Skip to main content
Open Access Publications from the University of California

Maps of the Southern Millimeter-wave Sky from Combined 2500 deg2 SPT-SZ and Planck Temperature Data

  • Author(s): Chown, R
  • Omori, Y
  • Aylor, K
  • Benson, BA
  • Bleem, LE
  • Carlstrom, JE
  • Chang, CL
  • Cho, H-M
  • Crawford, TM
  • Crites, AT
  • de Haan, T
  • Dobbs, MA
  • Everett, WB
  • George, EM
  • Henning, JW
  • Halverson, NW
  • Harrington, NL
  • Holder, G
  • Holzapfel, WL
  • Hou, Z
  • Hrubes, JD
  • Knox, L
  • Lee, AT
  • Luong-Van, D
  • Marrone, DP
  • McMahon, JJ
  • Meyer, SS
  • Millea, M
  • Mocanu, LM
  • Mohr, JJ
  • Natoli, T
  • Padin, S
  • Pryke, C
  • Reichardt, CL
  • Ruhl, JE
  • Sayre, JT
  • Schaffer, KK
  • Shirokoff, E
  • Simard, G
  • Staniszewski, Z
  • Stark, AA
  • Story, KT
  • Vanderlinde, K
  • Vieira, JD
  • Williamson, R
  • Wu, WLK
  • et al.

Published Web Location
No data is associated with this publication.

© 2018. The American Astronomical Society. All rights reserved. We present three maps of the millimeter-wave sky created by combining data from the South Pole Telescope (SPT) and the Planck satellite. We use data from the SPT-SZ survey, a survey of 2540 deg2 of the the sky with arcminute resolution in three bands centered at 95, 150, and 220 GHz, and the full-mission Planck temperature data in the 100, 143, and 217 GHz bands. A linear combination of the SPT-SZ and Planck data is computed in spherical harmonic space, with weights derived from the noise of both instruments. This weighting scheme results in Planck data providing most of the large-angular-scale information in the combined maps, with the smaller-scale information coming from SPT-SZ data. A number of tests have been done on the maps. We find their angular power spectra to agree very well with theoretically predicted spectra and previously published results.

Item not freely available? Link broken?
Report a problem accessing this item