Michael William Coughlin
Affiliations: | California Institute of Technology, Pasadena, CA |
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Gravitational wavesGoogle:
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Publications
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Pang PTH, Dietrich T, Coughlin MW, et al. (2023) An updated nuclear-physics and multi-messenger astrophysics framework for binary neutron star mergers. Nature Communications. 14: 8352 |
Andreoni I, Coughlin MW, Perley DA, et al. (2023) Publisher Correction: A very luminous jet from the disruption of a star by a massive black hole. Nature |
Andreoni I, Coughlin MW, Perley DA, et al. (2022) A very luminous jet from the disruption of a star by a massive black hole. Nature |
Burdge KB, Marsh TR, Fuller J, et al. (2022) A 62-minute orbital period black widow binary in a wide hierarchical triple. Nature. 605: 41-45 |
Dietrich T, Coughlin MW, Pang PTH, et al. (2020) Multimessenger constraints on the neutron-star equation of state and the Hubble constant. Science (New York, N.Y.). 370: 1450-1453 |
Abbott R, Abbott TD, Abraham S, et al. (2020) GW190521: A Binary Black Hole Merger with a Total Mass of 150 M_{⊙}. Physical Review Letters. 125: 101102 |
Coughlin MW, Antier S, Dietrich T, et al. (2020) Measuring the Hubble constant with a sample of kilonovae. Nature Communications. 11: 4129 |
Graham MJ, Ford KES, McKernan B, et al. (2020) Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational-Wave Event S190521g. Physical Review Letters. 124: 251102 |
Abbott R, Abbott TD, Abraham S, et al. (2020) Properties and Astrophysical Implications of the 150 M ⊙ Binary Black Hole Merger GW190521 The Astrophysical Journal. 900 |
Abbott R, Abbott TD, Abraham S, et al. (2020) GW190814: Gravitational Waves from the Coalescence of a 23 Solar Mass Black Hole with a 2.6 Solar Mass Compact Object The Astrophysical Journal. 896: 1-20 |