PBjam: A Python package for automating asteroseismology of solar-like oscillators. (arXiv:2012.00580v1 [astro-ph.SR])
<a href="http://arxiv.org/find/astro-ph/1/au:+Nielsen_M/0/1/0/all/0/1">M. B. Nielsen</a> (1 and 2 and 3), <a href="http://arxiv.org/find/astro-ph/1/au:+Davies_G/0/1/0/all/0/1">G. R. Davies</a> (1), <a href="http://arxiv.org/find/astro-ph/1/au:+Ball_W/0/1/0/all/0/1">W. H. Ball</a> (1 and 2), <a href="http://arxiv.org/find/astro-ph/1/au:+Lyttle_A/0/1/0/all/0/1">A. J. Lyttle</a> (1 and 2), <a href="http://arxiv.org/find/astro-ph/1/au:+Li_T/0/1/0/all/0/1">T. Li</a> (1 and 2), <a href="http://arxiv.org/find/astro-ph/1/au:+Hall_O/0/1/0/all/0/1">O. J. Hall</a> (1 and 2), <a href="http://arxiv.org/find/astro-ph/1/au:+Chaplin_W/0/1/0/all/0/1">W. J. Chaplin</a> (1 and 2), <a href="http://arxiv.org/find/astro-ph/1/au:+Gaulme_P/0/1/0/all/0/1">P. Gaulme</a> (4), <a href="http://arxiv.org/find/astro-ph/1/au:+Carboneau_L/0/1/0/all/0/1">L. Carboneau</a> (1 and 2), <a href="http://arxiv.org/find/astro-ph/1/au:+Ong_J/0/1/0/all/0/1">J. M. J. Ong</a> (5), <a href="http://arxiv.org/find/astro-ph/1/au:+Garcia_R/0/1/0/all/0/1">R. A. Garc&#xed;a</a> (6 and 7), <a href="http://arxiv.org/find/astro-ph/1/au:+Mosser_B/0/1/0/all/0/1">B. Mosser</a> (8), <a href="http://arxiv.org/find/astro-ph/1/au:+Roxburgh_I/0/1/0/all/0/1">I. W. Roxburgh</a> (9 and 1), <a href="http://arxiv.org/find/astro-ph/1/au:+Corsaro_E/0/1/0/all/0/1">E. Corsaro</a> (10), <a href="http://arxiv.org/find/astro-ph/1/au:+Benomar_O/0/1/0/all/0/1">O. Benomar</a> (11 and 3), <a href="http://arxiv.org/find/astro-ph/1/au:+Moya_A/0/1/0/all/0/1">A. Moya</a> (12 and 1), <a href="http://arxiv.org/find/astro-ph/1/au:+Lund_M/0/1/0/all/0/1">M. N. Lund</a> (2) ((1) School of Physics and Astronomy, University of Birmingham, (2) Stellar Astrophysics Centre (SAC), Department of Physics and Astronomy, Aarhus University, (3) Center for Space Science, NYUAD Institute, New York University Abu Dhabi, (4) Max-Planck-Institut f&#xfc;r Sonnensystemforschung, (5) Department of Astronomy, Yale University, (6) IRFU, CEA, Universit&#xe9; Paris-Saclay, (7) AIM, CEA, CNRS, Universit&#xe9; Paris-Saclay, Universit&#xe9; Paris Diderot, Sorbonne Paris Cit&#xe9;, (8) LESIA, Observatoire de Paris, Universit&#xe9; PSL, CNRS, Sorbonne Universit&#xe9;, Universit&#xe9; de Paris, (9) Astronomy Unit, School of Physics and Astronomy, Queen Mary University of London, (10) INAF – Osservatorio Astrofisico di Catania, (11) Solar Science Observatory, NAOJ and Department of Astronomical Science, Sokendai (GUAS), (12) Electrical Engineering, Electronics, Automation and Applied Physics Department, E.T.S.I.D.I, Polytechnic University of Madrid (UPM))

Asteroseismology is an exceptional tool for studying stars by using the
properties of observed modes of oscillation. So far the process of performing
an asteroseismic analysis of a star has remained somewhat esoteric and
inaccessible to non-experts. In this software paper we describe PBjam, an
open-source Python package for analyzing the frequency spectra of solar-like
oscillators in a simple but principled and automated way. The aim of PBjam is
to provide a set of easy-to-use tools to extract information about the radial
and quadrupole oscillations in stars that oscillate like the Sun, which may
then be used to infer bulk properties such as stellar mass, radius and age or
even structure. Asteroseismology and its data analysis methods are becoming
increasingly important as space-based photometric observatories are producing a
wealth of new data, allowing asteroseismology to be applied in a wide range of
contexts such as exoplanet, stellar structure and evolution, and Galactic
population studies.

Asteroseismology is an exceptional tool for studying stars by using the
properties of observed modes of oscillation. So far the process of performing
an asteroseismic analysis of a star has remained somewhat esoteric and
inaccessible to non-experts. In this software paper we describe PBjam, an
open-source Python package for analyzing the frequency spectra of solar-like
oscillators in a simple but principled and automated way. The aim of PBjam is
to provide a set of easy-to-use tools to extract information about the radial
and quadrupole oscillations in stars that oscillate like the Sun, which may
then be used to infer bulk properties such as stellar mass, radius and age or
even structure. Asteroseismology and its data analysis methods are becoming
increasingly important as space-based photometric observatories are producing a
wealth of new data, allowing asteroseismology to be applied in a wide range of
contexts such as exoplanet, stellar structure and evolution, and Galactic
population studies.

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