Large Imaging Surveys For Cosmology: Cosmic Magnification And Photometric Calibration
Creators: name: Boucaud, Alexandre
Publisher: name: Zenodo
Year: 2013
Subjects: cosmology
dark energy
gravitational lensing
cosmic magnification
photometric calibration
LSST

description: This work focuses on the use of deep, wide field surveys to extract new cosmo- logical information. Precise photometry plays a large role in this quest, through the determination of photometric redshifts and the propagation of photometric errors into the cosmological results. This is a unifying theme which effectively ties both parts of the thesis together.

After a general review of cosmology and the measurements that support the ΛCDM model, and a description of the Large Synoptic Survey Telescope (LSST), the first part of this work deals with the influence of the variation of main atmospheric con- stituents on ground-based photometry, focusing particularly on the LSST site at Cerro Pachón, Chile. We process all recent available data on ozone, water vapor and aerosols to construct a long-term atmospheric simulation and estimate quanti- tatively how the spatial and temporal gradients of these constituents would affect LSST calibration process.

The second part of this work starts with a theoretical description of gravitational lensing, concentrating on the weak lensing aspect. After discussing the advantages and difficulties of cosmic shear measurements, we explore the use of cosmic magni- fication, together with the redshift tomography enabled by the LSST, to constrain cosmological models. We find that cosmic magnification covariance is beset by in- trinsic clustering but nevertheless represents a useful probe of galaxy bias and dark energy that complements cosmic shear, and which can increase the robustness of cosmological constraints from lensing surveys.
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