Related papers: A Particle Detector Array deployed to the Murchiso…

An image-based blind search for Fast Radio Bursts in 88 hours of data from the EoR0 Field, with the Murchison Widefield Array

This work is part of ongoing efforts to detect Fast Radio Bursts (FRBs) using the Murchison Widefield Array (MWA) in a spectral window below 300 MHz. We used an image-based method based on the pilot study of Tingay et al. 2015, scaled up…

Instrumentation and Methods for Astrophysics · Physics 2024-09-06 Ian Kemp , Steven Tingay , Stuart Midgley , Daniel Mitchell

The challenges of low-frequency radio polarimetry: lessons from the Murchison Widefield Array

We present techniques developed to calibrate and correct Murchison Widefield Array (MWA) low frequency (72-300 MHz) radio observations for polarimetry. The extremely wide field-of-view, excellent instantaneous (u, v)-coverage and…

Instrumentation and Methods for Astrophysics · Physics 2017-10-04 Emil Lenc , C. S. Anderson , N. Barry , J. D. Bowman , I. H. Cairns , J. S. Farnes , B. M. Gaensler , G. Heald , M. Johnston-Hollitt , D. L. Kaplan , C. R. Lynch , P. I. McCauley , D. A. Mitchell , J. Morgan , M. F. Morales , T. Murphy , A. R. Offringa , S. M. Ord , B. Pindor , C. Riseley , E. M. Sadler , C. Sobey , M. Sokolowski , I. S. Sullivan , S. P. O'Sullivan , X. H. Sun , S. E. Tremblay , C. M. Trott , R. B. Wayth

Influence of a planar boundary on the electric field emitted by a particle shower

The radio detection of cosmic rays consists in the estimation of the properties of a primary cosmic ray by observing the electric field emitted by the extensive air shower (EAS) created when the primary cosmic ray enters the atmosphere.…

High Energy Astrophysical Phenomena · Physics 2019-03-27 Daniel García-Fernández , Benoît Revenu , Antony Escudie , Lilian Martin

A search for Fast Radio Bursts at low frequencies with Murchison Widefield Array high time resolution imaging

We present the results of a pilot study search for Fast Radio Bursts (FRBs) using the Murchison Widefield Array (MWA) at low frequencies (139 - 170 MHz). We utilised MWA data obtained in a routine imaging mode from observations where the…

Cosmology and Nongalactic Astrophysics · Physics 2015-12-16 S. J. Tingay , C. M. Trott , R. B. Wayth , G. Bernardi , J. D. Bowman , F. Briggs , R. J. Cappallo , A. A. Deshpande , L. Feng , B. M. Gaensler , L. J. Greenhill , P. J. Hancock , B. J. Hazelton , M. Johnston-Hollitt , D. L. Kaplan , C. J. Lonsdale , S. R. McWhirter , D. A. Mitchell , M. F. Morales , E. Morgan , T. Murphy , D. Oberoi , T. Prabu , N. Udaya Shankar , K. S. Srivani , R. Subrahmanyan , R. L. Webster , A. Williams , C. L. Williams

Multi-epoch Low Radio Frequency Surveys of the Kepler K2 Mission Campaign Fields 3, 4, and 5 with the Murchison Widefield Array

We present Murchison Widefield Array (MWA) monitoring of the Kepler K2 mission Fields 3, 4, and 5 at frequencies of 155 and 186 MHz, from observations contemporaneous with the K2 observations. This work follows from previous MWA and GMRT…

High Energy Astrophysical Phenomena · Physics 2019-07-10 S. J. Tingay , P. J Hancock

A Model-Independent Method of Determining Energy Scale and Muon Number in Cosmic Ray Surface Detectors

Surface detector arrays are designed to measure the spectrum and composition of high-energy cosmic rays by detecting the secondary particle flux of the Extensive Air Showers (EAS) induced by the primary cosmic rays. Electromagnetic…

Astrophysics · Physics 2008-11-26 Fabian Schmidt , Maximo Ave , Lorenzo Cazon , Aaron Chou

Radio detection of cosmic rays with the Auger Engineering Radio Array

The very low statistics of cosmic rays above the knee region make their study possible only through the detection of the extensive air showers (EAS) produced by their interaction with the constituents of the atmosphere. The Pierre Auger…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Florian Gaté

