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%% This BibTeX bibliography file was created using BibDesk.
%% http://bibdesk.sourceforge.net/
%% Created for Adam Beardsley at 2016-03-07 08:23:55 -0700
%% Saved with string encoding Unicode (UTF-8)
@techreport{jac15,
Author = {{Jacobs}, D.~C. and {Beardsley}, A.~P. and {Hazelton}, B.~J. and {Thyagarajan}, N. and {Trott}, C.},
Date-Added = {2016-03-07 15:22:16 +0000},
Date-Modified = {2016-03-07 15:23:54 +0000},
Number = {10},
Title = {{System Temperatures of 21cm Arrays}},
Type = {HERA Memo},
Year = {2015}}
@article{abb16b,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2016arXiv160208492A},
Archiveprefix = {arXiv},
Author = {{Abbott}, B.~P. and {Abbott}, R. and {Abbott}, T.~D. and {Abernathy}, M.~R. and {Acernese}, F. and {Ackley}, K. and {Adams}, C. and {Adams}, T. and {Addesso}, P. and {Adhikari}, R.~X. and et al.},
Date-Added = {2016-03-02 18:24:52 +0000},
Date-Modified = {2016-03-02 18:24:57 +0000},
Eprint = {1602.08492},
Journal = {ArXiv e-prints},
Keywords = {Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology},
Month = feb,
Primaryclass = {astro-ph.HE},
Title = {{Localization and broadband follow-up of the gravitational-wave transient GW150914}},
Year = 2016}
@article{lor07,
Abstract = {Pulsar surveys offer a rare opportunity to monitor the radio sky for impulsive burst-like events with millisecond durations. We analyzed archival survey data and found a 30-jansky dispersed burst, less than 5 milliseconds in duration, located 3{\textdegree} from the Small Magellanic Cloud. The burst properties argue against a physical association with our Galaxy or the Small Magellanic Cloud. Current models for the free electron content in the universe imply that the burst is less than 1 gigaparsec distant. No further bursts were seen in 90 hours of additional observations, which implies that it was a singular event such as a supernova or coalescence of relativistic objects. Hundreds of similar events could occur every day and, if detected, could serve as cosmological probes.},
Author = {Lorimer, D. R. and Bailes, M. and McLaughlin, M. A. and Narkevic, D. J. and Crawford, F.},
Date-Added = {2016-02-29 16:30:42 +0000},
Date-Modified = {2016-02-29 16:30:46 +0000},
Doi = {10.1126/science.1147532},
Eprint = {http://science.sciencemag.org/content/318/5851/777.full.pdf},
Issn = {0036-8075},
Journal = {Science},
Number = {5851},
Pages = {777--780},
Publisher = {American Association for the Advancement of Science},
Title = {A Bright Millisecond Radio Burst of Extragalactic Origin},
Url = {http://science.sciencemag.org/content/318/5851/777},
Volume = {318},
Year = {2007},
Bdsk-Url-1 = {http://science.sciencemag.org/content/318/5851/777},
Bdsk-Url-2 = {http://dx.doi.org/10.1126/science.1147532}}
@article{abb16a,
Author = {Abbott, B. P. and Abbott, R. and Abbott, T. D. and Abernathy, M. R. and Acernese, F. and Ackley, K. and Adams, C. and Adams, T. and Addesso, P. and Adhikari, R. X. and Adya, V. B. and Affeldt, C. and Agathos, M. and Agatsuma, K. and Aggarwal, N. and Aguiar, O. D. and Aiello, L. and Ain, A. and Ajith, P. and Allen, B. and Allocca, A. and Altin, P. A. and Anderson, S. B. and Anderson, W. G. and Arai, K. and Arain, M. A. and Araya, M. C. and Arceneaux, C. C. and Areeda, J. S. and Arnaud, N. and Arun, K. G. and Ascenzi, S. and Ashton, G. and Ast, M. and Aston, S. M. and Astone, P. and Aufmuth, P. and Aulbert, C. and Babak, S. and Bacon, P. and Bader, M. K. M. and Baker, P. T. and Baldaccini, F. and Ballardin, G. and Ballmer, S. W. and Barayoga, J. C. and Barclay, S. E. and Barish, B. C. and Barker, D. and Barone, F. and Barr, B. and Barsotti, L. and Barsuglia, M. and Barta, D. and Bartlett, J. and Barton, M. A. and Bartos, I. and Bassiri, R. and Basti, A. and Batch, J. C. and Baune, C. and Bavigadda, V. and Bazzan, M. and Behnke, B. and Bejger, M. and Belczynski, C. and Bell, A. S. and Bell, C. J. and Berger, B. K. and Bergman, J. and Bergmann, G. and Berry, C. P. L. and Bersanetti, D. and Bertolini, A. and Betzwieser, J. and Bhagwat, S. and Bhandare, R. and Bilenko, I. A. and Billingsley, G. and Birch, J. and Birney, R. and Birnholtz, O. and Biscans, S. and Bisht, A. and Bitossi, M. and Biwer, C. and Bizouard, M. A. and Blackburn, J. K. and Blair, C. D. and Blair, D. G. and Blair, R. M. and Bloemen, S. and Bock, O. and Bodiya, T. P. and Boer, M. and Bogaert, G. and Bogan, C. and Bohe, A. and Bojtos, P. and