Faint white dwarf flux standards: data and models
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| Main Authors: | , , , , , , , , , |
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| Format: | Preprint |
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2024
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| _version_ | 1866915019450482688 |
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| author | Bohlin, Ralph C. Deustua, Susana Narayan, Gautham Saha, Abhijit Calamida, Annalisa Gordon, Karl D. Holberg, Jay B. Hubeny, Ivan Matheson, Thomas Rest, Armin |
| author_facet | Bohlin, Ralph C. Deustua, Susana Narayan, Gautham Saha, Abhijit Calamida, Annalisa Gordon, Karl D. Holberg, Jay B. Hubeny, Ivan Matheson, Thomas Rest, Armin |
| contents | Fainter standard stars are essential for the calibration of larger telescopes. This work adds to the CALSPEC (calibration spectra) database 19 faint white dwarfs (WDs) with all-sky coverage and V magnitudes between 16.5 and 18.7. Included for these stars is new UV (ultraviolet) HST (Hubble Space Telescope) STIS (Space Telescope Imaging Spectrometer) spectrophotometry between 1150 and 3000~Å with a resolution of $\sim$500. Pure hydrogen WD models are fit to these UV spectra and to six-band HST/WFC3 (Wide Field Camera 3) photometry at 0.28 to 1.6~\micron\ to construct predicted model SEDs (spectral energy distributions) covering wavelengths from 900~Å to the JWST (James Webb Space Telescope) limit of 30~\micron\ using well-established CALSPEC procedures for producing flux standards with the goal of 1\% accuracy. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2411_09049 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Faint white dwarf flux standards: data and models Bohlin, Ralph C. Deustua, Susana Narayan, Gautham Saha, Abhijit Calamida, Annalisa Gordon, Karl D. Holberg, Jay B. Hubeny, Ivan Matheson, Thomas Rest, Armin Instrumentation and Methods for Astrophysics Fainter standard stars are essential for the calibration of larger telescopes. This work adds to the CALSPEC (calibration spectra) database 19 faint white dwarfs (WDs) with all-sky coverage and V magnitudes between 16.5 and 18.7. Included for these stars is new UV (ultraviolet) HST (Hubble Space Telescope) STIS (Space Telescope Imaging Spectrometer) spectrophotometry between 1150 and 3000~Å with a resolution of $\sim$500. Pure hydrogen WD models are fit to these UV spectra and to six-band HST/WFC3 (Wide Field Camera 3) photometry at 0.28 to 1.6~\micron\ to construct predicted model SEDs (spectral energy distributions) covering wavelengths from 900~Å to the JWST (James Webb Space Telescope) limit of 30~\micron\ using well-established CALSPEC procedures for producing flux standards with the goal of 1\% accuracy. |
| title | Faint white dwarf flux standards: data and models |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2411.09049 |