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Cosmological lensing ratios with DES Y1, SPT and Planck

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Correlations between tracers of the matter density field and gravitational lensing are sensitive to the evolution of the matter power spectrum and the expansion rate across cosmic time. Appropriately defined ratios of such correlation functions, on the other hand, depend only on the angular diameter distances to the tracer objects and to the gravitational lensing source planes. Because of their simple cosmological dependence, such ratios can exploit available signal-to-noise down to small angular scales, even where directly modeling the correlation functions is difficult. We present a measurement of lensing ratios using galaxy position and lensing data from the Dark Energy Survey, and CMB lensing data from the South Pole Telescope and Planck, obtaining the highest precision lensing ratio measurements to date. Relative to the concordance ΛCDM model, we find a best fit lensing ratio amplitude of A = 1.1 ± 0.1. We use the ratio measurements to generate cosmological constraints, focusing on the curvature parameter. We demonstrate that photometrically selected galaxies can be used to measure lensing ratios, and argue that future lensing ratio measurements with data from a combination of LSST and Stage-4 CMB experiments can be used to place interesting cosmological constraints, even after considering the systematic uncertainties associated with photometric redshift and galaxy shear estimation.
Original languageEnglish
Number of pages17
JournalMonthly Notices of the Royal Astronomical Society
Early online date14 May 2019
DOIs
Publication statusEarly online - 14 May 2019

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  • Cosmological lensing ratios

    Rights statement: This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record, J. Prat, et.al. (2019). 'Cosmological lensing ratios with DES Y1, SPT and Planck'. MNRAS, stz1309. is available online at: https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stz1309/5489191.

    Accepted author manuscript (Post-print), 1.33 MB, PDF document

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