The Yet-Unobserved Multi-Messenger Gravitational-Wave Universe. (arXiv:1903.09224v1 [astro-ph.HE])

The Yet-Unobserved Multi-Messenger Gravitational-Wave Universe. (arXiv:1903.09224v1 [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:+Bizouard_M/0/1/0/all/0/1">Marrie-Anne Bizouard</a> (CNRS, OCA), <a href="http://arxiv.org/find/astro-ph/1/au:+Burrows_A/0/1/0/all/0/1">Adam Burrows</a> (Princeton U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Janka_T/0/1/0/all/0/1">Thomas Janka</a> (MPA), <a href="http://arxiv.org/find/astro-ph/1/au:+Kotake_K/0/1/0/all/0/1">Kei Kotake</a> (Fukuoka U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Messer_B/0/1/0/all/0/1">Bronson Messer</a> (ORNL & U. Tennessee), <a href="http://arxiv.org/find/astro-ph/1/au:+Mezzacappa_T/0/1/0/all/0/1">Tony Mezzacappa</a> (ORNL & U. Tennessee), <a href="http://arxiv.org/find/astro-ph/1/au:+Mueller_B/0/1/0/all/0/1">Bernhard Mueller</a> (Monash U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Mueller_E/0/1/0/all/0/1">Ewald Mueller</a> (MPA), <a href="http://arxiv.org/find/astro-ph/1/au:+Papa_M/0/1/0/all/0/1">Maria Alessandra Papa</a> (AEI), <a href="http://arxiv.org/find/astro-ph/1/au:+Reddy_S/0/1/0/all/0/1">Sanjay Reddy</a> (U. Washington), <a href="http://arxiv.org/find/astro-ph/1/au:+Rosswog_S/0/1/0/all/0/1">Stephan Rosswog</a> (Stockholms U.)

Observations with next-generation ground-based detectors further enhanced
with multi-messenger (electromagnetic and neutrino) detections will allow us to
probe new extreme astrophysics. Target sources included: core-collapse
supernovae, continuous emission from isolated or accreting neutron stars, and
bursts from magnetars and other pulsars.

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