First Season MWA EoR Power Spectrum Results at Redshift 7

The Murchison Widefield Array (MWA) has collected hundreds of hours of Epoch of Reionization (EoR) data and now faces the challenge of overcoming foreground and systematic contamination to reduce the data to a cosmological measurement. We…

Instrumentation and Methods for Astrophysics · Physics 2016-12-13 A. P. Beardsley , B. J. Hazelton , I. S. Sullivan , P. Carroll , N. Barry , M. Rahimi , B. Pindor , C. M. Trott , J. Line , Daniel C. Jacobs , M. F. Morales , J. C. Pober , G. Bernardi , Judd D. Bowman , M. P. Busch , F. Briggs , R. J. Cappallo , B. E. Corey , A. de Oliveira-Costa , Joshua S. Dillon , D. Emrich , A. Ewall-Wice , L. Feng , B. M. Gaensler , R. Goeke , L. J. Greenhill , J. N. Hewitt , N. Hurley-Walker , M. Johnston-Hollitt , D. L. Kaplan , J. C. Kasper , H. S. Kim , E. Kratzenberg , E. Lenc , A. Loeb , C. J. Lonsdale , M. J. Lynch , B. McKinley , S. R. McWhirter , D. A. Mitchell , E. Morgan , A. R. Neben , Nithyanandan Thyagarajan , D. Oberoi , A. R. Offringa , S. M. Ord , S. Paul , T. Prabu , P. Procopio , J. Riding , A. E. E. Rogers , A. Roshi , N. Udaya Shankar , Shiv K. Sethi , K. S. Srivani , R. Subrahmanyan , M. Tegmark , S. J. Tingay , M. Waterson , R. B. Wayth , R. L. Webster , A. R. Whitney , A. Williams , C. L. Williams , C. Wu , J. S. B. Wyithe

Trigger and Aperture of the Surface Detector Array of the Pierre Auger Observatory

The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detectors, for the study of extensive air showers (EAS) generated by ultra-high-energy cosmic rays. We describe the trigger hierarchy, from the…

