TY - JOUR
T1 - KiDS-450
T2 - Enhancing cosmic shear with clipping transformations
AU - Giblin, Benjamin
AU - Heymans, Catherine
AU - Harnois-Déraps, Joachim
AU - Simpson, Fergus
AU - Dietrich, Jörg P.
AU - Waerbeke, Ludovic Van
AU - Amon, Alexandra
AU - Asgari, Marika
AU - Erben, Thomas
AU - Hildebrandt, Hendrik
AU - Joachimi, Benjamin
AU - Kuijken, Konrad
AU - Martinet, Nicolas
AU - Schneider, Peter
AU - Tröster, Tilman
N1 - Publisher Copyright:
© 2018 The Author(s).
PY - 2018
Y1 - 2018
N2 - We present the first 'clipped' cosmic shear measurement using data from the Kilo-Degree Survey (KiDS-450). 'Clipping' transformations suppress the signal from the highest density, non-linear regions of cosmological fields. We demonstrate that these transformations improve constraints on S8 = σ8(Ωm/0.3)0.5 when used in combination with conventional two-point statistics. For the KiDS-450 data, we find that the combined measurements improve the constraints on S8 by 17 per cent, compared to shear correlation functions alone. We determine the expectation value of the clipped shear correlation function using a suite of numerical simulations, and develop methodology to mitigate the impact of masking and shot noise. Future improvements in numerical simulations and mass reconstruction methodology will permit the precise calibration of clipped cosmic shear statistics such that clipping can become a standard tool in weak-lensing analyses.
AB - We present the first 'clipped' cosmic shear measurement using data from the Kilo-Degree Survey (KiDS-450). 'Clipping' transformations suppress the signal from the highest density, non-linear regions of cosmological fields. We demonstrate that these transformations improve constraints on S8 = σ8(Ωm/0.3)0.5 when used in combination with conventional two-point statistics. For the KiDS-450 data, we find that the combined measurements improve the constraints on S8 by 17 per cent, compared to shear correlation functions alone. We determine the expectation value of the clipped shear correlation function using a suite of numerical simulations, and develop methodology to mitigate the impact of masking and shot noise. Future improvements in numerical simulations and mass reconstruction methodology will permit the precise calibration of clipped cosmic shear statistics such that clipping can become a standard tool in weak-lensing analyses.
KW - Cosmological parameters
KW - Cosmology: observations
KW - Gravitational lensing: weak
KW - Surveys
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U2 - 10.1093/MNRAS/STY2271
DO - 10.1093/MNRAS/STY2271
M3 - Article
AN - SCOPUS:85055159585
SN - 0035-8711
VL - 480
SP - 5529
EP - 5549
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 4
ER -