A sample of 182 planets from the NASA Exoplanet Archive queried on 2023 March 6 for planets with masses and radii $> 3\sigma$ precision, planetary radii $<$ 4 \earthradius~ and stellar masses $<$ 1.5 \solmass described in Section 2 of Kanodia et al. 2023. We then perform a 4-D fit to the dataset described above, across planetary masses, radii, insolation fluxes, and stellar masses. We use 40 degrees across all four dimensions, and perform 100 trials for Monte-Carlo and Bootstrap simulations each. This is described in Section 3.1 of Kanodia et al. 2023. For ease of download, we have broken up the fit into three separate .zip files - 1. Without the bootstrap or Monte-Carlo results (AllPlanet_RpLt4_StMlt1.5_MRSStM_d40_0MC_0BS.zip) 2. With the bootstrap but not Monte-Carlo results (AllPlanet_RpLt4_StMlt1.5_MRSStM_d40_0MC_100BS.zip) 3. Without the bootstrap but with the Monte-Carlo results (AllPlanet_RpLt4_StMlt1.5_MRSStM_d40_100MC_0BS.zip) Beyond 2-D Mass-Radius Relationships: A Nonparametric and Probabilistic Framework for Characterizing Planetary Samples in Higher Dimensions: Kanodia et al. 2023