Bond, C. and Bondu, F. and Bonnand, R. and Boom, B. A. and Bork, R. and Boschi, V. and Bose, S. and Bouffanais, Y. and Bozzi, A. and Bradaschia, C. and Brady, P. R. and Braginsky, V. B. and Branchesi, M. and Brau, J. E. and Briant, T. and Brillet, A. and Brinkmann, M. and Brisson, V. and Brockill, P. and Brooks, A. F. and Brown, D. A. and Brown, D. D. and Brown, N. M. and Buchanan, C. C. and Buikema, A. and Bulik, T. and Bulten, H. J. and Buonanno, A. and Buskulic, D. and Buy, C. and Byer, R. L. and Cabero, M. and Cadonati, L. and Cagnoli, G. and Cahillane, C. and Bustillo, J. Calder\'on and Callister, T. and Calloni, E. and Camp, J. B. and Cannon, K. C. and Cao, J. and Capano, C. D. and Capocasa, E. and Carbognani, F. and Caride, S. and Diaz, J. Casanueva and Casentini, C. and Caudill, S. and Cavagli\`a, M. and Cavalier, F. and Cavalieri, R. and Cella, G. and Cepeda, C. B. and Baiardi, L. Cerboni and Cerretani, G. and Cesarini, E. and Chakraborty, R. and Chalermsongsak, T. and Chamberlin, S. J. and Chan, M. and Chao, S. and Charlton, P. and Chassande-Mottin, E. and Chen, H. Y. and Chen, Y. and Cheng, C. and Chincarini, A. and Chiummo, A. and Cho, H. S. and Cho, M. and Chow, J. H. and Christensen, N. and Chu, Q. and Chua, S. and Chung, S. and Ciani, G. and Clara, F. and Clark, J. A. and Cleva, F. and Coccia, E. and Cohadon, P.-F. and Colla, A. and Collette, C. G. and Cominsky, L. and Constancio, M. and Conte, A. and Conti, L. and Cook, D. and Corbitt, T. R. and Cornish, N. and Corsi, A. and Cortese, S. and Costa, C. A. and Coughlin, M. W. and Coughlin, S. B. and Coulon, J.-P. and Countryman, S. T. and Couvares, P. and Cowan, E. E. and Coward, D. M. and Cowart, M. J. and Coyne, D. C. and Coyne, R. and Craig, K. and Creighton, J. D. E. and Creighton, T. D. and Cripe, J. and Crowder, S. G. and Cruise, A. M. and Cumming, A. and Cunningham, L. and Cuoco, E. and Canton, T. Dal and Danilishin, S. L. and D'Antonio, S. and Danzmann, K. and Darman, N. S. and Da Silva Costa, C. F. and Dattilo, V. and Dave, I. and Daveloza, H. P. and Davier, M. and Davies, G. S. and Daw, E. J. and Day, R. and De, S. and DeBra, D. and Debreczeni, G. and Degallaix, J. and De Laurentis, M. and Del\'eglise, S. and Del Pozzo, W. and Denker, T. and Dent, T. and Dereli, H. and Dergachev, V. and DeRosa, R. T. and De Rosa, R. and DeSalvo, R. and Dhurandhar, S. and D\'{\i}az, M. C. and Di Fiore, L. and Di Giovanni, M. and Di Lieto, A. and Di Pace, S. and Di Palma, I. and Di Virgilio, A. and Dojcinoski, G. and Dolique, V. and Donovan, F. and Dooley, K. L. and Doravari, S. and Douglas, R. and Downes, T. P. and Drago, M. and Drever, R. W. P. and Driggers, J. C. and Du, Z. and Ducrot, M. and Dwyer, S. E. and Edo, T. B. and Edwards, M. C. and Effler, A. and Eggenstein, H.-B. and Ehrens, P. and Eichholz, J. and Eikenberry, S. S. and Engels, W. and Essick, R. C. and Etzel, T. and Evans, M. and Evans, T. M. and Everett, R. and Factourovich, M. and Fafone, V. and Fair, H. and Fairhurst, S. and Fan, X. and Fang, Q. and Farinon, S. and Farr, B. and Farr, W. M. and Favata, M. and Fays, M. and Fehrmann, H. and Fejer, M. M. and Feldbaum, D. and Ferrante, I. and Ferreira, E. C. and Ferrini, F. and Fidecaro, F. and Finn, L. S. and Fiori, I. and Fiorucci, D. and Fisher, R. P. and Flaminio, R. and Fletcher, M. and Fong, H. and Fournier, J.-D. and Franco, S. and Frasca, S. and Frasconi, F. and Frede, M. and Frei, Z. and Freise, A. and Frey, R. and Frey, V. and Fricke, T. T. and Fritschel, P. and Frolov, V. V. and Fulda, P. and Fyffe, M. and Gabbard, H. A. G. and Gair, J. R. and Gammaitoni, L. and Gaonkar, S. G. and Garufi, F. and Gatto, A. and Gaur, G. and Gehrels, N. and Gemme, G. and Gendre, B. and Genin, E. and Gennai, A. and George, J. and Gergely, L. and Germain, V. and Ghosh, Abhirup and Ghosh, Archisman and Ghosh, S. and Giaime, J. A. and Giardina, K. D. and Giazotto, A. and Gill, K. and Glaefke, A. and Gleason, J. R. and Goetz, E. and Goetz, R. and Gondan, L. and Gonz\'alez, G. and Castro, J. M. Gonzalez and Gopakumar, A. and Gordon, N. A. and Gorodetsky, M. L. and Gossan, S. E. and Gosselin, M. and Gouaty, R. and Graef, C. and Graff, P. B. and Granata, M. and Grant, A. and Gras, S. and Gray, C. and Greco, G. and Green, A. C. and Greenhalgh, R. J. S. and Groot, P. and Grote, H. and Grunewald, S. and Guidi, G. M. and Guo, X. and Gupta, A. and Gupta, M. K. and Gushwa, K. E. and Gustafson, E. K. and Gustafson, R. and Hacker, J. J. and Hall, B. R. and Hall, E. D. and Hammond, G. and Haney, M. and Hanke, M. M. and Hanks, J. and Hanna, C. and Hannam, M. D. and Hanson, J. and Hardwick, T. and Harms, J. and Harry, G. M. and Harry, I. W. and Hart, M. J. and Hartman, M. T. and Haster, C.