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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Journal ArticleDOI
Spider optimization : probing the systematics of a large-scale b-mode experiment
C. J. MacTavish,Peter A. R. Ade,Elia S. Battistelli,S. J. Benton,R. Bihary,James J. Bock,James J. Bock,J. R. Bond,Justus A. Brevik,Sean Bryan,Carlo R. Contaldi,B. P. Crill,Olivier Doré,Laura M. Fissel,Sunil Golwala,Mark Halpern,Gene C. Hilton,Warren Holmes,Viktor Hristov,Kent D. Irwin,W. C. Jones,W. C. Jones,Chao-Lin Kuo,Andrew E. Lange,C. Lawrie,T. G. Martin,Peter Mason,T. E. Montroy,Calvin B. Netterfield,Daniel Riley,J. E. Ruhl,Marcus Runyan,Amy Trangsrud,Carole Tucker,Anthony D. Turner,Marco P. Viero,Donald Wiebe +36 more
TL;DR: Spider is a long-duration, balloon-borne polarimeter designed to measure large-scale cosmic microwave background (CMB) polarization with very high sensitivity and control of systematics as mentioned in this paper.
Journal ArticleDOI
Breaking the Redshift Deadlock - I: Constraining the star formation history of galaxies with sub-millimetre photometric redshifts
David H. Hughes,Itziar Aretxaga,E. L. Chapin,Enrique Gaztanaga,James Dunlop,Mark J. Devlin,Mark Halpern,J. O. Gundersen,Jacob Klein,Calvin B. Netterfield,Luca Olmi,Douglas Scott,Gregory S. Tucker +12 more
TL;DR: In this paper, Monte-Carlo simulations of ground-based, balloon-borne and satellite sub-millimetre surveys were used to derive photometric redshifts with an r.m.s accuracy of +/- 0.4 over the range 0 3 x 10^12 Lsun] with an accuracy of 20 per cent.
Journal ArticleDOI
Quantifying the BICEP2-Planck tension over gravitational waves.
TL;DR: It is shown that measurements of TE and EE power spectra in the near future will discriminate between the hypotheses that this tension is either a statistical fluke or a sign of new physics.
Journal ArticleDOI
A SCUBA scan-map of the Hubble Deep Field: measuring the bright end of the submillimetre source counts
TL;DR: In this article, the authors used the 850-μm SCUBA camera on the JCMT and a scanning technique different from other sub-mm surveys to obtain a 125 arcmin 2 map centred on the Hubble Deep Field.
Posted Content
The First CHIME/FRB Fast Radio Burst Catalog
Chime,Mandana Amiri,B. C. Andersen,Kevin Bandura,Sabrina Berger,Mohit Bhardwaj,M. M. Boyce,P. J. Boyle,Charanjot Brar,Daniela Breitman,Tomas Cassanelli,P. Chawla,Tianyue Chen,J. F. Cliche,Amanda Cook,D. Cubranic,Alice P. Curtin,Meiling Deng,Matt Dobbs,Fengqiu,Dong,Gwendolyn Eadie,M. Fandino,Emmanuel Fonseca,Bryan Gaensler,Utkarsh Giri,Deborah C. Good,Mark Halpern,Alex S. Hill,Gary Hinshaw,A. Josephy,Jane F. Kaczmarek,Zarif Kader,Joseph W. Kania,Victoria M. Kaspi,T. L. Landecker,Dustin Lang,Calvin Leung,D. Z. Li,Hsiu-Hsien Lin,Kiyoshi Masui,R. Mckinven,J. Mena-Parra,M. Merryfield,B. W. Meyers,Daniele Michilli,N. Milutinovic,Arash Mirhosseini,Moritz Münchmeyer,A. Naidu,Laura Newburgh,Cherry Ng,C. Patel,Ue-Li Pen,Emily Petroff,T. Pinsonneault-Marotte,Ziggy Pleunis,M. Rafiei-Ravandi,Mubdi Rahman,Scott M. Ransom,A. Renard,Pranav Sanghavi,Paul Scholz,J. Richard Shaw,Kaitlyn Shin,Seth Siegel,Andrew E. Sikora,Saurabh Singh,Kendrick M. Smith,Ingrid H. Stairs,C. M. Tan,Shriharsh P. Tendulkar,K. Vanderlinde,Haochen Wang,Dallas Wulf,A. V. Zwaniga +75 more
TL;DR: In this article, the authors presented a catalog of 536 fast radio bursts (FRBs) detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) Project between 400 and 800 MHz from 2018 July 25 to 2019 July 1, including 62 bursts from 18 previously reported repeating sources.