#! /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__ = '2.3.0'
__date__ = '2022-11-29'
__citation__ = r"""
% 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}
}
"""
