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The Atacama Cosmology Telescope: Calibration with the Wilkinson Microwave Anisotropy Probe using cross-correlations

  • Amir Hajian
  • , Viviana Acquaviva
  • , Peter A.R. Ade
  • , Paula Aguirre
  • , Mandana Amiri
  • , John William Appel
  • , L. Felipe Barrientos
  • , Elia S. Battistelli
  • , John R. Bond
  • , Ben Brown
  • , Bryce Burger
  • , Jay Chervenak
  • , Sudeep Das
  • , Mark J. Devlin
  • , Simon R. Dicker
  • , W. Bertrand Doriese
  • , Joanna Dunkley
  • , Rolando Dünner
  • , Thomas Essinger-Hileman
  • , Ryan P. Fisher
  • Joseph W. Fowler, Mark Halpern, Matthew Hasselfield, Carlos Hernández-Monteagudo, Gene C. Hilton, Matt Hilton, Adam D. Hincks, Renée Hlozek, Kevin M. Huffenberger, David H. Hughes, John P. Hughes, Leopoldo Infante, Kent D. Irwin, Jean Baptiste Juin, Madhuri Kaul, Jeff Klein, Arthur Kosowsky, Judy M. Lau, Michele Limon, Yen Ting Lin, Robert H. Lupton, Tobias A. Marriage, Danica Marsden, Phil Mauskopf, Felipe Menanteau, Kavilan Moodley, Harvey Moseley, Calvin B. Netterfield, Michael D. Niemack, Michael R. Nolta, Lyman A. Page, Lucas Parker, Bruce Partridge, Beth Reid, Neelima Sehgal, Blaked Sherwin, Jon Sievers, David N. Spergel, Suzanne T. Staggs, Daniel S. Swetz, Eric R. Switzer, Robert Thornton, Hy Trac, Carole Tucker, Ryan Warne, Ed Wollack, Yue Zhao
  • University of Toronto
  • Princeton University
  • Rutgers - The State University of New Jersey, New Brunswick
  • Cardiff University
  • Pontificia Universidad Católica de Chile
  • University of British Columbia
  • University of Rome La Sapienza
  • University of Pittsburgh
  • NASA Goddard Space Flight Center
  • Lawrence Berkeley National Laboratory
  • University of Pennsylvania
  • National Institute of Standards and Technology
  • University of Oxford
  • Max Planck Institute for Astrophysics
  • University of KwaZulu-Natal
  • Council for Scientific and Industrial Research
  • University of Miami
  • Instituto Nacional de Astrofisica Optica y Electronica
  • Kavli Institute for Particle Astrophysics and Cosmology
  • Stanford University
  • Columbia University
  • The University of Tokyo
  • Johns Hopkins University
  • Haverford College
  • University of Barcelona
  • The University of Chicago
  • West Chester University
  • Harvard University

Research output: Contribution to journalArticlepeer-review

33 Scopus citations

Abstract

We 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.

Original languageEnglish
Article number86
JournalAstrophysical Journal
Volume740
Issue number2
DOIs
StatePublished - Oct 20 2011

Keywords

  • cosmic background radiation
  • cosmology: observations
  • methods: data analysis
  • methods: statistical

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