CBI   Cosmic Background Imager  

Supplementary Data (2004)

Here we present supplementary numerical data for the CBI observations reported by A. C. S. Readhead et al. (2004 ApJ, 609, 498-512, preprinted as astro-ph/0402359). If you use these data in a publication, please cite the appropriate papers and also give the URL of this web page and the date of publication (given at the bottom of this page).

The CBI even binning data (bins 2 to 14) formatted for use with the COSMOMC Markov Chain Monte Carlo package (Lewis & Bridle 2002, Phys. Rev. D, 66, 103511) can be found in the compressed tar file CBI2.0_newdat.tgz (revised 2006 Aug 25). Note: this replaces the file cbi2.0.tgz (revised 2004 Mar 3), in which the Fisher matrix was incorrectly transformed for the offset-lognormal approximation. Thanks to Loison Hoi for pointing out the error. For more information, see the discussion in the CosmoCoffee CMB forum.

Calibration

The CBI 2000+2001 data have been scaled to a 32 GHz Jupiter temperature of 147.3 ± 1.8 K. This is a weighted mean between the WMAP 32 GHz value and the OVRO absolute measurement (see the paper).

The CBI overall calibration error should be taken as 1.3% in flux density (2.6% in power).

Band Powers

Band power measurements are given in Table 1 of Readhead et al. There are two alternate binnings of the power spectrum, which are not independent. We recommend use of the even binning, reproduced here. Bins 1 and 15 were not used in the parameter analysis of Readhead et al.

bin     C_B    Fisher error X_B   lmin  lmax

1       7091   1882        3176     0   300
2       2059    717         489   300   400
3       1688    457         377   400   500
4       2415    545         449   500   600
5       1562    391         424   600   700
6       2201    490         577   700   800
7       2056    436         631   800   900
8       1158    396         744   900  1000
9        797    275         675  1000  1140
10       780    263         726  1140  1280
11       586    278         934  1280  1420
12      1166    361        1064  1420  1560
13       196    223         941  1560  1760
14        -4    203         386  1760  1960
15       355    103        2184  1960+ 

Bandpower Covariance Matrix (normalized)

  1.000 -0.264  0.037 -0.014  0.002 -0.002 -0.001 -0.001 -0.001  0.000  0.000  0.000  0.000  0.000 -0.001
 -0.264  1.000 -0.253  0.046 -0.015  0.001 -0.002 -0.001 -0.001 -0.001 -0.001 -0.001 -0.001  0.000 -0.002
  0.037 -0.253  1.000 -0.297  0.055 -0.017  0.001 -0.002 -0.002 -0.002 -0.001 -0.001 -0.002 -0.001 -0.004
 -0.014  0.046 -0.297  1.000 -0.283  0.054 -0.017  0.000 -0.002 -0.002 -0.002 -0.001 -0.002 -0.001 -0.005
  0.002 -0.015  0.055 -0.283  1.000 -0.290  0.053 -0.014 -0.001 -0.003 -0.002 -0.002 -0.003 -0.002 -0.007
 -0.002  0.001 -0.017  0.054 -0.290  1.000 -0.288  0.048 -0.014 -0.001 -0.002 -0.002 -0.002 -0.002 -0.007
 -0.001 -0.002  0.001 -0.017  0.053 -0.288  1.000 -0.278  0.047 -0.012 -0.003 -0.003 -0.004 -0.002 -0.010
 -0.001 -0.001 -0.002  0.000 -0.014  0.048 -0.278  1.000 -0.303  0.041 -0.009 -0.003 -0.005 -0.003 -0.011
 -0.001 -0.001 -0.002 -0.002 -0.001 -0.014  0.047 -0.303  1.000 -0.256  0.023 -0.009 -0.010 -0.007 -0.021
  0.000 -0.001 -0.002 -0.002 -0.003 -0.001 -0.012  0.041 -0.256  1.000 -0.264  0.028 -0.016 -0.008 -0.025
  0.000 -0.001 -0.001 -0.002 -0.002 -0.002 -0.003 -0.009  0.023 -0.264  1.000 -0.277  0.035 -0.017 -0.027
  0.000 -0.001 -0.001 -0.001 -0.002 -0.002 -0.003 -0.003 -0.009  0.028 -0.277  1.000 -0.289  0.053 -0.034
  0.000 -0.001 -0.002 -0.002 -0.003 -0.002 -0.004 -0.005 -0.010 -0.016  0.035 -0.289  1.000 -0.357 -0.031
  0.000  0.000 -0.001 -0.001 -0.002 -0.002 -0.002 -0.003 -0.007 -0.008 -0.017  0.053 -0.357  1.000 -0.257
 -0.001 -0.002 -0.004 -0.005 -0.007 -0.007 -0.010 -0.011 -0.021 -0.025 -0.027 -0.034 -0.031 -0.257  1.000

Band Power Window Functions

See Figure 5 of Readhead et al. The even window functions are tabulated in file total_joint-tot_x50_a_even-win.txt . This file has 15 columns, one for each bin (1...15), and 4599 rows, for l = 2...4600. The numbers tabulated are WB(l), but are not normalized:

Band power calculation

Last update: 2006 Aug 25

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