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Found 7 papers, 2 papers with code
Impact of magnetic activity on inferred stellar properties of main sequence Sun-like stars
We also warn that for stars with very high or low inclination angles, the response of modes to activity is more easily observable in the separation ratios and hence will incur a larger bias.
Solar and Stellar Astrophysics
Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the $\it{TESS}$ Continuous Viewing Zones and beyond
Better quality astrometry and simpler target selection than the $\it{Kepler}$ sample makes this data ideal for studies of the local star formation history and evolution of the Galactic disc.
Astrophysics of Galaxies
Fundamental Parameters of Main-Sequence Stars in an Instant with Machine Learning
Our method is open source and freely available for the community to use.
New axion and hidden photon constraints from a solar data global fit
We present a new statistical analysis that combines helioseismology (sound speed, surface helium and convective radius) and solar neutrino observations (the $^8$B and $^7$Be fluxes) to place upper limits to the properties of non standard weakly interacting particles.
Solar and Stellar Astrophysics
New solar opacities, abundances, helioseismology, and neutrino fluxes
We construct solar models with the newly calculated radiative opacities from the Opacity Project (OP) and recently determined (lower) heavy element abundances.
Solar Models: current epoch and time dependences, neutrinos, and helioseismological properties
We calculate accurate solar models and report the detailed time dependences of important solar quantities.
How Uncertain Are Solar Neutrino Predictions?
Solar neutrino fluxes and sound speeds are calculated using a systematic reevaluation of nuclear fusion rates.
