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
Proceedings ArticleDOI
Characterising the SCUBA-2 superconducting bolometer arrays
Dan Bintley,Michael J. MacIntosh,Wayne S. Holland,Per Friberg,Craig Walther,David Atkinson,Dennis Kelly,Xiaofeng Gao,Peter A. R. Ade,William F. Grainger,Julian Steven House,Lorenzo Moncelsi,Matthew I. Hollister,Matthew I. Hollister,Adam Woodcraft,Camelia Dunare,William Parkes,Anthony J. Walton,Kent D. Irwin,Gene C. Hilton,Michael D. Niemack,Carl D. Reintsema,Mandana Amiri,B. Burger,Mark Halpern,Matthew Hasselfield,Jeff T. Hill,Jan Kycia,C. G. A. Mugford,Lauren Persaud +29 more
TL;DR: The SCUBA-2 is a state-of-the-art 10,000 pixel submillimeter camera installed at the James Clerk Maxwell Telescope (JCMT) providing wide-field simultaneous imaging at wavelengths of 450 and 850 microns.
Journal ArticleDOI
A panchromatic study of BLAST counterparts: total star formation rate, morphology, active galactic nucleus fraction, and stellar mass
Lorenzo Moncelsi,Peter A. R. Ade,Edward L. Chapin,Luca Cortese,Luca Cortese,Mark J. Devlin,Simon Dye,Stephen Anthony Eales,Matthew Joseph Griffin,Mark Halpern,Peter Charles Hargrave,Gaelen Marsden,Philip Daniel Mauskopf,Calvin B. Netterfield,Enzo Pascale,Douglas Scott,Matthew D. P. Truch,Carole Tucker,Marco P. Viero,Donald V. Wiebe +19 more
TL;DR: In this paper, the authors carried out a multi-wavelength study of individual galaxies detected by the Balloon-borne Large Aperture Submillimeter Telescope (BLAST) and identified at other wavelengths, using data spanning the radio to the ultraviolet (UV).
Posted Content
The Atacama B-Mode Search: CMB Polarimetry with Transition-Edge-Sensor Bolometers
Thomas Essinger-Hileman,John W. Appel,J. A. Beall,H. M. Cho,J B. Fowler,Mark Halpern,M. Hasselfield,Kent D. Irwin,Tobias A. Marriage,Michael D. Niemack,L. A. Page,L. P. Parker,S. Pufu,S. T. Staggs,O. R. Stryzak,C. Visnjic,K. W. Yoon,Yue Zhao +17 more
TL;DR: The Atacama B-mode Search (ABS) experiment is a 145 GHz polarimeter designed to measure the Bmode polarization of the Cosmic Microwave Background (CMB) at large angular scales as discussed by the authors.
Proceedings ArticleDOI
Design and characterization of the Cosmology Large Angular Scale Surveyor (CLASS) 93 GHz focal plane
Sumit Dahal,Aamir Ali,J. W. Appel,Thomas Essinger-Hileman,Charles L. Bennett,Michael K. Brewer,Ricardo Bustos,Manwei Chan,David T. Chuss,Joseph Cleary,Felipe Colazo,Jullianna Couto,Kevin L. Denis,Rolando Dünner,Joseph Eimer,Trevor Van Engelhoven,Pedro Fluxa,Mark Halpern,Kathleen Harrington,Kyle Helson,Gene C. Hilton,Gary Hinshaw,Johannes Hubmayr,Jeffrey Iuliano,Tobias A. Marriage,Jeff McMahon,Nathan P Miller,Carolina Núñez,Ivan L. Padilla,Gonzalo A. Palma,Lucas Parker,Matthew Petroff,Bastián Pradenas,Rodrigo Reeves,Carl D. Reintsema,Karwan Rostem,Marco Sagliocca,Kongpop U-Yen,Deniz Augusto Nunes Valle,Bingjie Wang,Qinan Wang,Duncan J. Watts,Janet Weiland,Edward J. Wollack,Zhilei Xu,Ziang Yan,Lingzhen Zen +46 more
TL;DR: The first 93 GHz detector array of the Cosmology Large Angular Scale Surveyor (Class) was constructed on mono-crystalline silicon wafers to maintain TES uniformity and optimize optical efficiency throughout the wafer as discussed by the authors.
Proceedings ArticleDOI
BICEP Array cryostat and mount design
M. Crumrine,Peter A. R. Ade,Zeeshan Ahmed,Randol W. Aikin,Kate D. Alexander,Denis Barkats,S. J. Benton,Colin A. Bischoff,J. J. Bock,R. Bowens-Rubin,Justus A. Brevik,I. Buder,E. Bullock,Victor Buza,Jake Connors,J. Cornelison,B. P. Crill,Marion Dierickx,Lionel Duband,Cora Dvorkin,Jeffrey P. Filippini,S. Fliescher,J. A. Grayson,G. Hall,Mark Halpern,Sarah M. Harrison,S. R. Hildebrandt,Gene C. Hilton,Howard Hui,Kent D. Irwin,J. Kang,Kirit Karkare,E. Karpel,J. P. Kaufman,Brian Keating,S. Kefeli,S. A. Kernasovskiy,John M Kovac,C. L. Kuo,N. A. Larsen,King Tong Lau,E. M. Leitch,M. Lueker,K. G. Megerian,Lorenzo Moncelsi,Toshiya Namikawa,Calvin B. Netterfield,H. T. Nguyen,Roger O'Brient,R. W. Ogburn,S. Palladino,C. Pryke,B. Racine,S. Richter,R. Schwarz,Alessandro Schillaci,C. D. Sheehy,C. D. Sheehy,Ahmed Soliman,T. St. Germaine,Z. K. Staniszewski,Bryan Steinbach,R. V. Sudiwala,Grant Teply,K. L. Thompson,J. E. Tolan,Carole Tucker,A. D. Turner,C. Umilta,Abigail G. Vieregg,A. Wandui,A. C. Weber,D. V. Wiebe,J. Willmert,C. L. Wong,W. L. K. Wu,W. L. K. Wu,E. Yang,K. W. Yoon,C. Zhang +79 more
TL;DR: The Bicep Array as mentioned in this paper is a cosmic microwave background (CMB) polarization experiment that will begin observing at the South Pole in early 2019, and it is a CMB polarization experiment at six frequencies from 30 to 270 GHz.