GLADE+ : an extended galaxy catalogue for multimessenger searches with advanced gravitational-wave detectors

Author:

Dálya G12ORCID,Díaz R1,Bouchet F R3ORCID,Frei Z14ORCID,Jasche J5ORCID,Lavaux G3ORCID,Macas R6ORCID,Mukherjee S7ORCID,Pálfi M1ORCID,de Souza R S8ORCID,Wandelt B D3910ORCID,Bilicki M11ORCID,Raffai P14ORCID

Affiliation:

1. Institute of Physics, Eötvös Loránd University , 1117 Budapest, Hungary

2. Department of Physics and Astronomy, Universiteit Gent , B-9000 Ghent, Belgium

3. Institut d’Astrophysique de Paris , UMR 7095, CNRS, Sorbonne Université, 98bis Boulevard Arago, F-75014 Paris, France

4. MTA-ELTE Astrophysics Research Group , 1117 Budapest, Hungary

5. The Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova University Centre , SE 106 91 Stockholm, Sweden

6. Institute of Cosmology and Gravitation, University of Portsmouth , Portsmouth PO1 3FX, UK

7. Perimeter Institute for Theoretical Physics , 31 Caroline Street N., Waterloo, ON N2L 2Y5, Canada

8. Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences , 80 Nandan Rd, Shanghai 200030, China

9. Sorbonne Université, Institut Lagrange de Paris , 98 bis Boulevard Arago, F-75014 Paris, France

10. Center for Computational Astrophysics, Flatiron Institute , 162 5th Avenue, New York, NY 10010, USA

11. Center for Theoretical Physics, Polish Academy of Sciences , al. Lotników 32/46, PL-02-668 Warsaw, Poland

Abstract

ABSTRACT We present GLADE+, an extended version of the GLADE galaxy catalogue introduced in our previous paper for multimessenger searches with advanced gravitational-wave detectors. GLADE+ combines data from six separate but not independent astronomical catalogues: the GWGC, 2MPZ, 2MASS XSC, HyperLEDA, and WISExSCOSPZ galaxy catalogues, and the SDSS-DR16Q quasar catalogue. To allow corrections of CMB-frame redshifts for peculiar motions, we calculated peculiar velocities along with their standard deviations of all galaxies having B-band magnitude data within redshift z = 0.05 using the ‘Bayesian Origin Reconstruction from Galaxies’ formalism. GLADE+ is complete up to luminosity distance $d_L=47^{+4}_{-2}$ Mpc in terms of the total expected B-band luminosity of galaxies, and contains all of the brightest galaxies giving 90 per cent of the total B-band and K-band luminosity up to dL ≃ 130 Mpc. We include estimations of stellar masses and individual binary neutron star merger rates for galaxies with W1 magnitudes. These parameters can help in ranking galaxies in a given gravitational wave localization volume in terms of their likelihood of being hosts, thereby possibly reducing the number of pointings and total integration time needed to find the electromagnetic counterpart.

Funder

ANR

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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