Instrumentation and Methods for Astrophysics · Physics 2014-07-03 J. Abraham , P. Abreu , M. Aglietta , C. Aguirre , E. J. Ahn , D. Allard , I. Allekotte , J. Allen , J. Alvarez-Muñiz , M. Ambrosio , L. Anchordoqui , S. Andringa , A. Anzalone , C. Aramo , E. Arganda , S. Argirò , K. Arisaka , F. Arneodo , F. Arqueros , T. Asch , H. Asorey , P. Assis , J. Aublin , M. Ave , G. Avila , T. Bäcker , D. Badagnani , K. B. Barber , A. F. Barbosa , S. L. C. Barroso , B. Baughman , P. Bauleo , J. J. Beatty , T. Beau , B. R. Becker , K. H. Becker , A. Bellétoile , J. A. Bellido , S. BenZvi , C. Berat , P. Bernardini , X. Bertou , P. L. Biermann , P. Billoir , O. Blanch-Bigas , F. Blanco , C. Bleve , H. Blümer , M. Boháčová , D. Boncioli , C. Bonifazi , R. Bonino , N. Borodai , J. Brack , P. Brogueira , W. C. Brown , R. Bruijn , P. Buchholz , A. Bueno , R. E. Burton , N. G. Busca , K. S. Caballero-Mora , L. Caramete , R. Caruso , W. Carvalho , A. Castellina , O. Catalano , L. Cazon , R. Cester , J. Chauvin , A. Chiavassa , J. A. Chinellato , A. Chou , J. Chudoba , J. Chye , R. W. Clay , E. Colombo , R. Conceição , B. Connolly , F. Contreras , J. Coppens , A. Cordier , U. Cotti , S. Coutu , C. E. Covault , A. Creusot , A. Criss , J. Cronin , A. Curutiu , S. Dagoret-Campagne , R. Dallier , K. Daumiller , B. R. Dawson , R. M. de Almeida , M. De Domenico , C. De Donato , S. J. de Jong , G. De La Vega , W. J. M. de Mello Junior , J. R. T. de Mello Neto , I. De Mitri , V. de Souza , K. D. de Vries , G. Decerprit , L. del Peral , O. Deligny , A. Della Selva , C. Delle Fratte , H. Dembinski , C. Di Giulio , J. C. Diaz , P. N. Diep , C. Dobrigkeit , J. C. D'Olivo , P. N. Dong , A. Dorofeev , J. C. dos Anjos , M. T. Dova , D. D'Urso , I. Dutan , M. A. DuVernois , R. Engel , M. Erdmann , C. O. Escobar , A. Etchegoyen , P. Facal San Luis , H. Falcke , G. Farrar , A. C. Fauth , N. Fazzini , F. Ferrer , A. Ferrero , B. Fick , A. Filevich , A. Filipčič , I. Fleck , S. Fliescher , C. E. Fracchiolla , E. D. Fraenkel , W. Fulgione , R. F. Gamarra , S. Gambetta , B. García , D. García Gámez , D. Garcia-Pinto , X. Garrido , G. Gelmini , H. Gemmeke , P. L. Ghia , U. Giaccari , M. Giller , H. Glass , L. M. Goggin , M. S. Gold , G. Golup , F. Gomez Albarracin , M. Gómez Berisso , P. Gonçalves , M. Gonçalves do Amaral , D. Gonzalez , J. G. Gonzalez , D. Góra , A. Gorgi , P. Gouffon , S. R. Gozzini , E. Grashorn , S. Grebe , M. Grigat , A. F. Grillo , Y. Guardincerri , F. Guarino , G. P. Guedes , J. Gutiérrez , J. D. Hague , V. Halenka , P. Hansen , D. Harari , S. Harmsma , J. L. Harton , A. Haungs , M. D. Healy , T. Hebbeker , G. Hebrero , D. Heck , C. Hojvat , V. C. Holmes , P. Homola , J. R. Hörandel , A. Horneffer , M. Hrabovský , T. Huege , M. Hussain , M. Iarlori , A. Insolia , F. Ionita , A. Italiano , S. Jiraskova , M. Kaducak , K. H. Kampert , T. Karova , P. Kasper , B. Kégl , B. Keilhauer , E. Kemp , R. M. Kieckhafer , H. O. Klages , M. Kleifges , J. Kleinfeller , R. Knapik , J. Knapp , D. -H. Koang , A. Krieger , O. Krömer , D. Kruppke-Hansen , F. Kuehn , D. Kuempel , K. Kulbartz , N. Kunka , A. Kusenko , G. La Rosa , C. Lachaud , B. L. Lago , P. Lautridou , M. S. A. B. Leão , D. Lebrun , P. Lebrun , J. Lee , M. A. Leigui de Oliveira , A. Lemiere , A. Letessier-Selvon , M. Leuthold , I. Lhenry-Yvon , R. López , A. Lopez Agüera , K. Louedec , J. Lozano Bahilo , A. Lucero , H. Lyberis , M. C. Maccarone , C. Macolino , S. Maldera , D. Mandat , P. Mantsch , A. G. Mariazzi , I. C. Maris , H. R. Marquez Falcon , D. Martello , O. Martínez Bravo , H. J. Mathes , J. Matthews , J. A. J. Matthews , G. Matthiae , D. Maurizio , P. O. Mazur , M. McEwen , R. R. McNeil , G. Medina-Tanco , M. Melissas , D. Melo , E. Menichetti , A. Menshikov , R. Meyhandan , M. I. Micheletti , G. Miele , W. Miller , L. Miramonti , S. Mollerach , M. Monasor , D. Monnier Ragaigne , F. Montanet , B. Morales , C. Morello , J. C. Moreno , C. Morris , M. Mostafá , C. A. Moura , S. Mueller , M. A. Muller , R. Mussa , G. Navarra , J. L. Navarro , S. Navas , P. Necesal , L. Nellen , C. Newman-Holmes , D. Newton , P. T. Nhung , N. Nierstenhoefer , D. Nitz , D. Nosek , L. Nožka , M. Nyklicek , J. Oehlschläger , A. Olinto , P. Oliva , V. M. Olmos-Gilbaja , M. Ortiz , N. Pacheco , D. Pakk Selmi-Dei , M. Palatka , J. Pallotta , G. Parente , E. Parizot , S. Parlati , S. Pastor , M. Patel , T. Paul , V. Pavlidou , K. Payet , M. Pech , J. Pȩkala , I. M. Pepe , L. Perrone , R. Pesce , E. Petermann , S. Petrera , P. Petrinca , A. Petrolini , Y. Petrov , J. Petrovic , C. Pfendner , R. Piegaia , T. Pierog , M. Pimenta , T. Pinto , V. Pirronello , O. Pisanti , M. Platino , J. Pochon , V. H. Ponce , M. Pontz , P. Privitera , M. Prouza , E. J. Quel , J. Rautenberg , O. Ravel , D. Ravignani , A. Redondo , B. Revenu , F. A. S. Rezende , J. Ridky , S. Riggi , M. Risse , C. Rivière , V. Rizi , C. Robledo , G. Rodriguez , J. Rodriguez Martino , J. Rodriguez Rojo , I. Rodriguez-Cabo , M. D. Rodríguez-Frías , G. Ros , J. Rosado , T. Rossler , M. Roth , B. Rouillé-d'Orfeuil , E. Roulet , A. C. Rovero , F. Salamida , H. Salazar , G. Salina , F. Sánchez , M. Santander , C. E. Santo , E. M. Santos , F. Sarazin , S. Sarkar , R. Sato , N. Scharf , V. Scherini , H. Schieler , P. Schiffer , A. Schmidt , F. Schmidt , T. Schmidt , O. Scholten , H. Schoorlemmer , J. Schovancova , P. Schovánek , F. Schroeder , S. Schulte , F. Schüssler , D. Schuster , S. J. Sciutto , M. Scuderi , A. Segreto , D. Semikoz , M. Settimo , R. C. Shellard , I. Sidelnik , B. B. Siffert , G. Sigl , A. Śmiałkowski , R. Šmída , B. E. Smith , G. R. Snow , P. Sommers , J. Sorokin , H. Spinka , R. Squartini , E. Strazzeri , A. Stutz , F. Suarez , T. Suomijärvi , A. D. Supanitsky , M. S. Sutherland , J. Swain , Z. Szadkowski , A. Tamashiro , A. Tamburro , T. Tarutina , O. Taşcău , R. Tcaciuc , D. Tcherniakhovski , D. Tegolo , N. T. Thao , D. Thomas , R. Ticona , J. Tiffenberg , C. Timmermans , W. Tkaczyk , C. J. Todero Peixoto , B. Tomé , A. Tonachini , I. Torres , P. Travnicek , D. B. Tridapalli , G. Tristram , E. Trovato , M. Tueros , R. Ulrich , M. Unger , M. Urban , J. F. Valdés Galicia , I. Valiño , L. Valore , A. M. van den Berg , J. R. Vázquez , R. A. Vázquez , D. Veberič , A. Velarde , T. Venters , V. Verzi , M. Videla , L. Villaseñor , S. Vorobiov , L. Voyvodic , H. Wahlberg , P. Wahrlich , O. Wainberg , D. Warner , A. A. Watson , S. Westerhoff , B. J. Whelan , G. Wieczorek , L. Wiencke , B. Wilczyńska , H. Wilczyński , C. Wileman , M. G. Winnick , H. Wu , B. Wundheiler , T. Yamamoto , P. Younk , G. Yuan , A. Yushkov , E. Zas , D. Zavrtanik , M. Zavrtanik , I. Zaw , A. Zepeda , M. Ziolkowski

