Published April 16, 2025
| Version v3
Dataset
Open
DAmodel: Hierarchical Bayesian Modelling of DA White Dwarfs for Spectrophotometric Calibration - Data and SEDs v1.0
Authors/Creators
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Boyd, Benjamin M.1
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Narayan, Gautham2
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Mandel, Kaisey3
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Grayling, Matthew4
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Berres, Aidan
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Li, Mai2
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Do, Aaron5
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Saha, Abhijit6
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Axelrod, Tim
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Matheson, Thomas6
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Olszewski, Edward W
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Bohlin, Ralph C.
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Calamida, Annalisa7
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Deustua, Susana
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Holberg, Jay B.
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Hubeny, Ivan
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MacKenty, John W.
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Rest, Armin8, 7
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Sabbi, Elena
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Stubbs, Christopher W.
- 1. University of Cambridge Institute of Astronomy
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2.
University of Illinois Urbana-Champaign
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3.
Smithsonian Astrophysical Observatory
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4.
University of Cambridge
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5.
University of Hawaiʻi at Mānoa
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6.
National Optical Astronomy Observatory
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7.
Space Telescope Science Institute
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8.
Johns Hopkins University
Description
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