B F Schutz 1996 Class. Quantum Grav. 13 A219 doi:10.1088/0264-9381/13/11A/031
B F Schutz
Show affiliationsThe sources of gravitational radiation that seem to be most likely to be detected by planned ground- and space-based gravitational-wave detectors are reviewed, with particular attention to the likely information that observations of them will reveal. A particular emphasis is placed on observations by LISA, the fundamental-physics Cornerstone project of the European Space Agency's Horizon 2000+ programme.
04.30.Db Wave generation and sources
Issue 11A (November 1996)
B F Schutz 1996 Class. Quantum Grav. 13 A219
M. Simon et al. 1999 The Astronomical Journal 117 1594
I Csabai 1994 J. Phys. A: Math. Gen. 27 L417
Russell L Herman 2004 J. Phys. A: Math. Gen. 37 4753
John Baker 2003 Class. Quantum Grav. 20 S201
Scott A Hughes 2001 Class. Quantum Grav. 18 4067
Scott A Hughes and Daniel E Holz 2003 Class. Quantum Grav. 20 S65
Longhua Jiang and Jinwu Ye 2006 J. Phys.: Condens. Matter 18 6907
E Coccia 2003 Class. Quantum Grav. 20 S135
M T Herd et al 2005 J. Phys. D: Appl. Phys. 38 3304