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casper-2016.bib
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@article{Foley01082016,
author = {Foley, A. R. and Alberts, T. and Armstrong, R. P. and Barta, A. and Bauermeister, E. F. and Bester, H. and Blose, S. and Booth, R. S. and Botha, D. H. and Buchner, S. J. and Carignan, C. and Cheetham, T. and Cloete, K. and Coreejes, G. and Crida, R. C. and Cross, S. D. and Curtolo, F. and Dikgale, A. and de Villiers, M. S. and du Toit, L. J. and Esterhuyse, S. W. P. and Fanaroff, B. and Fender, R. P. and Fijalkowski, M. and Fourie, D. and Frank, B. and George, D. and Gibbs, P. and Goedhart, S. and Grobbelaar, J. and Gumede, S. C. and Herselman, P. and Hess, K. M. and Hoek, N. and Horrell, J. and Jonas, J. L. and Jordaan, J. D. B. and Julie, R. and Kapp, F. and Kotzé, P. and Kusel, T. and Langman, A. and Lehmensiek, R. and Liebenberg, D. and Liebenberg, I. J. V. and Loots, A. and Lord, R. T. and Lucero, D. M. and Ludick, J. and Macfarlane, P. and Madlavana, M. and Magnus, L. and Magozore, C. and Malan, J. A. and Manley, J. R. and Marais, L. and Marais, N. and Marais, S. J. and Maree, M. and Martens, A. and Mokone, O. and Moss, V. and Mthembu, S. and New, W. and Nicholson, G. D. and van Niekerk, P. C. and Oozeer, N. and Passmoor, S. S. and Peens-Hough, A. and Pińska, A. B. and Prozesky, P. and Rajan, S. and Ratcliffe, S. and Renil, R. and Richter, L. L. and Rosekrans, D. and Rust, A. and Schröder, A. C. and Schwardt, L. C. and Seranyane, S. and Serylak, M. and Shepherd, D. S. and Siebrits, R. and Sofeya, L. and Spann, R. and Springbok, R. and Swart, P. S. and Thondikulam, Venkatasubramani L. and Theron, I. P. and Tiplady, A. and Toruvanda, O. and Tshongweni, S. and van den Heever, L. and van der Merwe, C. and van Rooyen, R. and Wakhaba, S. and Walker, A. L. and Welz, M. and Williams, L. and Wolleben, M. and Woudt, P. A. and Young, N. J. and Zwart, J. T. L.},
title = {Engineering and science highlights of the KAT-7 radio telescope},
volume = {460},
number = {2},
pages = {1664-1679},
year = {2016},
doi = {10.1093/mnras/stw1040},
abstract ={The construction of the seven-dish Karoo Array Telescope (KAT-7) array in the Karoo region of the Northern Cape in South Africa was intended primarily as an engineering prototype for technologies and techniques applicable to the MeerKAT telescope. This paper looks at the main engineering and scientific highlights from this effort, and discusses their applicability to both MeerKAT and other next-generation radio telescopes. In particular, we found that the composite dish surface works well, but it becomes complicated to fabricate for a dish lacking circular symmetry; the Stirling cycle cryogenic system with ion pump to achieve vacuum works but demands much higher maintenance than an equivalent Gifford–McMahon cycle system; the ROACH (Reconfigurable Open Architecture Computing Hardware)-based correlator with SPEAD (Streaming Protocol for Exchanging Astronomical Data) protocol data transfer works very well and KATCP (Karoo Array Telescope Control Protocol) control protocol has proven very flexible and convenient. KAT-7 has also been used for scientific observations where it has a niche in mapping low surface-brightness continuum sources, some extended H i
haloes and OH masers in star-forming regions. It can also be used to monitor continuum source variability, observe pulsars, and make Very Long Baseline Interferometry observations.},
URL = {http://mnras.oxfordjournals.org/content/460/2/1664.abstract},
eprint = {http://mnras.oxfordjournals.org/content/460/2/1664.full.pdf+html},
journal = {Monthly Notices of the Royal Astronomical Society}
}
@Article{Alpert2015,
author="Alpert, B.
and Balata, M.
and Bennett, D.
and Biasotti, M.
and Boragno, C.
and Brofferio, C.
and Ceriale, V.
and Corsini, D.
and Day, K. P.
and De Gerone, M.
and Dressler, R.
and Faverzani, M.
and Ferri, E.
and Fowler, J.
and Gatti, F.
and Giachero, A.
and Hays-Wehle, J.
and Heinitz, S.
and Hilton, G.
and K{\"o}ster, U.
and Lusignoli, M.
and Maino, M.
and Mates, J.
and Nisi, S.
and Nizzolo, R.
and Nucciotti, A.
and Pessina, G.
and Pizzigoni, G.
and Puiu, A.
and Ragazzi, S.
and Reintsema, C.
and Gomes, M. Ribeiro
and Schmidt, D.
and Schumann, D.
and Sisti, M.
and Swetz, D.
and Terranova, F.
