All-sky upper limit for gravitational radiation from spinning neutron stars

Details All-sky upper limit for gravitational radiation from spinning neutron stars All-sky upper limit for gravitational radiation from spinning neutron stars

2003-04-30

arxiv.org/abs/gr-qc/0304107v1

Class.Quant.Grav. 20 (2003) S665-S676

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

12 pages, 4 figures, submitted to Proceedings of 7th Gravitational Wave Data Analysis Workshop, December 17-19, 2002, Kyoto, J

Scientific paper

10.1088/0264-9381/20/17/310

We present results of the all-sky search for gravitational-wave signals from spinning neutron stars in the data of the EXPLORER resonant bar detector. Our data analysis technique was based on the maximum likelihood detection method. We briefly describe the theoretical methods that we used in our search. The main result of our analysis is an upper limit of ${\bf 2\times10^{-23}}$ for the dimensionless amplitude of the continuous gravitational-wave signals coming from any direction in the sky and in the narrow frequency band from 921.00 Hz to 921.76 Hz.

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