Time-frequency analysis of extreme-mass-ratio inspiral signals in mock LISA data
Creators
Abstract
Extreme-mass-ratio inspirals (EMRIs) of compact objects with mass m ~ 1–10 M⊙ into massive black holes with mass M ~ 10^6 M⊙ can serve as excellent probes of strong-field general relativity. The Laser Interferometer Space Antenna (LISA) is expected to detect gravitational wave signals from ~ 100 EMRIs per year, but the data analysis of EMRI signals poses a unique set of challenges due to their long duration and the extensive parameter space of possible signals. One possible approach is to carry out a search for EMRI tracks in the time-frequency domain. We have applied a time-frequency search to the data from the Mock LISA Data Challenge (MLDC) with promising results. Our analysis used the Hierarchical Algorithm for Clusters and Ridges to identify tracks in the time-frequency spectrogram corresponding to EMRI sources. We then estimated the EMRI source parameters from these tracks. In these proceedings, we discuss the results of this analysis of the MLDC round 1.3 data.
Additional Information
© 2008 IOP Publishing Ltd. JG acknowledges support from St Catharine's College. IM would like to thank the Brinson Foundation, NASA grant NNG04GK98G and NSF grant PHY-0601459 for nancial support. LW's work is supported by the Alexander von Humboldt Foundation's Sofja Kovalevskaja Programme funded by the German Federal Ministry of Education and Research.Attached Files
Published - GAIjpcs08.pdf
Files
GAIjpcs08.pdf
Additional details
Identifiers
- Eprint ID
- 14259
- Resolver ID
- CaltechAUTHORS:20090518-135533616
Funding
- NASA
- NNG04GK98G
- NSF
- PHY-0601459
- German Federal Ministry of Education and Research
Dates
- Created
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2009-08-20Created from EPrint's datestamp field
- Updated
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2022-07-12Created from EPrint's last_modified field