A Synthetic Sample of Short-cadence Solar-like Oscillators for TESS

被引:16
作者
Ball, Warrick H. [1 ,2 ]
Chaplin, William J. [1 ,2 ]
Schofield, Mathew [1 ,2 ]
Miglio, Andrea [1 ,2 ]
Bossini, Diego [3 ]
Davies, Guy R. [1 ,2 ]
Girardi, Leo [3 ]
机构
[1] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[2] Aarhus Univ, Dept Phys & Astron, Stellar Astrophys Ctr, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
[3] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy
基金
欧洲研究理事会; 英国科学技术设施理事会;
关键词
stars: oscillations (including pulsations); STELLAR OSCILLATIONS; FREQUENCY-SHIFTS; ROTATION; HOUNDS; HARE; TRILEGAL; MODES; I;
D O I
10.3847/1538-4365/aaedbc
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
NASA's Transiting Exoplanet Survey Satellite (TESS) has begun a two-year survey of most of the sky, which will include light curves for thousands of solar-like oscillators sampled at a cadence of two minutes. To prepare for this steady stream of data, we present a mock catalog of light curves, designed to realistically mimic the properties of the TESS sample. In the process, we also present the first public release of the asteroFLAG Artificial DataSet Generator, which simulates light curves of solar-like oscillators based on input mode properties. The targets are drawn from a simulation of the Milky Way's populations and are selected in the same way as TESS's true Asteroseismic Target List. The light curves are produced by combining stellar models, pulsation calculations and semi-empirical models of solar-like oscillators. We describe the details of the catalog and provide several examples. We provide pristine light curves to which noise can be added easily. This mock catalog will be valuable in testing asteroseismology pipelines for TESS and our methods can be applied in preparation and planning for other observatories and observing campaigns.
引用
收藏
页数:10
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