52 datasets found

Keywords: star

Filter Results
  • 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
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