-J. and Haughian, K. and Healy, J. and Heefner, J. and Heidmann, A. and Heintze, M. C. and Heinzel, G. and Heitmann, H. and Hello, P. and Hemming, G. and Hendry, M. and Heng, I. S. and Hennig, J. and Heptonstall, A. W. and Heurs, M. and Hild, S. and Hoak, D. and Hodge, K. A. and Hofman, D. and Hollitt, S. E. and Holt, K. and Holz, D. E. and Hopkins, P. and Hosken, D. J. and Hough, J. and Houston, E. A. and Howell, E. J. and Hu, Y. M. and Huang, S. and Huerta, E. A. and Huet, D. and Hughey, B. and Husa, S. and Huttner, S. H. and Huynh-Dinh, T. and Idrisy, A. and Indik, N. and Ingram, D. R. and Inta, R. and Isa, H. N. and Isac, J.-M. and Isi, M. and Islas, G. and Isogai, T. and Iyer, B. R. and Izumi, K. and Jacobson, M. B. and Jacqmin, T. and Jang, H. and Jani, K. and Jaranowski, P. and Jawahar, S. and Jim\'enez-Forteza, F. and Johnson, W. W. and Johnson-McDaniel, N. K. and Jones, D. I. and Jones, R. and Jonker, R. J. G. and Ju, L. and Haris, K. and Kalaghatgi, C. V. and Kalogera, V. and Kandhasamy, S. and Kang, G. and Kanner, J. B. and Karki, S. and Kasprzack, M. and Katsavounidis, E. and Katzman, W. and Kaufer, S. and Kaur, T. and Kawabe, K. and Kawazoe, F. and K\'ef\'elian, F. and Kehl, M. S. and Keitel, D. and Kelley, D. B. and Kells, W. and Kennedy, R. and Keppel, D. G. and Key, J. S. and Khalaidovski, A. and Khalili, F. Y. and Khan, I. and Khan, S. and Khan, Z. and Khazanov, E. A. and Kijbunchoo, N. and Kim, C. and Kim, J. and Kim, K. and Kim, Nam-Gyu and Kim, Namjun and Kim, Y.-M. and King, E. J. and King, P. J. and Kinzel, D. L. and Kissel, J. S. and Kleybolte, L. and Klimenko, S. and Koehlenbeck, S. M. and Kokeyama, K. and Koley, S. and Kondrashov, V. and Kontos, A. and Koranda, S. and Korobko, M. and Korth, W. Z. and Kowalska, I. and Kozak, D. B. and Kringel, V. and Krishnan, B. and Kr\'olak, A. and Krueger, C. and Kuehn, G. and Kumar, P. and Kumar, R. and Kuo, L. and Kutynia, A. and Kwee, P. and Lackey, B. D. and Landry, M. and Lange, J. and Lantz, B. and Lasky, P. D. and Lazzarini, A. and Lazzaro, C. and Leaci, P. and Leavey, S. and Lebigot, E. O. and Lee, C. H. and Lee, H. K. and Lee, H. M. and Lee, K. and Lenon, A. and Leonardi, M. and Leong, J. R. and Leroy, N. and Letendre, N. and Levin, Y. and Levine, B. M. and Li, T. G. F. and Libson, A. and Littenberg, T. B. and Lockerbie, N. A. and Logue, J. and Lombardi, A. L. and London, L. T. and Lord, J. E. and Lorenzini, M. and Loriette, V. and Lormand, M. and Losurdo, G. and Lough, J. D. and Lousto, C. O. and Lovelace, G. and L\"uck, H. and Lundgren, A. P. and Luo, J. and Lynch, R. and Ma, Y. and MacDonald, T. and Machenschalk, B. and MacInnis, M. and Macleod, D. M. and Maga\~na-Sandoval, F. and Magee, R. M. and Mageswaran, M. and Majorana, E. and Maksimovic, I. and Malvezzi, V. and Man, N. and Mandel, I. and Mandic, V. and Mangano, V. and Mansell, G. L. and Manske, M. and Mantovani, M. and Marchesoni, F. and Marion, F. and M\'arka, S. and M\'arka, Z. and Markosyan, A. S. and Maros, E. and Martelli, F. and Martellini, L. and Martin, I. W. and Martin, R. M. and Martynov, D. V. and Marx, J. N. and Mason, K. and Masserot, A. and Massinger, T. J. and Masso-Reid, M. and Matichard, F. and Matone, L. and Mavalvala, N. and Mazumder, N. and Mazzolo, G. and McCarthy, R. and McClelland, D. E. and McCormick, S. and McGuire, S. C. and McIntyre, G. and McIver, J. and McManus, D. J. and McWilliams, S. T. and Meacher, D. and Meadors, G. D. and Meidam, J. and Melatos, A. and Mendell, G. and Mendoza-Gandara, D. and Mercer, R. A. and Merilh, E. and Merzougui, M. and Meshkov, S. and Messenger, C. and Messick, C. and Meyers, P. M. and Mezzani, F. and Miao, H. and Michel, C. and Middleton, H. and Mikhailov, E. E. and Milano, L. and Miller, J. and Millhouse, M. and Minenkov, Y. and Ming, J. and Mirshekari, S. and Mishra, C. and Mitra, S. and Mitrofanov, V. P. and Mitselmakher, G. and Mittleman, R. and Moggi, A. and Mohan, M. and Mohapatra, S. R. P. and Montani, M. and Moore, B. C. and Moore, C. J. and Moraru, D. and Moreno, G. and Morriss, S. R. and Mossavi, K. and Mours, B. and Mow-Lowry, C. M. and Mueller, C. L. and Mueller, G. and Muir, A. 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Collaboration = {LIGO Scientific Collaboration and Virgo Collaboration},
