Search for gravitational waves from the millisecond pulsar PSR 0437-471
| dc.contributor.author | Mohanty, S.D. | |
| dc.contributor.author | Heng, I.S. | |
| dc.contributor.author | Blair, D.G | |
| dc.contributor.author | Dhurandhar, S.V. | |
| dc.contributor.author | Tobar, M. | |
| dc.contributor.author | Ivanov, E. | |
| dc.date.accessioned | 2015-03-11T10:57:34Z | |
| dc.date.available | 2015-03-11T10:57:34Z | |
| dc.date.issued | 2015-03-11 | |
| dc.description.abstract | A search for gravitational waves from the millisecond pulsar PSR 0437-471has been initiated using the bar detector NIOBE which is located at the University of Western Australia. This search involves a very long coherent integration of the bar output which may stretch over a few years. We present a detailed report on the data analysis algorithm, called phase plane rotation,which will be used in this search. A discussion of the actual implementation of the algorithm is presented. | en_US |
| dc.identifier.uri | http://hdl.handle.net/11007/2994 | |
| dc.language.iso | en | en_US |
| dc.relation.ispartofseries | IUCAA Preprints; 14/1998; | |
| dc.subject | Gravitational waves | en_US |
| dc.title | Search for gravitational waves from the millisecond pulsar PSR 0437-471 | en_US |
| dc.type | Article | en_US |