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
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The Herschel Multi-Tiered Extragalactic Survey: Source Extraction and Cross-Identifications in Confusion-Dominated SPIRE Images
Isaac Roseboom,Seb Oliver,Martin Kunz,Bruno Altieri,Alexandre Amblard,V. Arumugam,Robbie Richard Auld,Herve Aussel,T. Babbedge,Matthieu Béthermin,Andrew Blain,James J. Bock,James J. Bock,Alessandro Boselli,Drew Brisbin,V. Buat,Denis Burgarella,N. Castro-Rodríguez,N. Castro-Rodríguez,Antonio Cava,Antonio Cava,Pierre Chanial,Edward L. Chapin,David L. Clements,A. Conley,L. Conversi,Asantha Cooray,Asantha Cooray,C. D. Dowell,C. D. Dowell,Eli Dwek,Simon Dye,Stephen Anthony Eales,David Elbaz,Duncan Farrah,M. Fox,Alberto Franceschini,Walter Kieran Gear,Jason Glenn,E. A. González Solares,Matthew Joseph Griffin,Mark Halpern,Martin Harwit,Evanthia Hatziminaoglou,J.-S. Huang,Edo Ibar,Kate Gudrun Isaak,Rob Ivison,Rob Ivison,Guilaine Lagache,L. R. Levenson,L. R. Levenson,N. Lu,Suzanne C. Madden,Bruno Maffei,G. Mainetti,Lucia Marchetti,G. Marsden,A. M. J. Mortier,Hien Nguyen,Hien Nguyen,B. O'Halloran,Alain Omont,Mat Page,Pasquale Panuzzo,Andreas Papageorgiou,H. Patel,C. P. Pearson,C. P. Pearson,Ismael Perez-Fournon,Ismael Perez-Fournon,Michael Pohlen,Jonathan Rawlings,Gwenifer Raymond,Dimitra Rigopoulou,Dimitra Rigopoulou,D. Rizzo,Michael Rowan-Robinson,M. Sanchez Portal,Benjamin L. Schulz,Douglas Scott,Nick Seymour,D. L. Shupe,A. J. Smith,Jamie Stevens,M. Symeonidis,Markos Trichas,K. E. Tugwell,Mattia Vaccari,Ivan Valtchanov,Joaquin Vieira,L. Vigroux,Lian-Tao Wang,Robyn L. Ward,G. Wright,C. K. Xu,Michael Zemcov,Michael Zemcov +97 more
TL;DR: In this article, the cross-identification and source photometry techniques used to process Herschel SPIRE imaging taken as part of the Herschel Multi-Tiered Extragalactic Survey (HerMES) were presented.
Posted Content
The XFaster Power Spectrum and Likelihood Estimator for the Analysis of Cosmic Microwave Background Maps
A. E. Gambrel,Alexandra S. Rahlin,Alexandra S. Rahlin,X. Song,Carlo R. Contaldi,P. A. R. Ade,Mandana Amiri,Steven J. Benton,A. S. Bergman,R. Bihary,James J. Bock,James J. Bock,John Bond,J. A. Bonetti,Sean Bryan,H. C. Chiang,H. C. Chiang,Adriaan J. Duivenvoorden,Adriaan J. Duivenvoorden,H. K. Eriksen,Marzieh Farhang,Marzieh Farhang,Jeffrey P. Filippini,A. A. Fraisse,Katherine Freese,Katherine Freese,M. Galloway,N. N. Gandilo,R. Gualtieri,Jon E. Gudmundsson,Mark Halpern,J. Hartley,Matthew Hasselfield,Gene C. Hilton,Warren Holmes,Viktor Hristov,Zhiqi Huang,Kent D. Irwin,Kent D. Irwin,W. C. Jones,A. Karakci,Chao-Lin Kuo,Zigmund Kermish,J. S.-Y. Leung,S. Li,D. S. Y. Mak,P. V. Mason,K. G. Megerian,Lorenzo Moncelsi,T. A. Morford,J. M. Nagy,Calvin B. Netterfield,Michael R. Nolta,Roger O'Brient,B. Osherson,Ivan L. Padilla,Ivan L. Padilla,B. Racine,Carl D. Reintsema,J. E. Ruhl,T. M. Ruud,Jamil A. Shariff,E. C. Shaw,C. Shiu,Juan D. Soler,Amy Trangsrud,Amy Trangsrud,Carole Tucker,R. S. Tucker,Anthony D. Turner,J. F. van der List,A. C. Weber,Ingunn Kathrine Wehus,S. Wen,Donald V. Wiebe,E. Y. Young,E. Y. Young +76 more
TL;DR: XFaster as discussed by the authors is a fast, iterative angular power spectrum estimator based on a diagonal approximation to the quadratic Fisher matrix estimator, which uses Monte Carlo simulations to compute noise biases and filter transfer functions.
