2015MNRAS.446.2887S


Query : 2015MNRAS.446.2887S

2015MNRAS.446.2887S - Mon. Not. R. Astron. Soc., 446, 2887-2894 (2015/January-3)

Probability distribution function for inclinations of merging compact binaries detected by gravitational wave interferometers.

SETO N.

Abstract (from CDS):

We analytically discuss probability distribution functions (PDFs) for inclinations of merging compact binaries whose gravitational waves are coherently detected by a network of ground-based interferometers. These PDFs would be useful for studying the possibility of (1) simultaneously detecting electromagnetic signals (such as gamma-ray bursts) associated with binary mergers and (2) statistically constraining the related theoretical models using actual observational data from multi-messenger astronomy. Our approach is similar to Schutz , but we explicitly include the dependence of the polarization angles of the binaries, based on the concise formulation given in Cutler & Flanagan . We find that the overall profiles of the PDFs are similar for any network of second-generation detectors (Advanced-LIGO, Advanced-Virgo, KAGRA and LIGO-India). For example, 5.1 percent of detected binaries would have inclination angle less than 10° with at most 0.1 percent differences between the potential networks. A perturbative expression is also provided for generating the PDFs with a small number of parameters given by directional averages of the quantity ε that characterizes the asymmetry of network sensitivities to two incoming orthogonal polarization modes.

Abstract Copyright: © 2014 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)

Journal keyword(s): gravitational waves - 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 SDSS J112848.22+170418.5 G 11 28 48.22989 +17 04 18.5014           ~ 393 0

Query : 2015MNRAS.446.2887S

Basic data :
SDSS J112848.22+170418.5 -- Galaxy
Other object types:
otypes_help
G (2020ApJS,[FND2022]), gB (2018ApJ,GRB), Rad (2018MNRAS), Opt (SDSS)
ICRS coord. (ep=J2000) :
11 28 48.22989 +17 04 18.5014 (Optical) [ ] C 2020ApJS..249....3A
FK4 coord. (ep=B1950 eq=1950) :
11 26 11.55334 +17 20 50.5659 [ ]
Gal coord. (ep=J2000) :
236.42460712 +68.42409732 [ ]
Radial velocity / Redshift / cz :
V(km/s) 88738 [150] / z(spectroscopic) 0.356800 [0.000500] / cz 106965.95 [149.90]
   (Opt) C 2022ApJ...940...56F
Fluxes (5) :
u (AB) 22.461 [0.366] D 2020ApJS..249....3A
g (AB) 22.059 [0.103] D 2020ApJS..249....3A
r (AB) 20.948 [0.063] C 2020ApJS..249....3A
i (AB) 20.708 [0.070] C 2020ApJS..249....3A
z (AB) 20.541 [0.250] D 2020ApJS..249....3A
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Identifiers (3) :
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SDSS J112848.22+170418.5 GRB 130603B [FND2022] GRB 130603B Host G

References (393 between 1850 and 2026) (Total 393)
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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Velocities : 1   

   


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Data at NED - NASA/IPAC Extragalactic Database : SDSS J112848.22+170418.5

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SDSS J112848.22+170418.5

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