submitted version

paper/makefile

@@ -25,7 +25,7 @@ diff:
 	$(LATEX) diff_$(FILE_TEX)
 
 submit:
-	tar -xzvf submit.tgz paper.tex  CLARA-TOL-main.pdf P_cl.pdf emcee_results.pdf sigma_cl.pdf tolfit.pdf vinf_cl.pdf
+	tar -czvf submit.tgz paper.tex  CLARA-TOL-main.pdf P_cl.pdf emcee_results.pdf sigma_cl.pdf vinf_cl.pdf
 
 clean:
 		rm -f $(FILE_NAME).aux

paper/paper.tex

@@ -100,9 +100,8 @@
 
 \begin{abstract}
   Star-forming Compact Dwarf Galaxies (CDGs) resemble the expected
-  pristine conditions of the first galaxies in the Universe.    
-Before the observational detection of the first galaxies becomes
-reality, CDGs are the best systems to test our ideas on primordial
+  pristine conditions of the first galaxies in the Universe and
+  are the best systems to test models on primordial
 galaxy formation and evolution.    
 Here we report on one of such CDGs, \tol, which presents
 a broad symmetric \lya\ line emission that had evaded theoretical
@@ -117,7 +116,8 @@
 (either a  a clump velocity dispersion of \sigmaclump\ with outflows of
 \inftyclump\ or a bulk rotation of $348^{+75}_{-48}$ km s$^{-1}$)
 consistent with a dynamical mass of at 
-least a $10^{10}$ M$_{\odot}$, ten times larger than its estimated baryonic mass.   
+least a $10^{10}$ M$_{\odot}$, ten times larger than its estimated
+baryonic mass.     
 We argue that a possible explanation for this excess of
 dynamical mass is the presence of a supermassive black hole at the
 center of \tol. 
@@ -131,7 +131,7 @@
 \end{abstract}
 
 \begin{keywords}
-Methods: data analysis - numerical 
+galaxies: dwarf --- galaxies: individual:\tol\ --- radiative transfer --- Methods: numerical 
 \end{keywords}