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Until now, there were erros in the citation of Astrometry-net and Scamp
papers.
With this commit, we fix these problems. The Swarp bibtex has also been
modify to follow the stetic of the citation style we have right now in
the project.
We also added the `dependency-bib.tex' as a prerequisite of `paper.bbl'.
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SWarp resamples and co-adds together FITS images using any arbitrary
astrometric projection defined in the WCS standard. It is a very useful
program for astronomy and that is why we added it to the pipeline.
With this commit, we also cite the paper for Astrometry-net that until
now was missing.
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With this commit, we include Astrometry-net software and one remaining
dependency of it (Swig). In principle it should work as far as we tested
all of this software in GNU/Linux, but we need to test also in Mac OS.
As a result, this commit is just for setting all the rules and
dependencies, but more tests are necessaries to ensure it works
properly, specially in Mac OS systems.
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Until now, the software building and analysis steps of the pipeline were
intertwined. However, these steps (of how to build a software, and how to
use it) are logically completely independent.
Therefore with this commit, the pipeline now has a new architecture
(particularly in the `reproduce' directory) to emphasize this distinction:
The `reproduce' directory now has the two `software' and `analysis'
subdirectories and the respective parts of the previous architecture have
been broken up between these two based on their function. There is also no
more `src' directory. The `config' directory for software and analysis is
now mixed with the language-specific directories.
Also, some of the software versions were also updated after some checks
with their webpages.
This new architecture will allow much more focused work on each part of the
pipeline (to install the software and to run them for an analysis).
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