Published August 2022
| Accepted Version
Journal Article
Open
Chemical Abundances for 25 JWST Exoplanet Host Stars with KeckSpec
Chicago
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Abstract
Using a data-driven machine learning tool we report T_(eff), log(g), vsin(i), and elemental abundances for 15 elements (C, N, O, Na, Mg, Al, Si, Ca, Ti, V, Cr, Mn, Fe, Ni, Y) for a sample of 25 exoplanet host stars targeted by JWST's first year of observations. The chemical diversity of these stars show that, while a number of their companion planets may have formed in a disk with chemistry similar to Solar, some JWST targets likely experienced different disk compositions. This sample is part of a larger forthcoming catalog that will report homogeneous abundances of ∼4,500 FGK stars derived from Keck/HIRES spectra.
Additional Information
© 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Received July 2022. Revised August 2022. Accepted August 2022. Published August 2022.Attached Files
Accepted Version - 2207.13662.pdf
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Additional details
- Eprint ID
- 116226
- Resolver ID
- CaltechAUTHORS:20220810-402964000
- Created
-
2022-08-12Created from EPrint's datestamp field
- Updated
-
2022-08-12Created from EPrint's last_modified field
- Caltech groups
- Astronomy Department