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Project Supported by
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NSF, National Science Foundation
KICP, Kavli Institute for Cosmological Physics
USAP, United States Antarctic Program
Antarctic Support Contract (ASC)
DOE Office of Science High Energy Physics
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Related Websites
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CBI, Cosmic Background Imager
DASI, Degree Angular Scale Interferometer
WMAP, Wilkinson Microwave Anisotropy Probe
Planck
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 | Map products |
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Temperature maps in micro-Kelvins in SFL and ZEA projections (Section 5):
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Bright source thumbnail temperature maps for all bands in micro-Kelvins in the ZEA projection (Section 3.4):
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Apodization masks in SFL and ZEA projections (Section 5.1.1):
Binay pixel masks in SFL and ZEA projections (Section 5.1.1) used in the cluster and source catalog constructions, respectively. The EDF-S mask was used to flag objects as inside or outside the Q1 region.
Telescope beams (Section 5.1.2). The file contains the B_ells for each band (one per column).
Noise amplitude spectral densities in micro-Kelvins used only in the cluster catalog construction (Section 5.1.3):
Transfer function (Section 5.1.4):
CLEAN beam maps in mJy (see Section 4.1, Section 6) associated with the emissive source catalog:
Signal-to-noise ratio maps (see Section 4.2, Section 7) associated with the galaxy cluster catalog:
 | Catalogs |
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Emissive source catalog (Section 6):
Galaxy cluster catalog (Section 7):
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