ACBAR Band Powers and Window Functions
This page contains supplementary numerical data that are not
included in the Reichardt et al. power spectrum paper. If you use
these data in a publication, please cite the appropriate papers
and give the URL of this web page.
(For the Year 2006 Release of the ACBAR Band Powers and
Window Functions, please visit
this page.)
(For the Year 2002 Release of the ACBAR Band Powers and
Window Functions, please visit
this page.)
Decorrelated Band Powers:
text file
File format:
Band # |
Band Power (uK^2) |
Uncertainty (uK^2) |
Log-normal Offset |
ACBAR only. (Click on plot for higher resolution version.)
ACBAR + WMAP3 + BOOMERANG03. (Click on plot for higher resolution version.)
High-l only. (Click on plot for higher resolution version.)
ACBAR + WMAP3. (Click on plot for higher resolution version.)
Decorrelated Window Functions:
text file
File Format:
Band # |
Mupltipole |
Decorrelated Window Function (W_l/l) |
ACBAR Window functions, normalized to unity. (Click on plot for higher resolution version.)
Please contact Christian Reichardt with
questions about the usage of this data.
Beam Uncertainty:
text file
File Format:
Mupltipole |
Fractional Beam Error (delta_B_l/B_l) |
ACBAR CosmoMC Files:
gzipped tar file
Untar the file in the main cosmomc directories. Files will be added to
the data and data/windows directories. The newdat file is a standard
format that can be included in the cosmomc .ini files. The calibration
and beam errors are already set as described in Reichardt et al. 2008.
Please contact
Christian Reichardt or
Carlo Contaldi with
questions about the usage of this data.
Postscript
preprint of the paper available at astro-ph/0801.1491.
The initial draft of this paper used WMAP3 as a calibration source. The original band-powers can be found here . The original CosmoMC files can be found here. The file types are the same as above.
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