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%% This BibTeX bibliography file was created using BibDesk.
%% http://bibdesk.sourceforge.net/
%% Created for Adam Beardsley at 2015-10-15 13:24:42 -0700
%% Saved with string encoding Unicode (UTF-8)
@inproceedings{ban14,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2014SPIE.9145E..22B},
Archiveprefix = {arXiv},
Author = {{Bandura}, K. and {Addison}, G.~E. and {Amiri}, M. and {Bond}, J.~R. and {Campbell-Wilson}, D. and {Connor}, L. and {Cliche}, J.-F. and {Davis}, G. and {Deng}, M. and {Denman}, N. and {Dobbs}, M. and {Fandino}, M. and {Gibbs}, K. and {Gilbert}, A. and {Halpern}, M. and {Hanna}, D. and {Hincks}, A.~D. and {Hinshaw}, G. and {H{\"o}fer}, C. and {Klages}, P. and {Landecker}, T.~L. and {Masui}, K. and {Mena Parra}, J. and {Newburgh}, L.~B. and {Pen}, U.-l. and {Peterson}, J.~B. and {Recnik}, A. and {Shaw}, J.~R. and {Sigurdson}, K. and {Sitwell}, M. and {Smecher}, G. and {Smegal}, R. and {Vanderlinde}, K. and {Wiebe}, D.},
Booktitle = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
Date-Added = {2015-10-15 17:14:21 +0000},
Date-Modified = {2015-10-15 17:14:26 +0000},
Doi = {10.1117/12.2054950},
Eid = {914522},
Eprint = {1406.2288},
Month = jul,
Pages = {22},
Primaryclass = {astro-ph.IM},
Series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
Title = {{Canadian Hydrogen Intensity Mapping Experiment (CHIME) pathfinder}},
Volume = 9145,
Year = 2014,
Bdsk-Url-1 = {http://dx.doi.org/10.1117/12.2054950}}
@article{bha08,
Author = {{Bhatnagar, S.} and {Cornwell, T. J.} and {Golap, K.} and {Uson, J. M.}},
Date-Added = {2015-10-15 20:24:36 +0000},
Date-Modified = {2015-10-15 20:24:41 +0000},
Doi = {10.1051/0004-6361:20079284},
Encoding = {tex},
Journal = {A\&A},
Number = 1,
Pages = {419-429},
Title = {Correcting direction-dependent gains in the deconvolution of radio interferometric images},
Url = {http://dx.doi.org/10.1051/0004-6361:20079284},
Volume = 487,
Year = 2008,
Bdsk-Url-1 = {http://dx.doi.org/10.1051/0004-6361:20079284}}
@article{bun04,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2004ExA....17..251B},
Author = {{Bunton}, J.~D.},
Date-Added = {2015-10-15 15:37:41 +0000},
Date-Modified = {2015-10-15 15:37:45 +0000},
Doi = {10.1007/s10686-005-5661-5},
Journal = {Experimental Astronomy},
Keywords = {correlator, FX, XF, filterbank, radio astronomy, SKA},
Month = jun,
Pages = {251-259},
Title = {{Ska Correlator Advances}},
Volume = 17,
Year = 2004,
Bdsk-Url-1 = {http://dx.doi.org/10.1007/s10686-005-5661-5}}
@article{dai00,
Abstract = {An 8 X 8 equals 64 element digital interferometer was developed at Waseda University (1989 - 1995). It was an equally spaced two dimensional array of 2.4 m dishes at 10.6 GHz, and a 2D FFT processor was used for Nyquist rate imaging. Recently a spatial-temporal (2 + 1)D FFT processor has been developed for pulsar survey (1996 - 2000), in which a first 2D spatial FFT transforms the electric fields of coordinate represented to those of momentum represented. We obtain the electric fields in each 64 direction at Nyquist rate by the 2D spatial Fourier transform. The following temporal 1D FFT gives the spectrum of 64ch or 256ch to 64 directions respectively also at Nyquist rate. The total bandwidths of each direction are 20 MHz and the resulting frequency resolutions are 20/64 MHz or 20/256 MHz. For sensitive pulsar survey, we also have developed an interferometric array of 20 m spherical dishes in Nasu flat, 160 km north of Tokyo. Five dishes are completed at present. Normal temperature receivers of high electron mobility transistors (HEMT) are used at 1.4 GHz observation and the receiver noise temperatures are below 40 K. Expected rms detection limit (Delta) T is about 10-2K under the condition of 20 MHz band widths and 1s integration time. Preliminary results of zenith survey at (delta) equals 40 deg using a single dish show (Delta) T equals 0.03 K without switching. Sub-reflectors and feed horns were designed so as to observe 5 deg off directions from zenith and they rotate around Az axis. It enable us to survey the declination zone of 32 <EQ (delta) <EQ 42 deg.},
