PBjam: A Python']Python Package for Automating Asteroseismology of Solar-like Oscillators

被引:28
|
作者
Nielsen, M. B. [1 ,2 ,3 ]
Davies, G. R. [1 ]
Ball, W. H. [1 ,2 ]
Lyttle, A. J. [1 ,2 ]
Li, T. [1 ,2 ]
Hall, O. J. [1 ,2 ]
Chaplin, W. J. [1 ,2 ]
Gaulme, P. [4 ]
Carboneau, L. [1 ,2 ]
Ong, J. M. J. [5 ]
Garcia, R. A. [6 ,7 ]
Mosser, B. [8 ]
Roxburgh, I. W. [1 ,9 ]
Corsaro, E. [10 ]
Benomar, O. [3 ,11 ,12 ]
Moya, A. [1 ,13 ]
Lund, M. N. [2 ]
机构
[1] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[2] Aarhus Univ, Dept Phys & Astron, Stellar Astrophys Ctr SAC, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
[3] New York Univ Abu Dhabi, NYUAD Inst, Ctr Space Sci, POB 129188, Abu Dhabi, U Arab Emirates
[4] Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany
[5] Yale Univ, Dept Astron, 52 Hillhouse Ave, New Haven, CT 06511 USA
[6] Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette, France
[7] Univ Paris Diderot, Sorbonne Paris Cite, Univ Paris Saclay, AIM,CEA,CNRS, F-91191 Gif Sur Yvette, France
[8] Univ Paris, Sorbonne Univ, CNRS, LESIA,Observ Paris,Univ PSL, F-92195 Meudon, France
[9] Queen Mary Univ London, Sch Phys & Astron, Astron Unit, London E1 4NS, England
[10] Osserv Astrofis Catania, INAF, Via S Sofia 78, I-95123 Catania, Italy
[11] NAOJ, Solar Sci Observ, Mitaka, Tokyo, Japan
[12] Sokendai GUAS, Dept Astron Sci, Mitaka, Tokyo, Japan
[13] Polytech Univ Madrid UPM, Elect Engn Elect Automat & Appl Phys Dept, ETSIDI, E-28012 Madrid, Spain
基金
欧洲研究理事会; 英国科学技术设施理事会; 新加坡国家研究基金会; 欧盟地平线“2020”;
关键词
DIFFERENTIAL ROTATION; RED GIANTS; STARS; FREQUENCIES; MISSION; AGES;
D O I
10.3847/1538-3881/abcd39
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Asteroseismology is an exceptional tool for studying stars 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 nonexperts. 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 quadropole oscillations in stars that oscillate like the Sun, which may then be used to infer bulk properties such as stellar mass, radius, 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.
引用
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页数:9
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