references.bib

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@article{wiener1928,
	Author = {Wiener, N},
	Date-Added = {2015-01-06 01:53:55 +0000},
	Date-Modified = {2015-01-06 01:55:27 +0000},
	Journal = {J. Mat. Phys.},
	Pages = {109--125},
	Title = {Coherency matrices and quantum theory},
	Volume = {7},
	Year = {1928}}

@article{wiener1930,
	Author = {Wiener, Norbert},
	Date-Added = {2015-01-06 01:45:41 +0000},
	Date-Modified = {2015-01-06 01:49:32 +0000},
	Journal = {Acta Mathematica},
	Month = dec,
	Number = {1},
	Pages = {117--258},
	Title = {{Generalized harmonic analysis}},
	Volume = {55},
	Year = {1930}}

@article{Barakat:1963,
	Author = {Barakat, Richard},
	Journal = {J. Opt. Soc. Am.},
	Number = {3},
	Pages = {317--322},
	Title = {{Theory of the Coherency Matrix for Light of Arbitrary Spectral Bandwidth}},
	Volume = {53},
	Year = {1963}}

@article{Whitney:1971,
	Author = {Whitney, Cynthia},
	Journal = {J. Opt. Soc. Am.},
	Number = {9},
	Pages = {1207},
	Title = {{Pauli-Algebraic Operators in Polarization Optics}},
	Volume = {61},
	Year = {1971}}

@article{cocke:1972,
	Author = {Cocke, W J and Holm, D A},
	Journal = {Nature Physical Science},
	Month = dec,
	Number = {103},
	Pages = {161--162},
	Title = {{Lorentz Transformation Properties of the Stokes Parameters}},
	Volume = {240},
	Year = {1972}}

@article{Santos:2012,
	Author = {Santos, Adler G and Sugon, Jr, Quirino M and McNamara, Daniel J},
	Journal = {Journal of the Optical Society of America A},
	Number = {1},
	Pages = {89--98},
	Title = {{Polarization ellipse and Stokes parameters in geometric algebra}},
	Volume = {29},
	Year = {2012}}

@article{Baylis:1993,
	Author = {Baylis, W E and Bonenfant, J and Derbyshire, J},
	Date-Modified = {2014-11-04 17:34:09 +0000},
	Journal = {Am. J. Phys.},
	Pages = {534},
	Title = {{Light polarization: A geometric-algebra approach}},
	Volume = {61},
	Year = {1993}}

@article{Bowman:2010,
	Annote = {10.1038/nature09601},
	Author = {Bowman, Judd and Rogers, Alan},
	Journal = {Nature},
	Month = dec,
	Number = {7325},
	Pages = {796--798},
	Title = {{A lower limit of [Dgr]z[thinsp]>[thinsp]0.06 for the duration of the reionization epoch}},
	Volume = {468},
	Year = {2010}}

@article{Baars:1977,
	Annote = {A{\&}amp;AA ID. AAA020.141.048},
	Author = {Baars, J W M and Genzel, R and Pauliny-Toth, I I K and Witzel, A},
	Date-Modified = {2014-11-04 17:57:09 +0000},
	Journal = {A\&A},
	Month = oct,
	Pages = {99},
	Title = {{The absolute spectrum of CAS A - an accurate flux density scale and a set of secondary calibrators}},
	Volume = {61},
	Year = {1977}}

@article{Kellermann:2009,
	Author = {Kellermann, K I},
	Journal = {A{\&}A},
	Month = jun,
	Number = {1},
	Pages = {143--144},
	Title = {{Setting the radio astronomy flux density scale}},
	Volume = {500},
	Year = {2009}}

@article{Karlsson:2013tj,
	Author = {Karlsson, Magnus},
	Eprint = {1303.1836v1},
	Eprintclass = {physics.optics},
	Eprinttype = {arxiv},
	Journal = {arXiv.org},
	Month = mar,
	Title = {{The connection between polarization calculus and four-dimensional rotations}},
	Year = {2013}}

@article{Britton:2000wr,
	Author = {Britton, M C},
	Journal = {The Astrophysical Journal},
	Title = {{Radio Astronomical Polarimetry and the Lorentz Group}},
	Year = {2000}}

@article{Han:1997jones,
	Author = {Han, D and Kim, Y S and Noz, Marilyn E},
	Date-Modified = {2014-11-04 17:46:10 +0000},
	Eprint = {physics/9703032v1},
	Eprintclass = {physics.optics},
	Eprinttype = {arxiv},
	Journal = {J. Opt. Soc. Am.},
	Month = mar,
	Pages = {2290--2298},
	Title = {{Jones-matrix Formalism as a Representation of the Lorentz Group}},
	Volume = {14},
	Year = {1997}}

@article{Han:1997stokes,
	Author = {Han, D and Kim, Y and Noz, Marilyn},
	Date-Modified = {2014-11-04 17:44:11 +0000},
	Journal = {Phys. Rev. E},
	Month = nov,
	Number = {5},
	Pages = {6065--6076},
	Title = {{Stokes parameters as a Minkowskian four-vector}},
	Volume = {56},
	Year = {1997}}

@article{Sundkvist:2006cl,
	Author = {Sundkvist, David},
	Journal = {Journal of Mathematical Physics},
	Number = {1},
	Pages = {012901},
	Title = {{Covariant irreducible parametrization of electromagnetic fields in arbitrary space-time}},
	Volume = {47},
	Year = {2006}}

@article{Carozzi:2006bj,
	Author = {Carozzi, T D and Bergman, J E S},
	Date-Modified = {2014-11-04 17:58:04 +0000},
	Journal = {J. Mat. Phys.},
	Month = mar,
	Pages = {2903},
	Title = {{Real irreducible sesquilinear-quadratic tensor concomitants of complex bivectors}},
	Volume = {47},
	Year = {2006}}

@article{Rogers:2012hd,
	Author = {Rogers, Alan E E and Bowman, Judd D},
	Date-Added = {2014-03-04 22:00:41 +0000},
	Date-Modified = {2014-11-04 17:53:21 +0000},
	Journal = {Radio Science},
	Month = jul,
	Number = {6},
	Pages = {RS0K06},
	Title = {{Absolute calibration of a wideband antenna and spectrometer for accurate sky noise temperature measurements}},
	Volume = {47},
	Year = {2012}}

@conference{leda2012,
	Author = {L. J. Greenhill and G. Bernardi},
	Booktitle = {NARIT Conf. Ser.},
	Date-Added = {2014-03-04 21:56:10 +0000},
	Date-Modified = {2014-11-04 17:39:23 +0000},
	Editor = {S. S. Komonjinda and Y. Y. Kovalev and D. Ruffolo},
	Title = {HI Epoch of Reionization Arrays},
	Volume = {1},
	Year = {2012}}

@book{ThompsonMoranSwenson2004,
	Author = {A. Richard Thompson and James M. Moran and George W. Swenson Jr.},
	Date-Added = {2012-12-17 11:16:30 +0000},
	Date-Modified = {2012-12-17 11:16:30 +0000},
	Edition = {Second},
	Keywords = {Interferometry synthesis imaging},
	Publisher = {WILEY-VCH Verlag},
	Title = {Interferometry and Synthesis in Radio Astronomy},
	Year = {2004}}

@article{VanCittertZernicke1938,
	Author = {F. Zernicke},
	Date-Added = {2012-12-17 11:16:09 +0000},
	Date-Modified = {2012-12-17 11:16:09 +0000},
	Journal = {Physica},
	Number = {758},
	Volume = {5},
	Year = {1938}}

@article{Pen:2008p9860,
	Abstract = {We propose to scan the 2dF survey field with Parkes multibeam in driftscan mode to make a map to cross correlate with galaxy redshifts. This allows a statistical detection of HI large scale structure out to z=0.15. In this cross correlation, the HI in ALL galaxies contributes, not only the bright ones, which significantly boosts the sensitivity. The proposed 40 hours on the fields result in a forecasted 20 sigma detection. The survey volume is 10 million cubic megaparsec, which contain 10^15 solar masses of hydrogen.},
	Affiliation = {AA(University of Toronto, Canada pen@cita.utoronto.ca), AB(University of Western Australia, Australia lister.staveley-smith@uwa.edu.au), AC(Academia Sinica Institute of Astronomy {\&} Astrophysics, Taiwan tchang@cita.utoronto.ca), AD(Carnegie Mellon University, USA jbp@cmu.edu), AE(Carnegie Mellon University, USA kbandura@andrew.cmu.edu)},
	Author = {Ue-Li Pen and Lister Staveley-Smith and Tzu-Ching Chang and Jeff Peterson and Kevin Bandura},
	Date-Added = {2012-09-18 15:05:46 +0000},
	Date-Modified = {2012-09-18 15:05:46 +0000},
	Journal = {ATNF proposal P641},
	Keywords = {Parkes, Extragalactic},
	Month = {Apr},
	Note = {Parkes},
	Pages = {1629},
	Pmid = {2008atnf.prop.1629P},
	Rating = {0},
	Title = {HI Surface brightness mapping},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p9860},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atnf.prop.1629P&link_type=ABSTRACT},
	Year = {2008},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atnf.prop.1629P&link_type=ABSTRACT}}

@article{Pen:2009p9865,
	Abstract = {We present the first statistically significant detection of cosmic structure using broadly distributed hydrogen radio emission. This is accomplished using a cross-correlation with optical galaxies. Statistical noise levels of 20μK are achieved, unprecedented in this frequency band. The signal is consistent with arising from the collective flux of known populations of galaxies. This lends support to the idea that large volumes of the Universe can be rapidly mapped without the need to resolve individual faint galaxies, enabling precise constraints to dark energy models. We discuss strategies for improved intensity mapping.},
	Affiliation = {AA(CITA, University of Toronto, 60 St George Str, Toronto, ON M5S 3H8, Canada), AB(School of Physics, M013, University of Western Australia, 35 Stirling Highway, Crawley WA 6009, Australia), AC(Department of Physics, Carnegie Mellon University, 500 Forbes Ave, Pittsburgh, PA 15213, USA), AD(CITA, University of Toronto, 60 St George Str, Toronto, ON M5S 3H8, Canada; Institute for Astronomy and Astrophysics, Academia Sinica, PO Box 23-141, Taipei 10617, Taiwan)},
	Author = {Ue-Li Pen and Lister Staveley-Smith and Jeffrey B Peterson and Tzu-Ching Chang},
	Date-Added = {2012-09-18 11:25:28 +0000},
	Date-Modified = {2012-09-18 11:25:28 +0000},
	Doi = {10.1111/j.1745-3933.2008.00581.x},
	Journal = {Monthly Notices of the Royal Astronomical Society: Letters},
	Keywords = {large-scale structure of Universe, radio lines: galaxies, galaxies: statistics},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2009/Pen/Monthly%20Notices%20of%20the%20Royal%20Astronomical%20Society%20Letters%202009%20Pen.pdf},
	Month = {Mar},
	Pages = {L6},
	Pmid = {2009MNRAS.394L...6P},
	Rating = {0},
	Title = {First detection of cosmic structure in the 21-cm intensity field},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p9865},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009MNRAS.394L...6P&link_type=ABSTRACT},
	Volume = {394},
	Year = {2009},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009MNRAS.394L...6P&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1111/j.1745-3933.2008.00581.x}}

@article{Peterson:2009p9204,
	Abstract = {Using the 21 cm line, observed all-sky and across the redshift range from 0 to 5, the large scale structure of the Universe can be mapped in three dimensions. This can be accomplished by studying specific intensity with resolution ~ 10 Mpc, rather than via the usual galaxy redshift survey. The data set can be analyzed to determine Baryon Acoustic Oscillation wavelengths, in order to address the question: 'What is the nature of Dark Energy?' In addition, the study of Large Scale Structure across this range addresses the questions: 'How does Gravity effect very large objects?' and 'What is the composition our Universe?' The same data set can be used to search for and catalog time variable and transient radio sources.},
	Author = {Jeffrey B Peterson and Roy Aleksan and R{\'e}za Ansari and Kevin Bandura and Dick Bond and John Bunton and Kermit Carlson and Tzu-Ching Chang and Fritz DeJongh and Matt Dobbs and Scott Dodelson and Hassane Darhmaoui and Nick Gnedin and Mark Halpern and Craig Hogan and Jean-Marc Le Goff and Tiehui Ted Liu and Ahmed Legrouri and Avi Loeb and Khalid Loudiyi and Christophe Magneville and John Marriner and David P McGinnis and Bruce McWilliams and Marc Moniez and Nathalie Palanque-Delabruille and Ralph J Pasquinelli and Ue-Li Pen and Jim Rich and Vic Scarpine and Hee-Jong Seo and Kris Sigurdson and Uros Seljak and Albert Stebbins and Jason H Steffen and Chris Stoughton and Peter T Timbie and Alberto Vallinotto and Christophe Teche},
	Date-Added = {2012-06-21 09:36:35 +0000},
	Date-Modified = {2012-06-21 09:36:35 +0000},
	Journal = {Astro2010: The Astronomy and Astrophysics Decadal Survey},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2009/Peterson/Astro2010%20The%20Astronomy%20and%20Astrophysics%20Decadal%20Survey%202009%20Peterson.pdf},
	Month = {Jan},
	Pages = {234},
	Pmid = {2009astro2010S.234P},
	Rating = {0},
	Title = {21-cm Intensity Mapping},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p9204},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009astro2010S.234P&link_type=ABSTRACT},
	Volume = {2010},
	Year = {2009},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009astro2010S.234P&link_type=ABSTRACT}}