Author = {Daishido, Tsuneaki and Tanaka, Naoki and Takeuchi, Hiroshi and Akamine, Yukinori and Fujii, Fumiyuki and Kuniyoshi, Masaya and Suemitsu, Taisei and Gotoh, Kentaro and Mizuki, Saori and Mizuno, Keiju and Suzuki, Tomoya and Asuma, Kuniyuki},
Date-Added = {2015-10-15 20:00:21 +0000},
Date-Modified = {2015-10-15 20:00:26 +0000},
Doi = {10.1117/12.390458},
Journal = {Proc. SPIE},
Pages = {73-85},
Title = {Pulsar huge array with Nyquist-rate digital lens and prism},
Url = {http://dx.doi.org/10.1117/12.390458},
Volume = {4015},
Year = {2000},
Bdsk-Url-1 = {http://dx.doi.org/10.1117/12.390458}}
@article{del07,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2007PASP..119..318D},
Author = {{Deller}, A.~T. and {Tingay}, S.~J. and {Bailes}, M. and {West}, C.},
Doi = {10.1086/513572},
Eprint = {astro-ph/0702141},
Journal = {\pasp},
Keywords = {Techniques: Interferometric, Instrumentation: Interferometers, Stars: Pulsars: General, Radio Continuum: General, Radio Lines: General},
Month = mar,
Pages = {318-336},
Title = {{DiFX: A Software Correlator for Very Long Baseline Interferometry Using Multiprocessor Computing Environments}},
Volume = 119,
Year = 2007,
Bdsk-Url-1 = {http://dx.doi.org/10.1086/513572}}
@article{dev09,
Author = {de Vos, M. and Gunst, A.W. and Nijboer, R.},
Date-Added = {2015-10-15 17:11:19 +0000},
Date-Modified = {2015-10-15 17:11:25 +0000},
Doi = {10.1109/JPROC.2009.2020509},
Issn = {0018-9219},
Journal = {Proceedings of the IEEE},
Keywords = {antenna phased arrays;aperture antennas;array signal processing;directive antennas;radiotelescopes;LOFAR telescope;aperture synthesis array;distributed radio telescope;flexible station-based signal processing;low frequency array;omnidirectional antennas;phased array antenna;software correlator;square kilometer array;system architecture;tied array beamformer;Antenna arrays;Aperture antennas;Array signal processing;Calibration;Frequency synthesizers;Phased arrays;Radio astronomy;Signal processing;Signal synthesis;Telescopes;Aperture synthesis;low-frequency astronomy;multibeaming;phased array;radio astronomy},
Month = {Aug},
Number = {8},
Pages = {1431-1437},
Title = {The LOFAR Telescope: System Architecture and Signal Processing},
Volume = {97},
Year = {2009},
Bdsk-Url-1 = {http://dx.doi.org/10.1109/JPROC.2009.2020509}}
@article{ell13,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2013ITAP...61.2540E},
Archiveprefix = {arXiv},
Author = {{Ellingson}, S.~W. and {Taylor}, G.~B. and {Craig}, J. and {Hartman}, J. and {Dowell}, J. and {Wolfe}, C.~N. and {Clarke}, T.~E. and {Hicks}, B.~C. and {Kassim}, N.~E. and {Ray}, P.~S. and {Rickard}, L.~J. and {Schinzel}, F.~K. and {Weiler}, K.~W.},
Date-Added = {2015-10-15 17:17:57 +0000},
Date-Modified = {2015-10-15 17:18:01 +0000},
Doi = {10.1109/TAP.2013.2242826},
Eprint = {1204.4816},
Journal = {IEEE Transactions on Antennas and Propagation},
Month = may,
Pages = {2540-2549},
Primaryclass = {astro-ph.IM},
Title = {{The LWA1 Radio Telescope}},
Volume = 61,
Year = 2013,
Bdsk-Url-1 = {http://dx.doi.org/10.1109/TAP.2013.2242826}}
@article{fos14,
Abstract = {A new digital backend has been developed for the Basic Element for SKA Training II (BEST-2) array at Radiotelescopi di Medicina, INAF-IRA, Italy, which allows concurrent operation of an FX correlator, and a direct-imaging correlator and beamformer. This backend serves as a platform for testing some of the spatial Fourier transform concepts which have been proposed for use in computing correlations on regularly gridded arrays. While spatial Fourier transform-based beamformers have been implemented previously, this is, to our knowledge, the first time a direct-imaging correlator has been deployed on a radio astronomy array. Concurrent observations with the FX and direct-imaging correlator allow for direct comparison between the two architectures. Additionally, we show the potential of the direct-imaging correlator for time-domain astronomy, by passing a subset of beams though a pulsar and transient detection pipeline. These results provide a timely verification for spatial Fourier transform-based instruments that are currently in commissioning. These instruments aim to detect highly redshifted hydrogen from the epoch of reionization and/or to perform wide-field surveys for time-domain studies of the radio sky. We experimentally show the direct-imaging correlator architecture to be a viable solution for correlation and beamforming.},
