2002年6月
Long-term operation of the Laser Interferometer Space Antenna and Galactic close white dwarf binaries
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- 巻
- 333
- 号
- 2
- 開始ページ
- 469
- 終了ページ
- 474
- 記述言語
- 英語
- 掲載種別
- 研究論文(学術雑誌)
- DOI
- 10.1046/j.1365-8711.2002.05432.x
- 出版者・発行元
- BLACKWELL PUBLISHING LTD
The binary confusion noise spectrum in the Laser Interferometer Space Antenna (LISA ) band depends strongly on the observational period and abundance of Galactic close white dwarf binaries (CWDBs). We have investigated how the number of the resolved Galactic CWDBs varies with the operation period of LISA , and found that the resolved number would typically grow by a factor of 5 when the operation period increases from 1 to 10 yr. We have also made a similar estimation for the number of CWDBs, the chirp signal of which can be measured using matched filtering analysis.
- リンク情報
- ID情報
-
- DOI : 10.1046/j.1365-8711.2002.05432.x
- ISSN : 0035-8711
- Web of Science ID : WOS:000176299500027