-
NextGen
The NextGen Model grid of theoretical spectra. -
TMAP
TMAP. Hydrogen+Helium NLTE Models -
TMAP (Grid 1)
TMAP. Hydrogen+Helium NLTE Models -
ATMO 2020, CEQ
A set of atmosphere models for cool T-Y brown dwarfs and giant exoplanets. Equilibrium chemistry. Valid temperature range: 200-2000K. Only for solar metallicity. -
ATMO 2020, NEQ weak
A set of atmosphere models for cool T-Y brown dwarfs and giant exoplanets. Non equilibrium chemistry (weak). Valid temperature range: 200-2000K. Only for solar metallicity. -
Kurucz ODFNEW /NOVER (2003) alpha:0.0
ATLAS9 Kurucz ODFNEW /NOVER models. Newly computed ODFs with better opacities and better abundances have been used. -
Kurucz ODFNEW /NOVER (2003)
ATLAS9 Kurucz ODFNEW /NOVER models. Newly computed ODFs with better opacities and better abundances have been used. -
Kurucz ODFNEW /NOVER (2003) alpha:0.4
ATLAS9 Kurucz ODFNEW /NOVER models. Newly computed ODFs with better opacities and better abundances have been used. -
ATMO 2020, NEQ strong
A set of atmosphere models for cool T-Y brown dwarfs and giant exoplanets. Non equilibrium chemistry (strong). Valid temperature range: 200-2000K. Only for solar metallicity. -
BT-Settl (GNS93)
The BT-Settl Model grid of theoretical spectra; With a cloud model, valid across the entire parameter range. Using GNS93 abundances. Wavelengths have been converted to air... -
Pacheco et al 2021
A Grid of Synthetic Spectra for Subdwarfs: NLTE line-blanketed atmosphere models -
Morley2015 Cloudy
Cloudy models of GJ 1214b “analogs” from Morley et al. 2015. Emission spectra.