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Phys. Rev. D 65, 022001 (2001) [11 pages]

Search for periodic gravitational wave sources with the Explorer detector

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P. Astone1, M. Bassan2, P. Bonifazi3, P. Carelli4, E. Coccia2, C. Cosmelli5, S. D’Antonio6, V. Fafone6, S. Frasca5, Y. Minenkov2, I. Modena2, G. Modestino6, A. Moleti2, G. V. Pallottino5, M. A. Papa7, G. Pizzella2,6, L. Quintieri6, F. Ronga6, R. Terenzi3, and M. Visco3
1Istituto Nazionale di Fisica Nucleare INFN, Rome, Italy
2University of Rome “Tor Vergata” and INFN, Rome, Italy
3IFSI-CNR, Roma, Italy
4University of L’Aquila, L’Aquila, Italy
5University of Rome “La Sapienza” and INFN, Rome, Italy
6Laboratori Nazionali di Frascati-INFN, Frascati, Italy
7Max Planck Institute of Gravitational Physics, AEI, Golm, Germany

Received 2 February 2001; published 19 December 2001

We have developed a procedure for the search of signals from periodic sources in the data of gravitational wave detectors. We report here the analysis of one year of data from the resonant detector Explorer, searching for sources located in the Galactic Center (GC). No signals with amplitude greater than h̅ =2.9×10-24, in the range 921.32–921.38 Hz, were observed using data collected over a time period of 95.7 days, for a source located at α=17.70±0.01h and δ=-29.00±0.05deg. Our procedure can be extended for any assumed position in the sky and for a more general all-sky search, with the proper frequency correction to account for the spin-down and Doppler effects.

© 2001 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.65.022001
DOI:
10.1103/PhysRevD.65.022001
PACS:
04.80.Nn