More out of less: an excess integrated Sachs-Wolfe signal from supervoids mapped out by the Dark Energy Survey
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The largest structures in the cosmic web probe the dynamical nature of dark energy through their integrated Sachs–Wolfe imprints. In the strength of the signal, typical cosmic voids have shown good consistency with expectation AISW = ΔTdata/ΔTtheory = 1, given the substantial cosmic variance. Discordantly, large-scale hills in the gravitational potential, or supervoids, have shown excess signals. In this study, we mapped out 87 new supervoids in the total 5000 deg2 footprint of the Dark Energy Survey at 0.2 < z < 0.9 to probe these anomalous claims. We found an excess imprinted profile with AISW ≈ 4.1 ± 2.0 amplitude. The combination with independent BOSS data reveals an ISW imprint of supervoids at the 3.3σ significance level with an enhanced AISW ≈ 5.2 ± 1.6 amplitude. The tension with ΛCDM predictions is equivalent to 2.6σ and remains unexplained.
Original language | English |
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Article number | stz341 |
Pages (from-to) | 5267-5277 |
Number of pages | 11 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 484 |
Issue number | 4 |
Early online date | 6 Feb 2019 |
DOIs | |
Publication status | Published - 21 Apr 2019 |
Documents
- 1811.07812v2
Rights statement: This is a pre-copyedited, author-produced version of an article accepted for publication in MNRAS following peer review. The version of record A Kovács et al., More out of less: an excess integrated Sachs–Wolfe signal from supervoids mapped out by the Dark Energy Survey, Monthly Notices of the Royal Astronomical Society, Volume 484, Issue 4, 21 April 2019, Pages 5267–5277 is available online at: https://academic.oup.com/mnras/article/484/4/5267/5307893 and DOI: 10.1093/mnras/stz341.
Accepted author manuscript (Post-print), 0.98 MB, PDF document
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