and Ullom, J.",
title="HOLMES",
journal="The European Physical Journal C",
year="2015",
volume="75",
number="3",
pages="1--11",
abstract="The European Research Council has recently funded HOLMES, a new experiment to directly measure the neutrino mass. HOLMES will perform a calorimetric measurement of the energy released in the decay of {\$}{\$}^{\{}163{\}}{\$}{\$} 163 Ho. The calorimetric measurement eliminates systematic uncertainties arising from the use of external beta sources, as in experiments with beta spectrometers. This measurement was proposed in 1982 by A. De Rujula and M. Lusignoli, but only recently the detector technological progress allowed to design a sensitive experiment. HOLMES will deploy a large array of low temperature microcalorimeters with implanted {\$}{\$}^{\{}163{\}}{\$}{\$} 163 Ho nuclei. The resulting mass sensitivity will be as low as 0.4Â eV. HOLMES will be an important step forward in the direct neutrino mass measurement with a calorimetric approach as an alternative to spectrometry. It will also establish the potential of this approach to extend the sensitivity down to 0.1Â eV. We outline here the project with its technical challenges and perspectives.",
issn="1434-6052",
doi="10.1140/epjc/s10052-015-3329-5",
url="http://dx.doi.org/10.1140/epjc/s10052-015-3329-5"
}
@article{Ferri2016179,
title = "Microwave multiplex readout for superconducting sensors ",
journal = "Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment ",
volume = "824",
number = "",
pages = "179 - 181",
year = "2016",
note = "Frontier Detectors for Frontier Physics: Proceedings of the 13th Pisa Meeting on Advanced Detectors ",
issn = "0168-9002",
doi = "http://dx.doi.org/10.1016/j.nima.2015.10.019",
url = "http://www.sciencedirect.com/science/article/pii/S0168900215012267",
author = "E. Ferri and D. Becker and D. Bennett and M. Faverzani and J. Fowler and J. Gard and A. Giachero and J. Hays-Wehle and G. Hilton and M. Maino and J. Mates and A. Puiu and A. Nucciotti and C. Reintsema and D. Schmidt and D. Swetz and J. Ullom and L. Vale",
keywords = "Neutrino mass",
keywords = "Microwave multiplexed readout",
keywords = "Low temparature detectors ",
abstract = "Abstract The absolute neutrino mass scale is still an outstanding challenge in both particle physics and cosmology. The calorimetric measurement of the energy released in a nuclear beta decay is a powerful tool to determine the effective electron-neutrino mass. In the last years, the progress on low temperature detector technologies has allowed to design large scale experiments aiming at pushing down the sensitivity on the neutrino mass below 1 eV. Even with outstanding performances in both energy (~ eV on keV) and time resolution (~ 1 μs) on the single channel, a large number of detectors working in parallel is required to reach a sub-eV sensitivity. Microwave frequency domain readout is the best available technique to readout large array of low temperature detectors, such as Transition Edge Sensors (TESs) or Microwave Kinetic Inductance Detectors (MKIDs). In this way a multiplex factor of the order of thousands can be reached, limited only by the bandwidth of the available commercial fast digitizers. This microwave multiplexing system will be used to readout the \{HOLMES\} detectors, an array of 1000 microcalorimeters based on \{TES\} sensors in which the 163Ho will be implanted. \{HOLMES\} is a new experiment for measuring the electron neutrino mass by means of the electron capture (EC) decay of 163Ho. We present here the microwave frequency multiplex which will be used in the \{HOLMES\} experiment and the microwave frequency multiplex used to readout the \{MKID\} detectors developed in Milan as well. "
}
@PHDTHESIS{jon10,
author = {{Jones}, G.},
title = {Instrumentation for wide bandwidth radio astronomy},
school = {California Institute of Technology},
year = {2010},
owner = {Glenn},
timestamp = {2010.05.29},
url = {http://resolver.caltech.edu/CaltechTHESIS:10122009-094525715}
}
@inproceedings{JonesDSS28,
author = {Jones, Glenn and Weinreb, Sander and Mani, Hamdi and Smith, Stephen and Teitelbaum, Lawrence and Hofstadter, Mark and Kuiper, Thomas B. H. and Imbriale, William A. and Dorcey, Ryan and Leflang, John},
title = {DSS-28: a novel wide bandwidth radio telescope devoted to educational outreach},
journal = {Proc. SPIE},
volume = {7733},
number = {},
pages = {77333O-77333O-12},
year = {2010},
doi = {10.1117/12.856642},
URL = { http://dx.doi.org/10.1117/12.856642}
}
@ARTICLE{mccarrick_2014,
author = {{McCarrick}, H. and {Flanigan}, D. and {Jones}, G. and {Johnson},
B.~R. and {Ade}, P. and {Araujo}, D. and {Bradford}, K. and {Cantor},
R. and {Che}, G. and {Day}, P. and {Doyle}, S. and {Leduc}, H. and
{Limon}, M. and {Luu}, V. and {Mauskopf}, P. and {Miller}, A. and
{Mroczkowski}, T. and {Tucker}, C. and {Zmuidzinas}, J.},
title = {{Horn-coupled, commercially-fabricated aluminum lumped-element kinetic
inductance detectors for millimeter wavelengths}},
journal = {Review of Scientific Instruments},
year = {2014},
volume = {85},
pages = {123117},
number = {12},
month = dec,
eid = {123117},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2014RScI...85l3117M},
archiveprefix = {arXiv},
doi = {10.1063/1.4903855},
eprint = {1407.7749},
primaryclass = {astro-ph.IM}
}
@INPROCEEDINGS{2012evn..confE..53A,
author = {{Alef}, W. and {Anderson}, J. and {Rottmann}, H. and {Roy}, A. and
{Crew}, G. and {Doeleman}, S. and {Hecht}, M. and {Ruszczyk}, C. and
{Fish}, V. and {Lonsdale}, C. and {Hiriart}, R. and {Greenberg}, J. and
{Lacasse}, R. and {Shillue}, B. and {Amestica}, R. and {Honma}, M. and
{Pradel}, N. and {Makoto}, I. and {Nagar}, N. and {Saez}, A.
