Published June 22, 2023
| Version v1
Dataset
Open
A calibration point for stellar evolution from massive star asteroseismology: supplementary dataset
Authors/Creators
- 1. Institute of Astronomy, KU Leuven, Leuven, Belgium
- 2. Instituto de Astrofísica de Canarias, La Laguna, Spain; Departamento de Astrofísica, Universidad de La Laguna, La Laguna, Spain.
- 3. Institute of Astronomy, KU Leuven, Leuven, Belgium; Department of Astrophysics, IMAPP, Radboud University Nijmegen, Nijmegen, the Netherlands; Max Planck Institute for Astronomy, Heidelberg, Germany.
- 4. Laboratoire Lagrange, UMR7293, Observatoire de la Côte d'Azur, Université de Nice Sophia-Antipolis, CNRS, Nice, France.
- 5. Department of Astronomy, University of Wisconsin-Madison, Madison, WI, USA; Kavli Institute for Theoretical Physics, University of California, Santa Barbara, CA, USA.
- 6. Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland.
- 7. IRAP, UPS, CNES, Université de Toulouse, CNRS, Toulouse, France; Institute of Astronomy, KU Leuven, Leuven, Belgium
- 8. Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA.
Description
Dataset related to the article "A calibration point for stellar evolution from massive star asteroseismology" by Burssens et al. 2022 published in Nature Astronomy on the 22nd of June 2023.
This dataset contains:
1) The frequency list derived from the cycle 2 TESS data set of HD192575 in machine-readable format. Units are provided in the article.
2) The MESA/GYRE inlists needed to reproduce models and figures.
See the article for more detailed information.
Files
HD192575_Supp_data.zip
Files
(32.7 kB)
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