J
Jo Dunkley
Researcher at Princeton University
Publications - 133
Citations - 88031
Jo Dunkley is an academic researcher from Princeton University. The author has contributed to research in topics: Cosmic microwave background & Planck. The author has an hindex of 56, co-authored 113 publications receiving 82943 citations. Previous affiliations of Jo Dunkley include University of Oxford.
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Journal ArticleDOI
The Atacama Cosmology Telescope: Summary of DR4 and DR5 Data Products and Data Access
Maya Mallaby-Kay,Zachary Atkins,Simone Aiola,Stefania Amodeo,Jason E. Austermann,James A. Beall,Daniel T. Becker,J. Richard Bond,Erminia Calabrese,Grace E. Chesmore,Steve K. Choi,Kevin T. Crowley,Omar Darwish,Edwawd V. Denison,Mark J. Devlin,Shannon M. Duff,Adriaan J. Duivenvoorden,Jo Dunkley,Simone Ferraro,Kyra Fichman,Patricio A. Gallardo,Joseph E. Golec,Yilun Guan,Dongwon Han,Matthew Hasselfield,J. Colin Hill,Gene C. Hilton,Matt Hilton,Renée Hlozek,Johannes Hubmayr,Kevin M. Huffenberger,John P. Hughes,Brian J. Koopman,Thibaut Louis,Amanda MacInnis,Mathew S. Madhavacheril,Jeff McMahon,Kavilan Moodley,Sigurd Naess,Toshiya Namikawa,Federico Nati,Laura Newburgh,John P. Nibarger,Michael D. Niemack,Lyman A. Page,Maria Salatino,Emmanuel Schaan,Alessandro Schillaci,Neelima Sehgal,Blake D. Sherwin,Cristóbal Sifón,Sara M. Simon,Suzanne T. Staggs,Emilie Storer,Joel N. Ullom,Alexander van Engelen,Jeff Van Lanen,Leila R. Vale,Edward J. Wollack,Zhilei Xu +59 more
TL;DR: The Atacama Cosmology Telescope (ACT) data are available for public access as discussed by the authors, including temperature and polarization maps that cover nearly half the sky at arcminute resolution in three frequency bands, lensing maps and component-separated maps covering 2,100 deg^2 of sky.
Posted Content
Planck intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353GHz with optical interstellar polarization
P. A. R. Ade,Nabila Aghanim,D. Alina,G. Aniano,C. Armitage-Caplan,M. Arnaud,M. Ashdown,Fernando Atrio-Barandela,Jonathan Aumont,C. Baccigalupi,A. J. Banday,R. B. Barreiro,E. Battaner,C. A. Beichman,K. Benabed,Stéphane Colombi,L. P. L. Colombo,C. Combet,F. Couchot,A. Coulais,B. P. Crill,A. Curto,F. Cuttaia,L. Danese,R. D. Davies,R. J. Davis,P. de Bernardis,A. De Rosa,G. de Zotti,J. Delabrouille,Clive Dickinson,Jose M. Diego,S. Donzelli,M. Douspis,Jo Dunkley,X. Dupac,H. K. Eriksen,E. Falgarone,Lapo Fanciullo,Fabio Finelli,Olivier Forni,M. Frailis,Aurelien A. Fraisse,E. Franceschi,S. Galeotta,K. Ganga,Tuhin Ghosh,M. Giard,J. Gonz,A. Gregorio,A. Gruppuso,Vincent Guillet,F. K. Hansen,D. L. Harrison,George Helou,C. Hern,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,W. C. Jones,Mika Juvela,R. Keskitalo,Theodore Kisner,R. Kneissl,J. Knoche,M. Kunz,Hannu Kurki-Suonio,G. Lagache,Anthony Lasenby,R. Leonardi,François Levrier,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,A. M. Magalh,Davide Maino,Nazzareno Mandolesi,Michele Maris,D. J. Marshall,Pierrick Martin,Serena Masi,S. Matarrese,Pasquale Mazzotta,Alessandro Melchiorri,L. Mendes,A. Mennella,M. Migliaccio,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Pavel D. Naselsky,Federico Nati,P. Natoli,Calvin B. Netterfield,F. Noviello,Dmitry Novikov,I. D. Novikov,Carol Anne Oxborrow,L. Pagano,F. Pajot,R. Paladini,D. Paoletti,Fabio Pasian,O. Perdereau,L. Perotto,F. Perrotta,F. Piacentini,M. Piat,D. Pietrobon,Stéphane Plaszczynski,Frédérick Poidevin,E. Pointecouteau,G. Polenta,L. Popa,G. W. Pratt,Simon Prunet,L. Puget,Rafael Rebolo,Martin Reinecke,Mathieu Remazeilles,C. Renault,S. Ricciardi,T. Riller,I. Ristorcelli,G. Rocha,C. Rosset,G. Roudier,B. Rusholme,M. Sandri,Giorgio Savini,Locke D. Spencer,V. Stolyarov,R. Stompor,R. V. Sudiwala,D. Sutton,J. A. Tauber,Luca Terenzi,M. Tomasi,M. Tristram,M. Tucci,G. Umana,Luca Valenziano,J. Valiviita,B. Van Tent,P. Vielva,F. Villa,Lawrence A. Wade,B. D. Wandelt,A. Zonca +153 more
TL;DR: In this article, the authors used ancillary catalogues of interstellar polarization and extinction of starlight to obtain the degree of polarization, pV, and optical depth in the V band to the star, V.
