ligo-cgmi

This package computes a source frame coarse-grained chirp mass estimate for gravitational-wave events. This is provided in the form of the probabilities that the chirp mass falls within a set of predetermined bins. In the case of Burst events, the estimate assumes a reshift of zero. There are two types of estimates:

LL (Low-Latency) based: found using the template point estimate, and in the case of CBC events, using the distance information provided by the Bayestar skymap to shift to the source frame
PE (Parameter Estimation) based: found using the source frame parameter estimation samples

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