Multimessenger Universe with Gravitational Waves from Binaries. (arXiv:1903.09277v1 [astro-ph.HE])

Multimessenger Universe with Gravitational Waves from Binaries. (arXiv:1903.09277v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Sathyaprakash_B/0/1/0/all/0/1">B.S. Sathyaprakash</a> (Penn State and Cardiff University), <a href="http://arxiv.org/find/astro-ph/1/au:+Bailes_M/0/1/0/all/0/1">Matthew Bailes</a> (Swinburne U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Kasliwal_M/0/1/0/all/0/1">Mansi M. Kasliwal</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Nissanke_S/0/1/0/all/0/1">Samaya Nissanke</a> (U. of Amsterdam), <a href="http://arxiv.org/find/astro-ph/1/au:+Anand_S/0/1/0/all/0/1">Shreya Anand</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Andreoni_I/0/1/0/all/0/1">Igor Andreoni</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Colpi_M/0/1/0/all/0/1">Monica Colpi</a> (U. of Milano – Bicocca), <a href="http://arxiv.org/find/astro-ph/1/au:+Coughlin_M/0/1/0/all/0/1">Michael Coughlin</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Hall_E/0/1/0/all/0/1">Evan Hall</a> (MIT), <a href="http://arxiv.org/find/astro-ph/1/au:+Kalogera_V/0/1/0/all/0/1">Vicky Kalogera</a> (Northwestern U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Kasen_D/0/1/0/all/0/1">Dan Kasen</a> (UC Berkeley), <a href="http://arxiv.org/find/astro-ph/1/au:+Sesana_A/0/1/0/all/0/1">Alberto Sesana</a> (U. Birmingham)

Future GW detector networks and EM observatories will provide a unique
opportunity to observe the most luminous events in the Universe involving
matter in extreme environs. They will address some of the key questions in
physics and astronomy: formation and evolution of compact binaries, sites of
formation of heavy elements and the physics of jets.

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