Date-Added = {2016-02-29 16:27:19 +0000},
Date-Modified = {2016-02-29 16:27:28 +0000},
Doi = {10.1103/PhysRevLett.116.061102},
Issue = {6},
Journal = {Phys. Rev. Lett.},
Month = {Feb},
Numpages = {16},
Pages = {061102},
Publisher = {American Physical Society},
Title = {Observation of Gravitational Waves from a Binary Black Hole Merger},
Url = {http://link.aps.org/doi/10.1103/PhysRevLett.116.061102},
Volume = {116},
Year = {2016},
Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.116.061102},
Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.116.061102}}
@article{neb15,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2015RaSc...50..614N},
Archiveprefix = {arXiv},
Author = {{Neben}, A.~R. and {Bradley}, R.~F. and {Hewitt}, J.~N. and {Bernardi}, G. and {Bowman}, J.~D. and {Briggs}, F. and {Cappallo}, R.~J. and {Deshpande}, A.~A. and {Goeke}, R. and {Greenhill}, L.~J. and {Hazelton}, B.~J. and {Johnston-Hollitt}, M. and {Kaplan}, D.~L. and {Lonsdale}, C.~J. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and {Morales}, M.~F. and {Morgan}, E. and {Oberoi}, D. and {Ord}, S.~M. and {Prabu}, T. and {Shankar}, N.~U. and {Srivani}, K.~S. and {Subrahmanyan}, R. and {Tingay}, S.~J. and {Wayth}, R.~B. and {Webster}, R.~L. and {Williams}, A. and {Williams}, C.~L.},
Date-Added = {2016-01-28 18:57:39 +0000},
Date-Modified = {2016-01-28 18:57:42 +0000},
Doi = {10.1002/2015RS005678},
Eprint = {1505.07114},
Journal = {Radio Science},
Keywords = {antenna arrays, radio astronomy, antennas},
Month = jul,
Pages = {614-629},
Primaryclass = {astro-ph.IM},
Title = {{Measuring phased-array antenna beampatterns with high dynamic range for the Murchison Widefield Array using 137 MHz ORBCOMM satellites}},
Volume = 50,
Year = 2015,
Bdsk-Url-1 = {http://dx.doi.org/10.1002/2015RS005678}}
@article{vir14,
Author = {Virone, G. and Lingua, A.M. and Piras, M. and Cina, A. and Perini, F. and Monari, J. and Paonessa, F. and Peverini, O.A. and Addamo, G. and Tascone, R.},
Date-Added = {2016-01-28 18:54:23 +0000},
Date-Modified = {2016-01-28 18:54:28 +0000},
Doi = {10.1109/LAWP.2014.2298250},
Issn = {1536-1225},
Journal = {Antennas and Wireless Propagation Letters, IEEE},
Keywords = {HF antennas;UHF antennas;antenna radiation patterns;autonomous aerial vehicles;position measurement;wire antennas;UAV flying path;antenna radiation pattern verification system;autonomous flight;data processing;frequency 150 MHz;frequency 408 MHz;low-frequency antenna;microunmanned aerial vehicle;position measurement;remote topographic instrument;wire antenna;Accuracy;Antenna measurements;Antenna radiation patterns;Arrays;Power measurement;Soil;Soil measurements;Antenna measurements;antenna radiation pattern;radio astronomy;unmanned aerial vehicles},
Pages = {169-172},
Title = {Antenna Pattern Verification System Based on a Micro Unmanned Aerial Vehicle (UAV)},
Volume = {13},
Year = {2014},
Bdsk-Url-1 = {http://dx.doi.org/10.1109/LAWP.2014.2298250}}
@article{kaz13,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2013MNRAS.430.1457K},
Archiveprefix = {arXiv},
Author = {{Kazemi}, S. and {Yatawatta}, S. and {Zaroubi}, S.},
Date-Added = {2016-01-27 21:12:59 +0000},
Date-Modified = {2016-01-27 21:13:03 +0000},
Doi = {10.1093/mnras/stt018},
Eprint = {1301.0633},
Journal = {\mnras},
Keywords = {methods: numerical, methods: statistical, techniques: interferometric},
Month = apr,
Pages = {1457-1472},
Primaryclass = {astro-ph.IM},
Title = {{Clustered calibration: an improvement to radio interferometric direction-dependent self-calibration}},
Volume = 430,
Year = 2013,
Bdsk-Url-1 = {http://dx.doi.org/10.1093/mnras/stt018}}
@book{kay93,
Author = {Kay, Steven M.},
Date-Added = {2016-01-27 21:11:53 +0000},
Date-Modified = {2016-01-27 21:56:26 +0000},
Isbn = {0-13-345711-7},
Publisher = {{Prentice-Hall, Inc.}},
Title = {Fundamentals of Statistical Signal Processing: Estimation Theory},
Year = {1993}}
@article{deo08,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2008MNRAS.388..247D},
Archiveprefix = {arXiv},
Author = {{de Oliveira-Costa}, A. and {Tegmark}, M. and {Gaensler}, B.~M. and {Jonas}, J. and {Landecker}, T.~L. and {Reich}, P.},
Date-Added = {2016-01-25 16:45:57 +0000},
Date-Modified = {2016-01-25 16:46:03 +0000},
Doi = {10.1111/j.1365-2966.2008.13376.x},
Eprint = {0802.1525},
Journal = {\mnras},
