Accompanying Files for "M/K-Dwarf Exoplanets With Similar Sizes and Instellations to Earth Typically Follow Near-Circular Orbits"

=== gammaposteriors.tar.gz ===

Each file (in the tarball) is named after the corresponding planetary object. The file contains samples drawn from the a-posteriori distribution of rho_{*,transit}/rho_{*,independent}. This ratio is referred to as gamma in the paper.

=== stellarposteriors.tar.gz ===

Each file contains the joint posterior distribution for the fundamental stellar parameters. The columns are:

Mass (Solar masses), Radius (Solar radii), Density (kg/m^3)

=== transittimes.tar.gz ===

A pair of files are produced for each KOI/TOI, named appropriately. The pdf figure is a summary figure showing the TTV data with errors (black), along with the best fitting sinusoidal model in brown. We also report the FAP (false alarm probability) of that signal, the associated TTV period and amplitude as annotations on the figure. We also provide the actual transit times for each epoch, in the files *times.dat, using the columns...

Epoch, Transit Time (BJD_UTC - 2,457,000), Error, TTV (mins), Error (mins)

=== lightcurves.tar.gz ===

Each file contains a detrended light curve, detrended using the method marginalisation process described in the paper. The columns are:

Time (BJD_UTC - 2,400,000*)
Relative Intensity
Uncertainty

For the TOIs, we include a fourth column which is the CROWDSAP value.

* For TOIs, this becomes 2,457,000

=== hbms -> *.tar.gz ===

Each tarball contains samples drawn from the a-posteriori joint distribution of the Hierarchical Bayesian Model (HBM) fits. Each tarball is a distinct model, and thus HBM:

exp.tar.gz - exponential distribution
beta.tar.gz - Beta distribution
rayleigh.tar.gz - Rayleigh distribution
tremaine.tar.gz - Tremaine distribution
exp_without4087.tar.gz - exponential distribution excluding KOI-4087.01
beta_without4087.tar.gz - Beta distribution excluding KOI-4087.01
exp_without4087_fake_0p0.tar.gz - exponential distribution excluding KOI-4087.01, but applied to fake data where e=0.0

There are two types of files in each container.

popchain_*.dat contains posterior samples of the population/hyper-parameters.
hkplate_*.dat contains posterior samples of the population/hyper-parameters.

There are 20 walkers for each file type, labelled 1-20 at the suffix of the file. The columns in each file are organised as follows...

popchain_exp*.dat
mu_e, var_e, loglike
popchain_rayl*.dat
mu_e, var_e, loglike
popchain_trem*.dat
mu_e, var_e, loglike
popchain_beta*.dat
mu_e, var_e, alpha, beta, loglike

hkplatechain_*.dat
h'_1, k'_1, h'_2, k'_2,...