Bayesian latent model augments negative-binomial globular cluster scaling with a Gaussian observation layer for error propagation and releases Nimble/PyMC code.
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New SBF distance confirms NGC5846_UDG1 lies in the NGC 5846 group and reconciles prior GC counts to ~50 members, supporting a massive dark matter halo.
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Modeling Globular Cluster Counts with Bayesian Latent Models
Bayesian latent model augments negative-binomial globular cluster scaling with a Gaussian observation layer for error propagation and releases Nimble/PyMC code.
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Revisiting the distance and the globular cluster system of the remarkable galaxy UDG1 in the NGC 5846 group
New SBF distance confirms NGC5846_UDG1 lies in the NGC 5846 group and reconciles prior GC counts to ~50 members, supporting a massive dark matter halo.