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Matteo Cantiello added We_use_a_a_theoretical__.tex
about 8 years ago
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We use a a theoretical (numerical relativity) template, generated with parameters favored by the output from the GW150914 parameter estimation (see the GW150914 \href{https://dcc.ligo.org/P150914/public}{detection paper}, \citet{Abbott_2016}) This NR template corresponds to the signal expected from a pair of black holes with masses of around 36 and 29 solar masses, merging into a single black hole of 62 solar masses, at a distance of around 410 Mpc.