@article{Smoot:1992p9283,
	Abstract = {Results of the first year of data from the differential microwave radiometers on the Cosmic Background Explorer are presented. Statistically significant structure that is well described as scale-invariant fluctuations with a Gaussian distribution is shown. The rms sky variation, smoothed to a total 10-deg FWHM Gaussian, is 30 +/-5 micro-K for Galactic latitude greater than 20-deg data with the dipole anisotropy removed. The rms cosmic quadrupole amplitude is 13 +/-4 micro-K. The angular autocorrelation of the signal in each radiometer channel and cross-correlation between channels are consistent and give a primordial fluctuation power-law spectrum with index of 1.1 +/-0.5, and an rms-quadrupole-normalized amplitude of 16 +/-4 micro-K. These features are in accord with the Harrison-Zel'dovich spectrum predicted by models of inflationary cosmology.},
	Affiliation = {AA(Lawrence Berkeley Laboratory; California, University, Berkeley), AB(NASA, Goddard Space Flight Center, Greenbelt, MD), AC(Universities Space Research Association; NASA, Goddard Space Flight Center, Greenbelt, MD), AD(California, University, Los Angeles), AE(Lawrence Berkeley Laboratory; California, University, Berkeley), AF(Lawrence Berkeley Laboratory; California, University, Berkeley), AG(Lawrence Berkeley Laboratory; California, University, Berkeley), AH(Lawrence Berkeley Laboratory; California, Unive...},
	Author = {G. F Smoot and C. L Bennett and A Kogut and E. L Wright and J Aymon and N. W Boggess and E. S Cheng and G de Amici and S Gulkis and M. G Hauser and G Hinshaw and P. D Jackson and M Janssen and E Kaita and T Kelsall and P Keegstra and C Lineweaver and K Loewenstein and P Lubin and J Mather and S. S Meyer and S. H Moseley and T Murdock and L Rokke and R. F Silverberg and L Tenorio and R Weiss and D. T Wilkinson},
	Date-Added = {2012-06-19 14:52:38 +0000},
	Date-Modified = {2012-06-19 14:52:38 +0000},
	Doi = {10.1086/186504},
	Journal = {Astrophysical Journal},
	Keywords = {MILKY WAY GALAXY, NORMAL DENSITY FUNCTIONS, COSMIC BACKGROUND EXPLORER SATELLITE, MICROWAVE RADIOMETERS, ROOT-MEAN-SQUARE ERRORS, ASTRONOMICAL MAPS, RELIC RADIATION},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/1992/Smoot/Astrophysical%20Journal%201992%20Smoot.pdf},
	Month = {Sep},
	Pages = {L1},
	Pmid = {1992ApJ...396L...1S},
	Rating = {0},
	Title = {Structure in the COBE differential microwave radiometer first-year maps},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p9283},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ApJ...396L...1S&link_type=ABSTRACT},
	Volume = {396},
	Year = {1992},
	Bdsk-File-1 = {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},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ApJ...396L...1S&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1086/186504}}

@article{Penzias:1965p9209,
	Abstract = {Measurements of the effective zenith noise temperature of the 20-foot horn-reflector antenna (Crawford, Hogg, and Hunt 1961) at the Crawford Hill Laboratory, Holmdel, New Jersey, at 4080 Mc/s have yielded a value of about 3.5 K higher than expected. This excess temperature is, within the limits of our observations, isotropic, unpolarized, and free from seasonal variations (July, 1964 - April, 1965). A possible explanation for the observed excess noise temperature is the one given by Dicke, Peebles, Roll, and Wilkinson (1965) in a companion letter in this issue.},
	Affiliation = {AA(Bell Telephone Laboratories Inc.), AB(Bell Telephone Laboratories Inc.)},
	Author = {A. A Penzias and R. W Wilson},
	Date-Added = {2012-06-19 11:30:39 +0000},
	Date-Modified = {2012-06-19 11:30:39 +0000},
	Doi = {10.1086/148307},
	Journal = {Astrophysical Journal},
	Keywords = {Microwave Background, Cosmic Background Radiation},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/1965/Penzias/Astrophysical%20Journal%201965%20Penzias.pdf},
	Month = {Jul},
	Pages = {419},
	Pmid = {1965ApJ...142..419P},
	Rating = {0},
	Title = {A Measurement of Excess Antenna Temperature at 4080 Mc/s.},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p9209},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1965ApJ...142..419P&link_type=ABSTRACT},
	Volume = {142},
	Year = {1965},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1965ApJ...142..419P&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1086/148307}}

@article{Mueller1948,
	Author = {Hans Mueller},
	Date-Added = {2012-05-29 19:51:45 +0000},
	Date-Modified = {2014-11-04 17:48:37 +0000},
	Journal = {J. Opt. Soc. Am.},
	Pages = {661},
	Title = {The foundation of optics},
	Volume = {38},
	Year = {1948}}

@inproceedings{Kestur:2010:BCF:1848074.1848496,
	Acmid = {1848496},
	Address = {Washington, DC, USA},
	Author = {Kestur, Srinidhi and Davis, John D. and Williams, Oliver},
	Booktitle = {Proceedings of the 2010 IEEE Annual Symposium on VLSI},
	Date-Added = {2012-05-28 16:18:19 +0000},
	Date-Modified = {2012-05-28 16:18:19 +0000},
	Doi = {http://dx.doi.org/10.1109/ISVLSI.2010.84},
	Isbn = {978-0-7695-4076-4},
	Numpages = {6},
	Pages = {288--293},
	Publisher = {IEEE Computer Society},
	Series = {ISVLSI '10},
	Title = {BLAS Comparison on FPGA, CPU and GPU},
	Url = {http://dx.doi.org/10.1109/ISVLSI.2010.84},
	Year = {2010},
	Bdsk-Url-1 = {http://dx.doi.org/10.1109/ISVLSI.2010.84}}

@conference{Bergman:2005p7825,
	Abstract = {The ELVIS instrument was recently proposed by the authors for the Indian Chandrayaan-1 mission to the Moon and is presently under consideration by the Indian Space Research Organisation (ISRO). The scientific objective of ELVIS is to explore the electromagnetic environment of the moon. ELVIS samples the full three-dimensional (3D) electric field vector, E(x,t), up to 18 MHz, with selective Nyqvist frequency bandwidths down to 5 kHz, and one component of the magnetic field vector, B(x,t), from a few Hz up to 100 kHz.As a transient detector, ELVIS is capable of detecting pulses with a minimum pulse width of 5 ns. The instrument comprises three orthogonal electric dipole antennas, one magnetic search coil antenna and a four-channel digital sampling system, utilising flexible digital down conversion and filtering together with state-of-the-art onboard digital signal processing.},
	Annote = {8 pages, 3 figures. Submitted to the DGLR Int. Symposium "To Moon and Beyond", Bremen, Germany, 2005. Companion paper to arXiv:astro-ph/0509210},
	Author = {J. E. S Bergman and L {\AA}hl{\'e}n and O St{\aa}l and B Thid{\'e} and S Ananthakrishnan and J. -E Wahlund and R. L Karlsson and W Puccio and T. D Carozzi and P Kale},
	Booktitle = {DGLR intl. symp. ''To Moon and Beyond''},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2015-01-07 19:32:21 +0000},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2005/Bergman/eprint%20arXiv%202005%20Bergman.pdf},
	Month = {Sep},
	Rating = {0},
	Title = {ELVIS - ELectromagnetic Vector Information Sensor},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7825},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005astro.ph..9864B&link_type=ABSTRACT},
	Year = {2005},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005astro.ph..9864B&link_type=ABSTRACT}}

@article{Bergman:2005p7865,
	Abstract = { The ELVIS instrument was recently proposed by the authors for the Indian Chandrayaan-1 mission to the Moon and is presently under consideration by the Indian Space Research Organisation (ISRO). The scientific objective of ELVIS is to explore the electromagnetic environment of the moon. ELVIS samples the full three-dimensional (3D) electric field vector, E(x,t), up to 18 MHz, with selective Nyqvist frequency bandwidths down to 5 kHz, and one component of the magnetic field vector, B(x,t), from a few Hz up to 100 kHz.As a transient detector, ELVIS is capable of detecting pulses with a minimum pulse width of 5 ns. The instrument comprises three orthogonal electric dipole antennas, one magnetic search coil antenna and a four-channel digital sampling system, utilising flexible digital down conversion and filtering together with state-of-the-art onboard digital signal processing. },
	Annote = {8 pages, 3 figures. Submitted to the DGLR Int. Symposium "To Moon and
  Beyond", Bremen, Germany, 2005. Companion paper to arXiv:astro-ph/0509210},
	Author = {J. E. S Bergman and L {\AA}hl{\'e}n and O St{\aa}l and B Thid{\'e} and S Ananthakrishnan and J. -E Wahlund and R. L Karlsson and W Puccio and T. D Carozzi and P Kale},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Eprint = {astro-ph/0509864v1},
	Journal = {arXiv},
	Keywords = {astro-ph},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2005/Bergman/arXiv%202005%20Bergman.pdf},
	Month = {Sep},
	Pmid = {astro-ph/0509864v1},
	Rating = {0},
	Title = {ELVIS - ELectromagnetic Vector Information Sensor},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7865},
	Url = {http://arxiv.org/abs/astro-ph/0509864v1},
	Volume = {astro-ph},
	Year = {2005},
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	Bdsk-Url-1 = {http://arxiv.org/abs/astro-ph/0509864v1}}

@article{Bergman:2008p7859,
	Abstract = {We present a new characterization of partially coherent electric and magnetic wave vector fields.This characterization is based on the 36 auto/cross correlations of the 3+3 complex Cartesian components of the electric and magnetic wave fields and is particularly suited for analyzing electromagnetic wave data on board spacecraft. Data from spacecraft based electromagnetic wave instruments are usually processed as data arrays. These data arrays however do not have a physical interpretation in themselves; they are simply a convenient storage format. In contrast, the characterization proposed here contains exactly the same information but are in the form of manifestly covariant space-time tensors. We call this data format the Canonical Electromagnetic Observables (CEO) since they correspond to unique physical observables. Some of them are already known, such as energy density, Poynting flux, stress tensor, etc, while others should be relevant in future space research. As an example we use this formalism to analyze data from a chorus emission in the mid-latitude magnetosphere, as recorded by the STAFF-SA instrument on board the Cluster-II spacecraft.},
	Annote = {8 pages, 1 figure. Submitted to Annales Geophysicae},
	Author = {Jan E. S Bergman and Tobia D Carozzi},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2014-11-04 17:37:27 +0000},
	Journal = {arXiv},
	Keywords = {Physics - Space Physics, Physics - Geophysics},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2008/Bergman/eprint%20arXiv%202008%20Bergman.pdf},
	Month = {Apr},
	Pmid = {2008arXiv0804.2092B},
	Rating = {0},
	Title = {Canonical Electromagnetic Observables for Systematic Characterization of Electric and Magnetic Wave Field Data on board Spacecraft},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7859},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008arXiv0804.2092B&link_type=ABSTRACT},
	Volume = {astro-ph/0804.2092},
	Year = {2008},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008arXiv0804.2092B&link_type=ABSTRACT}}

@book{BookGriffiths,
	Author = {David J. Griffiths},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Publisher = {Prentice-Hall Inc.},
	Title = {Introduction to Electrodynamics},
	Year = {1999}}

@book{BookMandelWolf,
	Abstract = {{The advent of lasers in the 1960s led to the development of many new fields in optical physics. This book is a systematic treatment of one of these fields--the broad area that deals with the coherence and fluctuation of light. The authors begin with a review of probability theory and random processes, and follow this with a thorough discussion of optical coherence theory within the framework of classical optics.  They next treat the theory of photoelectric detection of light and photoelectric correlation.  They then discuss in some detail quantum systems and effects.  The book closes with two chapters devoted to laser theory and one on the quantum theory of nonlinear optics.    The sound introduction to coherence theory and the quantum nature of light and the chapter-end exercises will appeal to graduate students and newcomers to the field. Researchers will find much of interest in the new results on coherence-induced spectral line shifts, nonclassical states of light, higher-order squeezing, and quantum effects of down-conversion. Written by two of the world's most highly regarded optical physicists, this book is required reading of all physicists and engineers working in optics.}},
	Author = {Mandel, Leonard and Wolf, Emil},
	Citeulike-Article-Id = {797005},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Day = {29},
	Edition = {1},
	Howpublished = {Hardcover},
	Isbn = {0521417112},
	Keywords = {hong-ou-mandel, optics, physics, quantum-optics},
	Posted-At = {2006-08-11 09:32:55},
	Priority = {0},
	Publisher = {Cambridge University Press},
	Title = {Optical Coherence and Quantum Optics},
	Year = {1995},
	Bdsk-Url-1 = {http://www.amazon.com/exec/obidos/redirect?tag=citeulike07-20%5C&path=ASIN/0521417112}}

@book{BookStewartCalculus,
	Author = {James Stewart},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Edition = {Seventh},
	Editor = {Liz Covello},
	Keywords = {calculus},
	Publisher = {Cengage Learning},
	Title = {Calculus},
	Year = {2012},
	Bdsk-File-1 = {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}}

