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Evidence against a supervoid causing the CMB Cold Spot

Authors :
Mackenzie, Ruari
Shanks, Tom
Bremer, Malcolm N.
Cai, Yan-Chuan
Gunawardhana, Madusha L. P.
Kovács, András
Norberg, Peder
Szapudi, Istvan
Publication Year :
2017

Abstract

We report the results of the 2dF-VST ATLAS Cold Spot galaxy redshift survey (2CSz) based on imaging from VST ATLAS and spectroscopy from 2dF AAOmega over the core of the CMB Cold Spot. We sparsely surveyed the inner 5$^{\circ}$ radius of the Cold Spot to a limit of $i_{AB} \le 19.2$, sampling $\sim7000$ galaxies at $z<0.4$. We have found voids at $z=$ 0.14, 0.26 and 0.30 but they are interspersed with small over-densities and the scale of these voids is insufficient to explain the Cold Spot through the $\Lambda$CDM ISW effect. Combining with previous data out to $z\sim1$, we conclude that the CMB Cold Spot could not have been imprinted by a void confined to the inner core of the Cold Spot. Additionally we find that our 'control' field GAMA G23 shows a similarity in its galaxy redshift distribution to the Cold Spot. Since the GAMA G23 line-of-sight shows no evidence of a CMB temperature decrement we conclude that the Cold Spot may have a primordial origin rather than being due to line-of-sight effects.<br />Comment: Submitted to MNRAS

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.1704.03814
Document Type :
Working Paper
Full Text :
https://doi.org/10.1093/mnras/stx931