Author = {Foster, G. and Hickish, J. and Magro, A. and Price, D. and Zarb Adami, K.},
Date-Added = {2015-10-15 20:01:32 +0000},
Date-Modified = {2015-10-15 20:01:37 +0000},
Doi = {10.1093/mnras/stu188},
Eprint = {http://mnras.oxfordjournals.org/content/439/3/3180.full.pdf+html},
Journal = {Monthly Notices of the Royal Astronomical Society},
Number = {3},
Pages = {3180-3188},
Title = {Implementation of a direct-imaging and FX correlator for the BEST-2 array},
Url = {http://mnras.oxfordjournals.org/content/439/3/3180.abstract},
Volume = {439},
Year = {2014},
Bdsk-Url-1 = {http://mnras.oxfordjournals.org/content/439/3/3180.abstract},
Bdsk-Url-2 = {http://dx.doi.org/10.1093/mnras/stu188}}
@inproceedings{lon00,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2000SPIE.4015..126L},
Author = {{Lonsdale}, C.~J. and {Doeleman}, S.~S. and {Cappallo}, R.~J. and {Hewitt}, J.~N. and {Whitney}, A.~R.},
Booktitle = {Radio Telescopes},
Date-Added = {2015-10-15 15:33:15 +0000},
Date-Modified = {2015-10-15 15:33:29 +0000},
Editor = {{Butcher}, H.~R.},
Month = jul,
Pages = {126-134},
Series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
Title = {{Exploring the performance of large-N radio astronomical arrays}},
Volume = 4015,
Year = 2000}
@ARTICLE{man99,
author = {{Maneewongvatana}, S. and {Mount}, D.~M.},
title = "{Analysis of approximate nearest neighbor searching with clustered point sets}",
journal = {eprint arXiv:cs/9901013},
eprint = {cs/9901013},
keywords = {Computer Science - Computational Geometry, E.1, F.2.2},
year = 1999,
month = jan,
adsurl = {http://adsabs.harvard.edu/abs/1999cs........1013M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{mel13,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2013ExA....36..235M},
Archiveprefix = {arXiv},
Author = {{Mellema}, G. and {Koopmans}, L.~V.~E. and {Abdalla}, F.~A. and {Bernardi}, G. and {Ciardi}, B. and {Daiboo}, S. and {de Bruyn}, A.~G. and {Datta}, K.~K. and {Falcke}, H. and {Ferrara}, A. and {Iliev}, I.~T. and {Iocco}, F. and {Jeli{\'c}}, V. and {Jensen}, H. and {Joseph}, R. and {Labroupoulos}, P. and {Meiksin}, A. and {Mesinger}, A. and {Offringa}, A.~R. and {Pandey}, V.~N. and {Pritchard}, J.~R. and {Santos}, M.~G. and {Schwarz}, D.~J. and {Semelin}, B. and {Vedantham}, H. and {Yatawatta}, S. and {Zaroubi}, S.},
Date-Added = {2015-10-15 19:47:14 +0000},
Date-Modified = {2015-10-15 19:47:23 +0000},
Doi = {10.1007/s10686-013-9334-5},
Eprint = {1210.0197},
Journal = {Experimental Astronomy},
Keywords = {Cosmology: Observations, Dark ages, Reionization, First stars, Diffuse radiation, Intergalactic medium, Radio lines: General, Techniques: Interferometric},
Month = aug,
Pages = {235-318},
Title = {{Reionization and the Cosmic Dawn with the Square Kilometre Array}},
Volume = 36,
Year = 2013,
Bdsk-Url-1 = {http://dx.doi.org/10.1007/s10686-013-9334-5}}
@article{mor09,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2009MNRAS.400.1814M},
Archiveprefix = {arXiv},
Author = {{Morales}, M.~F. and {Matejek}, M.},
Doi = {10.1111/j.1365-2966.2009.15537.x},
Eprint = {0810.5107},
Journal = {\mnras},
Keywords = {instrumentation: interferometers , techniques: interferometric , cosmology: miscellaneous},
Month = dec,
Pages = {1814-1820},
Title = {{Software holography: interferometric data analysis for the challenges of next generation observatories}},
Volume = 400,
Year = 2009,
Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2009.15537.x}}
@article{mor11,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2011PASP..123.1265M},
