https://github.com/RadioAstronomySoftwareGroup/pyuvdata
Revision 408c4d30059e4461d16bf9ee7b157cf2043cdaab authored by Bryna Hazelton on 28 September 2020, 03:35:35 UTC, committed by Bryna Hazelton on 11 December 2020, 19:21:28 UTC
1 parent 5d80c5b
Tip revision: 408c4d30059e4461d16bf9ee7b157cf2043cdaab authored by Bryna Hazelton on 28 September 2020, 03:35:35 UTC
use np.longdouble rather than "f16" to fix numpy issues on Windows
use np.longdouble rather than "f16" to fix numpy issues on Windows
Tip revision: 408c4d3
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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