},
title = "{An ALMA beamformer for ultra high resolution VLBI and phased array science}",
booktitle = {Proceedings of Science: 11th European VLBI Network Sympositum, Bordeax, France 10 Oct 2012, 6 pages. Online at <A href=''http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=178''>http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=178</A>, id.53},
year = 2012,
month = oct,
eid = {53},
pages = {53},
adsurl = {http://adsabs.harvard.edu/abs/2012evn..confE..53A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{Zwart21122008,
author = {Zwart, J. T. L. and Barker, R. W. and Biddulph, P. and Bly, D. and Boysen, R. C. and Brown, A. R. and Clementson, C. and Crofts, M. and Culverhouse, T. L. and Czeres, J. and Dace, R. J. and Davies, M. L. and D'Alessandro, R. and Doherty, P. and Duggan, K. and Ely, J. A. and Felvus, M. and Feroz, F. and Flynn, W. and Franzen, T. M. O. and Geisbüsch, J. and Génova-Santos, R. and Grainge, K. J. B. and Grainger, W. F. and Hammett, D. and Hills, R. E. and Hobson, M. P. and Holler, C. M. and Hurley-Walker, N. and Jilley, R. and Jones, M. E. and Kaneko, T. and Kneissl, R. and Lancaster, K. and Lasenby, A. N. and Marshall, P. J. and Newton, F. and Norris, O. and Northrop, I. and Odell, D. M. and Petencin, G. and Pober, J. C. and Pooley, G. G. and Pospieszalski, M. W. and Quy, V. and Rodríguez-Gonzálvez, C. and Saunders, R. D. E. and Scaife, A. M. M. and Schofield, J. and Scott, P. F. and Shaw, C. and Shimwell, T. W. and Smith, H. and Taylor, A. C. and Titterington, D. J. and Velić, M. and Waldram, E. M. and West, S. and Wood, B. A. and Yassin, G.},
title = {The Arcminute Microkelvin Imager},
volume = {391},
number = {4},
pages = {1545-1558},
year = {2008},
doi = {10.1111/j.1365-2966.2008.13953.x},
abstract ={The Arcminute Microkelvin Imager is a pair of interferometer arrays operating with six frequency channels spanning 13.9–18.2 GHz, for observations on angular scales of 30 arcsec–10 arcmin and for declinations greater than −15°; the Small Array has a sensitivity of 30 mJy s−1/2 and the Large Array has a sensitivity of 3 mJy s−1/2. The telescope is aimed principally at Sunyaev–Zel'dovich imaging of clusters of galaxies. We discuss the design of the telescope and describe and explain its electronic and mechanical systems.},
URL = {http://mnras.oxfordjournals.org/content/391/4/1545.abstract},
eprint = {http://mnras.oxfordjournals.org/content/391/4/1545.full.pdf+html},
journal = {Monthly Notices of the Royal Astronomical Society}
}
@article{Foster11042014,
author = {Foster, G. and Hickish, J. and Magro, A. and Price, D. and Zarb Adami, K.},
title = {Implementation of a direct-imaging and FX correlator for the BEST-2 array},
volume = {439},
number = {3},
pages = {3180-3188},
year = {2014},
doi = {10.1093/mnras/stu188},
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.},
URL = {http://mnras.oxfordjournals.org/content/439/3/3180.abstract},
eprint = {http://mnras.oxfordjournals.org/content/439/3/3180.full.pdf+html},
journal = {Monthly Notices of the Royal Astronomical Society}
}
@ARTICLE{2014MNRAS.445.1084Z,
author = {{Zheng}, H. and {Tegmark}, M. and {Buza}, V. and {Dillon}, J.~S. and
{Gharibyan}, H. and {Hickish}, J. and {Kunz}, E. and {Liu}, A. and
{Losh}, J. and {Lutomirski}, A. and {Morrison}, S. and {Narayanan}, S. and
{Perko}, A. and {Rosner}, D. and {Sanchez}, N. and {Schutz}, K. and
{Tribiano}, S.~M. and {Valdez}, M. and {Yang}, H. and {Adami}, K.~Z. and
{Zelko}, I. and {Zheng}, K. and {Armstrong}, R.~P. and {Bradley}, R.~F. and
{Dexter}, M.~R. and {Ewall-Wice}, A. and {Magro}, A. and {Matejek}, M. and
{Morgan}, E. and {Neben}, A.~R. and {Pan}, Q. and {Penna}, R.~F. and
{Peterson}, C.~M. and {Su}, M. and {Villasenor}, J. and {Williams}, C.~L. and
{Zhu}, Y.},
title = "{MITEoR: a scalable interferometer for precision 21 cm cosmology}",
journal = {Monthly Notices of the Royal Astronomical Society},
archivePrefix = "arXiv",
eprint = {1405.5527},
primaryClass = "astro-ph.IM",
keywords = {instrumentation: interferometers, methods: data analysis, techniques: interferometric, cosmology: observations, dark ages, reionization, first stars},
year = 2014,
month = dec,
volume = 445,
pages = {1084-1103},
doi = {10.1093/mnras/stu1773},
adsurl = {http://adsabs.harvard.edu/abs/2014MNRAS.445.1084Z},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@booklet{cliff16,
author = "Clifford van Dyk",
title = "{SKARAB Hello World}",
howpublished = "Peralex",
address = "Cape Town, South Africa",
year = "2016"}
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author = "A. Parsons and D. Backer and C. Chang and D. Chapman and H. Chen and P. Droz and C. de Jesus and D. MacMahon and A. Siemion and J. Wawrzynek and D. Werthimer and M. Wright",
title = "{A New Approach to Radio Astronomy Signal Processing: Packet Switched, FPGA-based, Upgradeable, Modular Hardware and reusable, Platform-Independent Signal Processing Libraries}",
booktitle = "Proceedings of the 28th General Assembly of the International Union of Radio Science",
address = "Boulder, Colorado",
month = "Oct",
year = "2005",
pages = "18"}
@misc{Weinreb,
title={Digital radiometer},
author={Weinreb, Sander},
journal={Proceedings of the Institute of Radio Engineers},
volume={49},
number={6},
pages={1099},
year={1961}
}
@article{chennamangalam2014gpu,
title = {A gpu-based wide-band radio spectrometer},
author = {Chennamangalam, Jayanth and Scott, Simon and Jones, Glenn and Chen, Hong and Ford, John and Kepley, Amanda and Lorimer, DR and Nie, Jun and Prestage, Richard and Roshi, D Anish and others},
journal = {Publications of the Astronomical Society of Australia},
volume = {31},
pages = {e048},
year = {2014},
publisher={Cambridge Univ Press}
}
@misc{skynet,
author = "Ghigo, Frank and Heatherly, Sue Ann ",
title = "SKYNET",
year = "2015",
note = "\url{http://www.gb.nrao.edu/20m/}."