Archiveprefix = {arXiv},
Author = {{Morales}, M.~F.},
Doi = {10.1086/663092},
Eprint = {0812.3669},
Journal = {\pasp},
Keywords = {Astronomical Instrumentation},
Month = nov,
Pages = {1265-1272},
Title = {{Enabling Next-Generation Dark Energy and Epoch of Reionization Radio Observatories with the MOFF Correlator}},
Volume = 123,
Year = 2011,
Bdsk-Url-1 = {http://dx.doi.org/10.1086/663092}}
@article{oto94,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/1994PASJ...46..503O},
Author = {{Otobe}, E. and {Nakajima}, J. and {Nishibori}, K. and {Saito}, T. and {Kobayashi}, H. and {Tanaka}, N. and {Watanabe}, N. and {Aramaki}, Y. and {Hoshikawa}, T. and {Asuma}, K. and {Daishido}, T.},
Date-Added = {2015-10-15 20:11:55 +0000},
Date-Modified = {2015-10-15 20:12:00 +0000},
Journal = {\pasj},
Keywords = {Calibrating, Crab Nebula, Error Analysis, Fast Fourier Transformations, Image Processing, Imaging Techniques, Radio Astronomy, Radio Emission, Instrument Errors, Phase Error, Pulsars, Radio Interferometers},
Month = oct,
Pages = {503-510},
Title = {{Two-dimensional direct images with a spatial FFT interferometer}},
Volume = 46,
Year = 1994}
@article{par10,
Abstract = {We are developing the Precision Array for Probing the Epoch of Re-ionization (PAPER) to detect 21 cm emission from the early universe, when the first stars and galaxies were forming. We describe the overall experiment strategy and architecture and summarize two PAPER deployments: a four-antenna array in the low radio frequency interference (RFI) environment of Western Australia and an eight-antenna array at a prototyping site at the NRAO facilities near Green Bank, WV. From these activities we report on system performance, including primary beam model verification, dependence of system gain on ambient temperature, measurements of receiver and overall system temperatures, and characterization of the RFI environment at each deployment site. We present an all-sky map synthesized between 139 MHz and 174 MHz using data from both arrays that reaches down to 80 mJy (4.9 K, for a beam size of 2.15e--5 sr at 156 MHz), with a 10 mJy (620 mK) thermal noise level that indicates what would be achievable with better foreground subtraction. We calculate angular power spectra ( C ℓ ) in a cold patch and determine them to be dominated by point sources, but with contributions from galactic synchrotron emission at lower radio frequencies and angular wavemodes. Although the sample variance of foregrounds dominates errors in these power spectra, we measure a thermal noise level of 310 mK at ℓ = 100 for a 1.46 MHz band centered at 164.5 MHz. This sensitivity level is approximately 3 orders of magnitude in temperature above the level of the fluctuations in 21 cm emission associated with re-ionization.},
Author = {Aaron R. Parsons and Donald C. Backer and Griffin S. Foster and Melvyn C. H. Wright and Richard F. Bradley and Nicole E. Gugliucci and Chaitali R. Parashare and Erin E. Benoit and James E. Aguirre and Daniel C. Jacobs and Chris L. Carilli and David Herne and Mervyn J. Lynch and Jason R. Manley and Daniel J. Werthimer},
Date-Added = {2015-10-15 17:08:47 +0000},
Date-Modified = {2015-10-15 17:08:51 +0000},
Journal = {The Astronomical Journal},
Number = {4},
Pages = {1468},
Title = {The Precision Array for Probing the Epoch of Re-ionization: Eight Station Results},
Url = {http://stacks.iop.org/1538-3881/139/i=4/a=1468},
Volume = {139},
Year = {2010},
Bdsk-Url-1 = {http://stacks.iop.org/1538-3881/139/i=4/a=1468}}
@article{pob14,
