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 |
|