}
@inproceedings{guppi,
author = {DuPlain, Ron and Ransom, Scott and Demorest, Paul and Brandt, Patrick and Ford, John and Shelton, Amy L.},
title = {Launching GUPPI: the Green Bank Ultimate Pulsar Processing Instrument},
journal = {Proc. SPIE},
volume = {7019},
number = {},
pages = {70191D-70191D-10},
year = {2008},
doi = {10.1117/12.790003},
URL = { http://dx.doi.org/10.1117/12.790003},
}
@article{2016JLTP..184..460S,
author = {Stanchfield, S.~M. and Ade, P.~A.~R. and Aguirre, J. and Brevik, J.~A. and Cho, H.~M. and Datta, R. and Devlin, M.~J. and Dicker, S.~R. and Dober, B. and Egan, D. and Ford, P. and Hilton, G. and Hubmayr, J. and Irwin, K.~D. and Marganian, P. and Mason, B.~S. and Mates, J.~A.~B. and McMahon, J. and Mello, M. and Mroczkowski, T. and Romero, C. and Tucker, C. and Vale, L. and White, S. and Whitehead, M. and Young, A.~H.},
title = "{Development of a Microwave SQUID-Multiplexed TES Array for MUSTANG-2}",
journal = {Journal of Low Temperature Physics},
keywords = {Microwave-multiplexed SQUIDs, TES bolometers, Focal plane arrays, 90 GHz},
year = 2016,
month = jul,
volume = 184,
pages = {460-465},
doi = {10.1007/s10909-016-1570-4},
adsurl = {http://adsabs.harvard.edu/abs/2016JLTP..184..460S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2014JLTP..176..808D,
author = {Dicker, S.~R. and Ade, P.~A.~R. and Aguirre, J. and Brevik, J.~A. and Cho, H.~M. and Datta, R. and Devlin, M.~J. and Dober, B. and Egan, D. and Ford, J. and Ford, P. and Hilton, G. and Irwin, K.~D. and Mason, B.~S. and Marganian, P. and Mello, M. and McMahon, J.~J. and Mroczkowski, T. and Rosenman, M. and Tucker, C. and Vale, L. and White, S. and Whitehead, M. and Young, A.~H.},
title = "{MUSTANG 2: A Large Focal Plane Array for the 100 m Green Bank Telescope}",
journal = {Journal of Low Temperature Physics},
keywords = {TES bolometers, Focal plane arrays, 90 GHz, Green Bank Telescope, Frequency domain readout},
year = 2014,
month = sep,
volume = 176,
pages = {808-814},
doi = {10.1007/s10909-013-1070-8},
adsurl = {http://adsabs.harvard.edu/abs/2014JLTP..176..808D},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{gb_flag,
author = {Morgan, M.~A. and Fisher, J.~R. and Castro, J.~J.},
title = "{Unformatted Digital Fiber-Optic Data Transmission for Radio Astronomy Front-Ends}",
journal = {Publications of the Astronomical Society of the Pacific},
keywords = {},
year = 2013,
month = may,
volume = 125,
pages = {},
doi = {10.1086/671349},
adsurl = {},
adsnote = {}
}
@misc{gb_beamformer,
author = "FLAG and Beamformer",
title = "Wide-Field L-band Focal Plane Array Beamformer for Pulsar, Diffuse Hydrogen, and Fast Transient Surveys on the GBT",
year = "2016",
note = "\url{https://safe.nrao.edu/wiki/bin/view/Beamformer/WebHome}."
}
@misc{gbtrans,
author = "Steve Ellingson",
title = "Transient events",
year = "",
note = ""
}
@phdthesis{hickish14,
author = {Jack Hickish},
title = {Digital signal processing methods for large-N, low-frequency radio telescopes},
school = {University of Oxford},
year = 2014,
month = 7,
address = {Oxford, United Kingdom}
}
@phdthesis{price13,
author = {Daniel Price},
title = {Radio astronomy instrumentation for redshifted hydrogen line science},
school = {University of Oxford},
year = 2013,
month = 7,
address = {Oxford, United Kingdom}
}
@ARTICLE{2013arXiv1303.2131M,
author = {{Max-Moerbeck}, W. and {Richards}, J.~L. and {Pavlidou}, V. and
{Pearson}, T.~J. and {Readhead}, A.~C.~S. and {on behalf of the Fermi LAT collaboration} and
{Hovatta}, T. and {King}, O.~G. and {Reeves}, R.},
title = "{OVRO 40 m Blazar Monitoring Program: Location of the gamma-ray emission region in blazars by the study of correlated variability at radio and gamma-rays}",
journal = {ArXiv e-prints},
archivePrefix = "arXiv",
eprint = {1303.2131},
primaryClass = "astro-ph.HE",
keywords = {Astrophysics - High Energy Astrophysical Phenomena},
year = 2013,
month = mar,