Abstract = {A number of experiments are currently working toward a measurement of the 21 cm signal from the epoch of reionization (EoR). Whether or not these experiments deliver a detection of cosmological emission, their limited sensitivity will prevent them from providing detailed information about the astrophysics of reionization. In this work, we consider what types of measurements will be enabled by the next generation of larger 21 cm EoR telescopes. To calculate the type of constraints that will be possible with such arrays, we use simple models for the instrument, foreground emission, and the reionization history. We focus primarily on an instrument modeled after the ~0.1 km 2 collecting area Hydrogen Epoch of Reionization Array concept design and parameterize the uncertainties with regard to foreground emission by considering different limits to the recently described "wedge" footprint in k space. Uncertainties in the reionization history are accounted for using a series of simulations that vary the ionizing efficiency and minimum virial temperature of the galaxies responsible for reionization, as well as the mean free path of ionizing photons through the intergalactic medium. Given various combinations of models, we consider the significance of the possible power spectrum detections, the ability to trace the power spectrum evolution versus redshift, the detectability of salient power spectrum features, and the achievable level of quantitative constraints on astrophysical parameters. Ultimately, we find that 0.1 km 2 of collecting area is enough to ensure a very high significance ( ##IMG## [http://ej.iop.org/icons/Entities/gsim.gif] {gsim} 30σ) detection of the reionization power spectrum in even the most pessimistic scenarios. This sensitivity should allow for meaningful constraints on the reionization history and astrophysical parameters, especially if foreground subtraction techniques can be improved and successfully implemented.},
Author = {Jonathan C. Pober and Adrian Liu and Joshua S. Dillon and James E. Aguirre and Judd D. Bowman and Richard F. Bradley and Chris L. Carilli and David R. DeBoer and Jacqueline N. Hewitt and Daniel C. Jacobs and Matthew McQuinn and Miguel F. Morales and Aaron R. Parsons and Max Tegmark and Dan J. Werthimer},
Date-Added = {2015-10-15 17:09:09 +0000},
Date-Modified = {2015-10-15 17:09:14 +0000},
Journal = {The Astrophysical Journal},
Number = {2},
Pages = {66},
Title = {What Next-generation 21 cm Power Spectrum Measurements can Teach us About the Epoch of Reionization},
Url = {http://stacks.iop.org/0004-637X/782/i=2/a=66},
Volume = {782},
Year = {2014},
Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/782/i=2/a=66}}
@ARTICLE{teg97a,
author = {{Tegmark}, M.},
title = "{How to Make Maps from Cosmic Microwave Background Data without Losing Information}",
journal = {\apjl},
eprint = {astro-ph/9611130},
keywords = {COSMOLOGY: COSMIC MICROWAVE BACKGROUND, METHODS: DATA ANALYSIS, Cosmology: Cosmic Microwave Background, Methods: Data Analysis},
year = 1997,
month = may,
volume = 480,
pages = {L87-L90},
doi = {10.1086/310631},
adsurl = {http://adsabs.harvard.edu/abs/1997ApJ...480L..87T},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{teg97b,
Author = {Tegmark, M.},
Date-Added = {2015-10-15 20:20:26 +0000},
Date-Modified = {2015-10-15 20:20:31 +0000},
Doi = {10.1103/PhysRevD.55.5895},
Journal = {Phys. Rev. D},
Month = {May},
Number = {10},
Numpages = {12},
Pages = {5895--5907},
Publisher = {American Physical Society},
Title = {How to measure CMB power spectra without losing information},
Volume = {55},
Year = {1997},
Bdsk-Url-1 = {http://dx.doi.org/10.1103/PhysRevD.55.5895}}
@article{teg09,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2009PhRvD..79h3530T},
Archiveprefix = {arXiv},
Author = {{Tegmark}, M. and {Zaldarriaga}, M.},
Date-Added = {2015-10-15 15:40:01 +0000},
Date-Modified = {2015-10-15 15:40:05 +0000},
Doi = {10.1103/PhysRevD.79.083530},
Eid = {083530},
Eprint = {0805.4414},
Journal = {\prd},
Keywords = {Observational cosmology},
Month = apr,
Number = 8,
Pages = {083530},
Title = {{Fast Fourier transform telescope}},
Volume = 79,
Year = 2009,
Bdsk-Url-1 = {http://dx.doi.org/10.1103/PhysRevD.79.083530}}
@article{teg10,
Author = {Tegmark, Max and Zaldarriaga, Matias},
Date-Added = {2015-10-15 16:29:18 +0000},
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Adsurl = {http://adsabs.harvard.edu/abs/2014MNRAS.445.1084Z},
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