Differences between revisions 2 and 3
Revision 2 as of 2020-04-17 14:51:51
Size: 243
Comment:
Revision 3 as of 2020-04-18 06:37:46
Size: 1097
Comment:
Deletions are marked like this. Additions are marked like this.
Line 7: Line 7:

=== Minutes ===

 * There is no paper about the coupling function method, but this method is already used in LIGO and Virgo.
  * Ask Virgo member about the acoustic noise paper, then contact to LIGO member
 * How about seismic motion paper?
  * 1 year data (seasonal data) with suspension
  * Ask Miyo-san about paper
 * PEM related paper (or internal document) in LIGO and Virgo
  * https://arxiv.org/abs/1409.5160
  * https://pemcoupling.readthedocs.io/en/stable/how-it-works/how-coupling.html
  * GEO noise hunting
   * https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1693
 * Task management by GitHub
 * power line noise offline subtraction
  * Using ADC data in the OMC rack
  * by subtracting, amplitude became 1/10 (Other power line noise contribution?)
 * ADC assignment for offline subtraction
  

Weekly PEM meeting

  • 2020/04/17(Fri) 14:00-(JST)
  • Regular meeting meeting (Japanese)
  • Web meeting with Zoom2 (Zoom2)

  • member : Yokozaq, Ohkawa, Yokoyama, Fujikawa, Washimoi, Akutsu, Tomaru

Minutes

KAGRA/Subgroups/PEM/Meeting/200417/Minute (last edited 2020-04-18 06:37:46 by TakaakiYokozawa)