From c956467401ebddd80c214302f29695f235c8acba Mon Sep 17 00:00:00 2001 From: DhruvSondhi Date: Fri, 21 May 2021 22:16:29 +0530 Subject: [PATCH] Fixing relevant changes --- docs/physics/montecarlo/propagation.rst | 2 +- docs/tardis.bib | 7 +++++++ 2 files changed, 8 insertions(+), 1 deletion(-) diff --git a/docs/physics/montecarlo/propagation.rst b/docs/physics/montecarlo/propagation.rst index de4d705c74d..907ca40f3c1 100644 --- 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 index 2b1ce18a2ed..14c30348b17 100644 --- 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},