@book{BookTinbergenPolarim,
	Author = {Jaan Tinbergen},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Keywords = {Polarimetry, Polarization},
	Publisher = {Cambridge University Press},
	Title = {Astronomical Polarimetry},
	Year = {2005}}

@article{BrandaoFaria2002,
	Author = {J A Brand{\~a}o Faria},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Doi = {10.1002/mop.10261},
	Journal = {Microwave and Optical Technology Letters},
	Keywords = {transmission matrices, cascaded multiconductor transmission-line structures, ABCD parameters},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2002/Faria/Microwave%20and%20Optical%20Technology%20Letters%202002%20Faria.pdf},
	Number = {3},
	Pages = {151--154},
	Rating = {0},
	Read = {Yes},
	Title = {On the transmission matrix of 2n-port reciprocal networks},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7461},
	Url = {http://dx.doi.org/10.1002/mop.10261},
	Volume = {33},
	Year = {2002},
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	Bdsk-Url-1 = {http://dx.doi.org/10.1002/mop.10261}}

@article{Hamaker:1996p5733,
	Abstract = {In two companion papers (Paper I, Hamaker et al. 1996; Paper II, Sault et al. 1996), a new theory of radio-interferometric polarimetry and its application to the calibration of interferometer arrays are presented. To complete our study of radio polarimetry, we examine here the definition of the Stokes parameters adopted by Commission 40 of the IAU (1974) and the way this definition works out in the mathematical equations. Using the formalism of Paper I, we give a simplified derivation of the frequently-cited `black-box' formula originally derived by Morris et al. (1964). We show that their original version is in error in the sign of Stokes V, the correct sign being that given by Weiler (1973) and Thompson et al. (1986).},
	Author = {J. P Hamaker and J. D Bregman},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2014-11-04 17:42:57 +0000},
	Journal = {A\&A Supp.},
	Keywords = {TECHNIQUES: INTERFEROMETERS, TECHNIQUES: POLARIMETERS, METHODS: DATA ANALYSIS, POLARIZATION, METHODS: ANALYTICAL},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/1996/Hamaker/Astronomy%20and%20Astrophysics%20Supp.%201996%20Hamaker.pdf},
	Month = {Apr},
	Pages = {161},
	Pmid = {1996A&AS..117..161H},
	Rating = {0},
	Title = {Understanding radio polarimetry. III. Interpreting the IAU/IEEE definitions of the Stokes parameters.},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p5733},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996A%2526AS..117..161H&link_type=ABSTRACT},
	Volume = {117},
	Year = {1996},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996A%2526AS..117..161H&link_type=ABSTRACT}}

@article{Hamaker:1996p5735,
	Abstract = {The measurement of polarized radiation uses entirely different methods at optical and radio wavelengths. As a result, the algebraic analysis of polarimeter performance differs and, in the case of radio interferometry, is unnecessarily complicated. We demonstrate that the mathematical operation of outer matrix multiplication provides the missing link between the two approaches. Within one coherent framework, we then unite the concepts of Stokes parameters and Wolf coherency matrix, the Jones and Mueller calculi from optics, and the techniques of radio interferometry based on multiplying correlators. We relate the polarization performance of a complete radio interferometer to the (matrix) polarization properties of its successive signal processing stages, providing a clear view of how a radio polarimeter works. Our treatment also clarifies the nature of and the relations between the various types of transformations used in optical polarimetry. We develop the analysis from the radio interferometrist's point of view, but include enough background for a wider audience. In a companion paper, we discuss in more detail the application to the calibration of radio interferometer systems; in a third paper we investigate the IAU (1973) radio definition of the Stokes parameters and its precise translation into mathematical form.},
	Author = {J. P Hamaker and J. D Bregman and R. J Sault},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2014-11-04 17:43:00 +0000},
	Journal = {A\&A Supp.},
	Keywords = {TECHNIQUES: POLARIMETERS, METHODS: DATA ANALYSIS, METHODS: ANALYTICAL, TECHNIQUES: INTERFEROMETERS},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/1996/Hamaker/Astronomy%20and%20Astrophysics%20Supp.%201996%20Hamaker-1.pdf},
	Month = {Apr},
	Pages = {137},
	Pmid = {1996A&AS..117..137H},
	Rating = {0},
	Read = {Yes},
	Title = {Understanding radio polarimetry. I. Mathematical foundations.},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p5735},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996A%2526AS..117..137H&link_type=ABSTRACT},
	Volume = {117},
	Year = {1996},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996A%2526AS..117..137H&link_type=ABSTRACT}}

@article{Hamaker:2000p7625,
	Abstract = {Paper II of this series studied the calibration process in mostly qualitative terms. In developing the underlying mathematics this paper completes that analysis and extends it in several directions. It exploits the analogy between scalar and matrix algebras to reformulate the self-calibration method in terms of 2 x 2 Jones and coherency matrices. The basic condition that the solutions must satisfy in either case is developed and its consequences are investigated. The fourfold nature of the matrices and the non-commutativity of their multiplication are shown to lead to a number of new effects. In the same way that scalar selfcal leaves the brightness scale undefined, matrix selfcal gives rise to a more complicated indeterminacy. The calibration is far from complete: self-alignment describes more properly what is actually achieved. The true brightness is misrepresented in the image obtained by an unknown brightness-scale factor (as in scalar selfcal) and an undefined poldistortion of the Stokes brightness. The latter is the product of a polrotation of the polvector (Q,U,V) and a polconversion between unpolarized and polarized brightness. The relation of these concepts to conventional ``quasi-scalar'' calibration methods is demonstrated. Like scalar selfcal, matrix self-alignment is shown to suppress spatial scattering of brightness in the image, which is a condition for attaining high dynamic range. Poldistortion of the brightness is an in-place transformation, but must be controlled in order to obtain olarimetric fidelity. The theory is applied to reinterpret the quasi-scalar methods of polarimetry including those of Paper II, and to prove two major new assertions: (a.) An instrument calibrated on an unpolarized calibrator measures the degree of polarization correctly regardless of poldistortion; (b.) Under the usual a priori assumptions, a heterogeneous instrument (i.e. one with unequal feeds) can be completely calibrated without requiring a phase-difference measurement.},
	Affiliation = {AA(Netherlands Foundation for Research in Astronomy, Postbus 2, 7990 AA Dwingeloo, The Netherlands)},
	Author = {J. P Hamaker},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2014-11-04 17:43:05 +0000},
	Doi = {10.1051/aas:2000337},
	Journal = {A\&A Supp.},
	Keywords = {TECHNIQUES: POLARIMETRIC, TECHNIQUES: INTERFEROMETRIC, INSTRUMENTATION: POLARIMETERS, METHODS: OBSERVATIONAL, METHODS: ANALYTICAL, INSTRUMENTATION: INTERFEROMETERS},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2000/Hamaker/Astronomy%20and%20Astrophysics%20Supp.%202000%20Hamaker.pdf},
	Month = {May},
	Pages = {515},
	Pmid = {2000A&AS..143..515H},
	Rating = {0},
	Title = {Understanding radio polarimetry. IV. The full-coherency analogue of scalar self-calibration: Self-alignment, dynamic range and polarimetric fidelity},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7625},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000A%2526AS..143..515H&link_type=ABSTRACT},
	Volume = {143},
	Year = {2000},
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	Bdsk-Url-2 = {http://dx.doi.org/10.1051/aas:2000337}}

@article{Hamaker:2006p7626,
	Abstract = {Context: .This is Paper V in a series on polarimetric aperture synthesis based on the algebra of 2×2 matrices. Aims: .It validates the matrix self-calibration theory of the preceding Paper IV and outlines the algorithmic methods that had to be developed for its application. Methods: .New avenues of polarimetric self-calibration opened up in Paper IV are explored by processing a simulated observation. To focus on the polarimetric issues, it is set up so as to sidestep some of the common complications of aperture synthesis, yet properly represent physical conditions. In addition to a representative collection of observing errors, the simulated instrument includes strongly varying Faraday rotation and antennas with unequal feeds. The selfcal procedure is described in detail, including aspects in which it differs from the scalar case, and its effects are demonstrated with a number of intermediate image results. Results: .The simulation's outcome is in full agreement with the theory. The nonlinear matrix equations for instrumental parameters are readily solved by iteration; a convergence problem is easily remedied with a new ancillary algorithm. Instrumental effects are cleanly separated from source properties without reference to changes in parallactic rotation during the observation. Polarimetric images of high purity and dynamic range result. As theory predicts, polarimetric errors that are common to all sources inevitably remain; prior knowledge of the statistics of linear and circular polarization in a typical observed field can be applied to eliminate most of them. Conclusions: .The paper conclusively demonstrates that matrix selfcal per se is a viable method that may foster substantial advancement in the art of radio polarimetry. For its application in real observations, a number of issues must be resolved that matrix selfcal has in common with its scalar sibling, such as the treatment of extended sources and the familiar sampling and aliasing problems. The close analogy between scalar interferometry and its matrix-based generalisation suggests that one may apply well-developed methods of scalar interferometry. Marrying these methods to those of this paper will require a significant investment in new software. Two such developments are known to be foreseen or underway.},
	Affiliation = {AA(ASTRON, Netherlands Foundation for Research in Astronomy, Postbus 2, 7990 AA Dwingeloo, The Netherlands hamaker@astron.nl)},
	Author = {J. P Hamaker},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2014-11-04 17:43:11 +0000},
	Doi = {10.1051/0004-6361:20065145},
	Journal = {A\&A},
	Keywords = {TECHNIQUES: POLARIMETRIC, TECHNIQUES: INTERFEROMETRIC, INSTRUMENTATION: POLARIMETERS, METHODS: OBSERVATIONAL, methods: data analysis, INSTRUMENTATION: INTERFEROMETERS},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2006/Hamaker/Astronomy%20and%20Astrophysics%202006%20Hamaker.pdf},
	Month = {Sep},
	Pages = {395},
	Pmid = {2006A&A...456..395H},
	Rating = {0},
	Title = {Understanding radio polarimetry. V. Making matrix self-calibration work: processing of a simulated observation},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7626},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006A%2526A...456..395H&link_type=ABSTRACT},
	Volume = {456},
	Year = {2006},
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	Bdsk-Url-2 = {http://dx.doi.org/10.1051/0004-6361:20065145}}

@article{Jones1941,
	Author = {R Clark Jones},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Journal = {J. Opt. Soc. Am.},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/1941/Jones/J.%20Opt.%20Soc.%20Am.%201941%20Jones.pdf},
	Month = {Jul},
	Pages = {1--6},
	Rating = {0},
	Title = {A New Calculus for the Treatment of Optical Systems. I. Description and Discussion of the Calculus},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7753},
	Volume = {31},
	Year = {1941},
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@article{Maxwell1861,
	Author = {James Maxwell},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Journal = {Philosophical Magazine},
	Keywords = {Maxwells equations},
	Title = {On Physical Lines of Force},
	Volume = {21 \& 23 Series 4},
	Year = {1861},
	Bdsk-Url-1 = {en.wikisource.org/wiki/On_Physical_Lines_of_Force}}

@article{Sault:1996p5731,
	Abstract = {In a companion paper, a mathematical formalism to describe the polarimetric response of a radio interferometer was presented. Some of the instrumental parameters, however, are either unknown or poorly known. Here we consider the determination of these parameters both by a traditional radio-interferometry instrumental approach as well as by using optical polarimetry principles. In doing so, we establish links between the two fields. We show that some degrees of freedom cannot be solved for with various calibration or self-calibration schemes. These degrees of freedom are identified with instrumental parameters and physical source properties. The number of unsolvable degrees of freedom is reduced for a long synthesis with alt-az antennas. We also consider the effect of errors in the assumed instrumental parameters on the resultant calibrated data. The polarimetric calibration procedure for some telescopes is reviewed in the context of this analysis.},
	Author = {R. J Sault and J. P Hamaker and J. D Bregman},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2014-11-04 17:54:18 +0000},
	Journal = {A\&A Supp.},
	Keywords = {TECHNIQUES: POLARIMETERS, METHODS: DATA ANALYSIS, METHODS: ANALYTICAL, TECHNIQUES: INTERFEROMETERS},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/1996/Sault/Astronomy%20and%20Astrophysics%20Supp.%201996%20Sault.pdf},
	Month = {Apr},
	Pages = {149},
	Pmid = {1996A&AS..117..149S},
	Rating = {0},
	Read = {Yes},
	Title = {Understanding radio polarimetry. II. Instrumental calibration of an interferometer array.},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p5731},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996A%2526AS..117..149S&link_type=ABSTRACT},
	Volume = {117},
	Year = {1996},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996A%2526AS..117..149S&link_type=ABSTRACT}}

