THE ATACAMA COSMOLOGY TELESCOPE: CALIBRATION WITH THE <i>WILKINSON MICROWAVE ANISOTROPY PROBE</i> USING CROSS-CORRELATIONS

dc.contributor.authorHajian, Amir
dc.contributor.authorAcquaviva, Viviana
dc.contributor.authorAde, Peter A. R.
dc.contributor.authorAguirre, Paula
dc.contributor.authorAmiri, Mandana
dc.contributor.authorAppel, John William
dc.contributor.authorFelipe Barrientos, L.
dc.contributor.authorBattistelli, Elia S.
dc.contributor.authorBond, John R.
dc.contributor.authorBrown, Ben
dc.contributor.authorBurger, Bryce
dc.contributor.authorChervenak, Jay
dc.contributor.authorDas, Sudeep
dc.contributor.authorDevlin, Mark J.
dc.contributor.authorDicker, Simon R.
dc.contributor.authorDoriese, W. Bertrand
dc.contributor.authorDunkley, Joanna
dc.contributor.authorDuenner, Rolando
dc.contributor.authorEssinger-Hileman, Thomas
dc.contributor.authorFisher, Ryan P.
dc.contributor.authorFowler, Joseph W.
dc.contributor.authorHalpern, Mark
dc.contributor.authorHasselfield, Matthew
dc.contributor.authorHernandez-Monteagudo, Carlos
dc.contributor.authorHilton, Gene C.
dc.contributor.authorHilton, Matt
dc.contributor.authorHincks, Adam D.
dc.contributor.authorHlozek, Renee
dc.contributor.authorHuffenberger, Kevin M.
dc.contributor.authorHughes, David H.
dc.contributor.authorHughes, John P.
dc.contributor.authorInfante, Leopoldo
dc.contributor.authorIrwin, Kent D.
dc.contributor.authorBaptiste Juin, Jean
dc.contributor.authorKaul, Madhuri
dc.contributor.authorKlein, Jeff
dc.contributor.authorKosowsky, Arthur
dc.contributor.authorLau, Judy M.
dc.contributor.authorLimon, Michele
dc.contributor.authorLin, Yen-Ting
dc.contributor.authorLupton, Robert H.
dc.contributor.authorMarriage, Tobias A.
dc.contributor.authorMarsden, Danica
dc.contributor.authorMauskopf, Phil
dc.contributor.authorMenanteau, Felipe
dc.contributor.authorMoodley, Kavilan
dc.contributor.authorMoseley, Harvey
dc.contributor.authorNetterfield, Calvin B.
dc.contributor.authorNiemack, Michael D.
dc.contributor.authorNolta, Michael R.
dc.contributor.authorPage, Lyman A.
dc.contributor.authorParker, Lucas
dc.contributor.authorPartridge, Bruce
dc.contributor.authorReid, Beth
dc.contributor.authorSehgal, Neelima
dc.contributor.authorSherwin, Blake D.
dc.contributor.authorSievers, Jon
dc.contributor.authorSpergel, David N.
dc.contributor.authorStaggs, Suzanne T.
dc.contributor.authorSwetz, Daniel S.
dc.contributor.authorSwitzer, Eric R.
dc.contributor.authorThornton, Robert
dc.contributor.authorTrac, Hy
dc.contributor.authorTucker, Carole
dc.contributor.authorWarne, Ryan
dc.contributor.authorWollack, Ed
dc.contributor.authorZhao, Yue
dc.date.accessioned2025-01-21T00:00:32Z
dc.date.available2025-01-21T00:00:32Z
dc.date.issued2011
dc.description.abstractWe present a new calibration method based on cross-correlations with the Wilkinson Microwave Anisotropy Probe (WMAP) and apply it to data from the Atacama Cosmology Telescope (ACT). ACT's observing strategy and map-making procedure allows an unbiased reconstruction of the modes in the maps over a wide range of multipoles. By directly matching the ACT maps to WMAP observations in the multipole range of 400 < l < 1000, we determine the absolute calibration with an uncertainty of 2% in temperature. The precise measurement of the calibration error directly impacts the uncertainties in the cosmological parameters estimated from the ACT power spectra. We also present a combined map based on ACT and WMAP data that has a high signal-to-noise ratio over a wide range of multipoles.
dc.fuente.origenWOS
dc.identifier.doi10.1088/0004-637X/740/2/86
dc.identifier.eissn1538-4357
dc.identifier.issn0004-637X
dc.identifier.urihttps://doi.org/10.1088/0004-637X/740/2/86
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/95345
dc.identifier.wosidWOS:000296762900036
dc.issue.numero2
dc.language.isoen
dc.revistaAstrophysical journal
dc.rightsacceso restringido
dc.subjectcosmic background radiation
dc.subjectcosmology: observations
dc.subjectmethods: data analysis
dc.subjectmethods: statistical
dc.titleTHE ATACAMA COSMOLOGY TELESCOPE: CALIBRATION WITH THE <i>WILKINSON MICROWAVE ANISOTROPY PROBE</i> USING CROSS-CORRELATIONS
dc.typeartículo
dc.volumen740
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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