Additional source metrics should be generated automatically and then fed into a database. Values of interest will include: a quantified measure of source compactness in Stokes I; fractional polarization; RM at peak of the FDF. We should decide which values need to be calculated and stored, and then implement those additions to the script.
Additional source metrics should be generated automatically and then fed into a database. Values of interest will include: a quantified measure of source compactness in Stokes I; fractional polarization; RM at peak of the FDF. We should decide which values need to be calculated and stored, and then implement those additions to the script.