paper.bib

@TECHREPORT{aipy,
  author = {Aaron Parsons},
  title = {Astronomical Interferometry in PYthon},
  year = {2007},
  file = {http://astro.berkeley.edu/~aparsons/aipy.pdf},
  url = {https://casper.berkeley.edu/astrobaki/index.php/AIPY}}
@TECHREPORT{uvfits,
  author = {Eric W. Greisen},
  title = {AIPS FITS File Format},
  number = {AIPS Memo 117},
  institution = {National Radio Astronomy Observatory},
  abstract = {AIPS has been writing images and uv data in FITS-format files
              for a very long time. While these files have been used widely in
              the community, there is a perception that a detailed document is
              still required. This memo is an attempt to meet that perception.
              AIPS FITS files for uv are conventions layered upon the standard
              FITS format to assist in the interchange of data recorded by
              interferometric telescopes, particularly by radio telescopes such
              as the EVLA and VLBA.},
  keywords = {radio astronomy, uvfits},
  month = {February},
  year = {2016},
  pages = {107},
  file = {ftp://ftp.aoc.nrao.edu/pub/software/aips/TEXT/PUBL/AIPSMEM117.PS},
  url = {http://www.aips.nrao.edu/aipsmemo.html},
}

@INPROCEEDINGS{miriad,
  author = {{Sault}, R.~J. and {Teuben}, P.~J. and {Wright}, M.~C.~H.},
  title = "{A Retrospective View of MIRIAD}",
  booktitle = {Astronomical Data Analysis Software and Systems IV},
  abstract = {Miriad is a radio interferometry data-reduction package, designed
              for taking raw data through to the image analysis stage. The
              Miriad project, begun in 1988, is now middle-aged. With the wisdom
              of hindsight, we review design decisions and some of Miriad's
              characteristics.}
  year = 1995,
  series = {Astronomical Society of the Pacific Conference Series},
  volume = 77,
  eprint = {astro-ph/0612759},
  editor = {{Shaw}, R.~A. and {Payne}, H.~E. and {Hayes}, J.~J.~E.},
  pages = {433},
  adsurl = {http://adsabs.harvard.edu/abs/1995ASPC...77..433S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
  url = {http://www.atnf.csiro.au/computing/software/miriad/}
}

@ARTICLE{fhd,
  author = {{Sullivan}, I.~S. and {Morales}, M.~F. and {Hazelton}, B.~J. and
	          {Arcus}, W. and {Barnes}, D. and {Bernardi}, G. and {Briggs}, F.~H. and
	          {Bowman}, J.~D. and {Bunton}, J.~D. and {Cappallo}, R.~J. and
	          {Corey}, B.~E. and {Deshpande}, A. and {deSouza}, L. and {Emrich}, D. and
	          {Gaensler}, B.~M. and {Goeke}, R. and {Greenhill}, L.~J. and
	          {Herne}, D. and {Hewitt}, J.~N. and {Johnston-Hollitt}, M. and
	          {Kaplan}, D.~L. and {Kasper}, J.~C. and {Kincaid}, B.~B. and
	          {Koenig}, R. and {Kratzenberg}, E. and {Lonsdale}, C.~J. and
	          {Lynch}, M.~J. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and
	          {Morgan}, E. and {Oberoi}, D. and {Ord}, S.~M. and {Pathikulangara}, J. and
	          {Prabu}, T. and {Remillard}, R.~A. and {Rogers}, A.~E.~E. and
	          {Roshi}, A. and {Salah}, J.~E. and {Sault}, R.~J. and {Udaya Shankar}, N. and
	          {Srivani}, K.~S. and {Stevens}, J. and {Subrahmanyan}, R. and
	          {Tingay}, S.~J. and {Wayth}, R.~B. and {Waterson}, M. and {Webster}, R.~L. and
	          {Whitney}, A.~R. and {Williams}, A. and {Williams}, C.~L. and
	          {Wyithe}, J.~S.~B.},
  title = "{Fast Holographic Deconvolution: A New Technique for Precision Radio Interferometry}",
  journal = {\apj},
  archivePrefix = "arXiv",
  eprint = {1209.1653},
  primaryClass = "astro-ph.IM",
  keywords = {dark ages, reionization, first stars, techniques: image processing, techniques: interferometric},
  year = 2012,
  month = nov,
  volume = 759,
  eid = {17},
  pages = {17},
  doi = {10.1088/0004-637X/759/1/17},
  adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...759...17S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
  url = {https://github.com/EoRImaging/FHD}
}