@article{Smirnov:2011a,
	Abstract = { Since its formulation by Hamaker et al., the radio interferometer measurement equation (RIME) has provided a rigorous mathematical basis for the development of novel calibration methods and techniques, including various approaches to the problem of direction-dependent effects (DDEs). This series of papers aims to place recent developments in the treatment of DDEs into one RIME-based mathematical framework, and to demonstrate the ease with which the various effects can be described and understood. It also aims to show the benefits of a RIME-based approach to calibration.  Paper I re-derives the RIME from first principles, extends the formalism to the full-sky case, and incorporates DDEs. Paper II then uses the formalism to describe self-calibration, both with a full RIME, and with the approximate equations of older software packages, and shows how this is affected by DDEs. It also gives an overview of real-life DDEs and proposed methods of dealing with them. Applying this to WSRT data (Paper III) results in a noise-limited image of the field around 3C 147 with a very high dynamic range (1.6 million), and none of the off-axis artifacts that plague regular selfcal. The resulting differential gain solutions contain significant information on DDEs, and can be used for iterative improvements of sky models.  Perhaps most importantly, sources as faint as 2 mJy have been shown to yield meaningful differential gain solutions, and thus can be used as potential calibration beacons in other DDE-related schemes. },
	Annote = {Published in: A{\&}A 2011, 527, A106

12 pages, no figures, published in A{\&}A},
	Author = {Oleg M Smirnov},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2014-11-04 17:55:19 +0000},
	Doi = {10.1051/0004-6361/201016082},
	Eprint = {1101.1764v3},
	Journal = {A\&A},
	Keywords = {A\&A},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2011/Smirnov/arXiv%202011%20Smirnov-1.pdf},
	Month = {Jan},
	Pages = {A106},
	Pmid = {1101.1764v3},
	Rating = {0},
	Read = {Yes},
	Title = {Revisiting the radio interferometer measurement equation. I. A full-sky Jones formalism},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7129},
	Url = {http://arxiv.org/abs/1101.1764v3},
	Volume = {527},
	Year = {2011},
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	Bdsk-Url-1 = {http://arxiv.org/abs/1101.1764v3},
	Bdsk-Url-2 = {http://dx.doi.org/10.1051/0004-6361/201016082}}

@article{Smirnov:2011b,
	Abstract = { Paper I of the series re-derived the radio interferometry measurement equation (RIME) from first principles, and extended the Jones formalism to the full-sky case, incorporating direction-dependent effects (DDEs). This paper aims to describe both classical radio interferometric calibration (selfcal and related methods), and the recent developments in the treatment of DDEs, using the RIME-based mathematical framework developed in Paper I. It also aims to demonstrate the ease with which the various effects can be described and understood.  The first section of this paper uses the RIME formalism to describe self-calibration, both with a full RIME, and with the approximate equations of older software packages, and shows how this is affected by DDEs. The second section gives an overview of real-life DDEs and proposed methods of dealing with them. This results in a formal RIME-based description and comparison of existing and proposed approaches to the problem of DDEs. },
	Annote = {Published in: A{\&}A 2011, 527, A107

11 pages, no figures, accepted by A{\&}A},
	Author = {Oleg M Smirnov},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2014-11-04 17:55:25 +0000},
	Doi = {10.1051/0004-6361/201116434},
	Eprint = {1101.1765v3},
	Journal = {A\&A},
	Keywords = {A\&A},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2011/Smirnov/arXiv%202011%20Smirnov.pdf},
	Month = {Jan},
	Pages = {A107},
	Pmid = {1101.1765v3},
	Rating = {0},
	Read = {Yes},
	Title = {Revisiting the radio interferometer measurement equation. II. Calibration and direction-dependent effects},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7128},
	Url = {http://arxiv.org/abs/1101.1765v3},
	Volume = {527},
	Year = {2011},
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	Bdsk-Url-1 = {http://arxiv.org/abs/1101.1765v3},
	Bdsk-Url-2 = {http://dx.doi.org/10.1051/0004-6361/201116434}}

@article{Smirnov:2011c,
	Abstract = { Papers I and II of this series have extended the radio interferometry measurement equation (RIME) formalism to the full-sky case, and provided a RIME-based description of calibration and the problem of direction-dependent effects (DDEs). This paper aims to provide a practical demonstration of a RIME-based approach to calibration, via an example of extremely high-dynamic range calibration of WSRT observations of 3C 147 at 21 cm, with full treatment of DDEs.  A version of the RIME incorporating differential gains has been implemented in MeqTrees, and applied to the 3C 147 data. This was used to perform regular selfcal, then solve for interferometer-based errors and for differential gains. The resulting image of the field around 3C 147 is thermal noise-limited, has a very high dynamic range (1.6 million), and none of the off-axis artefacts that plague regular selfcal. The differential gain solutions show a high signal-to-noise ratio, and may be used to extract information on DDEs and errors in the sky model.  The differential gain approach can eliminate DDE-related artefacts, and provide information for iterative improvements of sky models. Perhaps most importantly, sources as faint as 2 mJy have been shown to yield meaningful differential gain solutions, and thus can be used as potential calibration beacons in other DDE-related schemes. },
	Annote = {Published in: A{\&}A 2011, 527, A108

11 pages, 17 figures, accepted by A{\&}A},
	Author = {Oleg M Smirnov},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2014-11-04 17:55:30 +0000},
	Doi = {10.1051/0004-6361/201116435},
	Eprint = {1101.1768v2},
	Journal = {A\&A},
	Keywords = {A\&A},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2011/Smirnov/arXiv%202011%20Smirnov-2.pdf},
	Month = {Jan},
	Pages = {A108},
	Pmid = {1101.1768v2},
	Rating = {0},
	Title = {Revisiting the radio interferometer measurement equation. III. Addressing direction-dependent effects in 21 cm WSRT observations of 3C 147},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7130},
	Url = {http://arxiv.org/abs/1101.1768v2},
	Volume = {527},
	Year = {2011},
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	Bdsk-Url-1 = {http://arxiv.org/abs/1101.1768v2},
	Bdsk-Url-2 = {http://dx.doi.org/10.1051/0004-6361/201116435}}

@article{Smirnov:2011d,
	Abstract = { The radio interferometer measurement equation (RIME), especially in its 2x2 form, has provided a comprehensive matrix-based formalism for describing classical radio interferometry and polarimetry, as shown in the previous three papers of this series. However, recent practical and theoretical developments, such as phased array feeds (PAFs), aperture arrays (AAs) and wide-field polarimetry, are exposing limitations of the formalism. This paper aims to develop a more general formalism that can be used to both clearly define the limitations of the matrix RIME, and to describe observational scenarios that lie outside these limitations. Some assumptions underlying the matrix RIME are explicated and analysed in detail. To this purpose, an array correlation matrix (ACM) formalism is explored. This proves of limited use; it is shown that matrix algebra is simply not a sufficiently flexible tool for the job. To overcome these limitations, a more general formalism based on tensors and the Einstein notation is proposed and explored both theoretically, and with a view to practical implementations. The tensor formalism elegantly yields generalized RIMEs describing beamforming, mutual coupling, and wide-field polarimetry in one equation. It is shown that under the explicated assumptions, tensor equations reduce to the 2x2 RIME. From a practical point of view, some methods for implementing tensor equations in an optimal way are proposed and analysed. The tensor RIME is a powerful means of describing observational scenarios not amenable to the matrix RIME. Even in cases where the latter remains applicable, the tensor formalism can be a valuable tool for understanding the limits of such applicability. },
	Annote = {Published in: A{\&}A 2011, 531, A159

16 pages, no figures, accepted by A{\&}A},
	Author = {Oleg M Smirnov},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2014-11-04 17:55:34 +0000},
	Doi = {10.1051/0004-6361/201116764},
	Eprint = {1106.0579v1},
	Journal = {A\&A},
	Keywords = {A\&A},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2011/Smirnov/arXiv%202011%20Smirnov-3.pdf},
	Month = {Jun},
	Pages = {A159},
	Pmid = {1106.0579v1},
	Rating = {0},
	Title = {Revisiting the radio interferometer measurement equation. IV. A generalized tensor formalism},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7132},
	Url = {http://arxiv.org/abs/1106.0579v1},
	Volume = {531},
	Year = {2011},
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	Bdsk-Url-1 = {http://arxiv.org/abs/1106.0579v1},
	Bdsk-Url-2 = {http://dx.doi.org/10.1051/0004-6361/201116764}}

@article{SoftwareAIPS,
	Affiliation = {National Radio Astronomy Observatory},
	Author = {Eric W Greisen},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Journal = {AIPS Memorandum Series},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/1988/Greisen/AIPS%20Memorandum%20Series%201988%20Greisen.pdf},
	Month = {Dec},
	Number = {61},
	Pages = {1--19},
	Rating = {0},
	Title = {The Astronomical Image Processing System},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7741},
	Year = {1988},
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@misc{SoftwareCASA,
	Author = {NRAO},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Howpublished = {[computer software]},
	Keywords = {CASA software},
	Title = {CASA 3.3.0},
	Year = {2011}}

@article{SoftwareMeqTrees,
	Abstract = { The formulation of the radio interferometer measurement equation (RIME) by Hamaker et al. has provided us with an elegant mathematical apparatus for better understanding, simulation and calibration of existing and future instruments. The calibration of the new radio telescopes (LOFAR, SKA) would be unthinkable without the RIME formalism, and new software to exploit it. MeqTrees is designed to implement numerical models such as the RIME, and to solve for arbitrary subsets of their parameters. The technical goal of MeqTrees is to provide a tool for rapid implementation of such models, while offering performance comparable to hand-written code. We are also pursuing the wider goal of increasing the rate of evolution of radio astronomical software, by offering a tool for rapid experimentation and exchange of ideas.  MeqTrees is implemented as a Python-based front-end called the meqbrowser, and an efficient (C++-based) computational back-end called the meqserver. Numerical models are defined on the front-end via a Python-based Tree Definition Language (TDL), then rapidly executed on the back-end. The use of TDL facilitates an extremely short turn-around time for experimentation with new ideas. This is also helped by unprecedented visualization capabilities for all final and intermediate results. A flexible data model and a number of important optimizations in the back-end ensures that the numerical performance is comparable to that of hand-written code.  MeqTrees is already widely used as the simulation tool for new instruments (LOFAR, SKA) and technologies (focal plane arrays). It has demonstrated that it can achieve a noise-limited dynamic range in excess of a million, on WSRT data. It is the only package that is specifically designed to handle what we propose to call third-generation calibration (3GC), which is needed for the new generation of giant radio telescopes. },
	Annote = {Published in: A{\&}A 2010, 524, A61

15 pages; 14 figures},
	Author = {Jan E Noordam and Oleg M Smirnov},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Doi = {10.1051/0004-6361/201015013},
	Eprint = {1101.1745v2},
	Journal = {A\&A},
	Keywords = {A\&A},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2011/Noordam/arXiv%202011%20Noordam.pdf},
	Month = {Jan},
	Pages = {A61},
	Pmid = {1101.1745v2},
	Rating = {0},
	Title = {The MeqTrees software system and its use for third-generation calibration of radio interferometers},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7131},
	Url = {http://arxiv.org/abs/1101.1745v2},
	Volume = {524},
	Year = {2010},
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	Bdsk-Url-1 = {http://arxiv.org/abs/1101.1745v2},
	Bdsk-Url-2 = {http://dx.doi.org/10.1051/0004-6361/201015013}}

@article{SoftwareMIRIAD,
	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.},
	Affiliation = {AA(Australia Telescope National Facility, CSIRO, P.O. Box 76, Epping, N.S.W., 2121, Australia), AB(Astronomy Department, University of Maryland, College Park, MD 20742), AC(Astronomy Department, University of California, Berkeley, CA 94720)},
	Author = {R. J Sault and P. J Teuben and M. C. H Wright},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Journal = {Astronomical Data Analysis Software and Systems IV},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/1995/Sault/Astronomical%20Data%20Analysis%20Software%20and%20Systems%20IV%201995%20Sault.pdf},
	Month = {Jan},
	Pages = {433},
	Pmid = {1995ASPC...77..433S},
	Rating = {0},
	Title = {A Retrospective View of MIRIAD},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7742},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ASPC...77..433S&link_type=ABSTRACT},
	Volume = {77},
	Year = {1995},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ASPC...77..433S&link_type=ABSTRACT}}

@misc{SoftwareOSKAR2,
	Author = {Ben Mort and Fred Dulwich and Stef Salvini},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-09-27 10:57:31 +0000},
	Keywords = {oskar2},
	Title = {OSKAR2 [computer software]},
	Year = {2012}}

@book{Taylor1999,
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2014-11-04 17:56:07 +0000},
	Editor = {G. B Taylor and C. L. Carilli and R. A. Perley},
	Keywords = {synthesis imaging interferometry},
	Publisher = {ASP},
	Title = {Synthesis Imaging in Radio Astronomy II},
	Volume = {180},
	Year = {1999},
	Bdsk-File-1 = {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}}

@book{Wilson2009,
	Author = {Thomas Wilson and Kristen Rohlfs and Susanne Huttemeister},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Edition = {Fifth},
	Keywords = {radio astronomy},
	Publisher = {Springer-Verlag},
	Title = {Tools of Radio Astronomy},
	Year = {2009},
	Bdsk-File-1 = {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}}

