File: CITATION

package info (click to toggle)
healpy 1.19.0-1
  • links: PTS, VCS
  • area: main
  • in suites: forky, sid
  • size: 17,464 kB
  • sloc: ansic: 113,657; cpp: 15,827; python: 10,793; sh: 8,443; yacc: 5,410; fortran: 2,613; lex: 553; makefile: 380
file content (37 lines) | stat: -rw-r--r-- 1,648 bytes parent folder | download | duplicates (4)
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
Use of the HEALPix/healpy software package should be explicitly acknowledged in all publications in the following form:

* an acknowledgment statement – "Some of the results in this paper have been derived using the healpy and HEALPix package"
* at the first use of the HEALPix acronym, a footnote placed in the main body of the paper referring to the HEALPix website – currently http://healpix.sourceforge.net

BibTeX record:

@article{Zonca2019,
  doi = {10.21105/joss.01298},
  url = {https://doi.org/10.21105/joss.01298},
  year = {2019},
  month = mar,
  publisher = {The Open Journal},
  volume = {4},
  number = {35},
  pages = {1298},
  author = {Andrea Zonca and Leo Singer and Daniel Lenz and Martin Reinecke and Cyrille Rosset and Eric Hivon and Krzysztof Gorski},
  title = {healpy: equal area pixelization and spherical harmonics transforms for data on the sphere in Python},
  journal = {Journal of Open Source Software}
}

@ARTICLE{2005ApJ...622..759G,
   author = {{G{\'o}rski}, K.~M. and {Hivon}, E. and {Banday}, A.~J. and 
	{Wandelt}, B.~D. and {Hansen}, F.~K. and {Reinecke}, M. and 
	{Bartelmann}, M.},
    title = "{HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere}",
  journal = {\apj},
   eprint = {arXiv:astro-ph/0409513},
 keywords = {Cosmology: Cosmic Microwave Background, Cosmology: Observations, Methods: Statistical},
     year = 2005,
    month = apr,
   volume = 622,
    pages = {759-771},
      doi = {10.1086/427976},
   adsurl = {http://adsabs.harvard.edu/abs/2005ApJ...622..759G},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}