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Published June 24, 2025 | Version v1

TESS-miner 100-pc M-dwarf Sample

  • 1. Anton Pannekoek Institute for Astronomy
  • 2. University of Amsterdam
  • 3. Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center
  • 4. Carnegie Institution for Science
  • 5. Department of Physics & Astronomy, The University of California, Irvine

Description

This dataset was used in the analysis presented in Glusman et al. (2025), which investigates the occurrence rates of giant planets orbiting low-mass stars observed by TESS. It contains astrometric, photometric, and stellar parameter data for 149,316 M dwarfs, compiled from Gaia DR3 and the TESS Input Catalog (TIC), as well as derived quantities such as absolute magnitudes, color indices, and stellar properties computed using the empirical relations of Mann et al. (2015, 2019). Each star is also labeled with its spectral type and a classification output from the TESS-Miner pipeline. The dataset provides the foundation for the sample definition and occurrence rate modeling described in the publication.

Files

tessminer_100pc_sample.csv

Files (495.0 MB)

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