Granulation signatures as seen by Kepler short-cadence data. II. A hierarchical route to inferring stellar radii from granulation
Jens R. Larsen, Mia S. Lundkvist, Guy R. Davies, Martin B. Nielsen
astro-ph.SR, astro-ph.EP
Submitted: 2026-05-26
Comments: 13 pages, 6 figures, accepted for publication in A&A, abstract abridged
Project page: https://www.cosmos.esa.int/gaia
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Diagnosing Suboptimal Cotangent Disintegrations in Hamiltonian Monte Carlo
- Hamiltonian Monte Carlo for Hierarchical Models
- Bayesian model averaging: A systematic review and conceptual classification
- The sensitivity and behaviour of the curvature in the 'echelle diagram of red-giant stars
- Granulation signatures as seen by Kepler short-cadence data. I. A decoupling between granulation and oscillation timescales for dwarfs
- The Stagger-grid: A grid of 3D stellar atmosphere models - VI. Surface appearance of stellar granulation
- APOKASC-3: The Third Joint Spectroscopic and Asteroseismic catalog for Evolved Stars in the Kepler Fields
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