no code implementations • 4 Feb 2021 • Alexandra E. L. Thomas, William J. Chaplin, Sarbani Basu, Ben Rendle, Guy Davies, Andrea Miglio
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
no code implementations • 30 Nov 2020 • J. Ted Mackereth, Andrea Miglio, Yvonne Elsworth, Benoit Mosser, Savita Mathur, Rafael A. Garcia, Domenico Nardiello, Oliver J. Hall, Mathieu Vrard, Warrick H. Ball, Sarbani Basu, Rachael L. Beaton, Paul G. Beck, Maria Bergemann, Diego Bossini, Luca Casagrande, Tiago L. Campante, William J. Chaplin, Christina Chiappini, Léo Girardi, Andreas Christ Sølvsten Jørgensen, Saniya Khan, Josefina Montalbán, Martin B. Nielsen, Marc H. Pinsonneault, Thaíse S. Rodrigues, Aldo Serenelli, Victor Silva Aguirre, Dennis Stello, Jamie Tayar, Johanna Teske, Jennifer L. van Saders, Emma Willett
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
1 code implementation • 6 Jul 2016 • Earl P. Bellinger, George C. Angelou, Saskia Hekker, Sarbani Basu, Warrick Ball, Elisabeth Guggenberger
Our method is open source and freely available for the community to use.
no code implementations • 7 Jan 2015 • Núria Vinyoles, Aldo Serenelli, Francesco L. Villante, Sarbani Basu, Javier Redondo, Jordi Isern
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
1 code implementation • 16 Dec 2004 • John N. Bahcall, Aldo M. Serenelli, Sarbani Basu
We construct solar models with the newly calculated radiative opacities from the Opacity Project (OP) and recently determined (lower) heavy element abundances.
no code implementations • 17 Oct 2000 • John N. Bahcall, M. H. Pinsonneault, Sarbani Basu
We calculate accurate solar models and report the detailed time dependences of important solar quantities.
no code implementations • 12 May 1998 • John N. Bahcall, Sarbani Basu, M. H. Pinsonneault
Solar neutrino fluxes and sound speeds are calculated using a systematic reevaluation of nuclear fusion rates.