adsurl = {http://adsabs.harvard.edu/abs/2013arXiv1303.2131M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2010MNRAS.409..619K,
author = {{Keith}, M.~J. and {Jameson}, A. and {van Straten}, W. and {Bailes}, M. and
{Johnston}, S. and {Kramer}, M. and {Possenti}, A. and {Bates}, S.~D. and
{Bhat}, N.~D.~R. and {Burgay}, M. and {Burke-Spolaor}, S. and
{D'Amico}, N. and {Levin}, L. and {McMahon}, P.~L. and {Milia}, S. and
{Stappers}, B.~W.},
title = "{The High Time Resolution Universe Pulsar Survey - I. System configuration and initial discoveries}",
journal = {Monthly Notices of the Royal Astronomical Society},
archivePrefix = "arXiv",
eprint = {1006.5744},
primaryClass = "astro-ph.HE",
keywords = {pulsars: general},
year = 2010,
month = dec,
volume = 409,
pages = {619-627},
doi = {10.1111/j.1365-2966.2010.17325.x},
adsurl = {http://adsabs.harvard.edu/abs/2010MNRAS.409..619K},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{doi:10.1142/S2251171715500038,
author = {Kocz, J. and Greenhill, L. J. and Barsdell, B. R. and Price, D. and Bernardi, G. and Bourke, S. and Clark, M. A. and Craig, J. and Dexter, M. and Dowell, J. and Eftekhari, T. and Ellingson, S. and Hallinan, G. and Hartman, J. and Jameson, A. and MacMahon, D. and Taylor, G. and Schinzel, F. and Werthimer, D.},
title = {Digital Signal Processing Using Stream High Performance Computing},
journal = {Journal of Astronomical Instrumentation},
volume = {04},
number = {01n02},
pages = {1550003},
year = {2015},
doi = {10.1142/S2251171715500038},
URL = {http://www.worldscientific.com/doi/abs/10.1142/S2251171715500038},
eprint = {http://www.worldscientific.com/doi/pdf/10.1142/S2251171715500038}
}
@ARTICLE{2014MNRAS.443.3752L,
author = {{Liu}, K. and {Desvignes}, G. and {Cognard}, I. and {Stappers}, B.~W. and
{Verbiest}, J.~P.~W. and {Lee}, K.~J. and {Champion}, D.~J. and
{Kramer}, M. and {Freire}, P.~C.~C. and {Karuppusamy}, R.},
title = "{Measuring pulse times of arrival from broad-band pulsar observations}",
journal = {Monthly Notices of the Royal Astronomical Society},
archivePrefix = "arXiv",
eprint = {1407.3827},
keywords = {methods: data analysis, pulsars: general, pulsars: individual (PSR J1909-3744)},
year = 2014,
month = oct,
volume = 443,
pages = {3752-3760},
doi = {10.1093/mnras/stu1420},
adsurl = {http://adsabs.harvard.edu/abs/2014MNRAS.443.3752L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@INPROCEEDINGS{7180719,
author={A. Morselli and P. Di Lizia and G. Bianchi and C. Bortolotti and S. Montebugnoli and G. Naldi and F. Perini and G. Pupillo and M. Roma and M. Schiaffino and A. Mattana and E. Salerno and A. Magro and K. Z. Adami and R. Armellin and A. L. Sergiusti and W. Villadei and F. Dolce and M. Reali and J. Paoli},
booktitle={Metrology for Aerospace (MetroAeroSpace), 2015 IEEE},
title={A new high sensitivity radar sensor for space debris detection and accurate orbit determination},
year={2015},
pages={562-567},
keywords={aerospace instrumentation;collision avoidance;space debris;spaceborne radar;Earth-orbiting object observation;accurate orbit determination;collision avoidance;debris trajectory prediction;high sensitivity radar sensor;innovative bistatic radar system;manned spacecraft;multibeaming techniques;numerical simulations;operative satellites;ranging techniques;space debris detection;space missions;Bistatic radar;Orbits;Radar antennas;Receivers;Space debris;Trajectory;Multibeam;beamforming;bistatic radar;orbit determination;pulse compression;space debris},
doi={10.1109/MetroAeroSpace.2015.7180719},
month={June},}
@Article{Pupillo2015,
author="Pupillo, G.
and Naldi, G.
and Bianchi, G.
and Mattana, A.
and Monari, J.
and Perini, F.
and Poloni, M.
and Schiaffino, M.
and Bolli, P.
and Lingua, A.
and Aicardi, I.
and Bendea, H.
and Maschio, P.
and Piras, M.
and Virone, G.
and Paonessa, F.
and Farooqui, Z.
and Tibaldi, A.
and Addamo, G.
and Peverini, O. A.
and Tascone, R.
