Mark Halpern
Affiliations: | University of British Columbia, Vancouver, Vancouver, BC, Canada |
Area:
Astronomy and AstrophysicsWebsite:
https://phas.ubc.ca/users/mark-halpernGoogle:
"Mark Halpern"Mean distance: 13975
Parents
Sign in to add mentorRainer Weiss | grad student | 1983 | MIT | |
(Measurement of the anisotropy of the cosmic background radiation at millimeter wavelengths) |
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Publications
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Weiland JL, Addison GE, Bennett CL, et al. (2020) An Examination of Galactic Polarization with Application to the Planck TB Correlation The Astrophysical Journal. 893: 119 |
Gralla MB, Marriage TA, Addison G, et al. (2020) Atacama Cosmology Telescope: Dusty Star-forming Galaxies and Active Galactic Nuclei in the Equatorial Survey The Astrophysical Journal. 893: 104 |
Madhavacheril MS, Hill JC, Næss S, et al. (2020) Atacama Cosmology Telescope: Component-separated maps of CMB temperature and the thermal Sunyaev-Zel’dovich effect Physical Review D. 102 |
Osherson B, Filippini JP, Fu J, et al. (2020) Particle Response of Antenna-Coupled TES Arrays: Results from SPIDER and the Laboratory Journal of Low Temperature Physics. 199: 1127-1136 |
Zhang C, Ade PAR, Ahmed Z, et al. (2020) Characterizing the Sensitivity of 40 GHz TES Bolometers for BICEP Array Journal of Low Temperature Physics. 199: 968-975 |
Schillaci A, Ade PAR, Ahmed Z, et al. (2020) Design and Performance of the First BICEP Array Receiver Journal of Low Temperature Physics. 199: 976-984 |
St Germaine T, Ade PAR, Ahmed Z, et al. (2020) Optical Characterization of the Keck Array and BICEP3 CMB Polarimeters from 2016 to 2019 Journal of Low Temperature Physics. 199: 824-832 |
Dahal S, Amiri M, Appel JW, et al. (2020) The CLASS 150/220 GHz Polarimeter Array: Design, Assembly, and Characterization Journal of Low Temperature Physics. 199: 289-297 |
Soliman A, Ade PAR, Ahmed Z, et al. (2020) Optical Design and Characterization of 40-GHz Detector and Module for the BICEP Array Journal of Low Temperature Physics. 199: 1118-1126 |
Switzer ER, Ade PAR, Baildon T, et al. (2019) Sub-Kelvin cooling for two kilopixel bolometer arrays in the PIPER receiver. The Review of Scientific Instruments. 90: 095104 |