Published May 16, 2024 | Version v1
Dataset Open

Data affiliated with "Evolution of Flare Activity in GKM Stars Younger than 300 Myr over Five Years of TESS Observations"

  • 1. ROR icon Laboratory for Atmospheric and Space Physics
  • 2. ROR icon Cornell University
  • 3. ROR icon University of Colorado Boulder
  • 4. ROR icon Université de Montréal
  • 5. ROR icon National Solar Observatory

Description

Data and Python scripts affiliated with the publication "Evolution of Flare Activity in GKM Stars Younger than 300 Myr over Five Years of TESS Observations" in the American Astronomical Journals. The manuscript pre-print can be found on arXiv.

This repository contains all of the data used to complete the analysis of the aforementioned manuscript, along with the Python scripts used to create all of the figures in the manuscript. Many of the data products from this manuscript are saved as CSVs, with appropriate column names and units, when applicable.

Additionally, we include the light curves for all targets in this sample, along with the 'probability light curves,' which were used to identify flares in the TESS data. These data products can be found in the zip file 'TESS_stella_outputs.zip'. The rest of the data product is structured as it is on the associated GitHub repository.

Files

data.zip

Files (6.2 GB)

Name Size Download all
md5:9fa85e0083b5c4c8fbdc82d73c9061ad
108.9 MB Preview Download
md5:376c9c56ba32cdbd443cd006e10d5998
24.4 kB Preview Download
md5:f8f9dbbbb0dd76e918088da741ebcc15
6.1 GB Preview Download

Additional details

Related works

Is supplement to
Preprint: 10.48550/arXiv.2405.00850 (DOI)

Software

Repository URL
https://github.com/afeinstein20/young-stellar-flares
Programming language
Python
Development Status
Inactive

References

  • Feinstein, A. D., Seligman, D. Z., France, K., et al. 2024, arXiv:2405.00850. doi:10.48550/arXiv.2405.00850