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[[http://gw.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=445|Slide]] (Somiya) [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=445|Slide]] (Somiya)
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[[http://gw.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=446|WG Report]] [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=446|WG Report]]

LCGT-LF Special WG

Final Report Meeting, 2011.6.7 13:00-15:00

Slide (Somiya)

WG Report

bLCGT spectrum and inspiral frequency,inspiral frequency before coalescence (Kanda)

* Answers to the questions from Prof Kawamura

  • Q: What is the IR for 100Ms BBH with bLCGT?
  • A: 2170Mpc
  • Q: Is it the peak at 117Hz or the low-freq slope that decreases the bLCGT BNS IR by 10%?
  • A: Without the vertical coupling, the IR would become 290Mpc. Without entire suspension TN, the IR would become 301Mpc.

1st Meeting, 2011.4.22 13:00-15:00

Slide (Somiya)

Type-A without HL (R. Takahashi)

LCGT/subgroup/ifo/LCGT-LF (last edited 2011-06-17 00:45:49 by OsamuMiyakawa)