| dc.contributor.author | Murzakhanov Z. | |
| dc.contributor.author | Levin S. | |
| dc.contributor.author | Belov I. | |
| dc.contributor.author | Krivilev M. | |
| dc.contributor.author | Sharnin L. | |
| dc.date.accessioned | 2018-09-18T20:09:26Z | |
| dc.date.available | 2018-09-18T20:09:26Z | |
| dc.date.issued | 2012 | |
| dc.identifier.issn | 0543-1972 | |
| dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/137079 | |
| dc.description.abstract | A new method for processing the output signal from a gravitational wave direction finder in the measurement problem of detecting and identifying gravitational waves from binary relativistic astrophysical objects is discussed and studied. © 2012 Springer Science+Business Media, Inc. | |
| dc.relation.ispartofseries | Measurement Techniques | |
| dc.subject | gravitational wave detector | |
| dc.subject | gravitational waves | |
| dc.title | The measurement problem of detecting gravitational waves from binary pulsars | |
| dc.type | Article in Press | |
| dc.collection | Публикации сотрудников КФУ | |
| dc.relation.startpage | 1 | |
| dc.source.id | SCOPUS05431972-2012-SID84856566784 |