14 citations · 33 across the 6 of their papers we have counts for
6 papers
All You Need is not : Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background
Haowen Zhong, Francesco Iacovelli, Vuk Mandic +1
Searches for the stochastic gravitational-wave background (SGWB) using ground-based detectors rely heavily on the cross-correlation estimator , whose statistical properti…
Hankel low-rank matrix approximation for gravitational-wave data analysis
Nicholas Geissler, Vladimir Strokov, Christian Kümmerle +2
Next-generation gravitational-wave (GW) detectors, such as the Laser Interferometer Space Antenna (LISA), will observe vast numbers of overlapping signals. Disentangling these sign…
Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors
Haowen Zhong, Bei Zhou, Luca Reali +2
Stochastic gravitational-wave backgrounds can be of either cosmological or astrophysical origin. The detection of an astrophysical stochastic gravitational-wave background with gro…
Intermediate-mass black hole binary parameter estimation with next-generation ground-based detector networks
Luca Reali, Roberto Cotesta, Andrea Antonelli +3
Astrophysical scenarios for the formation and evolution of intermediate-mass black holes (IMBHs) in the mass range remain uncertain,…
LISA double white dwarf binaries as Galactic accelerometers
Reza Ebadi, Vladimir Strokov, Erwin H. Tanin +2
Galactic double white dwarf (DWD) binaries are among the guaranteed sources for the Laser Interferometer Space Antenna (LISA), an upcoming space-based gravitational wave (GW) detec…
Quasimonochromatic LISA Sources in the Frequency Domain
Vladimir Strokov, Emanuele Berti
Among the binary sources of interest for LISA some are quasimonochromatic, in the sense that the change in the gravitational wave frequency $Δf\lesssim 1\;\mbox{yr}^{-1}$ during th…