Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 466, Issue 3, Pages 2799-2804Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stw3233
Keywords
cosmology : observations; large-scale structure of Universe
Categories
Funding
- CAPES
- Science without Borders Program of CAPES [88881.064966/20140-1]
- Science without Borders Program of CNPq [234529/2014-08]
- CNPq
- FAPERJ
- INEspaco
- ESA Member State, NASA
- ESA Member State, Canada
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We probe the statistical isotropy hypothesis of the large-scale structure with the second Planck Sunyaev-Zeldovich (PSZ2) galaxy clusters data set. Our analysis adopts a statistical-geometrical method that compares the two-point angular-correlation function of objects in antipodal patches of the sky. Given possible observational biases, such as the presence of anisotropic sky cuts and the non-uniform exposure of Planck's instrumentation, ensembles of Monte Carlo realizations are produced in order to assess the significance of our results. When these observational effects are properly taken into account, we find neither evidence for preferred directions in the sky nor signs of large-angle features in the galaxy clusters celestial distribution. The PSZ2 data set is, therefore, in good concordance with the fundamental hypothesis of large-angle isotropy of cosmic objects.
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