Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes. (arXiv:1903.09220v1 [astro-ph.HE])

Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes. (arXiv:1903.09220v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Kalogera_V/0/1/0/all/0/1">Vassiliki Kalogera</a> (Northwestern U), <a href="http://arxiv.org/find/astro-ph/1/au:+Berry_C/0/1/0/all/0/1">Christopher P L Berry</a> (Northwestern U.), <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:+Fairhurst_S/0/1/0/all/0/1">Steve Fairhurst</a> (Cardiff U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Justham_S/0/1/0/all/0/1">Stephen Justham</a> (UCAS, Beijing and U. of Amsterdam), <a href="http://arxiv.org/find/astro-ph/1/au:+Mandel_I/0/1/0/all/0/1">Ilya Mandel</a> (Monash U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Mangiagli_A/0/1/0/all/0/1">Alberto Mangiagli</a> (U. of Milano-Bicocca), <a href="http://arxiv.org/find/astro-ph/1/au:+Mapelli_M/0/1/0/all/0/1">Michela Mapelli</a> (U. of Padova), <a href="http://arxiv.org/find/astro-ph/1/au:+Mills_C/0/1/0/all/0/1">Cameron Mills</a> (Cardiff U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Sathyaprakash_B/0/1/0/all/0/1">B.S. Sathyaprakash</a> (Penn State U. and Cardiff U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Schneider_R/0/1/0/all/0/1">Raffaella Schneider</a> (INFN Roma), <a href="http://arxiv.org/find/astro-ph/1/au:+Tauris_T/0/1/0/all/0/1">Thomas Tauris</a> (Aarhus U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Valiante_R/0/1/0/all/0/1">Rosa Valiante</a> (INAF Roma)

Next-generation observations will revolutionize our understanding of binary
black holes and will detect new sources, such as intermediate-mass black holes.
Primary science goals include: Discover binary black holes throughout the
observable Universe; Reveal the fundamental properties of black holes; Uncover
the seeds of supermassive black holes.

Next-generation observations will revolutionize our understanding of binary
black holes and will detect new sources, such as intermediate-mass black holes.
Primary science goals include: Discover binary black holes throughout the
observable Universe; Reveal the fundamental properties of black holes; Uncover
the seeds of supermassive black holes.

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