Sonora 2018: Cloud-free, solar C/O substellar evolution and photometry

<p>These models of the evolution and predicted&nbsp;photometry for non-irradiated, substellar mass objects (brown dwarfs and extrasolar giant planets) belong to the Sonora 2018 model series, to be described in Marley et al., currently in preparation for submission&nbsp;to Astrophysical Journal. Evolution tables provide luminosity,&nbsp;effective temperature, radius, gravity, and moment of inertia as a function of object mass and age. Photometry tables provide expected brightness in a selection of commonly used passbands, including those of JWST.</p> <p>This particular set of tables are for cloudless, solar C/O ratio objects at three metallicities ([M/H]=-0.5, 0.0, +0.5)&nbsp;(relative to Lodders (2010) abundances) with&nbsp;3.25 &le; log g(cgs) &le; 5.5&nbsp;and&nbsp;200 &le; T_eff(K) &le; 2400.&nbsp;&quot;Rainout&quot; chemical equilibrium is assumed.&nbsp;</p> <p>&quot;co1.0&quot; in filename&nbsp;nomenclature refers to 1.0 times the solar C/O ratio.&nbsp;</p> <p>The solar composition [M/H]=0.0 files are the same as in&nbsp;https://zenodo.org/record/1309035#.XoKM6y-ZN3k except for the addition here of moment of inertia column.</p> <p>Errata:</p> <p>README.pdf</p> <p>- units on luminosity are erg/s not erg/s/cm^2&nbsp;(4/13/2020)</p> <p>&nbsp;</p>