Differences between revisions 1 and 2
Revision 1 as of 2018-04-03 10:44:08
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Revision 2 as of 2018-04-03 10:47:59
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 * Alignment, ETMY: Izumi  * IFO:


 * ETMs:
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 * Oplev:
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 * MIF: Izumi
  * k1bs, k1imc will be connected by Dolphin. ETMs are connected to k1imc by RFM.
Line 25: Line 27:
 * ETMX:
  * Connection between Type A and Cryopayload is done. Cabling is done.
  * Height somehow changed from the last week to this week. We are fixing it, but it seems to change daily.
  * Alignment will be roughly adjusted today, and first contact will be removed today.
  * Circuits and connection to digital system are done. We started matrix tuning.
  * Viewport of Oplev is missing. It will be placed the next, but we need indium.
 * RT model

 * DAQ
Line 33: Line 32:
== 2. ETMX pump-down ==
 * See the check list.
== 2. IFO check list ==
 * It will be prepared soon.
Line 43: Line 42:
 * DAQ fix -> Miyakawa, Yamamoto
Line 57: Line 57:
 * Next meeting: 4/3  * Next meeting: 4/10

Minute of KAGRA commissioning meeting


  • Date: 2018/4/3 11AM~12PM
  • Attendance: Uchiyama, Yamamoto, Ohashi, Miyoki
    • eZuce: Miyakawa, Shoda, Kimura, Suzuki, Yokozawa, Inoue, Ushiba, Tomaru


1. Report of work of the last week and plan of work

  • IFO:
  • ETMs:
    • Mirror motion has been suppressed to ~2urad. Requirement is 1urad.
    • Beam is checked almost every night.
  • Oplev:
  • CAL: Yamamoto, Yokozawa
    • Started using IMC as training of calibration.
      • Simple calibration will be implemented.
    • X end PD is removed at 3/27 today.
  • RT model
  • DAQ

2. IFO check list

  • It will be prepared soon.

3. Operation

  • Please reply accommodation mail from Uchiyama-san.
  • Think for emergency.

4. Tasks or discussions

  • DAQ fix -> Miyakawa, Yamamoto

  • Selection of full channel -> DGS Yamamoto

  • Selection of science channel -> Commissioning Izumi

  • Screens at control room
    • Sensitivity.
    • PEM.
    • Needs laser safety information.
  • GW alert: online alert in the control room might be prepared. -> Togoshi

  • Frequency noise can be measured by middle lock. Large intensity noise can be a problem.

Others

  • Next meeting: 4/10

KAGRA/Commissioning/Weekly/20180403/Minute (last edited 2018-04-03 12:05:59 by OsamuMiyakawa)