Using electromagnetic observations to aid gravitational-wave parameter estimation of compact binaries observed with LISA
We present a first-stage study of the effect of using knowledge from electromagnetic (EM) observations in the gravitational wave (GW) data analysis of Galactic binaries that are predicted to be observed by the new Laser Interferometer Space Antenna in the low-frequency range, \(10^{-4} \mathrm{Hz}
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Veröffentlicht in: | arXiv.org 2012-08 |
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Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
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Online-Zugang: | Volltext |
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Zusammenfassung: | We present a first-stage study of the effect of using knowledge from electromagnetic (EM) observations in the gravitational wave (GW) data analysis of Galactic binaries that are predicted to be observed by the new Laser Interferometer Space Antenna in the low-frequency range, \(10^{-4} \mathrm{Hz} |
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ISSN: | 2331-8422 |
DOI: | 10.48550/arxiv.1207.6770 |