Host galaxies catalog used in LIGO searches for compact binary coalescence events

被引:120
作者
Kopparapu, Ravi Kumar [1 ,2 ]
Hanna, Chad [2 ]
Kalogera, Vicky [3 ]
O'Shaughnessy, Richard [3 ]
Gonzalez, Gabriela [2 ]
Brady, Patrick R. [2 ,4 ]
Fairhurst, Stephen [4 ,5 ,6 ]
机构
[1] Louisiana State Univ, Ctr Computat & Technol, Baton Rouge, LA 70803 USA
[2] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA
[3] Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA
[4] Univ Wisconsin, Dept Phys, Milwaukee, WI 53201 USA
[5] Cardiff Univ, Sch Phys & Astron, Cardiff CF2 3YB, S Glam, Wales
[6] CALTECH, LIGO Lab, Pasadena, CA 91125 USA
基金
美国国家科学基金会;
关键词
binaries : close; catalogs; galaxies : luminosity function; mass function gravitational waves; stars : neutron;
D O I
10.1086/527348
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
An up-to-date catalog of nearby galaxies considered to be hosts of binary compact objects is provided, with complete information about sky position, distance, extinction-corrected blue luminosity, and error estimates. With our current understanding of binary evolution, rates of formation and coalescence for binary compact objects scale with massive-star formation, and hence the (extinction-corrected) blue luminosity of host galaxies. Coalescence events in binary compact objects are among the most promising gravitational-wave sources for ground-based gravitational-wave detectors such as LIGO. Our catalog and associated error estimates are important for the interpretation of analyses carried out for LIGO, in constraining the rates of compact binary coalescence, given an astrophysical population model for the sources considered. We discuss how the notion of effective distance, created to account for the antenna pattern of a gravitational-wave detector, must be used in conjunction with our catalog. We also note that the catalog provided can be used in other astronomical analysis of populations that scale with galaxy blue luminosity.
引用
收藏
页码:1459 / 1467
页数:9
相关论文
共 28 条
  • [1] ABBOTT B, 2007, ARXIV07043368
  • [2] ALLEN B, 2005, GRQC0509116
  • [3] Excess power statistic for detection of burst sources of gravitational radiation -: art. no. 042003
    Anderson, WG
    Brady, PR
    Creighton, JDE
    Flanagan, ÉÉ
    [J]. PHYSICAL REVIEW D, 2001, 63 (04): : 420031 - 4200320
  • [4] A comprehensive study of binary compact objects as gravitational wave sources: Evolutionary channels, rates, and physical properties
    Belczynski, K
    Kalogera, V
    Bulik, T
    [J]. ASTROPHYSICAL JOURNAL, 2002, 572 (01) : 407 - 431
  • [5] BELCZYNSKI K, 2007, ASTROPH0703131
  • [6] BINNEY J, 2000, GALACTIC DYNAMICS
  • [7] K-corrections and filter transformations in the ultraviolet, optical, and near-infrared
    Blanton, Michael R.
    Roweis, Sam
    [J]. ASTRONOMICAL JOURNAL, 2007, 133 (02) : 734 - 754
  • [8] The galaxy luminosity function and luminosity density at redshift z=0.1
    Blanton, MR
    Hogg, D
    Bahcall, NA
    Brinkmann, J
    Britton, M
    Connolly, AJ
    Csabai, I
    Fukugita, M
    Loveday, J
    Meiksin, A
    Munn, JA
    Nichol, RC
    Okamura, S
    Quinn, T
    Schneider, DP
    Shimasaku, K
    Strauss, MA
    Tegmark, M
    Vogeley, MS
    Weinberg, DH
    [J]. ASTROPHYSICAL JOURNAL, 2003, 592 (02) : 819 - 838
  • [9] DRIVER PS, 2007, APJ, V657, pL85
  • [10] Fairhurst S, 2007, ARXIV07072410