Posted Content
In-flight gain monitoring of SPIDER's transition-edge sensor arrays.
Jeffrey P. Filippini,A. E. Gambrel,Alexandra S. Rahlin,E. Y. Young,P. A. R. Ade,M. Amiri,S. J. Benton,A. S. Bergman,R. Bihary,J. J. Bock,J. R. Bond,J. A. Bonetti,Sean Bryan,H. C. Chiang,Carlo R. Contaldi,O. Doré,Adriaan J. Duivenvoorden,H. K. Eriksen,Marzieh Farhang,Aurelien A. Fraisse,Katherine Freese,M. Galloway,N. N. Gandilo,K. Ganga,R. Gualtieri,Jon E. Gudmundsson,Mark Halpern,J. Hartley,M. Hasselfield,Gene C. Hilton,W. A. Holmes,V. V. Hristov,Zhi-Feng Huang,Kent D. Irwin,W. C. Jones,A. Karakci,C. L. Kuo,Zigmund Kermish,J. S.-Y. Leung,S. Li,D. S. Y. Mak,Peter Mason,K. G. Megerian,Lorenzo Moncelsi,T. A. Morford,J. M. Nagy,Calvin B. Netterfield,M. R. Nolta,Roger O'Brient,B. Osherson,I. L. Padilla,B. Racine,C. D. Reintsema,J. E. Ruhl,M. C. Runyan,T. M. Ruud,Jamil A. Shariff,E. C. Shaw,C. Shiu,Juan D. Soler,X. Song,A. Trangsrud,C. Tucker,R. S. Tucker,A. D. Turner,J. F. van der List,A. C. Weber,I. K. Wehus,Shyang Wen,D. V. Wiebe +69 more
TL;DR: In this paper, a sensitive and non-intrusive method for monitoring variations in TES responsivity using small square waves applied to the TES bias is proposed, which may prove useful for future balloon-and space-based instruments, where observing time and ground control bandwidth are limited.
Submillimeter Spectra of Low Temperature Gases and Mixtures
TL;DR: In this article, the spectral signature of dimers which will likely appear in far-infrared spectra of Titan was obtained by the Composite Infrared Spectrometer (CIS) onboard the Cassini spacecraft.
Clover - Measuring the CMB B-mode polarization
C. North,Peter A. R. Ade,Michael D. Audley,C. Baines,Richard A. Battye,Michael L. Brown,P. Cabella,P. G. Calisse,Anthony Challinor,William Duncan,Pedro G. Ferreira,Walter Kieran Gear,Dorota Glowacka,David J. Goldie,Paul K. Grimes,Mark Halpern,Victor Haynes,Gene C. Hilton,Kent D. Irwin,Bradley R. Johnson,M. Jones,Anthony Lasenby,P. Leahy,Jamie Leech,S. Lewis,Bruno Maffei,L. Martinis,Philip Daniel Mauskopf,Simon J. Melhuish,D. O'Dea,S. M. Parsley,Lucio Piccirillo,Giampaolo Pisano,Carl D. Reintsema,Giorgio Savini,Rashmikant V. Sudiwala,D. Sutton,Angela C. Taylor,G. Teleberg,David Titterington,V. Tsaneva,Carole Tucker,Robert A. Watson,Stafford Withington,Ghassan Yassin,Jin Zhang +45 more
TL;DR: Cluster as mentioned in this paper is a fully-funded, UK-led experiment to measure the B-mode polarisation of the Cosmic Microwave Background (CMB) with three individual telescopes operating at 97, 150 and 225 GHz, each populated by up to 256 horns.