A
Abigail G. Vieregg
Researcher at University of Chicago
Publications - 202
Citations - 10921
Abigail G. Vieregg is an academic researcher from University of Chicago. The author has contributed to research in topics: Cosmic microwave background & Neutrino. The author has an hindex of 38, co-authored 183 publications receiving 9108 citations. Previous affiliations of Abigail G. Vieregg include University of Cincinnati & Harvard University.
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Journal ArticleDOI
The First Limits on the Ultra-high Energy Neutrino Fluence from Gamma-ray Bursts
Abigail G. Vieregg,Abigail G. Vieregg,K. J. Palladino,P. Allison,B. M. Baughman,J. J. Beatty,Konstantin Belov,David Zeke Besson,S. Bevan,W. R. Binns,Chiang-Mei Chen,Pisin Chen,John Clem,A. Connolly,M. Detrixhe,D. De Marco,Paul Dowkontt,Michael DuVernois,P. W. Gorham,E. Grashorn,B. Hill,S. Hoover,M. A. Huang,M. H. Israel,A. Javaid,Kurt Liewer,S. Matsuno,B. C. Mercurio,Christian Miki,M. Mottram,J. W. Nam,R. J. Nichol,A. Romero-Wolf,L. L. Ruckman,David Saltzberg,D. Seckel,G. S. Varner,Yuh-Lin Wang +37 more
TL;DR: In this paper, the authors set the first limits on the ultra-high energy neutrino fluence at energies greater than 10^9 GeV from gamma-ray bursts (GRBs) based on data from the second flight of the ANtarctic Impulsive Transient Antenna (ANITA).
Journal Article
The Next-Generation Radio Neutrino Observatory -- Multi-Messenger Neutrino Astrophysics at Extreme Energies
Amy Connolly,Juanan Aguilar,Patrick Allison,S. Archambault,S. Barnet,J. J. Beatty,D. Z. Besson,Olga Botner,Stijn Buitink,Po-Hsun Chen,Brian Clark,Cosmin Deaconu,S. De Kockere,Michael DuVernois,N. van Eijndhoven,C. B. Finley,D. Garcia,Allan Hallgren,Francis Halzen,J. C. Hanson,Kael Hanson,J. Haugen,C. Pérez de los Heros,K. D. Hoffman,Benjamin Hokanson-Fasig,K. Hughes,K. Hultqvist,A. Ishihara,A. Karle,J. L. Kelley,S. R. Klein,R. Khandelwal,M. Kowalski,I. Kravchenko,U. Latif,Tsung-Che Liu,M.-Y. Lu,K. Mase,R. Morse,Jiwoo Nam,A. Nelles,Eric Oberla,Carl Pfendner,Y. Pan,Ilse Plaisier,S. Prohira,S. H. Robertson,J. Rolla,Dirk Ryckbosch,Frank G. Schröder,D. Seckel,A. Shultz,David J. Smith,D. Southall,Erin O'Sullivan,T. Stezelberger,Simona Toscano,J. Torres-Espinosa,S. Unger,Abigail G. Vieregg,K. D. de Vries,S. H. Wang,Christoph Welling,Stephanie Wissel,S. Yoshida +64 more
TL;DR: RNO is the mid-scale discovery instrument designed to make the first observation of neutrinos from the cosmos at extreme energies, with sensitivity well beyond current instrument capabilities as mentioned in this paper.
Journal ArticleDOI
The simulation of the sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to Askaryan radiation from cosmogenic neutrinos interacting in the Antarctic Ice
L. Cremonesi,Amy Connolly,Patrick Allison,O. Banerjee,L. Batten,J. J. Beatty,Keith Bechtol,Konstantin Belov,D. Z. Besson,D. Z. Besson,W. R. Binns,V. Bugaev,P. Cao,C. C. Chen,Chun Hsiung Chen,Po-Hsun Chen,J. M. Clem,B. Dailey,Cosmin Deaconu,Paul Dowkontt,B. D. Fox,J. W. H. Gordon,Peter Gorham,Berkeley Hill,J. J. Huang,Kaeli Hughes,R. Hupe,M. H. Israel,Kurt Liewer,S. Y. Lin,Tsung-Che Liu,Andrew Ludwig,Luca Macchiarulo,S. Matsuno,K. McBride,C. Miki,K. Mulrey,K. Mulrey,Jiwoo Nam,R. J. Nichol,A. Novikov,A. Novikov,Eric Oberla,S. Prohira,Brian Rauch,Jarred Matthew Roberts,Andrew Romero-Wolf,B. Rotter,J. W. Russell,David Saltzberg,D. Seckel,Harm Schoorlemmer,J. Shiao,S. Stafford,J. Stockham,M. Stockham,B. Strutt,J. Stuhr,M. S. Sutherland,G. S. Varner,Abigail G. Vieregg,S. H. Wang,Stephanie Wissel +62 more
TL;DR: In this paper, a Monte Carlo simulation program for the radio detection of UHE neutrino interactions in the Antarctic ice as viewed by the Antarctic Impulsive Transient Antenna (ANITA) is described.
