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The Aeon Before Ours · source record · paper

Searching for concentric low variance circles in the cosmic microwave background

DeAbreu, A.; Contreras, D.; Scott, D. · 2015

AI-verified citationSRC-DEABREU-2015
identifier / locator
Journal of Cosmology and Astroparticle Physics 2015(12): 031. DOI: 10.1088/1475-7516/2015/12/031 (arXiv:1508.05158)
url
https://arxiv.org/pdf/1508.05158
verification note
DOI confirmed via Crossref; abstract confirmed via the arXiv API.
reliability notes
  • Extends the reanalysis to Planck data using the proponents' own published parameter choices; confirms the special directions exist and finds them at the same abundance in simulated Gaussian skies.

Evidence drawn from this source

Undermines· strongCCC-E008

DeAbreu, Contreras & Scott 2015: proponents' own parameters, Planck data, same verdict

what the source states
"We are able to reproduce the analysis these authors presented for data from the WMAP satellite and we confirm the existence of these apparently special directions in the newer Planck data. However, we also find that these features are present at the same level of abundance in simulated Gaussian CMB skies, i.e. they are entirely consistent with the predictions of the standard cosmological model."
what we infer
Methodologically the strictest of the circle reanalyses: it froze the search parameters to the proponents' own published choices (a de facto prespecification), extended the search to Planck data, and still found the features at chance abundance. The proponents' published response is that it did not repeat the sky-twist ellipticity test and did not explain the anisotropy of the centers — both true, both recorded (CCC-E006, CCC-C504).
limitations
  • Did not test the sky-twist/ellipticity statistic, which the proponents regard as their strongest point.