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authorMohammad Akhlaghi <mohammad@akhlaghi.org>2018-02-27 14:48:02 +0100
committerMohammad Akhlaghi <mohammad@akhlaghi.org>2018-02-27 15:07:23 +0100
commit30733df5d30e150a26d53173d14bf941f179f6f5 (patch)
tree515694e80bded278388fbc3ff65acb60c0599cf7 /tex/references.tex
parent4360fbd36203022fde68b12f90548ca3a39085ce (diff)
Default PDF now uses PGFPlots and BibLaTeX
Making plots and including references are integral parts of a scientific paper. Therefore to demonstrate how cleanly they can be used within the pipeline, they are now used to produce the final PDF. To use PGFPlots a random dataset is made (using AWK's random function) and is plotted using PGFPlots. The minimum and maximum values of the dataset are also included in the text to further show how such calculations can go into the macros and text. For the references, the NoiseChisel paper was added as a reference to cite when using this pipeline along with the MUSE UDF paper I, which uses this pipeline for two sections. Following this discussion, citation is also discussed in `README.md` and the NoiseChisel paper is also added as a published work with a reproduction pipeline.
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+@ARTICLE{bacon17,
+ author = {{Bacon}, R. and {Conseil}, S. and {Mary}, D. and {Brinchmann}, J. and
+ {Shepherd}, M. and {Akhlaghi}, M. and {Weilbacher}, P.~M. and
+ {Piqueras}, L. and {Wisotzki}, L. and {Lagattuta}, D. and {Epinat}, B. and
+ {Guerou}, A. and {Inami}, H. and {Cantalupo}, S. and {Courbot}, J.~B. and
+ {Contini}, T. and {Richard}, J. and {Maseda}, M. and {Bouwens}, R. and
+ {Bouch{\'e}}, N. and {Kollatschny}, W. and {Schaye}, J. and
+ {Marino}, R.~A. and {Pello}, R. and {Herenz}, C. and {Guiderdoni}, B. and
+ {Carollo}, M.},
+ title = "{The MUSE Hubble Ultra Deep Field Survey. I. Survey description, data reduction, and source detection}",
+ journal = {A\&A},
+archivePrefix = "arXiv",
+ eprint = {1710.03002},
+ keywords = {galaxies: distances and redshifts, galaxies: high-redshift, cosmology: observations, methods: data analysis, techniques: imaging spectroscopy, galaxies: formation},
+ year = 2017,
+ month = nov,
+ volume = 608,
+ eid = {A1},
+ pages = {A1},
+ doi = {10.1051/0004-6361/201730833},
+ adsurl = {http://adsabs.harvard.edu/abs/2017A\%26A...608A...1B},
+ adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+
+
+
+
+@ARTICLE{ai15,
+ author = {{Akhlaghi}, M. and {Ichikawa}, T.},
+ title = "{Noise-based Detection and Segmentation of Nebulous Objects}",
+ journal = {ApJS},
+archivePrefix = "arXiv",
+ eprint = {1505.01664},
+ primaryClass = "astro-ph.IM",
+ keywords = {galaxies: irregular, galaxies: photometry, galaxies: structure, methods: data analysis, techniques: image processing, techniques: photometric},
+ year = 2015,
+ month = sep,
+ volume = 220,
+ eid = {1},
+ pages = {1},
+ doi = {10.1088/0067-0049/220/1/1},
+ adsurl = {http://adsabs.harvard.edu/abs/2015ApJS..220....1A},
+ adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}