remove boldface

paper/paper.tex

@@ -99,11 +99,11 @@
 Here we report on one of such CDGs, \tol, which presents
 a broad, single peaked, highly symmetric \lya emission line that had
 evaded theoretical interpretation so far.  
-{\bf In this paper we reproduce for the first time these line features with two
+In this paper we reproduce for the first time these line features with two
 different physically motivated kinematic models: 
 an interstellar medium composed by outflowing clumps with 
 random motions and an homogeneous gaseous sphere undergoing solid body
-rotation.}
+rotation.
 The multiphase model requires a clump velocity dispersion of
 \sigmaclump\ with outflows of \inftyclump\, while the
 bulk rotation velocity is constrained to be $348^{+75}_{-48}$ \kms.
@@ -604,14 +604,14 @@ \subsection{Multiphase ISM}
 and its corresponding parameter value. 
 Under these conditions we find $\sigma_{\rm cl}=$\sigmaclump,
 $v_{\infty {\rm, cl}}=$\inftyclump\ and $P_{\rm cl}=$\probaclump, 
-  with the minimum $\chi^2/d.o.f.=11.7$. {\bf This relatively high value
+  with the minimum $\chi^2/d.o.f.=11.7$. This relatively high value
     for the reduced $\chi^2$ could be interpreted as low statistical
     significance. 
 However, we stress once more that the is the first time that the main
 features of \tol\ can be reproduced, making this model an useful tool
 to guide the interpretation of complex observational data. 
 These results certainly open up the path to future searches to
-construct new models.} 
+construct new models.
 
 The results from this model can be qualitatively explained as follows.
 Due to the large fraction of \lya photons being emitted within the