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ACTPol: on-sky performance and characterization

Author(s): Grace, E; Beall, J; Bond, JR; Cho, HM; Datta, R; et al

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dc.contributor.authorGrace, E-
dc.contributor.authorBeall, J-
dc.contributor.authorBond, JR-
dc.contributor.authorCho, HM-
dc.contributor.authorDatta, R-
dc.contributor.authorDevlin, MJ-
dc.contributor.authorDuenner, R-
dc.contributor.authorFox, AE-
dc.contributor.authorGallardo, P-
dc.contributor.authorHasselfield, M-
dc.contributor.authorHenderson, S-
dc.contributor.authorHilton, GC-
dc.contributor.authorHincks, AD-
dc.contributor.authorHlozek, R-
dc.contributor.authorHubmayr, J-
dc.contributor.authorIrwin, K-
dc.contributor.authorKlein, J-
dc.contributor.authorKoopman, B-
dc.contributor.authorLi, D-
dc.contributor.authorLungu, M-
dc.contributor.authorNewburgh, L-
dc.contributor.authorNibarger, JP-
dc.contributor.authorNiemack, MD-
dc.contributor.authorMaurin, L-
dc.contributor.authorMcMahon, J-
dc.contributor.authorNaess, S-
dc.contributor.authorPage Jr., Lyman A.-
dc.contributor.authorPappas, C-
dc.contributor.authorSchmitt, BL-
dc.contributor.authorSievers, J-
dc.contributor.authorStaggs, ST-
dc.contributor.authorThornton, R-
dc.contributor.authorVan Lanen, J-
dc.contributor.authorWollack, EJ-
dc.date.accessioned2022-01-25T16:10:14Z-
dc.date.available2022-01-25T16:10:14Z-
dc.date.issued2014en_US
dc.identifier.citationGrace, E, Beall, J, Bond, JR, Cho, HM, Datta, R, Devlin, MJ, Duenner, R, Fox, AE, Gallardo, P, Hasselfield, M, Henderson, S, Hilton, GC, Hincks, AD, Hlozek, R, Hubmayr, J, Irwin, K, Klein, J, Koopman, B, Li, D, Lungu, M, Newburgh, L, Nibarger, JP, Niemack, MD, Maurin, L, McMahon, J, Naess, S, Page, LA, Pappas, C, Schmitt, BL, Sievers, J, Staggs, ST, Thornton, R, Van Lanen, J, Wollack, EJ. (2014). ACTPol: on-sky performance and characterization. MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VII, 9153 (10.1117/12.2057243en_US
dc.identifier.issn0277-786X-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1rf5kf69-
dc.description.abstractACTPol is the polarization-sensitive receiver on the Atacama Cosmology Telescope. ACTPol enables sensitive millimeter wavelength measurements of the temperature and polarization anisotropies of the Cosmic Microwave Background (CMB) at arcminute angular scales. These measurements are designed to explore the process of cosmic structure formation, constrain or determine the sum of the neutrino masses, probe dark energy, and provide a foundation for a host of other cosmological tests. We present an overview of the first season of ACTPol observations focusing on the optimization and calibration of the first detector array as well as detailing the on-sky performance.en_US
dc.language.isoenen_US
dc.relation.ispartofMILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VIIen_US
dc.rightsFinal published version. This is an open access article.en_US
dc.titleACTPol: on-sky performance and characterizationen_US
dc.typeConference Articleen_US
dc.identifier.doi10.1117/12.2057243-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/conference-proceedingen_US

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