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  * IOO: Kitazawa, kokeyama   * IOO: kokeyama

2017/2/26(Mon.)

  • Remote participants by eZuce: Miyoki
  • Report of work (*:responsible person)
    • Alignment and ETMY: *Enomoto
      • Photo sensor noise was improved on Thursday and checked on Friday. We confirmed the noise becomes better.
      • Sampling model of RT model was changed from 16kHz to 2kHz to reduce 10min period glitch.
    • Camera: Inoue, Haino, Yokozawa, Cory, Binhua
      • ETMY Camera was broken by taking too many photos. Camera will be replaced.
      • ITMY camera is being set to look at BS.
      • BS PD will be replaced by Yokozawa.
    • CRY: mirror temperature ~110K.
      • The satellite amplifier has an oscillation for photo sensors at low temperature. Satellite amplifiers which will be used for photo sensors at low temperature should be modified.
  • Work plan (*:responsible person)
    • ETMY: Enomomoto, Ushiba
      • Check the glitch with the 2kHz model.
      • Original REFL port will be tested to pick up Mich signal.
    • IOO: kokeyama
      • IO chassis will be replaced and being prepared.
  • Laser hazard: AM: PSL, PM: Upstream SR2-3 line, and Y-end.
  • Weekly
    • Week of 2/26
      • ETMY tuninng.
      • Beam alignment to REFL port.
      • 2/28: Height change for PRs
    • week of 3/5
      • IYC door will be closed.
      • Exchanging items and cleaning inside the PR2 chamber
    • week of 3/12
      • TMS installation at ETMY.
      • Connecting ducts at the corner area.
    • week of 3/19
      • Vacuum test at at the corner area.
      • TMS alignment using green light at ETMY.
  • Issues
    • DAC output has sometimes zero voltage for 100ms~1s. IO chassis will be replaced.

KAGRA/Commissioning/DailyWork/2018-02-26 (last edited 2018-02-27 08:56:27 by OsamuMiyakawa)