This repository contains the implementation of the calibration algorithm used in the Planck/LFI 2015 data release. It is a Python3/Fortran program developed using literate programming techniques, and it uses MPI to distribute the workload among several processing units.
The full source code of the program can be found in the PDF document dacapo_calibration.pdf.
After you have downloaded the repository, just type make. You can
configure the programs make calls by setting variables in a new
file named configuration.mk. The following variables are
accepted:
NOWEAVENOTANGLECPIFTEX2PDFBIBTEXPYTHONF2PYAUTOPEP8DOCKERMPIRUNINKSCAPEMV
In the directory examples you will find a couple of parameter files
for index.py and calibrate.py. Refer to the PDF documentation for
a full reference of each parameter.
To run a number of unit tests, run the following command:
make check
To run a number of integration test, use the following command instead:
make fullcheck
The code is released under a permissive MIT license. See the file LICENSE.
If you use this code in your publications, please cite it using the following BibTeX entry:
@MISC{2016ascl.soft12007T,
author = {{Tomasi}, M.},
title = "{dacapo\_calibration: Photometric calibration code}",
keywords = {Software },
howpublished = {Astrophysics Source Code Library},
year = 2016,
month = dec,
archivePrefix = "ascl",
eprint = {1612.007},
adsurl = {http://adsabs.harvard.edu/abs/2016ascl.soft12007T},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}