Differences between revisions 9 and 12 (spanning 3 versions)
Revision 9 as of 2011-06-07 01:12:13
Size: 419
Comment:
Revision 12 as of 2011-06-07 14:44:37
Size: 948
Comment:
Deletions are marked like this. Additions are marked like this.
Line 9: Line 9:
[[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)