2006MNRAS.369..598C


Query : 2006MNRAS.369..598C

2006MNRAS.369..598C - Mon. Not. R. Astron. Soc., 369, 598-602 (2006/June-3)

No Higher Criticism of the Bianchi-corrected Wilkinson Microwave Anisotropy Probe data.

CAYON L., BANDAY A.J., JAFFE T., ERIKSEN H.K., HANSEN F.K., GORSKI K.M. and JIN J.

Abstract (from CDS):

Higher Criticism (HC) has been proposed by Donoho & Jin as an effective statistic to detect deviations from Gaussianity. Motivated by the success of the Bianchi VIIhmodel in addressing many of the anomalies observed in the Wilkinson Microwave Anisotropy Probe (WMAP) data (Jaffe et al.), we present calculations in real and in wavelet space of the HC statistic of the Bianchi-corrected WMAP first-year data. At the wavelet scale of 5°, the HC of the WMAP map drops from a value above the 99 per cent confidence level (c.l.) to a value below the 68 per cent CL when corrected by the Bianchi template. An important property of the HC statistic is its ability to locate the pixels that account for the deviation from Gaussianity. The analysis of the uncorrected WMAP data pointed to a cold spot in the Southern hemisphere, centred at l ∼ 209°, b ∼ -57°. The HC of the Bianchi-corrected map indicates that this spot remains prominent, albeit at a level completely consistent with Gaussian statistics. Consequently, it is debatable how much emphasis should be placed on this residual feature, but we consider the effect of modestly increasing the scaling of the template. A factor of only 1.2 renders the spot indistinguishable from the background level, with no noticeable impact on the results published in Jaffe et al. for the low-l anomalies, large-scale power asymmetry or wavelet kurtosis. A trivial interpretation would be that the Bianchi template may require a small enhancement of power on scales corresponding to the wavelet scale of 5°.

Abstract Copyright: 2006 The Authors. Journal compilation © 2006 RAS

Journal keyword(s): methods: statistical - cosmic microwave background - cosmology: miscellaneous

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME the Cold Spot ? 03 13 -20.5           ~ 52 0

Query : 2006MNRAS.369..598C

Basic data :
NAME the Cold Spot -- Object of Unknown Nature
Other object types:
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ICRS coord. (ep=J2000) :
03 13 00.0 -20 30 00 [ ] E 2005MNRAS.356...29C
FK4 coord. (ep=B1950 eq=1950) :
03 10 44.9 -20 41 11 [ ]
Gal coord. (ep=J2000) :
209.0818 -57.0643 [ ]
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Identifiers (2) :
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NAME the Cold Spot NAME the Spot

References (52 between 1850 and 2026) (Total 52)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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