2017MNRAS.466.2212A


Query : 2017MNRAS.466.2212A

2017MNRAS.466.2212A - Mon. Not. R. Astron. Soc., 466, 2212-2216 (2017/April-1)

Using galaxy formation simulations to optimize LIGO follow-up observations.

ANTOLINI E., CAIAZZO I., DAVE R. and HEYL J.S.

Abstract (from CDS):

The recent discovery of gravitational radiation from merging black holes poses a challenge of how to organize the electromagnetic follow-up of gravitational-wave events as well as observed bursts of neutrinos. We propose a technique to select the galaxies that are most likely to host the event given some assumptions of whether the particular event is associated with recent star formation, low-metallicity stars or simply proportional to the total stellar mass in the galaxy. We combine data from the 2-MASS Photometric Redshift Galaxy Catalogue with results from galaxy formation simulations to develop observing strategies that potentially reduce the area of sky to search by up to a factor of 2 relative to an unweighted search of galaxies, and a factor of 20 to a search over the entire LIGOlocalization region.

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

Journal keyword(s): gravitational waves - methods: observational - galaxies: distances and redshifts - galaxies: distances and redshifts

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 : 2017MNRAS.466.2212A

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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