StellarAtmospheres.markdown

@@ -287,7 +287,7 @@ In general, you will not need all the files listed on the Tlusty website (unless
 
 ### WMbasic O and B stars
 
-[wmbasic.ascii.gz](https://data.nublado.org/stars/wmbasic.ascii.gz).
+[wmbasic.ascii.gz](https://data.nublado.org/stars/wmbasic.ascii.gz)
 
 
 The WMbasic code was maintained by [Adi Pauldrach](http://www.usm.uni-muenchen.de/people/adi/Programs/Contact.html) who still has a home page [here](http://www.usm.uni-muenchen.de/people/adi/adi.html). He computed a small grid of non-LTE, line-blanketed, and wind-blanketed hot stars with metallicities log Z = 0.0 and -0.3. The original grid of models is [here](http://www.usm.uni-muenchen.de/people/adi/Models/Model.html) and is described in
@@ -297,7 +297,11 @@ This is a three-dimensional grid so you must specify temperature, log g, and log
 
 ### CoStar O and B stars
 
-These grids of non-LTE, line blanketed model atmospheres including stellar winds have been developed by Daniel Schaerer and are described in [Schaerer, D., & de Koter, A. 1997, A&A, 322, 598](http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1997A%26A...322..598S&db_key=AST&data_type=HTML&format=&high=45b49b8de123609).  There are two abundance sets, halo and solar.  They are available from the [STScI web site](http://www.stsci.edu/science/starburst99/docs/SdK96/). You need the files Sc1_costar_z020_lb.fluxes (solar abundances) and Sc1_costar_z004_lb.fluxes (halo abundances).
+[Sc1_costar_solar.ascii.gz](https://data.nublado.org/stars/costar/Sc1_costar_solar.ascii.gz)
+
+[Sc1_costar_halo.ascii.gz](https://data.nublado.org/stars/costar/Sc1_costar_halo.ascii.gz)
+
+These grids of non-LTE, line blanketed model atmospheres including stellar winds have been developed by Daniel Schaerer and are described in [Schaerer, D., & de Koter, A. 1997, A&A, 322, 598](http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1997A%26A...322..598S&db_key=AST&data_type=HTML&format=&high=45b49b8de123609).  There are two abundance sets, halo and solar.  They are no longer available from the STScI web site, so we have also made the original files computed by Shaerer & De Koter available here: [Sc1_costar_z020_lb.fluxes.gz](https://data.nublado.org/stars/costar/Sc1_costar_z020_lb.fluxes.gz) (solar abundances) and [Sc1_costar_z004_lb.fluxes.gz](https://data.nublado.org/stars/costar/Sc1_costar_z004_lb.fluxes.gz) (halo abundances). These last two files are *not* needed by Cloudy and only here in case you need to look up the original files for some other reason.
 
 
 ### Rauch PN Nuclei