Data and code to reproduce Section 2 in Tayar et al. (2020), which describes typical uncertainties on classical observables (bolometric fluxes and angular diameters) for the characterization of exoplanet host stars.
fbol/calcfbol.py requires a bolometric correction grid available here:
wget --no-check-certificate -r 'https://docs.google.com/uc?export=download&id=1u2CQ65UBHDDn_J4ipg2Bayv7i88R5wua' -O bcgrid.h5
Please cite Choi et al. 2016 and Huber et al. 2017 when using the grid for your research.