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Published December 11, 2024 | Version v2
Dataset Open

DAmodel: Hierarchical Bayesian Modelling of DA White Dwarfs for Spectrophotometric Calibration - Data and SEDs v1.0

  • 1. University of Cambridge Institute of Astronomy
  • 2. ROR icon University of Illinois Urbana-Champaign
  • 3. ROR icon Smithsonian Astrophysical Observatory
  • 4. ROR icon University of Cambridge
  • 5. ROR icon University of Hawaiʻi at Mānoa
  • 6. ROR icon National Optical Astronomy Observatory
  • 7. ROR icon Space Telescope Science Institute
  • 8. ROR icon Johns Hopkins University

Description

Data and published SEDs from Boyd et al 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. 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

Files

DA_WD_Boyd_et_al.zip

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