and Wijnholds, S. J.",
title="Medicina array demonstrator: calibration and radiation pattern characterization using a UAV-mounted radio-frequency source",
journal="Experimental Astronomy",
year="2015",
volume="39",
number="2",
pages="405--421",
abstract="One of the most challenging aspects of the new-generation Low-Frequency Aperture Array (LFAA) radio telescopes is instrument calibration. The operational LOw-Frequency ARray (LOFAR) instrument and the future LFAA element of the Square Kilometre Array (SKA) require advanced calibration techniques to reach the expected outstanding performance. In this framework, a small array, called Medicina Array Demonstrator (MAD), has been designed and installed in Italy to provide a test bench for antenna characterization and calibration techniques based on a flying artificial test source. A radio-frequency tone is transmitted through a dipole antenna mounted on a micro Unmanned Aerial Vehicle (UAV) (hexacopter) and received by each element of the array. A modern digital FPGA-based back-end is responsible for both data-acquisition and data-reduction. A simple amplitude and phase equalization algorithm is exploited for array calibration owing to the high stability and accuracy of the developed artificial test source. Both the measured embedded element patterns and calibrated array patterns are found to be in good agreement with the simulated data. The successful measurement campaign has demonstrated that a UAV-mounted test source provides a means to accurately validate and calibrate the full-polarized response of an antenna/array in operating conditions, including consequently effects like mutual coupling between the array elements and contribution of the environment to the antenna patterns. A similar system can therefore find a future application in the SKA-LFAA context.",
issn="1572-9508",
doi="10.1007/s10686-015-9456-z",
url="http://dx.doi.org/10.1007/s10686-015-9456-z"
}
@article {RDS:RDS20336,
author = {Bolli, P. and Pupillo, G. and Virone, G. and Farooqui, M. Z. and Lingua, A. and Mattana, A. and Monari, J. and Murgia, M. and Naldi, G. and Paonessa, F. and Perini, F. and Pluchino, S. and Rusticelli, S. and Schiaffino, M. and Schillirò, F. and Tartarini, G. and Tibaldi, A.},
title = {From MAD to SAD: The Italian experience for the low-frequency aperture array of SKA1-LOW},
journal = {Radio Science},
volume = {51},
number = {3},
issn = {1944-799X},
url = {http://dx.doi.org/10.1002/2015RS005922},
doi = {10.1002/2015RS005922},
pages = {160--175},
keywords = {Antenna arrays, Radio astronomy, Instruments and techniques, Instruments and techniques, aperture array, radio astronomy, calibration, unmanned aerial vehicle},
year = {2016},
note = {2015RS005922},
}
@article{10.1086/674013,
ISSN = {00046280, 15383873},
URL = {http://www.jstor.org/stable/10.1086/674013},
abstract = {We present the design, construction, and commissioning results of ARCONS, the Array Camera for Optical to Near-IR Spectrophotometry. ARCONS is the first ground-based instrument in the optical through near-IR wavelength range based on microwave kinetic inductance detectors (MKIDs). MKIDs are revolutionary cryogenic detectors, capable of detecting single photons and measuring their energy without filters or gratings, similar to an X-ray microcalorimeter. MKIDs are nearly ideal, noiseless photon detectors, as they do not suffer from read noise or dark current and have nearly perfect cosmic ray rejection. ARCONS is an integral field spectrograph (IFS) containing a lens-coupled 2024 pixel MKID array yielding a 20″ × 20″ field of view and has been deployed on the Palomar 200 inch and Lick 120 inch telescopes for 24 nights of observing. We present initial results showing that ARCONS and its MKID arrays are now a fully operational and powerful tool for astronomical observations.},
author = {B. A. Mazin and S. R. Meeker and M. J. Strader and P. Szypryt and D. Marsden and J. C. van Eyken and G. E. Duggan and A. B. Walter and G. Ulbricht and M. Johnson and B. Bumble and K. O’Brien and C. Stoughton},
journal = {Publications of the Astronomical Society of the Pacific},
number = {933},
pages = {1348-1361},
publisher = {[University of Chicago Press, Astronomical Society of the Pacific]},
title = {ARCONS: A 2024 Pixel Optical through Near-IR Cryogenic Imaging Spectrophotometer},
volume = {125},
year = {2013}
}
@mastersthesis{MScSalas2014,
author = {{Salas}, P.},
title = {A two element radio interferometer for education},
school = {Pontificia Universidad Cat\'olica de Chile},
year = 2014,
month = 8,
}
@INPROCEEDINGS{amiba-adc,
author={H. Jiang and H. Liu and K. Guzzino and D. Kubo and C. T. Li and R. Chang},
booktitle={Electronics, Circuits and Systems (ICECS), 2012 19th IEEE International Conference on},
title={Digitizing The Yuan Tseh Lee Array for Microwave Background Anisotropy by 5Gsps ADC boards},
year={2012},
pages={304-307},
keywords={radiotelescopes;ADC boards;ENOB;SFDR;SINAD;Yuan Tseh Lee Array for Microwave Background Anisotropy;analog-to-digital printed circuit board;bit rate 8 bit/s;digital correlator system;digitize input radio frequencies;field programmable gate array platform;frequency 2.5 GHz;radio telescopes;Arrays;Bandwidth;Connectors;Field programmable gate arrays;Gain;Noise;Tuning},
doi={10.1109/ICECS.2012.6463741},
month={Dec},}
@INPROCEEDINGS{amiba-interim,
author={H. Jiang and H. Liu and R. Chang},
booktitle={General Assembly and Scientific Symposium (URSI GASS), 2014 XXXIth URSI},
title={Design of an interim digital spectro-correlator for the Yuan Tseh Lee array for microwave background anisotropy},
year={2014},
pages={1-4},
