Arcminute Cosmology Bolometer Array Receiver

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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 Band Powers
ACBAR only. (Click on plot for higher resolution version.)

ACBAR + WMAP3 Band Powers
ACBAR + WMAP3 + BOOMERANG03. (Click on plot for higher resolution version.)

High-l Band Powers
High-l only. (Click on plot for higher resolution version.)

ACBAR + WMAP3 Band Powers
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
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.

 
Copyright © Holzapfel Group, 2006 Page last modified December 10, 2006