論文

査読有り
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
  • N Seto

333
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
DOI
https://doi.org/10.1046/j.1365-8711.2002.05432.x
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000176299500027&DestApp=WOS_CPL
ID情報
  • DOI : 10.1046/j.1365-8711.2002.05432.x
  • ISSN : 0035-8711
  • Web of Science ID : WOS:000176299500027

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