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[ascl:2403.003] kinematic_scaleheight: Infer the vertical distribution of clouds in the solar neighborhood

kinematic_scaleheight uses MCMC methods to kinematically estimate the vertical distribution of clouds in the Galactic plane, including the least squares analysis of Crovisier (1978), an updated least squares analysis using a modern Galactic rotation model, and a Bayesian model sampled via MCMC as described in Wenger et al. (2024).

Code site:
https://github.com/tvwenger/kinematic_scaleheight
Bibcode:
2024ascl.soft03003W
Preferred citation method:

https://doi.org/10.5281/zenodo.10818724


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ascl:2403.003
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