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== Final Report Meeting, 2011.6.7 13:00-15:00 == [[http://gwdoc.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=446|WG Report]] [[attachment:LCGTLF0607_bLCGTspectrum.pdf|bLCGT spectrum and inspiral frequency]],[[attachment:LCGTLF0607_freq_before_merger.pdf|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. |
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| [[attachment:110422.pdf|Slide]] | [[attachment:110422v3.pdf|Slide]] (Somiya) [[attachment:TypeAnoHL.pdf|Type-A without HL]] (R. Takahashi) |
LCGT-LF Special WG
Final Report Meeting, 2011.6.7 13:00-15:00
Slide (Somiya)
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)