Keywords = {methods: data analysis , astronomical data bases: miscellaneous , ISM: structure , diffuse radiation , radio continuum: ISM},
Month = jul,
Pages = {247-260},
Title = {{A model of diffuse Galactic radio emission from 10 MHz to 100 GHz}},
Volume = 388,
Year = 2008,
Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2008.13376.x}}
@article{hic12,
Abstract = {ABSTRACT. We describe an ``active'' antenna system for HF/VHF (long wavelength) radio astronomy that has been successfully deployed 256-fold as the first station (LWA1) of the planned Long Wavelength Array. The antenna system, consisting of crossed dipoles, an active balun/preamp, a support structure, and a ground screen has been shown to successfully operate over at least the band from 20 MHz (15 m wavelength) to 80 MHz (3.75 m wavelength) with a noise figure that is at least 6 dB better than the Galactic background emission-noise temperature over that band. Thus, we met the goal to design and construct a compact, inexpensive, rugged, and easily assembled antenna system that can be deployed many-fold to form numerous large individual ``stations'' for the purpose of building a large, long wavelength synthesis array telescope for radio astronomical and ionospheric observations.},
Author = {Hicks, Brian C. and Paravastu-Dalal, Nagini and Stewart, Kenneth P. and Erickson, William C. and Ray, Paul S. and Kassim, Namir E. and Burns, Steve and Clarke, Tracy and Schmitt, Henrique and Craig, Joe and Hartman, Jake and Weiler, Kurt W.},
Copyright = {Copyright {\copyright} 2012 The University of Chicago Press},
Date-Added = {2016-01-25 15:57:42 +0000},
Date-Modified = {2016-01-25 15:57:47 +0000},
Issn = {00046280},
Journal = {Publications of the Astronomical Society of the Pacific},
Jstor_Articletype = {research-article},
Jstor_Formatteddate = {October 2012},
Language = {English},
Number = {920},
Pages = {pp. 1090-1104},
Publisher = {The University of Chicago Press on behalf of the Astronomical Society of the Pacific},
Title = {A Wide-Band, Active Antenna System for Long Wavelength Radio Astronomy},
Url = {http://www.jstor.org/stable/10.1086/668121},
Volume = {124},
Year = {2012},
Bdsk-Url-1 = {http://www.jstor.org/stable/10.1086/668121}}
@article{mit08,
Author = {Mitchell, D.A. and Greenhill, L.J. and Wayth, R.B. and Sault, R.J. and Lonsdale, C.J. and Cappallo, R.J. and Morales, M.F. and Ord, S.M.},
Date-Added = {2015-11-17 17:48:54 +0000},
Date-Modified = {2015-11-17 17:48:57 +0000},
Doi = {10.1109/JSTSP.2008.2005327},
Issn = {1932-4553},
Journal = {Selected Topics in Signal Processing, IEEE Journal of},
Keywords = {VHF antennas;array signal processing;dipole antenna arrays;interferometers;Australia;Murchison Widefield array;antenna array;array signal processing;frequency 80 MHz to 300 MHz;galactic emission;high-throughput real-time computing cluster;interferometric technique;ionospheric condition;low-frequency fixed dipole array;low-frequency radio array;next-generation radio interferometer;real-time calibration;real-time peeling implementation;Australia;Calibration;Dipole antennas;Image resolution;Instruments;Polarization;Radio interferometry;Signal synthesis;Structural beams;Tiles;Antenna arrays;array signal processing;calibration;dipole arrays;radio astronomy;radio interferometry},
Month = {Oct},
Number = {5},
Pages = {707-717},
Title = {Real-Time Calibration of the Murchison Widefield Array},
Volume = {2},
Year = {2008},
Bdsk-Url-1 = {http://dx.doi.org/10.1109/JSTSP.2008.2005327}}
@article{kas07,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2007ApJS..172..686K},
Archiveprefix = {arXiv},
Author = {{Kassim}, N.~E. and {Lazio}, T.~J.~W. and {Erickson}, W.~C. and {Perley}, R.~A. and {Cotton}, W.~D. and {Greisen}, E.~W. and {Cohen}, A.~S. and {Hicks}, B. and {Schmitt}, H.~R. and {Katz}, D.},
Date-Added = {2015-11-13 16:30:05 +0000},
Date-Modified = {2015-11-13 16:30:08 +0000},
Doi = {10.1086/519022},
Eprint = {0704.3088},
Journal = {\apjs},
Keywords = {Astrometry, Instrumentation: Interferometers, Techniques: High Anular Resolution, Techniques: Image Processing, Techniques: Interferometric, cas-a},
Month = oct,
Pages = {686-719},
Title = {{The 74 MHz System on the Very Large Array}},
Volume = 172,
Year = 2007,
Bdsk-Url-1 = {http://dx.doi.org/10.1086/519022}}
@article{coh07,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2007AJ....134.1245C},
Archiveprefix = {arXiv},