First Array-Wide Search for Diffuse UHE Neutrinos with the Askaryan Radio Array

The Askaryan Radio Array (ARA) is an ultrahigh energy (UHE) neutrino detector at the South Pole, designed to search for radio pulses emitted by neutrino-initiated particle showers in ice. ARA consists of an array of five autonomous stations…

High Energy Astrophysical Phenomena · Physics 2025-09-23 Marco Stein Muzio

GIGAS: a set of microwave sensor arrays to detect molecular bremsstrahlung radiation from extensive air shower

We present the GIGAS (Gigahertz Identification of Giant Air Shower) microwave radio sensor arrays of the EASIER project (Extensive Air Shower Identification with Electron Radiometers), deployed at the site of the Pierre Auger cosmic ray…

Instrumentation and Methods for Astrophysics · Physics 2018-03-14 Romain Gaïor , Imen Al Samarai , Corinne Bérat , Miguel Blanco Otano , Jacques David , Oliver Deligny , Hervé Lebbolo , Sandra Lecoz , Antoine Letessier-Selvon , Isabelle Lhenry-Yvon , Ioana C. Mariş , François Montanet , Philippe Repain , Francesco Salamida , Mariangela Settimo , Patrick Stassi , Anne Stutz

Study of an Isolated Double-pulse Cosmic Ray Candidate Recorded with the Askaryan Radio Array

The radio-frequency emissions produced by particle showers on Earth, resulting from cosmic rays (CRs) and ultra-high energy neutrinos (UHE-$\nu$) originating from astrophysical sources share significant similarities, enabling radio…

