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Pulling work from scattering/width paper into main #73
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…cy with scattering paper
profxj
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wow, great stuff!
I've left comments, suggestions and the like but am approving too
| thresh, Emin, Emax, self.state.energy.gamma, self.use_log10 | ||
| ).T * w.T).T | ||
| ) | ||
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have you tested whether this changed code gives the same results as before (if run the same way)?
| Note that now, RA, DEC, Gl, and Gb will be present | ||
| But their default values are None | ||
| """ | ||
| # converts to float if in string. Will do nothing if None |
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Am trying to intuit why this would be needed..
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Basically, if people publish an FRB in RA/DEC, or in Gl Gb, but not the other. Makes it easier for entering data. You need Gl, Gb for NE2001 estimates, and to place cuts on Gl, Gb to remove fluctuations due to the Galactic Plane
As per title. This pull adds the capability to fit scattering and width distributions simultaneously with other FRB parameters. it includes work from the scattering paper.