David Shoemaker 2003 Class. Quantum Grav. 20 S11 doi:10.1088/0264-9381/20/10/302
David Shoemaker
Show affiliationsGround-based interferometry for gravitational-wave detection is in a state of rapid evolution. First-generation systems (LIGO, GEO, TAMA, VIRGO) are now (summer 2002) starting or will soon start observations, and second-generation instruments are well into the planning phases. By the time LISA joins the network of gravitational-wave detectors, we will have a mixture of second- and third-generation ground-based instruments observing. We give a description of some probable configurations for the ground-based instruments in that epoch.
95.55.Br Astrometric and interferometric instruments
Issue 10 (21 May 2003)
Received 13 December 2002
Published 25 April 2003
David Shoemaker 2003 Class. Quantum Grav. 20 S11
Pasquale Calabrese and Andrea Gambassi 2005 J. Phys. A: Math. Gen. 38 R133
D A Bruce 1981 J. Phys. C: Solid State Phys. 14 5195
Peter Kuchment 2005 J. Phys. A: Math. Gen. 38 4887
Xin-Fa Deng et al. 2009 ApJ 699 948
J E Burns 2006 Phys. Med. Biol. 51 R1
Stephen Fairhurst et al 2005 Class. Quantum Grav. 22 S1109
Toshikazu Shigeyama and Takuji Tsujimoto 2003 ApJ 598 L47
Tobias Galla 2006 J. Phys. A: Math. Gen. 39 3853
Wako Aoki et al 2000 ApJ 536 L97