Data used in the figures of the article "A cool runaway greenhouse without surface magma ocean"

These data have been generated with the codes Exo k and PCM.

Exo k is an open-source software. A complete documentation on how to install and use it can be found at http://perso.astrophy.u-bordeaux.fr/∼jleconte/ exo k-doc/index.html.
The generic Global Climate Model PCM (formerly known as LMDZ.generic) used in this work is the version 2528 that can be downloaded with documentation from the SVN repository at https://svn.lmd.jussieu.fr/Planeto/trunk/ LMDZ.GENERIC/. More information and documentation are available at http://www-planets.lmd.jussieu.fr.

The archive is organized as follows:
├─ Fig1 (comparison of atmospheric profiles with a same Outgoing Thermal Radiation)
│  ├─ OTR274.txt (profiles with a 274 W/m2 bolometric emission)
│  ├─ OTR10000txt (profiles with a 1000 W/m2 bolometric emission)
│
├─ Fig2 (Outgoing Thermal Radiation as a function of surface temperature)
│  ├─ Geoflux=0 (internal heat flux = 0 W/m2)
│  │  ├─ T1_0_ISR_Tsurf_OTR_ALB.dat
│  │  ├─ Proxima_0_ISR_Tsurf_OTR_ALB.dat
│  │  ├─ M3_0_ISR_Tsurf_OTR_ALB.dat
│  │  ├─ Sun_0_ISR_Tsurf_OTR_ALB.dat
│  │  ├─ F1_0_ISR_Tsurf_OTR_ALB.dat
│  ├─ Geoflux=0.09Wm-2 (internal heat flux = 0.09 W/m2)
│     ├─ T1_0.09_ISR_Tsurf_OTR_ALB.dat
│     ├─ Sun_0.09_ISR_Tsurf_OTR_ALB.dat
│
├─ Fig3 (Trappist-1b profiles and spectra)
│  ├─ Profiles
│  │  ├─ Adiabatic
│  │  │   ├─ Trappist1b_adiabatic_profile_1EO.txt (1x Earth Ocean)
│  │  │   ├─ Trappist1b_adiabatic_profile_3EO.txt (3x Earth Ocean)
│  │  │
│  │  ├─ Converged
│  │  │   ├─ Trappist1b_profile_1EO_geoflux=0W.txt (1x Earth Ocean, internal heat flux = 0 W/m2)
│  │  │   ├─ Trappist1b_profile_1EO_geoflux=5W.txt (1x Earth Ocean, internal heat flux = 5 W/m2)
│  │  │   ├─ Trappist1b_profile_3EO_geoflux=0W.txt (3x Earth Ocean, internal heat flux = 0 W/m2)
│  │  │   ├─ Trappist1b_profile_3EO_geoflux=5W.txt (3x Earth Ocean, internal heat flux = 5 W/m2)
│  │  │
│  ├─ Spectra
│  │  ├─ Adiabatic
│  │  │   ├─ Trappist1b_adiabatic_spectra_1EO.txt (1x Earth Ocean)
│  │  │   ├─ Trappist1b_adiabatic_spectra_3EO.txt (3x Earth Ocean)
│  │  │
│  │  ├─ Converged
│  │  │   ├─ Trappist1b_spectra_1EO_geoflux=0W.txt (1x Earth Ocean, internal heat flux = 0 W/m2)
│  │  │   ├─ Trappist1b_spectra_1EO_geoflux=5W.txt (1x Earth Ocean, internal heat flux = 5 W/m2)
│  │  │   ├─ Trappist1b_spectra_3EO_geoflux=0W.txt (3x Earth Ocean, internal heat flux = 0 W/m2)
│  │  │   ├─ Trappist1b_spectra_3EO_geoflux=5W.txt (3x Earth Ocean, internal heat flux = 5 W/m2)
│
├─ Fig4_(net stellar and emission fluxes for a converged and adiabatic profiles)
│  ├─profiles_Sun_adia_converged_netfluxes.txt
│
├─ Fig5 (Profiles for different instellations, for each star)
│  ├─ T1_profiles.txt
│  ├─ Proxima_profiles.txt
│  ├─ M3_profiles.txt
│  ├─ K5_profiles.txt
│  ├─ Sun_profiles.txt
│  ├─ F1_profiles.txt
│
├─ Fig6 (Comparison 1D vs 3D)
│  ├─ 1D
│  │  ├─ exok_1D_PTH_trappist1.txt
│  │  ├─ exok_1D_PTH_Proxima.txt
│  │  ├─ exok_1D_PTH_M3.txt
│  ├─ 3D
│     ├─ PT_trappist1_3D.dat
│     ├─ PT_Proxima_3D.dat
│     ├─ PT_M3_3D.dat
│     ├─ HeatingRates_3D_trappist1.dat
│     ├─ HeatingRates_3D_trappist1.dat
│     ├─ HeatingRates_3D_trappist1.dat
│
├─ Fig7 (Profiles for 2 values of instellation and 3 values of cp)
│  ├─ profiles_cp_Sun.txt  
│
├─ Fig8 (Profiles for 3 values of instellation and continuums from 2 version of MT_sCKD)
│  ├─ profiles_2continuums_Sun.txt  
│
├─ Fig9 (Profiles as a function of surface pressure and internal heat fluxes)
│  ├─ EarlyVenus
│  │  ├─ profiles_fig9_EarlyVenus_0.1bar.txt
│  │  ├─ profiles_fig9_EarlyVenus_1bar.txt
│  │  ├─ profiles_fig9_EarlyVenus_10bar.txt
│  │  ├─ profiles_fig9_EarlyVenus_100bar.txt
│  │  ├─ profiles_fig9_EarlyVenus_270bar.txt
│  ├─ Trappist1
│     ├─ profiles_fig9_Trappist1_0.1bar.txt
│     ├─ profiles_fig9_Trappist1_1bar.txt
│     ├─ profiles_fig9_Trappist1_10bar.txt
│     ├─ profiles_fig9_Trappist1_100bar.txt
│     ├─ profiles_fig9_Trappist1_270bar.txt
│
├─ readme.txt