2016MNRAS.462.2177K

Query : 2016MNRAS.462.2177K

2016MNRAS.462.2177K - Mon. Not. R. Astron. Soc., 462, 2177-2183 (2016/October-3)

Concise estimate of the expected number of detections for stellar-mass binary black holes by eLISA.

KYUTOKU K. and SETO N.

Abstract (from CDS):

We study prospects for detecting extragalactic binary black holes similar to GW150914 by evolved Laser Interferometer Space Antenna (eLISA). We find that the majority of detected binary black holes will not merge within reasonable observation periods of eLISA in any configuration. While long-arm detectors are highly desired for promoting multiband gravitational-wave astronomy by increasing the detections of merging binaries, the number of total detections can be increased also by improving the acceleration noise. A monochromatic approximation works well to derive semiquantitative features of observational prospects for non-merging binaries with clearly indicating the parameter dependence. Our estimate also suggests that the number of galaxies in the error volume is so small that the host galaxy may be determined uniquely with high confidence.

Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): gravitational waves - binaries: close - binaries: close

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 GrW 150914 GWE ~ ~           ~ 674 1

Query : 2016MNRAS.462.2177K

Basic data :
GrW 150914 -- Gravitational Wave Event
Other object types: otypes_help 		GWE (GrW)
ICRS coord. (ep=J2000) : 		No Coord.
Radial velocity / Redshift / cz : 		V(km/s) 25772 [~] / z(~) 0.09 [~] / cz 26981 [~]
   E 2016ApJ...823L..25K
notes:

Identifiers (3) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

GrW 150914 095045 GrW 150914 NAME GW150914

References (674 between 1850 and 2026) (Total 674)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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