Gamma ray bursts and gravitational waves: Triggered search strategy in the LIGO science runs - INSPIRE

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Gamma ray bursts and gravitational waves: Triggered search strategy in the LIGO science runs

S.D. Mohanty
(
- Potsdam, Max Planck Inst. and
- Caltech, Kellogg Lab and
- Oregon U. and
- NASA, Goddard
)
,
S. Marka
(
- Potsdam, Max Planck Inst. and
- Caltech, Kellogg Lab and
- Oregon U. and
- NASA, Goddard
)
,
R. Rahkola
(
- Potsdam, Max Planck Inst. and
- Caltech, Kellogg Lab and
- Oregon U. and
- NASA, Goddard
)
,
S. Mukherjee
(
- Potsdam, Max Planck Inst. and
- Caltech, Kellogg Lab and
- Oregon U. and
- NASA, Goddard
)
,
I. Leonor
(
- Potsdam, Max Planck Inst. and
- Caltech, Kellogg Lab and
- Oregon U. and
- NASA, Goddard
)

2004

Part of Gravitational waves. Proceedings, 5th Edoardo Amaldi Conference, Tirrenia, Italy, July 6-11, 2003

Published in:

Class.Quant.Grav. 21 (2004) S765-S774

Contribution to:

5th Edoardo Amaldi Conference on Gravitational Waves

DOI:

10.1088/0264-9381/21/5/055

Experiments:

LIGO

reference search9 citations

Citations per year

Abstract: (IOP)

We describe a complete analysis pipeline for detecting and estimating gravitational wave signals in conjunction with observations of astrophysical phenomena with an electromagnetic or particle signature, examples of such phenomena being gamma ray bursts (GRB) and supernovae neutrino bursts. Our data analysis methods explicitly account for non-Gaussian and non-stationary features in real interferometric data. This pipeline is meant for signal searches in conjunction with individual GRB triggers and is being used for the analysis of data from the LIGO science runs (S1 and S2). However, many aspects of the pipeline are quite general and can also be used for other broadband interferometric detectors.

talk: Tirrenia 2003/07/06
gravitational radiation: search for
trigger
gamma ray: burst
neutrino: supernova
data analysis method
LIGO

References(31)

Figures(0)

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