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tardis-sn · Jan 27, 2014 · 59ca13f · 59ca13f
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Showing 1 changed file with 2 additions and 2 deletions.
diff --git a/docs/uses.rst b/docs/uses.rst
@@ -4,10 +4,10 @@ What can I do with TARDIS?
 
 TARDIS is designed to carry out calculations of synthetic supernova spectra (see Kerzendorf & Sim 2014). A TARDIS calculation requires
 
-1) a model for the supernova eject (density and composition distribution) to be specified;
+1) a model for the supernova ejecta (density and composition distribution) to be specified;
 2) parameters determining the physical and numerical properties of the code are give.
 
-These inputs are specified via the input file (yaml file). As a starting point, examine the input file in the example download (above). The example file sets up a very simple model in which the density distribution is based on the well-known W7 model () and in which uniform abundances are specified. To get you started, here is a short list of settings that can be experimented with to get a feel for using TARDIS. Please contact us if you have questions or woudl like information on more advanced possibilities!
+These inputs are specified via the input file (yaml file). As a starting point, examine the input file in the example download (above). The example file sets up a very simple model in which the density distribution is based on the well-known W7 model (Nomoto et al. 1984; fit following Branch et al. 1985) and in which uniform abundances are specified. To get you started, here is a short list of settings that can be experimented with to get a feel for using TARDIS. Please contact us if you have questions or woudl like information on more advanced possibilities!
 
 Change the abundances
 ===============