Fixing relevant changes

tardis-sn · May 22, 2021 · c956467 · c956467
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diff --git a/docs/physics/montecarlo/propagation.rst b/docs/physics/montecarlo/propagation.rst
@@ -41,7 +41,7 @@ random number generator which provides uniformly distributed numbers :math:`z`
 on the interval :math:`[0,1]`. The frequency assignment is more involved than
 selecting an initial propagation direction, since the Planck function has to be
 sampled. TARDIS uses the technique described in :cite:`Carter1975` and
-summarized in :cite:`Bjorkmann1999` for this purpose.
+summarized in :cite:`Bjorkman2001` for this purpose.
 
 .. _expansion:
 

diff --git a/docs/tardis.bib b/docs/tardis.bib
@@ -147,6 +147,7 @@ @Article{Magee2016
   Eid                      = {A89},
   Eprint                   = {1603.04728},
 }
+
 @Article{Mazzali1993,
   Title                    = {{The application of Monte Carlo methods to the synthesis of early-time supernovae spectra}},
   Author                   = {{Mazzali}, P.~A. and {Lucy}, L.~B.},
@@ -157,6 +158,7 @@ @Article{Mazzali1993
   Volume                   = {279},
   Adsurl                   = {http://adsabs.harvard.edu/abs/1993A%26A...279..447M},
 }
+
 @PhdThesis{Noebauer2014,
   Title                    = {A Monte Carlo Approach to Radiation Hydrodynamics in Stellar Outflows},
   Author                   = {{Noebauer}, U.~M.},
@@ -166,6 +168,7 @@ @PhdThesis{Noebauer2014
   Type                     = {Dissertation},
   Url                      = {http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:91-diss-20140731-1219398-0-8}
 }
+
 @Article{Sim2010,
   Title                    = {{Multidimensional modelling of X-ray spectra for AGN accretion disc outflows - III. Application to a hydrodynamical simulation}},
   Author                   = {{Sim}, S.~A. and {Proga}, D. and {Miller}, L. and {Long}, K.~S. and {Turner}, T.~J.},
@@ -179,6 +182,7 @@ @Article{Sim2010
   Doi                      = {10.1111/j.1365-2966.2010.17215.x},
   Eprint                   = {1006.3449},
 }
+
 @Article{Magee2017,
   author        = {{Magee}, M. R. and {Kotak}, R. and {Sim}, S. A. and {Wright}, D. and {Smartt}, S. J. and {Berger}, E. and {Chornock}, R. and {Foley}, R. J. and {Howell}, D. A. and {Kaiser}, N. and {Magnier}, E. A. and {Wainscoat}, R. and {Waters}, C.},
   title         = {Growing evidence that SNe Iax are not a one-parameter family. The case of PS1-12bwh},
@@ -196,6 +200,7 @@ @Article{Magee2017
   primaryclass  = {astro-ph.HE},
   timestamp     = {2017.07.27},
 }
+
 @Article{Inserra2016,
   author        = {{Inserra}, C. and {Bulla}, M. and {Sim}, S. A. and {Smartt}, S. J.},
   title         = {Spectropolarimetry of Superluminous Supernovae: Insight into Their Geometry},
@@ -213,6 +218,7 @@ @Article{Inserra2016
   primaryclass  = {astro-ph.HE},
   timestamp     = {2017.07.27},
 }
+
 @Article{Boyle2017,
   author        = {{Boyle}, A. and {Sim}, S. A. and {Hachinger}, S. and {Kerzendorf}, W.},
   title         = {Helium in double-detonation models of type Ia supernovae},
@@ -251,6 +257,7 @@ @Article{Heringer2017
   doi           = {10.3847/1538-4357/aa8309},
   eid           = {15},
 }
+
 @Article{Barna2017,
   author        = {{Barna}, B. and {Szalai}, T. and {Kromer}, M. and {Kerzendorf}, W. E. and {Vink{\'o}}, J. and {Silverman}, J. M. and {Marion}, G. H. and {Wheeler}, J. C.},
   title         = {Abundance tomography of Type Iax SN 2011ay with tardis},