https://github.com/RadioAstronomySoftwareGroup/pyuvdata
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Tip revision: f7fe4c1c1394f84095b7984352b175a3132c0369 authored by Garrett 'Karto' Keating on 13 January 2022, 03:40:32 UTC
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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}
}
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