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19942026
most citedKiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing

1k citations · 19.5k across the 254 of their papers we have counts for

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Showing 2016 · astro-ph.COShow all

12 papers · 2 filters

astro-ph.CO2016★ 201 cited

KiDS-450: Testing extensions to the standard cosmological model

Shahab Joudaki, Alexander Mead, Chris Blake +16

We test extensions to the standard cosmological model with weak gravitational lensing tomography using 450 deg of imaging data from the Kilo Degree Survey (KiDS). In these exte…

astro-ph.CO2016★ 54 cited

Halo ellipticity of GAMA galaxy groups from KiDS weak lensing

Edo van Uitert, Henk Hoekstra, Benjamin Joachimi +14

We constrain the average halo ellipticity of ~2 600 galaxy groups from the Galaxy And Mass Assembly (GAMA) survey, using the weak gravitational lensing signal measured from the ove…

astro-ph.CO2016★ 73 cited

The-wiZZ: Clustering redshift estimation for everyone

Christopher B. Morrison, Hendrik Hildebrandt, Samuel J. Schmidt +5

We present The-wiZZ, an open source and user-friendly software for estimating the redshift distributions of photometric galaxies with unknown redshifts by spatially cross-correlati…

astro-ph.CO2016★ 14 cited

Weak-lensing shear estimates with general adaptive moments, and studies of bias by pixellation, PSF distortions, and noise

Patrick Simon, Peter Schneider

In weak gravitational lensing, weighted quadrupole moments of the brightness profile in galaxy images are a common way to estimate gravitational shear. We employ general adaptive m…

astro-ph.CO2016★ 21 cited

HIFLUGCS: X-ray luminosity -- dynamical mass relation and its implications for mass calibrations with the SPIDERS and 4MOST surveys

Yu-Ying Zhang, Thomas H. Reiprich, Peter Schneider +7

We present the X-ray luminosity (L) versus dynamical mass (M) relation for 63 nearby clusters in the HIFLUGCS. The luminosity measurements are obtained based on ~1.3 Ms of clean XM…

astro-ph.CO2016★ 12 cited

Confronting semi-analytic galaxy models with galaxy-matter correlations observed by CFHTLenS

Hananeh Saghiha, Patrick Simon, Peter Schneider +1

Testing predictions of semi-analytic models of galaxy evolution against observations help to understand the complex processes that shape galaxies. We compare predictions from the G…