Journal ArticleDOI
The Atacama Cosmology Telescope: Detection of mm-wave transient sources
Sigurd Naess,Nick Battaglia,J. Richard Bond,Erminia Calabrese,Steve K. Choi,Nicholas F. Cothard,Mark J. Devlin,Cody J. Duell,Adriaan J. Duivenvoorden,Jo Dunkley +9 more
TL;DR: In this paper, the Atacama Cosmology Telescope was used for the discovery of three transient mm-wave sources using data from the atacama cosmology telescope, two of which were coincident in position with M and K stars, while the third was coincident with a G star.
Journal ArticleDOI
The Atacama Cosmology Telescope: Microwave Intensity and Polarization Maps of the Galactic Center
Yilun Guan,Susan E. Clark,Brandon S. Hensley,Patricio A. Gallardo,Sigurd Naess,Cody J. Duell,Simone Aiola,Zachary Atkins,Erminia Calabrese,Steve K. Choi,Nicholas F. Cothard,Mark J. Devlin,Adriaan J. Duivenvoorden,Jo Dunkley,Rolando Dünner,Simone Ferraro,Simone Ferraro,Matthew Hasselfield,John P. Hughes,Brian J. Koopman,Arthur Kosowsky,Mathew S. Madhavacheril,Jeff McMahon,Federico Nati,Michael D. Niemack,Lyman A. Page,Maria Salatino,Emmanuel Schaan,Emmanuel Schaan,Neelima Sehgal,Cristóbal Sifón,Suzanne T. Staggs,Eve M. Vavagiakis,Edward J. Wollack,Zhilei Xu,Zhilei Xu +35 more
TL;DR: In this article, the Atacama Cosmology Telescope (ACT) was used to obtain arcminute-resolution intensity and polarization maps of the Galactic center made with the ACT at 98, 150, and 224 GHz.
Journal ArticleDOI
Concept Study of Optical Configurations for High-Frequency Telescope for LiteBIRD
T. Hasebe,Shingo Kashima,Peter A. R. Ade,Y. Akiba,David Alonso,Kam Arnold,Jonathan Aumont,Carlo Baccigalupi,Darcy Barron,Soumen Basak,Soumen Basak,S. Beckman,Julian Borrill,Julian Borrill,F. Boulanger,M. Bucher,Erminia Calabrese,Yuji Chinone,Yuji Chinone,H. M. Cho,A. Cukierman,D. W. Curtis,T. de Haan,M. A. Dobbs,A. Dominjon,Tadayasu Dotani,L. Duband,A. Ducout,Jo Dunkley,Jo Dunkley,J. M. Duval,Tucker Elleflot,H. K. Eriksen,Josquin Errard,J. Fischer,T. Fujino,T. Funaki,U. Fuskeland,K. Ganga,Neil Goeckner-Wald,J. Grain,N. W. Halverson,T. Hamada,Masaya Hasegawa,Kaori Hattori,Makoto Hattori,L. Hayes,Masashi Hazumi,N. Hidehira,Charles A. Hill,Charles A. Hill,Gene C. Hilton,Johannes Hubmayr,Kiyotomo Ichiki,Toshiaki Iida,H. Imada,M. Inoue,Yuki Inoue,Kent D. Irwin,Hirokazu Ishino,Oliver Jeong,H. Kanai,D. Kaneko,N. Katayama,T. Kawasaki,S. A. Kernasovskiy,Reijo Keskitalo,Reijo Keskitalo,A. Kibayashi,Y. Kida,Kimihiro Kimura,Theodore Kisner,Theodore Kisner,Kazunori Kohri,Eiichiro Komatsu,K. Komatsu,C. L. Kuo,Noah Kurinsky,Akito Kusaka,Akito Kusaka,Alex Lazarian,Aaron Lee,Aaron Lee,Dale Li,Eric V. Linder,Eric V. Linder,Bruno Maffei,Anna Mangilli,M. Maki,Tomotake Matsumura,Shuji Matsuura,D. Meilhan,Satoru Mima,Yuto Minami,Kazuhisa Mitsuda,L. Montier,M. Nagai,T. Nagasaki,R. Nagata,M. Nakajima,Shogo Nakamura,Toshiya Namikawa,Masato Naruse,H. Nishino,Tom Nitta,Takashi Noguchi,Hideo Ogawa,Shugo Oguri,Norio Okada,Atsushi Okamoto,Takahiro Okamura,Chiko Otani,G. Patanchon,Giampaolo Pisano,Gabriel M. Rebeiz,Mathieu Remazeilles,Paul L. Richards,Shin-ichiro Sakai,Yuki Sakurai,Y. Sato,N. Sato,Makoto Sawada,Y. Segawa,Yutaro Sekimoto,Yutaro Sekimoto,Uroš Seljak,Blake D. Sherwin,Blake D. Sherwin,Toshifumi Shimizu,Keisuke Shinozaki,R. Stompor,Hajime Sugai,Hiroyuki Sugita,Aritoki Suzuki,Jun-ichi Suzuki,Osamu Tajima,Suguru Takada,R. Takaku,S. Takakura,S. Takatori,D. Tanabe,E. Taylor,K. L. Thompson,B. Thorne,B. Thorne,Takayuki Tomaru,T. Tomida,N. Tomita,M. Tristram,Carole Tucker,Paul Turin,Masahiro Tsujimoto,S. Uozumi,Shin Utsunomiya,Yoshinori Uzawa,F. Vansyngel,Ingunn Kathrine Wehus,Benjamin Westbrook,M. Willer,Nathan Whitehorn,Yasuhiro Yamada,Ryo Yamamoto,Noriko Y. Yamasaki,T. Yamashita,Mitsuhiro Yoshida +164 more
TL;DR: In this paper, the anti-reflection (AR) coating on the lens for the refractive option is derived and the simulation result of a sub-wavelength AR structure on both surfaces of silicon, which shows a band-averaged reflection of 1.1-3.2% at 101-448 GHz.