keywords={correlators;microwave antenna arrays;ADC board;AMiBA;Allen deviation;CO intensity mapping;FX-type correlator;ROACH2;Yuan Tseh Lee array;analog system;analog to digital converter;bandwidth 1.6 GHz;correlation accumulators;cross-correlation;four reconfigurable open architecture computing hardware 2 systems;four-antenna digital spectro-correlator;interim digital spectro-correlator design;microwave background anisotropy;optimal input power;polarization;spectral channels;word length 8 bit;Antennas;Arrays;Correlators;Engines;Field programmable gate arrays;Hardware;Optical switches;Correlator;Field Programmable Gate Array (FPGA);Interferometer},
doi={10.1109/URSIGASS.2014.6930032},
month={Aug},}
@ARTICLE{2016arXiv160607473D,
author = {{DeBoer}, D.~R. and {Parsons}, A.~R. and {Aguirre}, J.~E. and
{Alexander}, P. and {Ali}, Z.~S. and {Beardsley}, A.~P. and
{Bernardi}, G. and {Bowman}, J.~D. and {Bradley}, R.~F. and
{Carilli}, C.~L. and {Cheng}, C. and {de Lera Acedo}, E. and
{Dillon}, J.~S. and {Ewall-Wice}, A. and {Fadana}, G. and {Fagnoni}, N. and
{Fritz}, R. and {Furlanetto}, S.~R. and {Glendenning}, B. and
{Greig}, B. and {Grobbelaar}, J. and {Hazelton}, B.~J. and {Hewitt}, J.~N. and
{Hickish}, J. and {Jacobs}, D.~C. and {Julius}, A. and {Kariseb}, M. and
{Kohn}, S.~A. and {Lekalake}, T. and {Liu}, A. and {Loots}, A. and
{MacMahon}, D. and {Malan}, L. and {Malgas}, C. and {Maree}, M. and
{Mathison}, N. and {Matsetela}, E. and {Mesinger}, A. and {Morales}, M.~F. and
{Neben}, A.~R. and {Patra}, N. and {Pieterse}, S. and {Pober}, J.~C. and
{Razavi-Ghods}, N. and {Ringuette}, J. and {Robnett}, J. and
{Rosie}, K. and {Sell}, R. and {Smith}, C. and {Syce}, A. and
{Tegmark}, M. and {Thyagarajan}, N. and {Williams}, P.~K.~G. and
{Zheng}, H.},
title = "{Hydrogen Epoch of Reionization Array (HERA)}",
journal = {ArXiv e-prints},
archivePrefix = "arXiv",
eprint = {1606.07473},
primaryClass = "astro-ph.IM",
keywords = {Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics},
year = 2016,
month = jun,
adsurl = {http://adsabs.harvard.edu/abs/2016arXiv160607473D},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2010AJ....139.1468P,
author = {{Parsons}, A.~R. and {Backer}, D.~C. and {Foster}, G.~S. and
{Wright}, M.~C.~H. and {Bradley}, R.~F. and {Gugliucci}, N.~E. and
{Parashare}, C.~R. and {Benoit}, E.~E. and {Aguirre}, J.~E. and
{Jacobs}, D.~C. and {Carilli}, C.~L. and {Herne}, D. and {Lynch}, M.~J. and
{Manley}, J.~R. and {Werthimer}, D.~J.},
title = "{The Precision Array for Probing the Epoch of Re-ionization: Eight Station Results}",
journal = {The Astrophysical Journal},
archivePrefix = "arXiv",
eprint = {0904.2334},
keywords = {cosmology: observations, instrumentation: interferometers, radio continuum: general, techniques: interferometric, site testing, telescopes},
year = 2010,
month = apr,
volume = 139,
pages = {1468-1480},
doi = {10.1088/0004-6256/139/4/1468},
adsurl = {http://adsabs.harvard.edu/abs/2010AJ....139.1468P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2014ApJ...788..106P,
author = {{Parsons}, A.~R. and {Liu}, A. and {Aguirre}, J.~E. and {Ali}, Z.~S. and
{Bradley}, R.~F. and {Carilli}, C.~L. and {DeBoer}, D.~R. and
{Dexter}, M.~R. and {Gugliucci}, N.~E. and {Jacobs}, D.~C. and
{Klima}, P. and {MacMahon}, D.~H.~E. and {Manley}, J.~R. and
{Moore}, D.~F. and {Pober}, J.~C. and {Stefan}, I.~I. and {Walbrugh}, W.~P.
},
title = "{New Limits on 21 cm Epoch of Reionization from PAPER-32 Consistent with an X-Ray Heated Intergalactic Medium at z = 7.7}",
journal = {The Astrophysical Journal},
archivePrefix = "arXiv",
eprint = {1304.4991},
keywords = {cosmology: observations, dark ages, reionization, first stars, early universe, instrumentation: interferometers, intergalactic medium, radio continuum: general},
year = 2014,
month = jun,
volume = 788,
eid = {106},
pages = {106},
doi = {10.1088/0004-637X/788/2/106},
adsurl = {http://adsabs.harvard.edu/abs/2014ApJ...788..106P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2015ApJ...809...61A,
author = {{Ali}, Z.~S. and {Parsons}, A.~R. and {Zheng}, H. and {Pober}, J.~C. and
{Liu}, A. and {Aguirre}, J.~E. and {Bradley}, R.~F. and {Bernardi}, G. and
{Carilli}, C.~L. and {Cheng}, C. and {DeBoer}, D.~R. and {Dexter}, M.~R. and
{Grobbelaar}, J. and {Horrell}, J. and {Jacobs}, D.~C. and {Klima}, P. and
{MacMahon}, D.~H.~E. and {Maree}, M. and {Moore}, D.~F. and
{Razavi}, N. and {Stefan}, I.~I. and {Walbrugh}, W.~P. and {Walker}, A.
},
title = "{PAPER-64 Constraints on Reionization: The 21 cm Power Spectrum at z = 8.4}",
journal = {The Astrophysical Journal},
archivePrefix = "arXiv",
eprint = {1502.06016},
keywords = {cosmology: observations, dark ages, reionization, first stars, early universe, instrumentation: interferometers, intergalactic medium},
year = 2015,
month = aug,
volume = 809,
eid = {61},
pages = {61},
doi = {10.1088/0004-637X/809/1/61},
adsurl = {http://adsabs.harvard.edu/abs/2015ApJ...809...61A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{flyseye,
author = {{Siemion}, A.~P.~V. and {Bower}, G.~C. and {Foster}, G. and
{McMahon}, P.~L. and {Wagner}, M.~I. and {Werthimer}, D. and
{Backer}, D. and {Cordes}, J. and {van Leeuwen}, J.},
title = "{The Allen Telescope Array Fly's Eye Survey for Fast Radio Transients}",
journal = {The Astrophysical Journal},
archivePrefix = "arXiv",
eprint = {1109.2659},
primaryClass = "astro-ph.HE",
keywords = {instrumentation: detectors, intergalactic medium, methods: data analysis, pulsars: general, radio continuum: general},
year = 2012,
month = jan,
volume = 744,
eid = {109},
pages = {109},
doi = {10.1088/0004-637X/744/2/109},
adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...744..109S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{seti,
author = {{Siemion}, A.~P.~V. and {Cobb}, J. and {Chen}, H. and {Cordes}, J. and
{Filiba}, T. and {Foster}, G. and {Fries}, A. and {Howard}, A. and
{von Korff}, J. and {Korpela}, E. and {Lebofsky}, M. and {McMahon}, P.~L. and
{Parsons}, A. and {Spitler}, L. and {Wagner}, M. and {Werthimer}, D.