@article{Wolf1954,
	Abstract = {A macroscopic theory of interference and diffraction of light in stationary fields produced by finite sources which emit light within a finite spectral range is formulated. It is shown that a generalized Huygens principle may be obtained for such fields, which involves only observable quantities. The generalized Huygens principle expresses the intensity at a typical point of the field in terms of an integral taken twice independently over an arbitrary surface, the integral involving the intensity distribution over the surface and the values of a certain correlation factor, which is found to be the 'degree of coherence' previously introduced by Zernike. Next it is shown that under fairly general conditions, this correlation factor is essentially the normalized integral over the source of the Fourier (frequency) transform of the spectral intensity function of the source, and that it may be determined from simple interference experiments. Further, it is shown that in regions where geometrical optics is a valid approximation, the coherence factor itself then obeys a simple geometrical law of propagation. Several results on partially coherent fields, established previously by Van Cittert, Zernike, Hopkins and Rogers, follow as special cases from these theorems. The results have a bearing on many optical problems and can also be applied in investigations concerned with other types of radiation.},
	Author = {Wolf, E.},
	Date-Added = {2012-05-28 16:18:11 +0000},
	Date-Modified = {2012-05-28 16:18:11 +0000},
	Journal = {Nuovo Cimento},
	Number = {884},
	Volume = {12},
	Year = {1954}}

@inproceedings{Kant2009,
	Author = {G.W. Kant and E. van der Wal and M. Ruiter and P. Benthem},
	Booktitle = {Widefield Science and Technology for the SKA},
	Date-Added = {2012-05-28 16:18:03 +0000},
	Date-Modified = {2012-05-28 16:18:03 +0000},
	Editor = {S.A. Torchinsky, A. van Ardenne, T. van den Brink-Havinga, A.J.J. van Es, A.J. Faulkner},
	Month = {November},
	Pages = {227-234},
	Title = {EMBRACE System Design and Realisation},
	Year = {2009},
	Bdsk-File-1 = {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}}

@misc{MoralesCARPE,
	Author = {M. Morales},
	Date-Added = {2012-05-28 16:18:03 +0000},
	Date-Modified = {2012-05-28 16:18:03 +0000},
	Howpublished = {online},
	Keywords = {CAPRE MOFF},
	Title = {CARPE},
	Url = {http://www.phys.washington.edu/users/mmorales/carpe/},
	Year = {2010},
	Bdsk-Url-1 = {http://www.phys.washington.edu/users/mmorales/carpe/}}

@article{McMahon:2008p1029,
	Abstract = {CASPER stuff, in particular spectrometers},
	Author = {Peter Leonard McMahon},
	Date-Added = {2012-05-28 16:17:57 +0000},
	Date-Modified = {2012-05-28 16:17:57 +0000},
	Journal = {CASPER Theses},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2008/McMahon/CASPER%20Theses%202008%20McMahon.pdf},
	Month = {Jul},
	Pages = {1--135},
	Rating = {0},
	Read = {Yes},
	Title = {Adventures in Radio Astronomy Instrumentation and Signal Processing},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p1029},
	Year = {2008},
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@manual{KATCP,
	Author = {S. Cross and R. Crida and T. Bennett and M. Welz},
	Date-Added = {2012-05-28 16:17:57 +0000},
	Date-Modified = {2012-05-28 16:17:57 +0000},
	Keywords = {katcp},
	Organization = {National Research Foundation (South Africa)},
	Title = {Guidelines for Communication with Devices},
	Year = {2009}}

@article{Campbell:2002p8252,
	Abstract = {This lecture covers the fundamentals of observations with a filled aperture antenna, basic receiver systems and sources of noise. A simple derivation is provided for the radiometer equation, which determines a telescope's ability to detect radio sources. The lecture ends with a discussion of antennas as filters on the spatial Fourier components of the sky brightness distribution.},
	Affiliation = {AA(National Astronomy and Ionosphere Center, Department of Astronomy, Cornell University, Ithaca, New York 14853-6801, USA)},
	Author = {Donald B Campbell},
	Date-Added = {2012-05-28 16:17:57 +0000},
	Date-Modified = {2012-05-28 16:17:57 +0000},
	Journal = {Single-Dish Radio Astronomy: Techniques and Applications},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2002/Campbell/Single-Dish%20Radio%20Astronomy%20Techniques%20and%20Applications%202002%20Campbell-2.pdf},
	Month = {Dec},
	Note = {ISBN: 1-58381-120-6},
	Pages = {81},
	Pmid = {2002ASPC..278...81C},
	Rating = {0},
	Title = {Measurement in Radio Astronomy},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p8252},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ASPC..278...81C&link_type=ABSTRACT},
	Volume = {278},
	Year = {2002},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ASPC..278...81C&link_type=ABSTRACT}}

@article{ONeil:2002p8156,
	Abstract = {Calibrating telescope data is one of the most important issues an observer faces. In this chapter we describe a number of the methods which are commonly used to calibrate radio telescope data in the centimeter wavelength regime. This includes a discussion of the various methods often used in determining the temperature and gain of a telescope, as well as some of the more common difficulties which can be encountered.},
	Affiliation = {AA(National Astronomy and Ionosphere Center, Arecibo Observatory, HC 3 Box 53995, Arecibo, Puerto Rico 00612, USA)},
	Author = {K O'Neil},
	Date-Added = {2012-05-28 16:17:57 +0000},
	Date-Modified = {2012-05-28 16:17:57 +0000},
	Journal = {Single-Dish Radio Astronomy: Techniques and Applications},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2002/O'Neil/Single-Dish%20Radio%20Astronomy%20Techniques%20and%20Applications%202002%20O'Neil.pdf},
	Month = {Dec},
	Note = {ISBN: 1-58381-120-6},
	Pages = {293},
	Pmid = {2002ASPC..278..293O},
	Rating = {0},
	Title = {Single-Dish Calibration Techniques at Radio Wavelengths},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p8156},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ASPC..278..293O&link_type=ABSTRACT},
	Volume = {278},
	Year = {2002},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ASPC..278..293O&link_type=ABSTRACT}}

@article{Nita:2010p4648,
	Abstract = {ABSTRACT Due to its conceptual simplicity and its proven effectiveness in real-time detection and removal of radio frequency interference (RFI) from radio astronomy data, the spectral kurtosis (SK) estimator is likely to become a standard tool of a new generation of radio telescopes. However, the SK estimator in its original form must be developed from instantaneous power spectral density estimates, and hence cannot be employed as an RFI excision tool downstream of the data pipeline in existing instruments where any time averaging is performed. In this Letter, we develop a generalized estimator with wider applicability for both instantaneous and averaged spectral data, which extends its practical use to a much larger pool of radio instruments.},
	Affiliation = {AA(Center for Solar-Terrestrial Research, New Jersey Institute of Technology, Newark, NJ 07102, USA; ), AB(Center for Solar-Terrestrial Research, New Jersey Institute of Technology, Newark, NJ 07102, USA; )},
	Author = {G. M Nita and D. E Gary},
	Date-Added = {2012-05-28 16:17:57 +0000},
	Date-Modified = {2012-05-28 16:17:57 +0000},
	Doi = {10.1111/j.1745-3933.2010.00882.x},
	Journal = {Monthly Notices of the Royal Astronomical Society: Letters},
	Keywords = {methods: statistical, instrumentation: spectrographs},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2010/Nita/Monthly%20Notices%20of%20the%20Royal%20Astronomical%20Society%20Letters%202010%20Nita.pdf},
	Month = {Jul},
	Note = {(c) Journal compilation {\copyright} 2010 RAS},
	Pages = {L60},
	Pmid = {2010MNRAS.406L..60N},
	Rating = {0},
	Read = {Yes},
	Title = {The generalized spectral kurtosis estimator},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p4648},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010MNRAS.406L..60N&link_type=ABSTRACT},
	Volume = {406},
	Year = {2010},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010MNRAS.406L..60N&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1111/j.1745-3933.2010.00882.x}}

@article{Keith:2010p6667,
	Abstract = {We have embarked on a survey for pulsars and fast transients using the 13-beam multibeam receiver on the Parkes Radio Telescope. Installation of a digital backend allows us to record 400 MHz of bandwidth for each beam, split into 1024 channels and sampled every 64 μs. Limits of the receiver package restrict us to a 340 MHz observing band centred at 1352 MHz. The factor of 8 improvement in frequency resolution over previous multibeam surveys allows us to probe deeper into the Galactic plane for short-duration signals such as the pulses from millisecond pulsars. We plan to survey the entire southern sky in 42641 pointings, split into low, mid and high Galactic latitude regions, with integration times of 4200, 540 and 270 s, respectively. Simulations suggest that we will discover 400 pulsars, of which 75 will be millisecond pulsars. With ~30 per cent of the mid-latitude survey complete, we have redetected 223 previously known pulsars and discovered 27 pulsars, five of which are millisecond pulsars. The newly discovered millisecond pulsars tend to have larger dispersion measures than those discovered in previous surveys, as expected from the improved time and frequency resolution of our instrument.},
	Affiliation = {AA(Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia), AB(Swinburne University of Technology, Centre for Astrophysics and Supercomputing, Mail H39, PO Box 218, VIC 3122, Australia), AC(Swinburne University of Technology, Centre for Astrophysics and Supercomputing, Mail H39, PO Box 218, VIC 3122, Australia), AD(Swinburne University of Technology, Centre for Astrophysics and Supercomputing, Mail H39, PO Box 218, VIC 3122, Australia), AE(Australia Telescope National Facility,...},
	Author = {M. J Keith and A Jameson and W van Straten and M Bailes and S Johnston and M Kramer and A Possenti and S. D Bates and N. D. R Bhat and M Burgay and S Burke-Spolaor and N D'Amico and L Levin and Peter L McMahon and S Milia and B. W Stappers},
	Date-Added = {2012-05-28 16:17:57 +0000},
	Date-Modified = {2012-09-27 10:56:22 +0000},
	Doi = {10.1111/j.1365-2966.2010.17325.x},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Keywords = {pulsars: general},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2010/Keith/Monthly%20Notices%20of%20the%20Royal%20Astronomical%20Society%202010%20Keith.pdf},
	Month = {Dec},
	Pages = {619},
	Pmid = {2010MNRAS.409..619K},
	Rating = {0},
	Read = {Yes},
	Title = {The High Time Resolution Universe Pulsar Survey - I. System configuration and initial discoveries},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p6667},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010MNRAS.409..619K&link_type=ABSTRACT},
	Volume = {409},
	Year = {2010},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010MNRAS.409..619K&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1111/j.1365-2966.2010.17325.x}}

@article{Keith:2012p7984,
	Abstract = {We present the discovery of six millisecond pulsars (MSPs) in the High Time Resolution Universe (HTRU) survey for pulsars and fast transients carried out with the Parkes radio telescope. All six are in binary systems with approximately circular orbits and are likely to have white dwarf companions. PSR J1017-7156 has a high flux density and a narrow pulse width, making it ideal for precision timing experiments. PSR J1446-4701 and PSR J1125-5825 are coincident with gamma-ray sources, and folding the high-energy photons with the radio timing ephemeris shows evidence of pulsed gamma-ray emission. PSR J1502-6752 has a spin period of 26.7 ms, and its low period derivative implies that it is a recycled pulsar. The orbital parameters indicate it has a very low mass function, and therefore a companion mass much lower than usually expected for such a mildly recycled pulsar. In addition we present polarization profiles for all 12 MSPs discovered in the HTRU survey to date. Similar to previous observations of MSPs, we find that many have large widths and a wide range of linear and circular polarization fractions. Their polarization profiles can be highly complex, and although the observed position angles often do not obey the rotating vector model, we present several examples of those that do. We speculate that the emission heights of MSPs are a substantial fraction of the light cylinder radius in order to explain broad emission profiles, which then naturally leads to a large number of cases where emission from both poles is observed.},
	Affiliation = {AA(Australia Telescope National Facility, CSIRO Astronomy {\&} Space Science, PO Box 76, Epping, NSW 1710, Australia), AB(Australia Telescope National Facility, CSIRO Astronomy {\&} Space Science, PO Box 76, Epping, NSW 1710, Australia), AC(Swinburne University of Technology, Centre for Astrophysics and Supercomputing Mail H39, PO Box 218, VIC 3122, Australia; University of California, Berkeley, 601 Campbell Hall 3411, Berkeley, CA 94720, USA; ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO)), AD(Unive...},
	Annote = {{\copyright} 2011 The Authors Monthly Notices of the Royal Astronomical Society {\copyright} 2011 RAS},
	Author = {M. J Keith and S Johnston and M Bailes and S. D Bates and N. D. R Bhat and M Burgay and S Burke-Spolaor and N D'Amico and A Jameson and M Kramer and L Levin and S Milia and A Possenti and B. W Stappers and W van Straten and D Parent},
	Date-Added = {2012-05-28 16:17:57 +0000},
	Date-Modified = {2012-05-28 16:17:57 +0000},
	Doi = {10.1111/j.1365-2966.2011.19842.x},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Keywords = {pulsars: individual: PSR J1446-4701, pulsars: general, pulsars: individual: PSR J1017-7156, pulsars: individual: PSR J1502-6752},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2012/Keith/Monthly%20Notices%20of%20the%20Royal%20Astronomical%20Society%202012%20Keith.pdf},
	Month = {Jan},
	Pages = {1752},
	Pmid = {2012MNRAS.419.1752K},
	Rating = {0},
	Title = {The High Time Resolution Universe Pulsar Survey - IV. Discovery and polarimetry of millisecond pulsars},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7984},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012MNRAS.419.1752K&link_type=ABSTRACT},
	Volume = {419},
	Year = {2012},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012MNRAS.419.1752K&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1111/j.1365-2966.2011.19842.x}}

