/
__init__.py
executable file
·55 lines (51 loc) · 1.82 KB
/
__init__.py
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
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
#! /usr/bin/env python
"""
-------------------
AegeanTools module.
-------------------
This module was written primarily for the Aegean source finder, and the tools BANE and MIMAS.
The wcs_helpers and angle_tools modules contain many useful classes and methods that would be useful more
generally.
"""
__author__ = 'Paul Hancock'
__version__ = '2.2.5'
__date__ = '2021-11-15'
__citation__ = """
% If your work makes use of AegeanTools please cite the following papers as appropriate:
% Advanced features of Aegean, plus description of BANE, MIMAS, and AeRes
@ARTICLE{Hancock_Aegean2_2018,
author = {{Hancock}, P.~J. and {Trott}, C.~M. and {Hurley-Walker}, N.},
title = "{Source Finding in the Era of the SKA (Precursors): Aegean 2.0}",
journal = {\pasa},
archivePrefix = "arXiv",
eprint = {1801.05548},
primaryClass = "astro-ph.IM",
keywords = {radio continuum: general, catalogs, methods: statistical},
year = 2018,
month = mar,
volume = 35,
eid = {e011},
pages = {e011},
doi = {10.1017/pasa.2018.3},
adsurl = {http://adsabs.harvard.edu/abs/2018PASA...35...11H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
% Basic description of Aegean
@ARTICLE{Hancock_Aegean_2012,
author = {{Hancock}, P.~J. and {Murphy}, T. and {Gaensler}, B.~M. and
{Hopkins}, A. and {Curran}, J.~R.},
title = "{Compact continuum source finding for next generation radio surveys}",
journal = {\mnras},
archivePrefix = "arXiv",
eprint = {1202.4500},
primaryClass = "astro-ph.IM",
keywords = {techniques: image processing, catalogues, surveys},
year = 2012,
month = may,
volume = 422,
pages = {1812-1824},
doi = {10.1111/j.1365-2966.2012.20768.x},
adsurl = {http://adsabs.harvard.edu/abs/2012MNRAS.422.1812H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
"""