Extragalactic Radio Sources and the WMAP Cold Spot

By L. Rudnick, S. Brown, L. Williams. 2007

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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.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/a43d04444dbf536f54575bae4e530e951ed67f99

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In Astronomy and Astrophysics

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  2. A. Riess
  3. Mark Halpern
  4. C. Bennett
  5. David N. Spergel
  6. J. Weiland
  7. Gary F. Hinshaw
  8. Volker Springel

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