Institute for Multi-messenger Astrophysics and Cosmology
Publications
ORCID ID: 0000-0002-3835-6729
Selected recent papers
- M. Cavaglia, “Characterization of gravitational-wave detector noise with fractals,” Class. Quant. Grav. 39, no.13, 135012 (2022).
- K. Mogushi et al., “NNETFIX: an artificial neural network-based denoising engine for gravitational-wave signals,” Mach. Learn. Sci. Tech. 2 (2021) 3, 035018.
- Barrett M. Frank et al., “Modeling spurious forces on the LISA spacecraft across a full solar cycle,” Class. Quant. Grav. 37 (2020) 17, 175007.
- Marco Cavaglia, Ashini Modi, “Two-dimensional correlation function of binary black hole coalescences,” Universe 6 (2020) 7, 93.
- M. Cavaglia, K. Staats and T. Gill, “Finding the origin of noise transients in LIGO data with machine learning,” Commun. Comput. Phys. 25, no.4, 963-987 (2019).
Top cite papers
- B. P. Abbott et al. , “GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral”, Phys. Rev. Lett. 119, 161101 (2017).
- B. P. Abbott et al. “Multi-messenger Observations of a Binary Neutron Star Merger”, ApJL 848, L12 (2017).
- B. P. Abbott et al., “GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence, Phys. Rev .Lett. 116 (2016) 24, 241103.