Pulsar Search using the Allegro Gravitational Wave Detector

Details Pulsar Search using the Allegro Gravitational Wave Detector Pulsar Search using the Allegro Gravitational Wave Detector

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aps..apr.c1103m&link_type=abstract

American Physical Society, APS/AAPT Joint Meeting, April 18-21, 1997, abstract #C11.03

Physics

Scientific paper

The majority of effort in analyzing the data from resonant gravitational wave detectors has been to search for burst signals emitted during a supernova explosion. However, resonant detectors have shown themselves capable of running for long time spans with a high duty cycle and a stable noise floor. These features make it worthwhile to examine the data for continuous wave (CW) signals of gravitational radiation produced by millisecond pulsars. We report on the search for a CW signal in the data taken by the Allegro detector. The search is directed towards the globular cluster 47 Tucanae (Tuc) as this area is rich with the millisecond pulsars needed to produce CW radiation in the Allegro bandwidth.

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