Long Term Operation of LISA and Galactic Close White Dwarf Binaries

Details Long Term Operation of LISA and Galactic Close White Dwarf Binaries Long Term Operation of LISA and Galactic Close White Dwarf Binaries

2002-02-20

arxiv.org/abs/astro-ph/0202364v1

Mon.Not.Roy.Astron.Soc. 333 (2002) 469

Astronomy and Astrophysics

Astrophysics

9 pages, 3 figures. To appear in MNRAS

Scientific paper

10.1046/j.1365-8711.2002.05432.x

The binary confusion noise spectrum at LISA band depends strongly on observational period and abundance of Galactic close white dwarf binaries (CWDBs). We have investigated how the number of the resolved Galactic CWDBs varies with operation period of LISA, and found that the resolved number would typically grows by a factor of 5 when the operation period increases from 1yr to 10yr. We have also made a similar estimation for number of CWDBs whose chirp signal can be measured in matched filtering analysis.

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