Uploaded July 2022 | Updated September 2026, 1 hour ago
LISA will observe millions of Galactic binaries which carry a unique information about the structure of Milky Way. We analyse LDC2a (Sangria) data set focusing on characterising inspiralling white dwarf binaries. We present the data analysis method for identification the signals, estimating the number of sources and their parameters. We do not rely on the exact knowledge of the instrumental noise and fit it together with GW sources. Finally we present comparison of our results with the catalogue used in producing the simulated data to assess the performance of our method.
Authors: Eric Plagnol, Stas Babak, Maude Lejeune
Presenter: Eric Plagnol
LISA will observe millions of Galactic binaries which carry a unique information about the structure of Milky Way. We analyse LDC2a (Sangria) data set focusing on characterising inspiralling white dwarf binaries. We present the data analysis method for identification the signals, estimating the number of sources and their parameters. We do not rely on the exact knowledge of the instrumental noise and fit it together with GW sources. Finally we present comparison of our results with the catalogue used in producing the simulated data to assess the performance of our method.
Authors: Eric Plagnol, Stas Babak, Maude Lejeune
Presenter: Eric Plagnol
