L Cadonati et al 2005 Class. Quantum Grav. 22 S1337 doi:10.1088/0264-9381/22/18/S47
L Cadonati1, L Baggio2,9, I S Heng3, W Johnson4, A Mion2, A Ortolan5, S Poggi2, G A Prodi2, F Salemi6, P Sutton7, G Vedovato8, M Zanolin1 and J P Zendri8
Show affiliationsOver the course of a two-week period, starting on Christmas Eve 2003, the recently upgraded AURIGA and the LIGO observatory were simultaneously acquiring data. This first coincidence run between the two projects triggered a new collaborative effort in the search for gravitational wave bursts. This paper introduces the goals of the AURIGA–LIGO joint analysis and the methods that have been formulated to address the challenges of a coincidence between detectors with different spectral sensitivities, bandwidths and antenna patterns. Two approaches are presented, both based on the exchange of event triggers between AURIGA and LIGO: a set of directional coincidence searches, which exploit measured amplitude information, and a cross-correlation search in the LIGO interferometers around the time of the AURIGA events, with minimal assumptions on the signal characteristics.
07.05.Kf Data analysis: algorithms and implementation; data management
Issue 18 (21 September 2005)
Received 1 April 2005, in final form 26 July 2005
Published 6 September 2005
L Cadonati et al 2005 Class. Quantum Grav. 22 S1337
Laura Cadonati and Szabolcs Márka 2005 Class. Quantum Grav. 22 S1159
Francesco Miniati et al. 2001 ApJ 562 233
Stephen M Merkowitz et al 1999 Class. Quantum Grav. 16 3035
P. Panuzzo et al. 2007 ApJ 656 206
Boris Khlebtsov et al 2006 Nanotechnology 17 5167
Eddy Ardonne et al 2005 J. Phys. A: Math. Gen. 38 9183
G V Ermolaev et al 2006 J. Phys. D: Appl. Phys. 39 4236
Charlie Torres and Warren G Anderson 2005 Class. Quantum Grav. 22 S1169
Cullen H. Blake et al. 2008 ApJ 684 635