High Energy Astrophysical Phenomena · Physics 2025-09-19 Shoukat Ali , Dave Z. Besson for ARA Collaboration

Detecting the Rise and Fall of 21 cm Fluctuations with the Murchison Widefield Array

We forecast the sensitivity with which the Murchison Widefield Array (MWA) can measure the 21 cm power spectrum of cosmic hydrogen, using radiative transfer simulations to model reionization and the 21 cm signal. The MWA is sensitive to…

Astrophysics · Physics 2009-11-13 Adam Lidz , Oliver Zahn , Matthew McQuinn , Matias Zaldarriaga , Lars Hernquist

Interplanetary Scintillation studies with the Murchison Wide-field Array II: Properties of sub-arcsecond compact sources at low radio frequencies

We report the first astrophysical application of the technique of wide-field Interplanetary Scintillation (IPS) with the Murchison Widefield Array (MWA). This powerful technique allows us to identify and measure sub-arcsecond compact…

High Energy Astrophysical Phenomena · Physics 2018-01-10 R. Chhetri , J. Morgan , R. D. Ekers , J-P Macquart , E. M. Sadler , M. Giroletti , J. R. Callingham , S. J. Tingay

Results and Perspectives of the Auger Engineering Radio Array

The Auger Engineering Radio Array (AERA) is an extension of the Pierre Auger Cosmic-Ray Observatory. It is used to detect radio emission from extensive air showers with energies beyond $10^{17}~$eV in the $30 - 80~$MHz frequency band. After…

High Energy Astrophysical Phenomena · Physics 2017-03-20 Christian Glaser

Radio detection of Extensive Air Showers (ECRS 2016)

Detection of the mostly geomagnetically generated radio emission of cosmic-ray air showers provides an alternative to air-Cherenkov and air-fluorescence detection, since it is not limited to clear nights. Like these established methods, the…

High Energy Astrophysical Phenomena · Physics 2017-01-20 Frank G. Schröder

Interplanetary Scintillation with the Murchison Widefield Array I: A sub-arcsecond Survey over 900 square degrees at 79 and 158 MHz

We present the first dedicated observations of Interplanetary Scintillation (IPS) with the Murchison Widefield Array (MWA). We have developed a synthesis imaging technique, tailored to the properties of modern "large-N" low-frequency radio…

Instrumentation and Methods for Astrophysics · Physics 2017-09-12 J . S. Morgan , J-P. Macquart , R. Ekers , R. Chhetri , M. Tokumaru , P. K. Manoharan , S. Tremblay , M. M. Bisi , B. V. Jackson

Calibration and Stokes Imaging with Full Embedded Element Primary Beam Model for the Murchison Widefield Array

The Murchison Widefield Array (MWA), located in Western Australia, is one of the low-frequency precursors of the international Square Kilometre Array (SKA) project. In addition to pursuing its own ambitious science program, it is also a…

Instrumentation and Methods for Astrophysics · Physics 2017-12-20 M. Sokolowski , T. Colegate , A. T. Sutinjo , D. Ung , R. B. Wayth , N. Hurley-Walker , E. Lenc , B. Pindor , J. Morgan , D. L. Kaplan , M. E. Bell , J. R. Callingham , K. S. Dwarakanath , Bi-Qing For , B. M. Gaensler , P. J. Hancock , L. Hindson , M. Johnston-Hollitt , A. D. Kapińska , B. McKinley , A. R. Offringa , P. Procopio , L. Staveley-Smith , C. Wu , Q. Zheng

Radio-detection of extensive air showers at the Pierre Auger Observatory - Results and enhancements

The Pierre Auger Collaboration is exploring the potential of radio-detection techniques to measure the extensive air showers. The main advantage of these setups is the possibility to cover a large area with no atmospheric attenuation and…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 K. Louedec

Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf

The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 10^16 eV. The most neutrino-like background stems from the radio emission of air showers. This article…

Instrumentation and Methods for Astrophysics · Physics 2017-03-02 S. W. Barwick , D. Z. Besson , A. Burgman , E. Chiem , A. Hallgren , J. C. Hanson , S. R. Klein , S. Kleinfelder , A. Nelles , C. Persichilli , S. Phillips , T. Prakash , C. Reed , S. R. Shively , J. Tatar , E. Unger , J. Walker , G. Yodh