@article{Winkel:2012p7953,
	Abstract = {Position and frequency switching techniques used for the removal of the bandpass dependence of radio astronomical spectra are presented and discussed in detail. Both methods are widely used, although the frequency dependence of the system temperature and/or noise diode is often neglected. This leads to systematic errors in the calibration that potentially have a significant impact on scientific results, especially when using large-bandwidth receivers or performing statistical analyses. We present methods to derive an unbiased calibration using a noise diode, which is part of many heterodyne receivers. We compare the proposed methods and describe the advantages and bottlenecks of the various approaches. Monte Carlo simulations are used to qualitatively investigate both systematics and the error distribution of the reconstructed flux estimates about the correct flux values for the new methods but also the 'classical' case. Finally, the determination of the frequency-dependent noise temperature of the calibration diode using hot-cold measurements or observations of well-known continuum sources is also briefly discussed.},
	Annote = {25 pages, 30 figures. Accepted for publication in A{\&}A},
	Author = {B Winkel and A Kraus and U Bach},
	Date-Added = {2012-05-28 16:17:57 +0000},
	Date-Modified = {2012-05-28 16:17:57 +0000},
	Journal = {eprint arXiv},
	Keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2012/Winkel/eprint%20arXiv%202012%20Winkel.pdf},
	Month = {Mar},
	Pages = {741},
	Pmid = {2012arXiv1203.0741W},
	Rating = {0},
	Title = {Unbiased flux calibration methods for spectral-line radio observations},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7953},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012arXiv1203.0741W&link_type=ABSTRACT},
	Volume = {1203},
	Year = {2012},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012arXiv1203.0741W&link_type=ABSTRACT}}

@techreport{minicircuitsAmplifier,
	Author = {Mini-Circuits},
	Date-Added = {2012-05-28 16:17:12 +0000},
	Date-Modified = {2012-05-28 16:17:12 +0000},
	Institution = {MiniCirctuis},
	Title = {ZRL-2150+ Low Noise Amplifier},
	Year = {2009}}

@techreport{minicircuitsBalun2009,
	Author = {Mini-Circuits},
	Date-Added = {2012-05-28 16:17:12 +0000},
	Date-Modified = {2012-05-28 16:17:12 +0000},
	Institution = {MiniCirctuis},
	Title = {ADTL2-18+ RF Transformer},
	Year = {2009}}

@techreport{minicircuitsPowerSplitter2009,
	Author = {Mini-Circuits},
	Date-Added = {2012-05-28 16:17:12 +0000},
	Date-Modified = {2012-05-28 16:17:12 +0000},
	Institution = {MiniCirctuis},
	Title = {ZC16PD-252+ Power Splitter/Combiner},
	Year = {2009}}

@article{Morales:2010p8596,
	Abstract = {Measurement of the spatial distribution of neutral hydrogen via the redshifted 21-cm line promises to revolutionize our knowledge of the epoch of reionization and the first galaxies, and may provide a powerful new tool for observational cosmology from redshifts 1<z<4. In this review we discuss recent advances in our theoretical understanding of the epoch of reionization (EoR), the application of 21-cm tomography to cosmology and measurements of the dark energy equation of state after reionization, and the instrumentation and observational techniques shared by 21-cm EoR and postreionization cosmology machines. We place particular emphasis on the expected signal and observational capabilities of first generation 21-cm fluctuation instruments.},
	Author = {Miguel F Morales and J. Stuart B Wyithe},
	Date-Added = {2012-05-28 16:17:12 +0000},
	Date-Modified = {2012-05-28 16:17:12 +0000},
	Doi = {10.1146/annurev-astro-081309-130936},
	Journal = {Annual Review of Astronomy and Astrophysics},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2010/Morales/Annual%20Review%20of%20Astronomy%20and%20Astrophysics%202010%20Morales.pdf},
	Month = {Sep},
	Pages = {127},
	Pmid = {2010ARA&A..48..127M},
	Rating = {0},
	Title = {Reionization and Cosmology with 21-cm Fluctuations},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p8596},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ARA%2526A..48..127M&link_type=ABSTRACT},
	Volume = {48},
	Year = {2010},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ARA%2526A..48..127M&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1146/annurev-astro-081309-130936}}

@article{Morales:2011p8536,
	Abstract = {Proposed 21 cm cosmology observatories for studying the epoch of reionization (z≈6-15) and dark energy (≈0-6) envision compact arrays with tens of thousands of antenna elements. Fully correlating this many elements is computationally expensive using traditional XF or FX correlators and has led some groups to reconsider direct imaging/FFT correlators. In this article we develop a variation of the direct imaging correlator that we call the MOFF correlator. The MOFF correlator shares the computational advantages of a direct imaging correlator, while avoiding a number of its shortcomings. In particular, the MOFF correlator makes no constraints on the antenna arrangement or type; provides a fully calibrated output image, including wide-field polarimetry and noncoplanar baseline effects; and can be orders of magnitude more efficient than XF or FX correlators for compact radio cosmology arrays.},
	Annote = {(c) year: {\copyright} 2011. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A.},
	Author = {Miguel F Morales},
	Date-Added = {2012-05-28 16:17:12 +0000},
	Date-Modified = {2012-05-28 16:17:12 +0000},
	Doi = {10.1086/663092},
	Journal = {Publications of the Astronomical Society of the Pacific},
	Keywords = {Astronomical Instrumentation},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2011/Morales/Publications%20of%20the%20Astronomical%20Society%20of%20the%20Pacific%202011%20Morales.pdf},
	Month = {Nov},
	Pages = {1265},
	Pmid = {2011PASP..123.1265M},
	Rating = {0},
	Title = {Enabling Next-Generation Dark Energy and Epoch of Reionization Radio Observatories with the MOFF Correlator},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p8536},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011PASP..123.1265M&link_type=ABSTRACT},
	Volume = {123},
	Year = {2011},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011PASP..123.1265M&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1086/663092}}

@article{Miller:2002p3590,
	Abstract = {We examine power spectra from the Abell/ACO rich cluster survey and the Two-Degree Field Galaxy Redshift Survey (2dFGRS) for observational evidence of features produced by the baryons. A nonnegligible baryon fraction produces relatively sharp oscillatory features at specific wavenumbers in the matter power spectrum. However, the mere existence of baryons will also produce a global suppression of the power spectrum. We look for both of these features using the false discovery rate statistic. We show that the window effects on the Abell/ACO power spectrum are minimal, which has allowed for the discovery of discrete oscillatory features in the power spectrum. On the other hand, there are no statistically significant oscillatory features in the 2dFGRS power spectrum, which is expected from the survey's broad window function. After accounting for window effects we apply a scale-independent bias to the 2dFGRS power spectrum, PAbell(k)=b2P2dF(k) and b=3.2. We find that the overall shapes of the Abell/ACO and the biased 2dFGRS power spectra are entirely consistent over the range 0.02<=k<=0.15h Mpc-1. We examine the range of Ωmatter and baryon fraction, for which these surveys could detect significant suppression in power. The reported baryon fractions for both the Abell/ACO and 2dFGRS surveys are high enough to cause a detectable suppression in power (after accounting for errors, windows, and k-space sampling). Using the same technique, we also examine, given the best-fit baryon density obtained from big bang nucleosynthesis, whether it is possible to detect additional suppression due to dark matter-baryon interaction. We find that the limit on dark matter cross section/mass derived from these surveys is the same as those ruled out in a recent study by Chen, Hannestad, {\&} Scherrer.},
	Affiliation = {AA(Department of Physics, Carnegie Mellon University, 5000 Forbes Avenue, Pittsburgh, PA 15232; chrism@cmu.edu, nichol@cmu.edu), AB(Department of Physics, Carnegie Mellon University, 5000 Forbes Avenue, Pittsburgh, PA 15232; chrism@cmu.edu, nichol@cmu.edu), AC(Institute for Theoretical Physics, University of California, Santa Barbara, CA 93106; xuelei@itp.ucsb.edu)},
	Author = {Christopher J Miller and Robert C Nichol and Xuelei Chen},
	Date-Added = {2012-05-28 16:17:03 +0000},
	Date-Modified = {2012-05-28 16:17:03 +0000},
	Doi = {10.1086/342795},
	Journal = {The Astrophysical Journal},
	Keywords = {Galaxies: General, Galaxies: Clusters: General, Methods: Statistical, Cosmology: Cosmological Parameters, Cosmology: Large-Scale Structure of Universe},
	Local-Url = {file://localhost/Volumes/Users/price/Documents/Papers/2002/Miller/The%20Astrophysical%20Journal%202002%20Miller.pdf},
	Month = {Nov},
	Pages = {483},
	Pmid = {2002ApJ...579..483M},
	Rating = {0},
	Title = {Detecting the Baryons in Matter Power Spectra},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p3590},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ApJ...579..483M&link_type=ABSTRACT},
	Volume = {579},
	Year = {2002},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ApJ...579..483M&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1086/342795}}

@article{Carilli:2004p3690,
	Abstract = {The Square Kilometer Array (SKA) represents the next major, and natural, step in radio astronomical facilities, providing two orders of magnitude increase in collecting area over existing telescopes. In a series of meetings, starting in Groningen, the Netherlands (August 2002) and culminating in a `science retreat' in Leiden (November 2003), the SKA International Science Advisory Committee (ISAC), conceived of, and carried-out, a complete revision of the SKA science case (to appear in New Astronomy Reviews). This preface includes: (i) general introductory material, (ii) summaries of the key science programs, and (iii) a detailed listing of standards and assumptions used in the revised science case.},
	Affiliation = {AA(National Radio Astronomy Observatory, P.O. Box O87801, Socorro, NM 87801, USAS.Rawlingss.rawlings1@physics.ox.ac.uk), AB(National Radio Astronomy Observatory, P.O. Box O87801, Socorro, NM 87801, USAS.Rawlingss.rawlings1@physics.ox.ac.uk)},
	Author = {C. L Carilli and S Rawlings},
	Date-Added = {2012-05-28 16:17:03 +0000},
	Date-Modified = {2012-05-28 16:17:03 +0000},
	Doi = {10.1016/j.newar.2004.09.001},
	Journal = {New Astronomy Reviews},
	Local-Url = {file://localhost/Volumes/Users/price/Documents/Papers/2004/Carilli/New%20Astronomy%20Reviews%202004%20Carilli.pdf},
	Month = {Dec},
	Pages = {979},
	Pmid = {2004NewAR..48..979C},
	Rating = {0},
	Title = {Motivation, key science projects, standards and assumptions},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p3690},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004NewAR..48..979C&link_type=ABSTRACT},
	Volume = {48},
	Year = {2004},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004NewAR..48..979C&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.newar.2004.09.001}}

@article{Schlegel:2007p3611,
	Abstract = {The Baryon Oscillation Spectroscopic Survey (BOSS) will map out the baryon acoustic oscillation (BAO) signature with unprecedented accuracy and greatly improve the constraints on the acceleration of the expansion rate of the Universe. BOSS will upgrade the SDSS fiber-fed spectrographs to 1000 fibers, and improve the throughput from 3600 - 10,050 Angstroms. For the five years from 2009-2014, we will map 1.5 million luminous red galaxies (LRGs) at z<0.7 over a footprint of 10,000 square degrees. A simultaneous survey of 160,000 QSOs will map the hydrogen gas in absorption at redshifts 2.3 < z < 3. BOSS will provide the definitive measurement of the low redshift (z<0.7) BAO scale, and it will pioneer a powerful new method of measuring BAO at high redshift with QSOs. This will achieve precise stand-alone constraints on the properties of dark energy, the curvature of space, and the Hubble constant. The absolute distance measurements will reach a precision of 1% at z=0.35, 1% at z=0.6, and 1.5% at z=2.5. As part of the SDSS-III project, BOSS will produce a large, well-calibrated public database to support a broad range of astronomical research.},
	Affiliation = {AA(LBNL), AB(NYU), AC(U Arizona), AD(Apache Point Observatory), AE(Princeton University), AF(Case Western Reserve University), AG(CITA, Canada), AH(University of Portsmouth, United Kingdom), AI(LBNL), AJ(University of Portsmouth, United Kingdom), AK(Drexel University), AL(University of California), AM(LBNL), AN(Penn State University), AO(Penn State University), AP(Princeton University), AQ(Ohio State University), AR(LBNL)},
	Author = {David J Schlegel and M Blanton and D Eisenstein and B Gillespie and J Gunn and P Harding and P McDonald and R Nichol and N Padmanabhan and W Percival and G Richards and C Rockosi and N Roe and N Ross and D Schneider and M Strauss and D Weinberg and M White},
	Date-Added = {2012-05-28 16:17:03 +0000},
	Date-Modified = {2012-05-28 16:17:03 +0000},
	Journal = {American Astronomical Society},
	Month = {Dec},
	Pages = {966},
	Pmid = {2007AAS...21113229S},
	Rating = {0},
	Title = {SDSS-III: The Baryon Oscillation Spectroscopic Survey (BOSS)},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p3611},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007AAS...21113229S&link_type=ABSTRACT},
	Volume = {211},
	Year = {2007},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007AAS...21113229S&link_type=ABSTRACT}}

