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Extragalactic Radio Sources and the WMAP Cold Spot

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Rudnick, Lawrence, Brown, Shea, Williams, Liliya R.·2007·The Astrophysical Journal

Abstract

We detect a dip of 20%-45% in the surface brightness and number counts of NRAO VLA Sky Survey (NVSS) sources smoothed to a few degrees at the location of the WMAP cold spot. The dip has structure on scales of ~1° to 10°. Together with independent all-sky wavelet analyses, our results suggest that the dip in extragalactic brightness and number counts and the WMAP cold spot are physically related, i.e., that the coincidence is neither a statistical anomaly nor a WMAP foreground-correction problem. If the cold spot does originate from structures at modest redshifts, as we suggest, then there is no remaining need for non-Gaussian processes at the last scattering surface of the cosmic microwave background (CMB) to explain the cold spot. The late integrated Sachs-Wolfe effect, already seen statistically for NVSS source counts, can now be seen to operate on a single region. To create the magnitude and angular size of the WMAP cold spot requires a ~140 Mpc radius completely empty void at z ≤ 1 along this line of sight. This is far outside the current expectations of the concordance cosmology, and adds to the anomalies seen in the CMB.

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Metadata

Authors
Rudnick, L., Brown, S., & Williams, L. R.
Venue
The Astrophysical Journal
Published
2007-12-10
Volume
671
Issue
1
Pages
40-44
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2090960271
Cited by
173
References
1
FWCI
12.28
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Extragalactic Radio Sources and the WMAP Cold Spot. https://app.cochat.ai/papers/10.1086/522222
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Rudnick, L., Brown, S., & Williams, L. R. (2007). Extragalactic Radio Sources and the WMAP Cold Spot. The Astrophysical Journal. https://doi.org/10.1086/522222

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