Author = {{Cohen}, A.~S. and {Lane}, W.~M. and {Cotton}, W.~D. and {Kassim}, N.~E. and {Lazio}, T.~J.~W. and {Perley}, R.~A. and {Condon}, J.~J. and {Erickson}, W.~C.},
Date-Added = {2015-11-13 16:29:52 +0000},
Date-Modified = {2015-11-13 16:29:56 +0000},
Doi = {10.1086/520719},
Eprint = {0706.1191},
Journal = {\aj},
Keywords = {atmospheric effects, catalogs, radio continuum: general, surveys, cyg-a},
Month = sep,
Pages = {1245-1262},
Title = {{The VLA Low-Frequency Sky Survey}},
Volume = 134,
Year = 2007,
Bdsk-Url-1 = {http://dx.doi.org/10.1086/520719}}
@article{thy15c,
Author = {{Thyagarajan}, N. and {Beardsley}, A.~P. and {Bowman}, J.~D. and {Morales}, M.~F.},
Date-Added = {2015-11-10 16:47:00 +0000},
Date-Modified = {2015-11-10 16:47:05 +0000},
Journal = {{arXiv:1510.08318}},
Title = {{A Generic and Efficient E-field Parallel Imaging Correlator for Next-Generation Radio Telescopes}},
Year = {2015}}
@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{bea12,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2012MNRAS.425.1781B},
Archiveprefix = {arXiv},
Author = {{Beardsley}, A.~P. and {Hazelton}, B.~J. and {Morales}, M.~F. and {Capallo}, R.~J. and {Goeke}, R. and {Emrich}, D. and {Lonsdale}, C.~J. and {Arcus}, W. and {Barnes}, D. and {Bernardi}, G. and {Bowman}, J.~D. and {Bunton}, J.~D. and {Corey}, B.~E. and {Deshpande}, A. and {deSouza}, L. and {Gaensler}, B.~M. and {Greenhill}, L.~J. and {Herne}, D. and {Hewitt}, J.~N. and {Kaplan}, D.~L. and {Kasper}, J.~C. and {Kincaid}, B.~B. and {Koenig}, R. and {Kratzenberg}, E. and {Lynch}, M.~J. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and {Morgan}, E. and {Oberoi}, D. and {Ord}, S.~M. and {Pathikulangara}, J. and {Prabu}, T. and {Remillard}, R.~A. and {Rogers}, A.~E.~E. and {Roshi}, A. and {Salah}, J.~E. and {Sault}, R.~J. and {Shankar}, N.~U. and {Srivani}, K.~S. and {Stevens}, J. and {Subrahmanyan}, R. and {Tingay}, S.~J. and {Wayth}, R.~B. and {Waterson}, M. and {Webster}, R.~L. and {Whitney}, A.~R. and {Williams}, A. and {Williams}, C.~L. and {Wyithe}, J.~S.~B.},
Doi = {10.1111/j.1365-2966.2012.20878.x},
Eprint = {1203.1293},
Journal = {\mnras},
Keywords = {instrumentation: interferometers, cosmology: miscellaneous},
Month = sep,
Pages = {1781-1788},
Primaryclass = {astro-ph.IM},
Title = {{A new layout optimization technique for interferometric arrays, applied to the Murchison Widefield Array}},
Volume = 425,
Year = 2012,
Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2012.20878.x}}
@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}}
@book{bri74,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/1974fft..book.....B},
Author = {{Brigham}, E.~O.},
Booktitle = {Englewood Cliffs, N.J.: Prentice-Hall, 1974},
Title = {{The fast Fourier Transform}},
Year = 1974}
@article{bow13,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2013PASA...30...31B},
Archiveprefix = {arXiv},
Author = {{Bowman}, J.~D. and {Cairns}, I. and {Kaplan}, D.~L. and {Murphy}, T. and {Oberoi}, D. and {Staveley-Smith}, L. and {Arcus}, W. and {Barnes}, D.~G. and {Bernardi}, G. and {Briggs}, F.~H. and {Brown}, S. and {Bunton}, J.~D. and {Burgasser}, A.~J. and {Cappallo}, R.~J. and {Chatterjee}, S. and {Corey}, B.~E. and {Coster}, A. and {Deshpande}, A. and {deSouza}, L. and {Emrich}, D. and {Erickson}, P. and {Goeke}, R.~F. and {Gaensler}, B.~M. and {Greenhill}, L.~J. and {Harvey-Smith}, L. and {Hazelton}, B.~J. and {Herne}, D. and {Hewitt}, J.~N. and {Johnston-Hollitt}, M. and {Kasper}, J.~C. and {Kincaid}, B.~B. and {Koenig}, R. and {Kratzenberg}, E. and {Lonsdale}, C.~J. and {Lynch}, M.~J. and {Matthews}, L.~D. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and {Morales}, M.~F. and {Morgan}, E.~H. and {Ord}, S.~M. and {Pathikulangara}, J. and {Prabu}, T. and {Remillard}, R.~A. and {Robishaw}, T. and {Rogers}, A.~E.~E. and {Roshi}, A.~A. and {Salah}, J.~E. and {Sault}, R.~J. and {Shankar}, N.~U. and {Srivani}, K.~S. and {Stevens}, J.~B. and {Subrahmanyan}, R. and {Tingay}, S.~J. and {Wayth}, R.~B. and {Waterson}, M. and {Webster}, R.~L. and {Whitney}, A.~R. and {Williams}, A.~J. and {Williams}, C.~L. and {Wyithe}, J.~S.~B.},
Doi = {10.1017/pas.2013.009},
Eid = {e031},
Eprint = {1212.5151},
Journal = {\pasa},
Keywords = {dark ages, reionisation, first stars, instrumentation: interferometers, radio continuum: general, radio lines: general, Sun: general},
Month = apr,
Pages = {31},
Primaryclass = {astro-ph.IM},
Title = {{Science with the Murchison Widefield Array}},
Volume = 30,
