A list of galaxies for gravitational wave searches

We present a list of galaxies within 100 Mpc, which we call the Gravitational Wave Galaxy Catalogue (GWGC), that is currently being used in follow-up searches of electromagnetic counterparts from gravitational wave searches. Due to the time constraints of rapid follow-up, a locally available catalogue of reduced, homogenized data is required. To achieve this we used four existing catalogues: an updated version of the Tully Nearby Galaxy Catalog, the Catalog of Neighboring Galaxies, the V8k catalogue and HyperLEDA. The GWGC contains information on sky position, distance, blue magnitude, major and minor diameters, position angle, and galaxy type for 53 255 galaxies. Errors on these quantities are either taken directly from the literature or estimated based on our understanding of the uncertainties associated with the measurement method. By using the PGC numbering system developed for HyperLEDA, the catalogue has a reduced level of degeneracies compared to catalogues with a similar purpose, and is easily updated. We also include 150 Milky Way globular clusters. Finally, we compare the GWGC to previously used catalogues, and find the GWGC to be more complete within 100 Mpc due to our use of more up-to-date input catalogues and the fact that we have not made a blue luminosity cut.

[1]  Joshua R. Smith,et al.  LIGO: The laser interferometer gravitational-wave observatory , 2006, QELS 2006.

[2]  J. P. Huchra,et al.  Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant , 1998, astro-ph/9801080.

[3]  S. Roweis,et al.  K-Corrections and Filter Transformations in the Ultraviolet, Optical, and Near-Infrared , 2006, astro-ph/0606170.

[4]  Herr Waldeyer,et al.  Sitzungsberichte der Königlich Preußischen Akademie der Wissenschaften , 2005, Naturwissenschaften.

[5]  H. Courtois,et al.  THE EXTRAGALACTIC DISTANCE DATABASE , 2009, 0902.3668.

[6]  David Blair,et al.  Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO's fifth science run , 2009 .

[7]  Tomasz Bulik,et al.  A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties , 2001, astro-ph/0111452.

[8]  W. K. Huchtmeier,et al.  A Catalog of Neighboring Galaxies , 2004 .

[9]  R. Nichol,et al.  The Galaxy Luminosity Function and Luminosity Density at Redshift z = 0.1 , 2002, astro-ph/0210215.

[10]  P. Peebles,et al.  Action Principle Solutions for Galaxy Motions within 3000 Kilometers per Second , 1995, astro-ph/9506144.

[11]  Expected Coalescence Rates of Ns-Ns Binaries for Laser Beam Interferometers , 2005, astro-ph/0510727.

[12]  M. Loupias,et al.  Status of VIRGO , 2004 .

[13]  D. Kocevski,et al.  Our Peculiar Motion Away from the Local Void , 2007, 0705.4139.

[14]  E. Phinney The Rate of Neutron Star Binary Mergers in the Universe: Minimal Predictions for Gravity Wave Detectors , 1991 .

[15]  P. Prugniel,et al.  Hyperleda. I. Identification and designation of galaxies , 2003 .

[16]  P. Schechter An analytic expression for the luminosity function for galaxies , 1976 .

[17]  Vicky Kalogera,et al.  Host Galaxies Catalog Used in LIGO Searches for Compact Binary Coalescence Events , 2007, 0706.1283.

[18]  Peter Shawhan,et al.  LOOC UP: locating and observing optical counterparts to gravitational wave bursts , 2008, 0803.0312.

[19]  William E. Harris,et al.  A Catalog of Parameters for Globular Clusters in the Milky Way , 1996 .

[20]  Wendy L. Freedman,et al.  The Tip of the Red Giant Branch as a Distance Indicator for Resolved Galaxies , 1993 .

[21]  R. Tully Nearby groups of galaxies. II - an all-sky survey within 3000 kilometers per second , 1987 .

[22]  L. Nuttall,et al.  Identifying the host galaxy of gravitational wave signals , 2010, 1009.1791.

[23]  An Overview of Gravitational-Wave Sources , 2002, gr-qc/0204090.

[24]  John L. Tonry,et al.  A new technique for measuring extragalactic distances , 1988 .

[25]  Bhasker K. Moorthy,et al.  The First Data Release of the Sloan Digital Sky Survey , 2003, astro-ph/0305492.