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[ascl:2202.020] distance-omnibus: Distance estimation method for molecular cloud clumps in the Milky Way

distance-omnibus computes posterior DPDFs for catalog sources using the Bayesian application of kinematic distance likelihoods derived from a Galactic rotation curve with prior Distance Probability Density Functions (DPDFs) derived from ancillary data. The methodology and code base are generalized for use with any (sub-)millimeter survey of the Galactic plane.

Code site:
https://github.com/BGPS/distance-omnibus
Described in:
https://ui.adsabs.harvard.edu/abs/2013ApJ...770...39E https://ui.adsabs.harvard.edu/abs/2015ApJ...799...29E
Bibcode:
2022ascl.soft02020E

Views: 2084

ascl:2202.020
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