five

An IDL routine to estimate the mass of low-mass stars and brown dwarfs (v2)

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DataCite Commons2020-09-04 更新2024-07-25 收录
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https://figshare.com/articles/dataset/An_IDL_routine_to_estimate_the_mass_of_low_mass_stars_and_brown_dwarfs_v2_/1460839/1
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This IDL routine uses the 2MASS and WISE J, H, Ks, W1 and W2 apparent magnitudes and the distance of a given object, along with an estimated age range, to determine its most probable mass range using BT-Settl isochrones (Allard et al. 2013; Baraffe et al. 2003) in a likelihood analysis. Errors on the distance and photometry, when input, are propagated to the estimated mass range. **IMPORTANT NOTE : Please read the header of banyan_mass.pro for installation instructions** Please cite Gagné et al. 2014, Baraffe et al. 2003, Allard et al. 2013 and Rajpurohit et al. 2013 (see links below) if you use this procedure.
提供机构:
figshare
创建时间:
2016-01-19
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