@article{Meyer:2004p3546,
	Abstract = {The HI Parkes All-Sky Survey (HIPASS) catalogue forms the largest uniform catalogue of HI sources compiled to date, with 4315 sources identified purely by their HI content. The catalogue data comprise the southern region δ < + 2$\,^{\circ}$ of HIPASS, the first blind HI survey to cover the entire southern sky. The rms noise for this survey is 13 mJy beam-1 and the velocity range is -1280 to 12 700 km s-1. Data search, verification and parametrization methods are discussed along with a description of measured quantities. Full catalogue data are made available to the astronomical community including positions, velocities, velocity widths, integrated fluxes and peak flux densities. Also available are on-sky moment maps, position-velocity moment maps and spectra of catalogue sources. A number of local large-scale features are observed in the space distribution of sources, including the super-Galactic plane and the Local Void. Notably, large-scale structure is seen at low Galactic latitudes, a region normally obscured at optical wavelengths.},
	Affiliation = {AA(School of Physics, University of Melbourne, VIC 3010, Australia; Space Telescope Science Institute, 3700 San Martin Drive, Baltimore MD 21218, USA), AB(School of Physics, University of Melbourne, VIC 3010, Australia; European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei M{\"u}nchen, Germany), AC(School of Physics, University of Melbourne, VIC 3010, Australia), AD(Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia), AE(School of Physics, University of M...},
	Author = {M. J Meyer and M. A Zwaan and R. L Webster and L Staveley-Smith and E Ryan-Weber and M. J Drinkwater and D. G Barnes and M Howlett and V. A Kilborn and J Stevens and M Waugh and M. J Pierce and R Bhathal and W. J. G de Blok and M. J Disney and R. D Ekers and K. C Freeman and D. A Garcia and B. K Gibson and J Harnett and P. A Henning and H Jerjen and M. J Kesteven and P. M Knezek and B. S Koribalski and S Mader and M Marquarding and R. F Minchin and J O'Brien and T Oosterloo and R. M Price and M. E Putman and S. D Ryder and E. M Sadler and I. M Stewart and F Stootman and A. E Wright},
	Date-Added = {2012-05-28 16:17:03 +0000},
	Date-Modified = {2012-05-28 16:17:03 +0000},
	Doi = {10.1111/j.1365-2966.2004.07710.x},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Keywords = {catalogues, radio lines: galaxies, methods: observational, Surveys},
	Local-Url = {file://localhost/Volumes/Users/price/Documents/Papers/2004/Meyer/Monthly%20Notices%20of%20the%20Royal%20Astronomical%20Society%202004%20Meyer.pdf},
	Month = {Jun},
	Pages = {1195},
	Pmid = {2004MNRAS.350.1195M},
	Rating = {0},
	Title = {The HIPASS catalogue - I. Data presentation},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p3546},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004MNRAS.350.1195M&link_type=ABSTRACT},
	Volume = {350},
	Year = {2004},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004MNRAS.350.1195M&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1111/j.1365-2966.2004.07710.x}}

@article{Perlmutter:1990p3192,
	Abstract = {Not Available},
	Author = {S Perlmutter and G Goldhaber and H. J Marvin and R. A Muller and C. R Pennypacker and W. J Couch and B. J Boyle},
	Date-Added = {2012-05-28 16:17:03 +0000},
	Date-Modified = {2012-05-28 16:17:03 +0000},
	Journal = {Bulletin of the American Astronomical Society},
	Local-Url = {file://localhost/Volumes/Users/price/Documents/Papers/1990/Perlmutter/Bulletin%20of%20the%20American%20Astronomical%20Society%201990%20Perlmutter.pdf},
	Month = {Sep},
	Pages = {1332},
	Pmid = {1990BAAS...22.1332P},
	Rating = {0},
	Title = {The Program to Measure qo Using Supernovae at Cosmological Distances},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p3192},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990BAAS...22.1332P&link_type=GIF},
	Volume = {22},
	Year = {1990},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990BAAS...22.1332P&link_type=GIF}}

@inproceedings{Ikin2009,
	Author = {T.S. Ikin and P.N. Wilkinson and A.J. Faulkner and M. Jones and A. Baird and A.K. Brown and D. George and G. Harris and P.L. Kibet and M. Panahi and D. Price and H.C. Reader and S. Schediwy and P.S. van der Merwe and K. Zarb-Adami and Y. Zhang},
	Booktitle = {Wide Field Astronomy \& Technology for the Square Kilometre Array},
	Date-Added = {2012-05-28 16:15:53 +0000},
	Date-Modified = {2012-05-28 16:15:53 +0000},
	Editor = {S.A. Torchinsky and A. van Ardenne and T. van den Brink-Havinga and A.J.J. van Es and A.J. Faulkner},
	Pages = {267-272},
	Title = {Progress on Analogue Front end for 2PAD},
	Year = {2009}}

@article{Khlebnikov:2010p5035,
	Abstract = {In this paper, we consider the problem of optimum multi-domain real-time beamforming and high-precision beam pattern positioning in application to very large wideband array antennas, particularly to the Square Kilometre Array (SKA) aperture array antenna. We present a new structure for wideband space-frequency beamforming and beamsteering that maximizes detectability of cosmic signals over the array operational frequency range.},
	Author = {Vasily A Khlebnikov and Kristian Zarb-Adami},
	Date-Added = {2012-05-28 16:15:53 +0000},
	Date-Modified = {2012-05-28 16:15:53 +0000},
	Doi = {10.1109/ARRAY.2010.5613254},
	Journal = {Phased Array Systems and Technology (ARRAY), 2010 IEEE International Symposium on},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2010/Khlebnikov/Phased%20Array%20Systems%20and%20Technology%20(ARRAY)%202010%20IEEE%20International%20Symposium%20on%202010%20Khlebnikov.pdf},
	Pages = {911 -- 916},
	Pmid = {5613254},
	Rating = {0},
	Title = {All-digital wideband space-frequency beamforming for the SKA aperture array},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p5035},
	Url = {http://ieeexplore.ieee.org/search/srchabstract.jsp?tp=&arnumber=5613254&queryText%253D%2528%2528Authors%253Aarmstrong%2529+AND+%2528Publication+Title%253Aarray%2529%2529%2526openedRefinements%253D*%2526sortType%253Ddesc_Publication+Year%2526ranges%253D2010_2010_Publication_Year%2526matchBoolean%253Dtrue%2526rowsPerPage%253D50%2526searchField%253DSearch+All},
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	Bdsk-Url-2 = {http://dx.doi.org/10.1109/ARRAY.2010.5613254}}

@article{Mort:2010p5096,
	Abstract = {Digital beamforming for the aperture array components of the Square Kilometre Array (SKA) poses considerable computational challenges. We propose a hierarchical scheme aimed at tackling them and introduce OSKAR, a beamforming simulator which implements these ideas and algorithms. The simulator continues to be developed to investigate possible designs for the custom devices envisaged for phase 1 of the SKA construction.},
	Author = {Mort},
	Date-Added = {2012-05-28 16:15:53 +0000},
	Date-Modified = {2012-05-28 16:15:53 +0000},
	Doi = {10.1109/ARRAY.2010.5613289},
	Journal = {Phased Array Systems and Technology (ARRAY), 2010 IEEE International Symposium on},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2010/Mort/Phased%20Array%20Systems%20and%20Technology%20(ARRAY)%202010%20IEEE%20International%20Symposium%20on%202010%20Mort.pdf},
	Pages = {690 -- 694},
	Pmid = {5613289},
	Rating = {0},
	Title = {OSKAR: Simulating digital beamforming for the SKA aperture array},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p5096},
	Url = {http://ieeexplore.ieee.org/search/srchabstract.jsp?tp=&arnumber=5613289&queryText%253D%2528%2528Authors%253Amort%2529%2529%2526openedRefinements%253D*%2526sortType%253Ddesc_Publication+Year%2526ranges%253D2010_2010_Publication_Year%2526matchBoolean%253Dtrue%2526rowsPerPage%253D50%2526searchField%253DSearch+All},
	Year = {2010},
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	Bdsk-Url-2 = {http://dx.doi.org/10.1109/ARRAY.2010.5613289}}

@electronic{PointingAccuracy,
	Date-Added = {2012-05-28 16:15:53 +0000},
	Date-Modified = {2012-05-28 16:15:53 +0000},
	Title = {http://www.jb.man.ac.uk/aboutus/lovell/anatomy.html},
	Url = {http://www.jb.man.ac.uk/aboutus/lovell/anatomy.html},
	Year = {2011},
	Bdsk-Url-1 = {http://www.jb.man.ac.uk/aboutus/lovell/anatomy.html}}

@book{Pozar2005,
	Author = {David M. Pozar},
	Date-Added = {2012-05-28 16:15:53 +0000},
	Date-Modified = {2012-06-20 19:53:20 +0000},
	Edition = {3rd},
	Keywords = {Microwave network analysis, scattering parameters},
	Publisher = {John Wiley and Sons Inc.},
	Title = {Microwave Engineering},
	Year = {2005}}

@article{Schediwy:2010p4914,
	Abstract = {We report on our work to quantity the effect of phase errors on the forward gain and pointing offset uncertainty of phased array beams using a combination of simulations, from the aperture array simulator OSKAR, and measurements taken with the aperture array telescope 2-PAD. We demonstrate that for small arrays the limit in phase error is 10$\,^{\circ}$, resulting in a 5% beamwidth pointing offset; while for larger arrays the limiting phase error is 25$\,^{\circ}$, resulting in a 5% reduction in array sensitivity. In addition we argue that a digital beamforming system is advantageous over an analogue beamformer, due to its ability to dynamically calibrate residual phase errors in individual frequency channels, thereby drastically improving the pointing offset uncertainty and the forward gain of phased arrays.},
	Author = {Schediwy},
	Date-Added = {2012-05-28 16:15:53 +0000},
	Date-Modified = {2012-05-28 16:15:53 +0000},
	Doi = {10.1109/ARRAY.2010.5613362},
	Journal = {Phased Array Systems and Technology (ARRAY), 2010 IEEE International Symposium on},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2010/Schediwy/Phased%20Array%20Systems%20and%20Technology%20(ARRAY)%202010%20IEEE%20International%20Symposium%20on%202010%20Schediwy.pdf},
	Pages = {256 -- 260},
	Pmid = {5613362},
	Rating = {0},
	Title = {A quantitative analysis of how phase errors affect the beam quality of phased arrays},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p4914},
	Url = {http://ieeexplore.ieee.org/search/srchabstract.jsp?tp=&arnumber=5613362&queryText%253D%2528%2528Authors%253Aschediwy%2529%2529%2526openedRefinements%253D*%2526sortType%253Ddesc_Publication+Year%2526ranges%253D2010_2010_Publication_Year%2526matchBoolean%253Dtrue%2526rowsPerPage%253D50%2526searchField%253DSearch+All},
	Year = {2010},
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	Bdsk-Url-2 = {http://dx.doi.org/10.1109/ARRAY.2010.5613362}}

@article{Schilizzi2007,
	Author = {R T Schilizzi and P Alexander and J M Cordes and P E Dewdney and R D Ekers and A J Faulkner and B M Gaensler and P J Hall and J L Jonas and K I Kellerman},
	Date-Added = {2012-05-28 16:15:53 +0000},
	Date-Modified = {2012-05-28 16:15:53 +0000},
	Journal = {SKA Memo Series},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2008/Schilizzi/SKA%20Memo%20Series%202008%20Schilizzi.pdf},
	Month = {Sep},
	Pages = {1--74},
	Rating = {0},
	Title = {Preliminary Specifications for the Square Kilometre Array},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p5415},
	Url = {www.skatelescope.org/pages/page_memos.htm},
	Volume = {100},
	Year = {20087},
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@inbook{Skolnik1969,
	Author = {Merrill Skolnik},
	Chapter = {6},
	Date-Added = {2012-05-28 16:15:53 +0000},
	Date-Modified = {2012-05-28 16:15:53 +0000},
	Editor = {Charles Susskind},
	Keywords = {non},
	Pages = {207-234},
	Publisher = {McGraw-Hill Book Company},
	Series = {Inter-University Electronics Series},
	Title = {Antenna Theory Part 1},
	Volume = {7},
	Year = {1969}}

@article{Wolf:1951p7552,
	Abstract = {Page 1. The  diffraction  theory  of  aberrations This article has been downloaded from IOPscience. Please scroll down to see the full text article. 1951 Rep. ... 95 p 1. {\S} 2. {\S} 3. THE  DIFFRACTION THEORY  OF  ABERRATIONS BY E. WOLF* The Observatory, Cambridge University ...},
	Author = {E Wolf},
	Date-Added = {2012-05-28 16:15:53 +0000},
	Date-Modified = {2012-05-28 16:15:53 +0000},
	Journal = {Reports on progress in physics},
	Month = {Jan},
	Pmid = {5784999762723211499related:6wjWSqJySFAJ},
	Rating = {0},
	Title = {The diffraction theory of aberrations},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p7552},
	Url = {http://iopscience.iop.org/0034-4885/14/1/304},
	Year = {1951},
	Bdsk-Url-1 = {http://iopscience.iop.org/0034-4885/14/1/304}}

