DAmodel: Hierarchical Bayesian Modelling of DA White Dwarfs for Spectrophotometric Calibration - Data and SEDs v1.0
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Data and published SEDs from Boyd et al. (2025) v1.0. Synthetic SEDs for each standard are in the "seds" subfolder. The coordinates of a the white dwarf faint standards can be found in "wdfs_coords.txt". Tables from the paper, including synthetic photometry for other surveys, can be found in "paper_tables.zip". Implementation of DAmodel can be found at: github.com/benboyd97/DAmodel wave = angstroms flux = erg cm−2 s −1 A−1 flux_err = erg cm−2 s −1 A−1
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Zenodo创建时间：
2024-12-11