Year = 2013,
Bdsk-Url-1 = {http://dx.doi.org/10.1017/pas.2013.009}}
@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{coo65,
Author = {Cooley, James W. and Tukey, John W.},
Journal = {Math. Comput.},
Pages = {297-301},
Title = {An algorithm for the machine calculation of complex Fourier series},
Volume = {19},
Year = {1965}}
@article{cor08,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2008ISTSP...2..647C},
Archiveprefix = {arXiv},
Author = {{Cornwell}, T.~J. and {Golap}, K. and {Bhatnagar}, S.},
Doi = {10.1109/JSTSP.2008.2005290},
Eprint = {0807.4161},
Journal = {IEEE Journal of Selected Topics in Signal Processing},
Month = nov,
Pages = {647-657},
Title = {{The Noncoplanar Baselines Effect in Radio Interferometry: The W-Projection Algorithm}},
Volume = 2,
Year = 2008,
Bdsk-Url-1 = {http://dx.doi.org/10.1109/JSTSP.2008.2005290}}
@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,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/1999cs........1013M},
Author = {{Maneewongvatana}, S. and {Mount}, D.~M.},
Eprint = {cs/9901013},
Journal = {eprint arXiv:cs/9901013},
Keywords = {Computer Science - Computational Geometry, E.1, F.2.2},
Month = jan,
Title = {{Analysis of approximate nearest neighbor searching with clustered point sets}},
Year = 1999}
@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,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/1997ApJ...480L..87T},
Author = {{Tegmark}, M.},
Doi = {10.1086/310631},
Eprint = {astro-ph/9611130},
Journal = {\apjl},
Keywords = {COSMOLOGY: COSMIC MICROWAVE BACKGROUND, METHODS: DATA ANALYSIS, Cosmology: Cosmic Microwave Background, Methods: Data Analysis},
Month = may,
Pages = {L87-L90},
Title = {{How to Make Maps from Cosmic Microwave Background Data without Losing Information}},
Volume = 480,
Year = 1997,
Bdsk-Url-1 = {http://dx.doi.org/10.1086/310631}}
@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},
Date-Modified = {2015-10-15 16:29:22 +0000},
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Journal = {Phys. Rev. D},
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Numpages = {10},
Pages = {103501},
Publisher = {American Physical Society},
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Url = {http://link.aps.org/doi/10.1103/PhysRevD.82.103501},
Volume = {82},
Year = {2010},
Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.82.103501},
Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.82.103501}}
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Date-Added = {2015-10-15 17:03:47 +0000},
Date-Modified = {2015-10-15 17:03:53 +0000},
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Issn = {1448-6083},
Journal = {PASA - Publications of the Astronomical Society of Australia},
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Title = {The Murchison Widefield Array: The Square Kilometre Array Precursor at Low Radio Frequencies},
Url = {http://journals.cambridge.org/article_S1323358012000070},
Volume = {30},
Year = {2013},
Bdsk-Url-1 = {http://journals.cambridge.org/article_S1323358012000070},
Bdsk-Url-2 = {http://dx.doi.org/10.1017/pasa.2012.007}}
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Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2001isra.book.....T},
Author = {{Thompson}, A.~R. and {Moran}, J.~M. and {Swenson}, Jr., G.~W.},
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Publisher = {Wiley},
Title = {{Interferometry and Synthesis in Radio Astronomy, 2nd Edition}},
Year = 2001}
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Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2013Sci...341...53T},
Archiveprefix = {arXiv},
Author = {{Thornton}, D. and {Stappers}, B. and {Bailes}, M. and {Barsdell}, B. and {Bates}, S. and {Bhat}, N.~D.~R. and {Burgay}, M. and {Burke-Spolaor}, S. and {Champion}, D.~J. and {Coster}, P. and {D'Amico}, N. and {Jameson}, A. and {Johnston}, S. and {Keith}, M. and {Kramer}, M. and {Levin}, L. and {Milia}, S. and {Ng}, C. and {Possenti}, A. and {van Straten}, W.},
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Eprint = {1307.1628},
Journal = {Science},
Month = jul,
Pages = {53-56},
Primaryclass = {astro-ph.HE},
Title = {{A Population of Fast Radio Bursts at Cosmological Distances}},
Volume = 341,
Year = 2013,
Bdsk-Url-1 = {http://dx.doi.org/10.1126/science.1236789}}
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Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2015ApJ...804...14T},
