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gr-qc2025
Effective-one-body modelling of eccentric supermassive black hole binaries for Pulsar Timing Array
Sara Manzini, Stanislav Babak
Pulsar Timing Arrays (PTAs) observations will detect gravitational waves (GWs) from the early inspiral phase of supermassive black hole binaries (SMBHBs) with orbital periods of we…
gr-qc2025
Contamination of transient gravitational waves in LISA data by gaps and glitches
Jonathan R. Gair, Senwen Deng, Stanislav Babak
We present a probabilistic framework to quantify the impact of artefacts (glitches and gaps) in LISA data on transient gravitational wave signals. By modeling both artefacts and tr…
gr-qc2025★ 3 cited
Fast detection and reconstruction of merging Massive Black Hole Binary signals
Senwen Deng, Stanislav Babak, Sylvain Marsat
The Laser Interferometer Space Antenna (LISA) will detect gravitational waves from the population of merging massive black holes binaries (MBHBs) throughout the Universe. The LISA…