Gravitational wave cosmology and astrophysics with large spectroscopic galaxy surveys
by Antonella Palmese, Or Graur, James T. Annis, Segev BenZvi, Eleonora Di Valentino, Juan Garcia-Bellido, Satya Gontcho A Gontcho, Ryan Keeley, Alex Kim, Ofer Lahav, Samaya Nissanke, Kerry Paterson, Masao Sako, Arman Shafieloo, and Yu-Dai Tsai
Published onMay 31, 2019
Gravitational wave cosmology and astrophysics with large spectroscopic galaxy surveys
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Abstract
During the next decade, measurements of the Hubble constant from gravitational wave standard sirens will potentially reach a 1-2% uncertainty. The next generation of spectroscopic galaxy surveys will play a crucial role towards achieving such precision, and towards improving our understanding of gravitational wave sources.
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