Weak lensing magnification in the Dark Energy Survey Science Verification data
Journal Article
·
· Monthly Notices of the Royal Astronomical Society
- Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas (CIEMAT), Madrid (Spain). et al.
In this paper, the effect of weak lensing magnification on galaxy number counts is studied by cross-correlating the positions of two galaxy samples, separated by redshift, using the Dark Energy Survey Science Verification data set. This analysis is carried out for galaxies that are selected only by its photometric redshift. An extensive analysis of the systematic effects, using new methods based on simulations is performed, including a Monte Carlo sampling of the selection function of the survey.
- Research Organization:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- Contributing Organization:
- The DES Collaboration
- Grant/Contract Number:
- AC02-76SF00515; AST-1138766; AYA2012-39559; ESP2013-48274; FPA2015-68048; SEV-2012-0234; MDM-2015-0509; FP7/2007-2013; 240672; 291329; 306478; AC02-07CH11359; AC05-00OR22725
- OSTI ID:
- 1434674
- Alternate ID(s):
- OSTI ID: 1362052; OSTI ID: 1435207
- Report Number(s):
- DES-2016-0203; FERMILAB-PUB-16-567-AE; arXiv:1611.10326; TRN: US1802686
- Journal Information:
- Monthly Notices of the Royal Astronomical Society, Vol. 476, Issue 1; ISSN 0035-8711
- Publisher:
- Royal Astronomical SocietyCopyright Statement
- Country of Publication:
- United States
- Language:
- English
Cited by: 15 works
Citation information provided by
Web of Science
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