    • Try closing ASC loops.
  • [B] Measure MICH/PRCL/SRCL to DARM coupling.

KAGRA/Subgroups/MIF/O4CommissioningTaskList (last edited 2021-07-07 09:31:56 by YutaMichimura)