M
Mark Halpern
Researcher at University of British Columbia
Publications - 560
Citations - 121832
Mark Halpern is an academic researcher from University of British Columbia. The author has contributed to research in topics: Cosmic microwave background & Galaxy. The author has an hindex of 126, co-authored 546 publications receiving 114409 citations. Previous affiliations of Mark Halpern include National Institute of Standards and Technology & Stanford University.
Papers
More filters
Posted Content
21 cm Intensity Mapping
Jeffrey B. Peterson,Roy Aleksan,Reza Ansari,Kevin Bandura,Dick Bond,John D. Bunton,Kermit Carlson,Tzu-Ching Chang,F. DeJongh,Matt Dobbs,Scott Dodelson,Hassane Darhmaoui,Nick Gnedin,Mark Halpern,Craig J. Hogan,Jean-Marc Le Goff,Tiehui Ted Liu,Ahmed Legrouri,Avi Loeb,Khalid Loudiyi,Christophe Magneville,John Marriner,D. McGinnis,Bruce McWilliams,Marc Moniez,Nathalie Palanque-Delabruille,Ralph J. Pasquinelli,Ue-Li Pen,Jim Rich,V. Scarpine,Hee-Jong Seo,Kris Sigurdson,Uroš Seljak,Albert Stebbins,Jason H. Steffen,Chris Stoughton,Peter T. Timbie,Alberto Vallinotto,S. Wyithe,Christophe Yèche +39 more
TL;DR: Using the 21 cm line, observed all-sky and across the redshift range from 0 to 5, the large scale structure of the Universe can be mapped in three dimensions as discussed by the authors.
Proceedings ArticleDOI
Instrument design and characterization of the Millimeter Bolometer Array Camera on the Atacama Cosmology Telescope
Daniel S. Swetz,Peter A. R. Ade,Christine A. Allen,Mandana Amiri,J. W. Appel,Elia S. Battistelli,Elia S. Battistelli,B. Burger,Jay Chervenak,A. J. Dahlen,Sudeep Das,S. Denny,Mark J. Devlin,Simon Dicker,William B. Doriese,R. Dunner,R. Dunner,Thomas Essinger-Hileman,R. P. Fisher,Joseph W. Fowler,X. Gao,Amir Hajian,Mark Halpern,Peter Charles Hargrave,M. Hasselfield,Gene C. Hilton,Adam D. Hincks,Kent D. Irwin,Norman Jarosik,Madhuri Kaul,Jacob Klein,S. Knotek,Judy M. Lau,Michele Limon,Robert H. Lupton,Tobias A. Marriage,K. L. Martocci,Philip Daniel Mauskopf,Samuel H. Moseley,Calvin B. Netterfield,Michael D. Niemack,M. R. Nolta,L. Page,L. P. Parker,B. Reid,Carl D. Reintsema,Audrey Sederberg,Neelima Sehgal,Jon Sievers,David N. Spergel,Suzanne T. Staggs,O. R. Stryzak,Eric R. Switzer,Robert Thornton,Carole Tucker,Edward J. Wollack,Yue Zhao +56 more
TL;DR: The Millimeter Bolometer Array Camera (MBAC) as mentioned in this paper was used to map the temperature anisotropies of theCosmic Microwave Background (CMB) with arc-minute resolution.
Journal ArticleDOI
Correlations in the (Sub)millimeter background from ACTxBLAST
Amir Hajian,Marco P. Viero,Graeme E. Addison,Paula Aguirre,J. W. Appel,Nick Battaglia,James J. Bock,J. Richard Bond,Sudeep Das,Mark J. Devlin,Simon Dicker,Joanna Dunkley,Rolando Dünner,Thomas Essinger-Hileman,John P. Hughes,Joseph W. Fowler,Mark Halpern,Matthew Hasselfield,Matt Hilton,Adam D. Hincks,Renée Hlozek,Kent D. Irwin,Jacob Klein,Arthur Kosowsky,Yen-Ting Lin,Tobias A. Marriage,Danica Marsden,Gaelen Marsden,Felipe Menanteau,Lorenzo Moncelsi,Kavilan Moodley,Calvin B. Netterfield,Michael D. Niemack,Michael R. Nolta,Lyman A. Page,Lucas Parker,Douglas Scott,Neelima Sehgal,Jon Sievers,David N. Spergel,Suzanne T. Staggs,Daniel S. Swetz,Eric R. Switzer,Robert Thornton,Edward J. Wollack +44 more
TL;DR: In this article, the authors present measurements of the auto-and cross-frequency correlation power spectra of the cosmic (sub)millimeter background at: 250, 350, and 500 um (1200, 860, and 600 GHz) from observations made with the Balloon-borne Large Aperture Submillimeter Telescope, BLAST; and at 1380 and 2030 um (218 and 148 GHz) by observations made by the Atacama Cosmology Telescope, ACT.
First-year wilkinson microwave anisotropy probe (wmap) 1 observations: foreground emission
C. L. Bennett,R. S. Hill,G. Hinshaw,M. R. Nolta,N. Odegard,David N. Spergel,Janet L. Weiland,E. L. Wright,Mark Halpern,N. Jarosik,Alan J. Kogut,Michele Limon,S. S. Meyer,Gregory S. Tucker,Edward J. Wollack +14 more
TL;DR: In this article, the authors used a maximum entropy method to construct a model of the Galactic emission components, and the individual model components are accurate to a few percent, leading to an improved understanding of Galactic astrophysical processes.
Journal ArticleDOI
Antenna-coupled TES bolometers used in BICEP2, Keck array, and SPIDER
Peter A. R. Ade,Randol W. Aikin,Mandana Amiri,Denis Barkats,S. J. Benton,Colin A. Bischoff,James J. Bock,J. A. Bonetti,Justus A. Brevik,I. Buder,E. Bullock,Goutam Chattopadhyay,G. Davis,Peter K. Day,C. D. Dowell,L. Duband,Jeffrey P. Filippini,Jeffrey P. Filippini,S. Fliescher,Sunil Golwala,Mark Halpern,Matthew Hasselfield,S. R. Hildebrandt,Gene C. Hilton,Viktor Hristov,Howard Hui,Kent D. Irwin,Kent D. Irwin,W. C. Jones,Kirit Karkare,J. P. Kaufman,Brian Keating,S. Kefeli,S. A. Kernasovskiy,John M Kovac,Chao-Lin Kuo,Chao-Lin Kuo,Henry G. LeDuc,E. M. Leitch,Nuria Llombart,M. Lueker,P. V. Mason,K. G. Megerian,Lorenzo Moncelsi,Calvin B. Netterfield,H. T. Nguyen,Roger O'Brient,R. W. Ogburn,A. Orlando,C. Pryke,Alexandra S. Rahlin,Carl D. Reintsema,S. Richter,Marcus Runyan,R. Schwarz,C. D. Sheehy,Z. K. Staniszewski,R. Sudiwala,Grant Teply,J. E. Tolan,Amy Trangsrud,R. S. Tucker,A. D. Turner,Abigail G. Vieregg,A. C. Weber,Donald V. Wiebe,P. Wilson,C. L. Wong,Ki Won Yoon,Jonas Zmuidzinas +69 more
TL;DR: In this paper, the authors have developed antenna-coupled transition-edge sensor (TES) bolometers for a wide range of cosmic microwave background (CMB) polarimetry experiments, including BICEP2, Keck Array, and balloon borne SPIDER.