Getting-started.md

-In this section we will describe how to quickly run an *Exo-REM* simulation. We will use the `inputs/example.nml` coming with all [distributed versions](https://gitlab.obspm.fr/dblain/exorem/-/tree/master/dist) of *Exo-REM* as a starting point. Before, please take the time to read the README.
+In this section we will describe how to quickly run an *Exo-REM* simulation. We will use the `inputs/example.nml` coming with all [distributed versions](https://gitlab.obspm.fr/dblain/exorem/-/tree/master/dist) of *Exo-REM* as a starting point. Before, please take the time to read the README and/or the [].
 
 Want some help with convergence issues ? Check the related page on this wiki.
 
@@ -15,11 +15,11 @@ Summary:
     - [Better figures](#better-figures)
 
 # Prerequisites
-If you downloaded the archive in the [_dist_](https://gitlab.obspm.fr/dblain/exorem/-/tree/master/dist) directory, you should have everything you need, except a stellar spectrum (see point 4 below). Otherwise, check the following:
+If you downloaded the archive in the [_dist_](https://gitlab.obspm.fr/dblain/exorem/-/tree/master/dist) directory, you should have everything you need, except a stellar spectrum (see point 4 below), and more importantly the k-coefficients tables (see point 3 below). Otherwise, check the following:
 
 1. Verify if the collision-induced absorption (CIA) files are inside the _data/cia_ directory. If you want to use other CIA files, respect the same format and use "CIAname.cia.txt" as file name (e.g. "H2-He.cia.txt").
 2. If you intend to use clouds, verify if the cloud optical constants (OCST) files are inside the _data/cloud_optical_constants_ directory. If you want to use other OCST files, respect the same format and use "cloudName.ocst.txt" as file name (e.g. "H2O.ocst.txt").
-3. Put k-coefficients of desired absorbers inside the _data/k_coefficients_tables_ directory. You can use directly *CKC* outputs converted into HDF5 using *txt2h5*, or e.g. *[petitRADTRANS](https://petitradtrans.readthedocs.io/en/latest/content/available_opacities.html)* k-tables. If your absorber name is "absorberName", the lines file needs to be named "absorberName.ktable.exorem.h5" (e.g. H2O.ktable.exorem.h5). You can download compressed *Exo-REM* k-tables [here](https://gitlab.obspm.fr/dblain/exorem/-/tree/master/data/k_coefficients). 
+3. Put k-coefficients of desired absorbers inside the _data/k_coefficients_tables_ directory. You can use directly *CKC* outputs converted into HDF5 using *txt2h5*, or e.g. *[petitRADTRANS](https://petitradtrans.readthedocs.io/en/latest/content/available_opacities.html)* k-tables. If your absorber name is "absorberName", the lines file needs to be named "absorberName.ktable.exorem.h5" (e.g. H2O.ktable.exorem.h5). You can download compressed *Exo-REM* k-tables [here](https://lesia.obspm.fr/exorem/). 
 4. If you intend to use stellar spectra, you can download them e.g. [here](http://svo2.cab.inta-csic.es/theory/newov2/index.php?models=bt-settl). You **must** modify them in order to respect the *Exo-REM* data format (see section data format).
 5. Verify if all the condensates and gases thermochemical tables are in the _data/thermochemical_tables_ directory. If you want to add more species to the chemical model, respect the same format and use "speciesName.tct.dat" as file name (e.g. "H2O.tct.dat").
 6. Put a temperature profile as a priori inside the _inputs/atmospheres/temperature_profiles_ directory. The *Exo-REM* data format must be respected. You should have received an example of such a file with your *Exo-REM* distribution.