},
title = "{Current and Nascent SETI Instruments}",
journal = {ArXiv e-prints},
archivePrefix = "arXiv",
eprint = {1109.1136},
primaryClass = "astro-ph.IM",
keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
year = 2011,
month = sep,
adsurl = {http://adsabs.harvard.edu/abs/2011arXiv1109.1136S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{fast,
author = {{Nan}, R. and {Li}, D. and {Jin}, C. and {Wang}, Q. and {Zhu}, L. and
{Zhu}, W. and {Zhang}, H. and {Yue}, Y. and {Qian}, L.},
title = "{The Five-Hundred Aperture Spherical Radio Telescope (fast) Project}",
journal = {International Journal of Modern Physics D},
archivePrefix = "arXiv",
eprint = {1105.3794},
primaryClass = "astro-ph.IM",
keywords = {Radio telescope, active main reflector, HI 21cm line, pulsar},
year = 2011,
volume = 20,
pages = {989-1024},
doi = {10.1142/S0218271811019335},
adsurl = {http://adsabs.harvard.edu/abs/2011IJMPD..20..989N},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{vegas,
author = {{Anish Roshi}, D. and {Bloss}, M. and {Brandt}, P. and {Bussa}, S. and
{Chen}, H. and {Demorest}, P. and {Desvignes}, G. and {Filiba}, T. and
{Fisher}, R.~J. and {Ford}, J. and {Frayer}, D. and {Garwood}, R. and
{Gowda}, S. and {Jones}, G. and {Mallard}, B. and {Masters}, J. and
{McCullough}, R. and {Molera}, G. and {O'Neil}, K. and {Ray}, J. and
{Scott}, S. and {Shelton}, A. and {Siemion}, A. and {Wagner}, M. and
{Watts}, G. and {Werthimer}, D. and {Whitehead}, M.},
title = "{Advanced Multi-beam Spectrometer for the Green Bank Telescope}",
journal = {ArXiv e-prints},
archivePrefix = "arXiv",
eprint = {1202.0938},
primaryClass = "astro-ph.IM",
keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
year = 2012,
month = feb,
adsurl = {http://adsabs.harvard.edu/abs/2012arXiv1202.0938A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@INPROCEEDINGS{dsn-transient-observatory,
author = {{Kuiper}, T.~B. and {Lazio}, T.~J. and {Majid}, W.~A. and {Navarro}, R. and
{Teitelbaum}, L.~P. and {Trinh}, J.~T.},
title = "{DSN Transient Observatory}",
booktitle = {American Astronomical Society Meeting Abstracts \#221},
year = 2013,
series = {American Astronomical Society Meeting Abstracts},
volume = 221,
month = jan,
eid = {439.14},
pages = {439.14},
adsurl = {http://adsabs.harvard.edu/abs/2013AAS...22143914K},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{specbook,
author = {{Price}, D.~C.},
title = "{Spectrometers and Polyphase Filterbanks in Radio Astronomy}",
journal = {ArXiv e-prints},
archivePrefix = "arXiv",
eprint = {1607.03579},
primaryClass = "astro-ph.IM",
keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
year = 2016,
month = jul,
adsurl = {http://adsabs.harvard.edu/abs/2016arXiv160703579P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{evla,
author={R. A. Perley and C. J. Chandler and B. J. Butler and J. M. Wrobel},
title={The Expanded Very Large Array: A New Telescope for New Science},
journal={The Astrophysical Journal Letters},
volume={739},
number={1},
pages={L1},
url={http://stacks.iop.org/2041-8205/739/i=1/a=L1},
year={2011},
abstract={Since its commissioning in 1980, the Very Large Array (VLA) has consistently demonstrated its scientific productivity. However, its fundamental capabilities have changed little since 1980, particularly in the key areas of sensitivity, frequency coverage, and velocity resolution. These limitations have been addressed by a major upgrade of the array, which began in 2001 and will be completed at the end of 2012. When completed, the Expanded VLA—the EVLA—will provide complete frequency coverage from 1 to 50 GHz, a continuum sensitivity of typically 1 μJy beam –1 (in 9 hr with full bandwidth), and a modern correlator with vastly greater capabilities and flexibility than the VLA's. In this Letter, we describe the goals of the EVLA project, its current status, and the anticipated expansion of capabilities over the next few years. User access to the array through the Open Shared Risk Observing and Resident Shared Risk Observing programs is described. The following papers in this special issue, derived from observations in its early science period, demonstrate the astonishing breadth of this most flexible and powerful general-purpose telescope.}
}
@ARTICLE{bee2,
author={C. Chang and J. Wawrzynek and R. W. Brodersen},
journal={IEEE Design Test of Computers},
title={BEE2: a high-end reconfigurable computing system},
year={2005},
volume={22},
number={2},
pages={114-125},
keywords={digital signal processing chips;microprocessor chips;performance evaluation;real-time systems;reconfigurable architectures;Berkeley Emulation Engine 2;DSP-based system;high-end reconfigurable computing system;microprocessor-based system;processing-module building block;Application software;Computational modeling;Digital signal processing;Digital signal processing chips;Emulation;Energy consumption;Field programmable gate arrays;Hardware;Radio astronomy;Throughput},
doi={10.1109/MDT.2005.30},
ISSN={0740-7475},
month={March},}
@misc{private-mo,
author = "Ohady, Mo",
date = "2016-07-21",
howpublished = "private communication"
}
@proceeding{uniboard,
author = {Hargreaves, J. E.},