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${LATEX} ch_software.tex  ${BIBTEX} ch_software  ${LATEX} ch_software.tex  h2co_lowdens:   @rm -f h2co_lowdens*.aux h2co_lowdens*.bbl h2co_lowdens*.blg h2co_lowdens*.dvi h2co_lowdens*.log h2co_lowdens*.lot h2co_lowdens*.lof  ${LATEX} h2co_lowdens.tex  ${BIBTEX} h2co_lowdens  ${LATEX} h2co_lowdens.tex  ${BIBTEX} h2co_lowdens  ${LATEX} h2co_lowdens.tex  diff --git a/ch_boundhii.tex b/ch_boundhii.tex  index a6f9604..d75c6dd 100644  --- a/ch_boundhii.tex  +++ b/ch_boundhii.tex 
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\input{tables_chboundhii/boundhiitable}  \section{Follow-up work}  In order to get a complete census of massive proto-clusters in the Galactic  plane, it is necessary to examine the southern plane as well.  \citet{Urquhart2013a} began this examination using ATLASGAL data and identified  6 new candidates in the southern sky. In principle, this indicates either some  incompleteness in the BGPS or a genuinely higher cluster formation rate in the  southern sky (which, with such small numbers, is easily consistent with uniform  sampling from a disk distribution).  However, we note that three of the candidates in \citet{Urquhart2013a} are  assigned the wrong kinematic distance - they are placed at the far distance  when strong evidence puts them at the near.  \subimport{/Users/adam/work/BoundHII/distance_massiveclumps/}{standalone}  \input{solobib}  \end{document}  diff --git a/ch_software.tex b/ch_software.tex  index 01229ef..9f0881c 100644  --- a/ch_software.tex  +++ b/ch_software.tex 
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\citet{Clauset2007}. I wrote a translation of his code into python (and  fortran and c). It was used in most of the publications in this thesis.  \section{Other codes}  I am the maintainer for a few other significant code projects, some of which  are specific to the University of Colorado and the Apache Point Observatory.  \subsection{Astropy: Astroquery}  \url{http://astroquery.readthedocs.org/en/latest/}\\  The \texttt{astroquery} project is an affiliate of the much larger  \texttt{astropy} project. It implements python-based query tools  for various astronomical data servers, e.g. IPAC, SIMBAD, Vizier, etc.  \subsection{CASARADIO}  \url{http://code.google.com/p/casaradio/}\\  Tools by and for radio astronomers at the Center for Astrophysics and Space  Astronomy (CASA).  \subsection{APO software}  \url{https://code.google.com/p/aposoftware/}\\  The APO software page includes reduction tools for DIS, TripleSpec, and NICFPS.  It also includes some observing preparation tools and observing scripts for  TUI.  \input{solobib}  \end{document}  diff --git a/ch_v2.tex b/ch_v2.tex  index 693efbe..a465086 100644  --- a/ch_v2.tex  +++ b/ch_v2.tex 
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(Section \ref{sec:bgpspipeline}). That software is described in \citet{Aguirre2011}  and this chapter.  \section{Version \subsection{Version  1} The Bolocam Galactic Plane Survey (BGPS) Version 1 (\vone) was released in 2009 and published in \citet{Aguirre2011} and \citet{Rosolowsky2010}. \citet{Aguirre2011} summarizes a great deal of the work in this thesis, on the BGPS pipeline,  in particular the reduction strategy implemented for the BGPS. we implemented.  However, since that paper was written in cooperation with James Aguirre, the text is not reproduced here and instead references to the paper are included within the description of \vtwo below. \Figure{gc_fullres_6_small.jpg}  {The `cover figure' for the BGPS: The Galactic Center seen at 1.1 mm (orange),  20 cm (purple), and 8 \um.  }{fig:gc}{0.05}{0}  %\standalonefalse  %\subimport{/Users/adam/Dropbox/BGPS_paper_v2/}{v2.tex}