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Measurement of the thermal Sunyaev-Zel'dovich effect around cosmic voids

Abstract:
We stack maps of the thermal Sunyaev-Zel’dovich effect produced by the Planck Collaboration around the centers of cosmic voids defined by the distribution of galaxies in the CMASS sample of the Baryon Oscillation Spectroscopic Survey, scaled by the void effective radii. We report a first detection of the associated cross-correlation at the 3.4σ level: voids are under-pressured relative to the cosmic mean. We compare the measured Compton-y profile around voids with a model based solely on the spatial modulation of halo abundance with environmental density. The amplitude of the detected signal is marginally lower than predicted by an overall amplitude αv = 0.67 ± 0.2. We discuss the possible interpretations of this measurement in terms of modelling uncertainties, excess pressure in low-mass halos, or non-local heating mechanisms.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1103/PhysRevD.97.063514

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author



Publisher:
American Physical Society
Journal:
Physical Review D More from this journal
Volume:
97
Issue:
6
Article number:
063514
Publication date:
2018-03-14
Acceptance date:
2018-02-14
DOI:
EISSN:
2470-0029
ISSN:
2470-0010


Pubs id:
pubs:824478
UUID:
uuid:4d0b7f78-129e-4f0f-b82b-cd31101cd20e
Local pid:
pubs:824478
Source identifiers:
824478
Deposit date:
2018-02-14

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