@article{Ikin:2009p8855,
	Abstract = {Not Available},
	Author = {T. S Ikin and P Wilkinson and A. J Faulkner and M Jones and A Baird and A. K Brown and D George and G Harris and P. L Kibet and M Panahi and D Price and H. C Reader and S Schediwy and P. S van der Merwe and K Zarb Adami and D Zhang},
	Date-Added = {2012-05-27 13:14:16 +0000},
	Date-Modified = {2012-05-27 13:14:16 +0000},
	Journal = {"Proceedings of Wide Field Astronomy {\&} Technology for the Square Kilometre Array (SKADS 2009). 4-6 November 2009. Chateau de Limelette},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2009/Ikin/%22Proceedings%20of%20Wide%20Field%20Astronomy%20&%20Technology%20for%20the%20Square%20Kilometre%20Array%20(SKADS%202009).%204-6%20November%202009.%20Chateau%20de%20Limelette%202009%20Ikin.pdf},
	Month = {Jan},
	Pages = {44},
	Pmid = {2009wska.confE..44I},
	Rating = {0},
	Title = {Progress on Analogue Front end for 2PAD},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p8855},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009wska.confE..44I&link_type=ARTICLE},
	Year = {2009},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009wska.confE..44I&link_type=ARTICLE}}

@article{Price:2009p8869,
	Abstract = {Not Available},
	Author = {D Price and S Schediwy},
	Date-Added = {2012-05-27 13:14:16 +0000},
	Date-Modified = {2012-05-27 13:14:16 +0000},
	Journal = {"Proceedings of Wide Field Astronomy {\&} Technology for the Square Kilometre Array (SKADS 2009). 4-6 November 2009. Chateau de Limelette},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2009/Price/%22Proceedings%20of%20Wide%20Field%20Astronomy%20&%20Technology%20for%20the%20Square%20Kilometre%20Array%20(SKADS%202009).%204-6%20November%202009.%20Chateau%20de%20Limelette%202009%20Price.pdf},
	Month = {Jan},
	Pages = {56},
	Pmid = {2009wska.confE..56P},
	Rating = {0},
	Title = {Database Design for Aperture Array Hardware Management},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p8869},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009wska.confE..56P&link_type=ARTICLE},
	Year = {2009},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009wska.confE..56P&link_type=ARTICLE}}

@article{Schediwy:2009p8881,
	Abstract = {Not Available},
	Author = {S Schediwy and D Price and F Dulwich and B Mort and C Williams},
	Date-Added = {2012-05-27 13:14:16 +0000},
	Date-Modified = {2012-05-27 13:14:16 +0000},
	Journal = {"Proceedings of Wide Field Astronomy {\&} Technology for the Square Kilometre Array (SKADS 2009). 4-6 November 2009. Chateau de Limelette},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2009/Schediwy/%22Proceedings%20of%20Wide%20Field%20Astronomy%20&%20Technology%20for%20the%20Square%20Kilometre%20Array%20(SKADS%202009).%204-6%20November%202009.%20Chateau%20de%20Limelette%202009%20Schediwy.pdf},
	Month = {Jan},
	Pages = {57},
	Pmid = {2009wska.confE..57S},
	Rating = {0},
	Title = {Phase Errors in Phased Arrays: Implications on Forward Gain, Pointing Offset, Calibration, and Beamforming},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p8881},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009wska.confE..57S&link_type=ARTICLE},
	Year = {2009},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009wska.confE..57S&link_type=ARTICLE}}

@misc{PriceSchediwy2009,
	Author = {Danny Price and Sascha Schediwy and Tim Ikin and Mike Jones},
	Date-Added = {2012-05-27 13:07:11 +0000},
	Date-Modified = {2012-05-27 13:09:27 +0000},
	Howpublished = {internal memo},
	Month = {January},
	Title = {The 2-PAD Analogue System: Characterisation, Commissioning, and Implications for Calibration and Beamforming},
	Year = {2010}}

@article{Percival:2010p8749,
	Abstract = {The spectroscopic Sloan Digital Sky Survey (SDSS) Data Release 7 (DR7) galaxy sample represents the final set of galaxies observed using the original SDSS target selection criteria. We analyse the clustering of galaxies within this sample, including both the luminous red galaxy and main samples, and also include the 2-degree Field Galaxy Redshift Survey data. In total, this sample comprises 893319 galaxies over 9100deg2. Baryon acoustic oscillations (BAO) are observed in power spectra measured for different slices in redshift; this allows us to constrain the distance-redshift relation at multiple epochs. We achieve a distance measure at redshift z = 0.275, of rs(zd)/DV(0.275) = 0.1390 +/- 0.0037 (2.7 per cent accuracy), where rs(zd) is the comoving sound horizon at the baryon-drag epoch, DV(z) ≡ [(1 + z)2D2Acz/H(z)]1/3, DA(z) is the angular diameter distance and H(z) is the Hubble parameter. We find an almost independent constraint on the ratio of distances DV(0.35)/DV(0.2) = 1.736 +/- 0.065, which is consistent at the 1.1σ level with the best-fitting Λ cold dark matter model obtained when combining our z = 0.275 distance constraint with the Wilkinson Microwave Anisotropy Probe 5-year (WMAP5) data. The offset is similar to that found in previous analyses of the SDSS DR5 sample, but the discrepancy is now of lower significance, a change caused by a revised error analysis and a change in the methodology adopted, as well as the addition of more data. Using WMAP5 constraints on Ωbh2 and Ωch2, and combining our BAO distance measurements with those from the Union supernova sample, places a tight constraint on Ωm = 0.286 +/- 0.018 and H0 = 68.2 +/- 2.2kms-1Mpc-1 that is robust to allowing Ωk ≠ 0 and w ≠ -1. This result is independent of the behaviour of dark energy at redshifts greater than those probed by the BAO and supernova measurements. Combining these data sets with the full WMAP5 likelihood constraints provides tight constraints on both Ωk = -0.006 +/- 0.008 and w = -0.97 +/- 0.10 for a constant dark energy equation of state.},
	Affiliation = {AA(Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama building, Portsmouth P01 3FX), AB(Institute of Space Sciences (CSIC-IEEC), UAB, Barcelona 08193, Spain; Institute for Sciences of the Cosmos (ICC), University of Barcelona, Barcelona 08028, Spain; Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USA), AC(Steward Observatory, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85121, USA), AD(Department of Astrophysical Sciences, Princeton Uni...},
	Author = {Will J Percival and Beth A Reid and Daniel J Eisenstein and Neta A Bahcall and Tamas Budavari and Joshua A Frieman and Masataka Fukugita and James E Gunn and {\v Z}eljko Ivezi{\'c} and Gillian R Knapp and Richard G Kron and Jon Loveday and Robert H Lupton and Timothy A McKay and Avery Meiksin and Robert C Nichol and Adrian C Pope and David J Schlegel and Donald P Schneider and David N Spergel and Chris Stoughton and Michael A Strauss and Alexander S Szalay and Max Tegmark and Michael S Vogeley and David H Weinberg and Donald G York and Idit Zehavi},
	Date-Added = {2012-05-26 12:18:38 +0000},
	Date-Modified = {2012-05-26 12:18:38 +0000},
	Doi = {10.1111/j.1365-2966.2009.15812.x},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Keywords = {large-scale structure of Universe, cosmology: observations, distance scale},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2010/Percival/Monthly%20Notices%20of%20the%20Royal%20Astronomical%20Society%202010%20Percival.pdf},
	Month = {Feb},
	Pages = {2148},
	Pmid = {2010MNRAS.401.2148P},
	Rating = {0},
	Title = {Baryon acoustic oscillations in the Sloan Digital Sky Survey Data Release 7 galaxy sample},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p8749},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010MNRAS.401.2148P&link_type=ABSTRACT},
	Volume = {401},
	Year = {2010},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010MNRAS.401.2148P&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1111/j.1365-2966.2009.15812.x}}

@article{Carilli:2004p8674,
	Abstract = {The epoch of reionization (EoR) sets a fundamental benchmark in cosmic structure formation, corresponding to the formation of the first luminous objects that act to ionize the neutral intergalactic medium (IGM). Recent observations at near-IR and radio wavelengths imply that we are finally probing into this key epoch of galaxy formation at z ⩾ 6. The Square Kilometer Array (SKA) will provide critical insight into the EoR, in a number of ways. First, the ability of the SKA to image the neutral IGM in 21-cm emission is a truly unique probe of the process of reionization, and is recognized as the next necessary and fundamental step in our study of the evolution of large scale structure and cosmic reionization. Second, study of HI 21-cm absorption toward the first radio loud objects probes small to intermediate scale structure in the neutral `cosmic web', as well as HI in the first collapsed structures (proto-disks and mini-halos). And third, the incomparable sensitivity of the SKA allows for the study of the molecular gas, dust, and star formation activity in the first galaxies, as well as the radio continuum emission from the first accreting massive black holes. Such objects will be obscured at optical wavelengths due to absorption by the neutral IGM.},
	Affiliation = {AA(National Radio Astronomy Observatory, Socorro, NM 87801, USA), AB(Caltech, Pasadena, CA, USA), AC(Australia Telescope National Facility, Sydney, Australia), AD(Astrophysics, Department of Physics, Keble Road, Oxford OX1 3RH, UK), AE(Astrophysics, Department of Physics, Keble Road, Oxford OX1 3RH, UK), AF(ASTRON, P.O. Box 2, 7990 AA Dwingeloo, The Netherlands)},
	Author = {C. L Carilli and S Furlanetto and F Briggs and M Jarvis and S Rawlings and H Falcke},
	Date-Added = {2012-05-26 11:02:37 +0000},
	Date-Modified = {2012-05-26 11:02:37 +0000},
	Doi = {10.1016/j.newar.2004.09.046},
	Journal = {New Astronomy Reviews},
	Local-Url = {file://localhost/Users/danny/Documents/Papers/2004/Carilli/New%20Astronomy%20Reviews%202004%20Carilli-1.pdf},
	Month = {Dec},
	Pages = {1029},
	Pmid = {2004NewAR..48.1029C},
	Rating = {0},
	Read = {Yes},
	Title = {Probing the dark ages with the Square Kilometer Array},
	Uri = {papers://854398C7-5EA2-48B7-9B84-E12F480BF696/Paper/p8674},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004NewAR..48.1029C&link_type=ABSTRACT},
	Volume = {48},
	Year = {2004},
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	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004NewAR..48.1029C&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.newar.2004.09.046}}

@article{skaSiteDecision,
	Author = {Geoff Brumfiel},
	Date-Added = {2012-05-25 14:34:50 +0000},
	Date-Modified = {2012-05-25 14:34:50 +0000},
	Journal = {Nature},
	Month = {May},
	Title = {Nations to split telescope project},
	Year = {2012}}

@unpublished{Schediwy2010,
	Author = {Sascha Schediwy},
	Date-Added = {2010-06-03 14:04:07 +0100},
	Date-Modified = {2010-06-03 14:04:39 +0100},
	Month = {February 2010},
	Note = {ARC Research Proposal},
	Title = {SANDGROPER ARC Proposal},
	Year = {2010}}

@article{Carozzi:2009hf,
	Author = {Carozzi, T D and Woan, G},
	Journal = {MNRAS},
	Month = may,
	Number = {3},
	Pages = {1558--1568},
	Title = {{A generalized measurement equation and van Cittert-Zernike theorem for wide-field radio astronomical interferometry}},
	Volume = {395},
	Year = {2009}}

@techreport{JEN:note185,
	Author = {{Noordam}, J.~E.},
	Date-Modified = {2014-11-04 17:49:41 +0000},
	Institution = {AIPS++},
	Series = {AIPS++ Notes Series},
	Title = {{AIPS++ Note 185}},
	Url = http://aips2.nrao.edu/docs/notes/185/185.html,
	Year = 1996,
	Bdsk-Url-1 = {http://aips2.nrao.edu/docs/notes/185/185.html}}

@article{Lyutikov2005,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2005MNRAS.360..869L},
	Author = {{Lyutikov}, M. and {Pariev}, V.~I. and {Gabuzda}, D.~C.},
	Doi = {10.1111/j.1365-2966.2005.08954.x},
	Eprint = {astro-ph/0406144},
	Journal = {MNRAS},
	Keywords = {MHD, radiation mechanisms: non-thermal, galaxies: active, galaxies: jets, galaxies: nuclei},
	Month = jul,
	Pages = {869-891},
	Title = {{Polarization and structure of relativistic parsec-scale AGN jets}},
	Volume = 360,
	Year = 2005,
	Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2005.08954.x}}

@article{Sparks1992,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1992Natur.355..804S},
	Author = {{Sparks}, W.~B. and {Fraix-Burnet}, D. and {Macchetto}, F. and {Owen}, F.~N.},
	Doi = {10.1038/355804a0},
	Journal = {Nature},
	Keywords = {Elliptical Galaxies, Radio Galaxies, Radio Jets (Astronomy), Synchrotron Radiation, Astronomical Observatories, Charge Coupled Devices},
	Month = feb,
	Pages = {804-806},
	Title = {{A counterjet in the elliptical galaxy M87}},
	Volume = 355,
	Year = 1992,
	Bdsk-Url-1 = {http://dx.doi.org/10.1038/355804a0}}

@techreport{Sault-AT-Calibration,
	Author = {Sault, R.J. and Killeen, N.E.B.K. and Kesteven, M.J.},
	Date-Modified = {2014-11-04 17:54:32 +0000},
	Institution = {ATNF},
	Number = {39.3/015},
	Series = {ATNF Technical Document Series},
	Title = {{AT polarisation calibration}},
	Url = {http://www.atnf.csiro.au/observers/memos/},
	Year = {1991},
	Bdsk-Url-1 = {http://www.atnf.csiro.au/observers/memos/}}