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Morley2015 Haze (Tholin) (Transm.)
Hazed (Tholin flavour) models of GJ 1214b “analogs” from Morley et al. 2015. Transmission spectra. -
Morley2015 Haze (Tholin)
Hazed (Tholin flavour) models of GJ 1214b “analogs” from Morley et al. 2015. Emission spectra. -
Morley2015 Haze (Soot) (Transm.)
Hazed (Soot flavour) models of GJ 1214b “analogs” from Morley et al. 2015. Transmission spectra. -
Morley2015 Haze (Soot)
Hazed (Soot flavour) models of GJ 1214b “analogs” from Morley et al. 2015. Emission spectra. -
Morley2015 Cloudy
Cloudy models of GJ 1214b “analogs” from Morley et al. 2015. Emission spectra. -
Morley2015 Cloudy (Transm.)
Cloudy models of GJ 1214b “analogs” from Morley et al. 2015. Transmission spectra. -
Morley2015 Cloud free (Transm.)
Cloud free models of GJ 1214b “analogs” from Morley et al. 2015. Transmission spectra. -
Morley2015 Cloud free
Cloud free models of GJ 1214b “analogs” from Morley et al. 2015. Emission spectra. -
Goyal (rainout)
Fully scalable forward model grid of exoplanet transmission spectra. Considering global condensation and removal of species from the atmospheric column (rainout). -
Goyal (local)
Fully scalable forward model grid of exoplanet transmission spectra. Considering local condensation only. -
Saumon 2012
Saumon et al. 2012 T dwarf models -
Pacheco et al 2021
A Grid of Synthetic Spectra for Subdwarfs: NLTE line-blanketed atmosphere models -
Kurucz ODFNEW /NOVER (2003) alpha:0.4
ATLAS9 Kurucz ODFNEW /NOVER models. Newly computed ODFs with better opacities and better abundances have been used. -
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. -
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... -
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. -
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. -
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. -
TMAP (Grid 1)
TMAP. Hydrogen+Helium NLTE Models