Data for "Wide Binary Orbits are Preferentially Aligned with the Orbits of Small Planets, but Probably Not Hot Jupiters"

Data accompanying the paper "Wide Binary Orbits are Preferentially Aligned with the Orbits of Small Planets, but Probably Not Hot Jupiters." The data is organized as follows: control_sample.csv and with_exoplanets_sample.csv are the parameters we use from LOFTI and TESS for each system, as well as the median parameters from the orbit fitting Four zipped folders are provided with_exoplanets_with_isochrones.tar.gz contains the orbit parameters of binary systems that contain exoplanets and are above separations of 3.6 arcseconds (which according to our procedure is the minimum separation that we don't use a generic prior of masses for) with_exoplanets_no_isochrones.tar.gz contains the orbit parameters of binary systems that contain exoplanets and are below separations of 3.6 arcseconds (which according to our procedure is the minimum separation that we don't use a generic prior of masses for) control_with_isochrones.tar.gz contains the orbit parameters of binary systems that compose our control sample and are above separations of 3.6 arcseconds (which according to our procedure is the minimum separation that we don't use a generic prior of masses for) control_no_isochrones.tar.gz contains the orbit parameters of binary systems that compose our control sample and are below separations of 3.6 arcseconds (which according to our procedure is the minimum separation that we don't use a generic prior of masses for) To open the chains of a given filepath, first download LOFTI (https://github.com/logan-pearce/lofti_gaia) and then run data = np.load(filePath,allow_pickle=True).tolist() print(data.inc) print(data.sma) print(data.ecc) data.help