Archiveprefix = {arXiv},
Author = {{Thyagarajan}, N. and {Jacobs}, D.~C. and {Bowman}, J.~D. and {Barry}, N. and {Beardsley}, A.~P. and {Bernardi}, G. and {Briggs}, F. and {Cappallo}, R.~J. and {Carroll}, P. and {Corey}, B.~E. and {de Oliveira-Costa}, A. and {Dillon}, J.~S. and {Emrich}, D. and {Ewall-Wice}, A. and {Feng}, L. and {Goeke}, R. and {Greenhill}, L.~J. and {Hazelton}, B.~J. and {Hewitt}, J.~N. and {Hurley-Walker}, N. and {Johnston-Hollitt}, M. and {Kaplan}, D.~L. and {Kasper}, J.~C. and {Kim}, H.-S. and {Kittiwisit}, P. and {Kratzenberg}, E. and {Lenc}, E. and {Line}, J. and {Loeb}, A. and {Lonsdale}, C.~J. and {Lynch}, M.~J. and {McKinley}, B. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and {Morales}, M.~F. and {Morgan}, E. and {Neben}, A.~R. and {Oberoi}, D. and {Offringa}, A.~R. and {Ord}, S.~M. and {Paul}, S. and {Pindor}, B. and {Pober}, J.~C. and {Prabu}, T. and {Procopio}, P. and {Riding}, J. and {Rogers}, A.~E.~E. and {Roshi}, A. and {Udaya Shankar}, N. and {Sethi}, S.~K. and {Srivani}, K.~S. and {Subrahmanyan}, R. and {Sullivan}, I.~S. and {Tegmark}, M. and {Tingay}, S.~J. and {Trott}, C.~M. and {Waterson}, M. and {Wayth}, R.~B. and {Webster}, R.~L. and {Whitney}, A.~R. and {Williams}, A. and {Williams}, C.~L. and {Wu}, C. and {Wyithe}, J.~S.~B.},
Doi = {10.1088/0004-637X/804/1/14},
Eid = {14},
Eprint = {1502.07596},
Journal = {\apj},
Keywords = {cosmology: observations, dark ages, reionization, first stars, large-scale structure of universe, methods: statistical, radio continuum: galaxies, techniques: interferometric},
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Pages = {14},
Primaryclass = {astro-ph.IM},
Title = {{Foregrounds in Wide-field Redshifted 21 cm Power Spectra}},
Volume = 804,
Year = 2015,
Bdsk-Url-1 = {http://dx.doi.org/10.1088/0004-637X/804/1/14}}
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Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2015ApJ...807L..28T},
Archiveprefix = {arXiv},
Author = {{Thyagarajan}, N. and {Jacobs}, D.~C. and {Bowman}, J.~D. and {Barry}, N. and {Beardsley}, A.~P. and {Bernardi}, G. and {Briggs}, F. and {Cappallo}, R.~J. and {Carroll}, P. and {Deshpande}, A.~A. and {de Oliveira-Costa}, A. and {Dillon}, J.~S. and {Ewall-Wice}, A. and {Feng}, L. and {Greenhill}, L.~J. and {Hazelton}, B.~J. and {Hernquist}, L. and {Hewitt}, J.~N. and {Hurley-Walker}, N. and {Johnston-Hollitt}, M. and {Kaplan}, D.~L. and {Kim}, H.-S. and {Kittiwisit}, P. and {Lenc}, E. and {Line}, J. and {Loeb}, A. and {Lonsdale}, C.~J. and {McKinley}, B. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and {Morales}, M.~F. and {Morgan}, E. and {Neben}, A.~R. and {Oberoi}, D. and {Offringa}, A.~R. and {Ord}, S.~M. and {Paul}, S. and {Pindor}, B. and {Pober}, J.~C. and {Prabu}, T. and {Procopio}, P. and {Riding}, J. and {Udaya Shankar}, N. and {Sethi}, S.~K. and {Srivani}, K.~S. and {Subrahmanyan}, R. and {Sullivan}, I.~S. and {Tegmark}, M. and {Tingay}, S.~J. and {Trott}, C.~M. and {Wayth}, R.~B. and {Webster}, R.~L. and {Williams}, A. and {Williams}, C.~L. and {Wyithe}, J.~S.~B.},
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Eprint = {1506.06150},
Journal = {\apjl},
Keywords = {cosmology: observations, dark ages, reionization, first stars, large-scale structure of universe, methods: statistical, radio continuum: galaxies, techniques: interferometric},
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Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
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Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2013A%26A...556A...2V},
Archiveprefix = {arXiv},
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Keywords = {instrumentation: interferometers, radio continuum: general, radio lines: general, dark ages, reionization, first stars, telescopes},
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Pages = {A2},
Primaryclass = {astro-ph.IM},
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Adsurl = {http://adsabs.harvard.edu/abs/1938Phy.....5..785Z},
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Adsurl = {http://adsabs.harvard.edu/abs/2014MNRAS.445.1084Z},
Archiveprefix = {arXiv},
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Keywords = {instrumentation: interferometers, methods: data analysis, techniques: interferometric, cosmology: observations, dark ages, reionization, first stars},
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