Planet-to-star radius ratios measured with TESS-Gaia Light Curves.

TGLC Transit Fit Summary This directory contains the script and results from fitting TGLC light curves using the exoplanet package. • The .dat files contain results from transit fits for stars observed in different TESS sectors. These targets are known planets discovered by TESS or Kepler. Each row corresponds to one TESS sector and includes key parameters from the transit model. • .py file — Python script used to fit the TGLC light curves. • PS*.csv files are taken from the NASA Exoplanet Archive. For TESS, we removed planets/publications not selected in our sample and renamed the Planet System table to the PS_reduced.csv • table*.csv files are machine-readable tables for tables in the appendix. Columns of .dat files: • Star_sector: TIC ID and TESS sector (e.g., TIC_410214986_28) • Tmag: TESS-band magnitude of the host star • rhat: Gelman-Rubin R̂ statistic for MCMC convergence (values close to 1.0 indicate good convergence) • p: Orbital period of the planet (in days) • pl_ratror: Planet-to-star radius ratio (Rp/R★) from the literature • pl_ratrorerr1: Positive uncertainty on pl_ratror • pl_ratrorerr2: Negative uncertainty on pl_ratror • value: Planet-to-star radius ratio (Rp/R★) from the TGLC fit • err1: Positive uncertainty on value • err2: Negative uncertainty on value