CMB lensing tomography with the DES Science Verification galaxies

Giannantonio, T.

doi:10.1093/mnras/stv2678

Title: CMB lensing tomography with the DES Science Verification galaxies

Journal Article · Thu Jan 07 00:00:00 EST 2016 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stv2678· OSTI ID:1247533

Giannantonio, T. ^[1]

Univ. of Cambridge, Cambridge (United Kingdom); Univ.-Sternwarte, Ludwig-Maximilians Univ. Munchen, Munchen (Germany). et al.

We measure the cross-correlation between the galaxy density in the Dark Energy Survey (DES) Science Verification data and the lensing of the cosmic microwave background (CMB) as reconstructed with the Planck satellite and the South Pole Telescope (SPT). When using the DES main galaxy sample over the full redshift range 0.2 < z_phot < 1.2, a cross-correlation signal is detected at 6σ and 4σ with SPT and Planck , respectively. We then divide the DES galaxies into five photometric redshift bins, finding significant (>2σ) detections in all bins. Comparing to the fiducial Planck cosmology, we find the redshift evolution of the signal matches expectations, although the amplitude is consistently lower than predicted across redshift bins. We test for possible systematics that could affect our result and find no evidence for significant contamination. Finally, we demonstrate how these measurements can be used to constrain the growth of structure across cosmic time. We find the data are fit by a model in which the amplitude of structure in the z < 1.2 universe is 0.73 ± 0.16 times as large as predicted in the Λ cold dark matter Planck cosmology, a 1.7σ deviation.

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Research Organization:: Argonne National Laboratory (ANL), Argonne, IL (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Univ. of Illinois at Urbana-Champaign, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Contributing Organization:: DES Collaboration

Grant/Contract Number:: AC02-07CH11359; SC0015640

OSTI ID:: 1247533

Alternate ID(s):: OSTI ID: 1594615

Report Number(s):: DES-2015-0048; FERMILAB-PUB-15-308-AE; arXiv:1507.05551; 1383854

Journal Information:: Monthly Notices of the Royal Astronomical Society, Vol. 456, Issue 3; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 87 works

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