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[[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.

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)