CMB lensing tomography with the DES Science Verification galaxies
Abstract
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.
- Authors:
-
- Univ. of Cambridge, Cambridge (United Kingdom); Univ.-Sternwarte, Ludwig-Maximilians Univ. Munchen, Munchen (Germany). et al.
- Publication Date:
- Research Org.:
- 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 Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- Contributing Org.:
- DES Collaboration
- OSTI Identifier:
- 1247533
- Alternate Identifier(s):
- OSTI ID: 1594615
- Report Number(s):
- DES-2015-0048; FERMILAB-PUB-15-308-AE; arXiv:1507.05551
Journal ID: ISSN 0035-8711; 1383854
- Grant/Contract Number:
- AC02-07CH11359; SC0015640
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 456; Journal Issue: 3; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; cosmic background radiation; gravitational lensing: weak; large-scale structure of Universe; mic background radiation | gravitational lensing: weak | large-scale structure of Universe | cosmic background radiation | gravitational lensing: weak | large-scale structure of Universe
Citation Formats
Giannantonio, T. CMB lensing tomography with the DES Science Verification galaxies. United States: N. p., 2016.
Web. doi:10.1093/mnras/stv2678.
Giannantonio, T. CMB lensing tomography with the DES Science Verification galaxies. United States. https://doi.org/10.1093/mnras/stv2678
Giannantonio, T. Thu .
"CMB lensing tomography with the DES Science Verification galaxies". United States. https://doi.org/10.1093/mnras/stv2678. https://www.osti.gov/servlets/purl/1247533.
@article{osti_1247533,
title = {CMB lensing tomography with the DES Science Verification galaxies},
author = {Giannantonio, T.},
abstractNote = {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.},
doi = {10.1093/mnras/stv2678},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 456,
place = {United States},
year = {Thu Jan 07 00:00:00 EST 2016},
month = {Thu Jan 07 00:00:00 EST 2016}
}
Web of Science
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