Journal ArticleDOI
Design and Performance of the First BICEP Array Receiver
Alessandro Schillaci,Peter A. R. Ade,Zeeshan Ahmed,Mandana Amiri,Denis Barkats,R. Basu Thakur,Colin A. Bischoff,James J. Bock,H. Boenish,E. Bullock,Victor Buza,J. Cheshire,Jake Connors,J. Cornelison,M. Crumrine,A. Cukierman,Marion Dierickx,Lionel Duband,S. Fatigoni,Jeffrey P. Filippini,G. Hall,Mark Halpern,Sarah M. Harrison,S. Henderson,Sergi R. Hildebrandt,Gene C. Hilton,Howard Hui,Kent D. Irwin,J. Kang,Kirit Karkare,E. Karpel,S. Kefeli,John M Kovac,Chao-Lin Kuo,King Tong Lau,K. G. Megerian,Lorenzo Moncelsi,Toshiya Namikawa,H. T. Nguyen,Roger O'Brient,S. Palladino,N. Precup,T. Prouvé,C. Pryke,B. Racine,Carl D. Reintsema,S. Richter,Benjamin L. Schmitt,R. Schwarz,C. D. Sheehy,Ahmed Soliman,T. St. Germaine,Bryan Steinbach,Rashmikant V. Sudiwala,Keith L. Thompson,Carole Tucker,Anthony D. Turner,C. Umiltà,Abigail G. Vieregg,A. Wandui,A. C. Weber,Donald V. Wiebe,J. Willmert,W. L. K. Wu,Eui-Hyeok Yang,Ki Won Yoon,Edward D. Young,Che-Hang Yu,Chao Zhang +68 more
TL;DR: The BICEP/Keck (BK) experiment targets this primordial signature, the amplitude of which is parameterized by the tensor-to-scalar ratio r, by observing the polarized microwave sky through the exceptionally clean and stable atmosphere at the South Pole as discussed by the authors.
Proceedings ArticleDOI
The Radio Neutrino Observatory Greenland (RNO-G)
Rno-g,Juan A. Aguilar,Patrick Allison,J. J. Beatty,Hans Bernhoff,David Zeke Besson,N. Bingefors,Olga Botner,Sjoerd Bouma,Stijn Buitink,Katie Carter,Maddalena Cataldo,Brian Clark,Zachary Curtis-Ginsberg,Amy Connolly,Paramita Dasgupta,Simon De Kockere,Krijn D. de Vries,Cosmin Deaconu,M. A. DuVernois,Christian Glaser,Allan Hallgren,Steffen Hallmann,Jordan C. Hanson,Bryan Hendricks,Benjamin Hokanson-Fasig,C. Hornhuber,Kaeli Hughes,A. Karle,John L. Kelley,Spencer Klein,Ryan Krebs,R. Lahmann,U. Latif,Mitchell Magnuson,Thomas Meures,Zachary S. Meyers,Katharine Mulrey,Anna Nelles,Alexander Novikov,Eric Oberla,Bob Oeyen,Hershal Pandya,Ilse Plaisier,Lilly Pyras,Dirk Ryckbosch,Olaf Scholten,D. Seckel,Daniel Smith,Daniel Southall,Jorge Torres,Simona Toscano,D. Tosi,Dieder J. Van Den Broeck,Nick van Eijndhoven,Abigail G. Vieregg,Christoph Welling,Stephanie Wissel,Robert Young,Adrian Zink +59 more
TL;DR: The Radio Neutrino Observatory Greenland (RNO-G) as discussed by the authors is scheduled for deployment in the summer of 2021, and it will target the detection of astrophysical and cosmogenic neutrinos above 10 PeV.