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20142022
most citedKiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics

778 citations · 2.4k across the 16 of their papers we have counts for

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14 papers · 1 filter

astro-ph.CO2020★ 134 cited

KiDS-1000 Cosmology: constraints beyond flat CDM

Tilman Tröster, Marika Asgari, Chris Blake +26

We present constraints on extensions to the flat CDM cosmological model by varying the spatial curvature , the sum of the neutrino masses , the dark energy equati…

astro-ph.CO2020★ 778 cited

KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics

Marika Asgari, Chieh-An Lin, Benjamin Joachimi +22

We present cosmological constraints from a cosmic shear analysis of the fourth data release of the Kilo-Degree Survey (KiDS-1000), doubling the survey area with nine-band optical a…

astro-ph.CO2020★ 752 cited

KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints

Catherine Heymans, Tilman Tröster, Marika Asgari +31

We present a joint cosmological analysis of weak gravitational lensing observations from the Kilo-Degree Survey (KiDS-1000), with redshift-space galaxy clustering observations from…

astro-ph.CO2020★ 160 cited

KiDS-1000 catalogue: Weak gravitational lensing shear measurements

Benjamin Giblin, Catherine Heymans, Marika Asgari +19

We present weak lensing shear catalogues from the fourth data release of the Kilo-Degree Survey, KiDS-1000, spanning 1006 square degrees of deep and high-resolution imaging. Our `g…

astro-ph.CO2020★ 20 cited

KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies

Andrej Dvornik, Henk Hoekstra, Konrad Kuijken +13

We simultaneously present constraints on the stellar-to-halo mass relation for central and satellite galaxies through a weak lensing analysis of spectroscopically classified galaxi…

astro-ph.CO2019★ 19 cited

The effects of varying depth in cosmic shear surveys

Sven Heydenreich, Peter Schneider, Hendrik Hildebrandt +7

We present a semi-analytic model for the shear two-point correlation function of a cosmic shear survey with non-uniform depth. Ground-based surveys are subject to depth variations…

astro-ph.CO2019★ 135 cited

KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs

Marika Asgari, Tilman Tröster, Catherine Heymans +12

We present cosmological constraints from a joint cosmic shear analysis of the Kilo-Degree Survey (KV450) and the Dark Energy Survey (DES-Y1), conducted using Complete Orthogonal Se…

astro-ph.CO2019★ 176 cited

Cosmology from large-scale structure: Constraining CDM with BOSS

Tilman Tröster, Ariel. G. Sánchez, Marika Asgari +9

We reanalyse the anisotropic galaxy clustering measurement from the Baryon Oscillation Spectroscopic Survey (BOSS), demonstrating that using the full shape information provides cos…

astro-ph.CO2017★ 13 cited

Quantifying systematics from the shear inversion on weak-lensing peak counts

Chieh-An Lin, Martin Kilbinger

Weak-lensing peak counts provide a straightforward way to constrain cosmology by linking local maxima of the lensing signal to the mass function. Recent applications to data have a…

astro-ph.CO2016★ 2 cited

Cosmology with weak-lensing peak counts

Chieh-An Lin

Weak gravitational lensing (WL) causes distortions of galaxy images and probes massive structures on large scales, allowing us to understand the late-time evolution of the Universe…

astro-ph.CO2016★ 49 cited

Cosmological constraints with weak lensing peak counts and second-order statistics in a large-field survey

Austin Peel, Chieh-An Lin, Francois Lanusse +3

Peak statistics in weak lensing maps access the non-Gaussian information contained in the large-scale distribution of matter in the Universe. They are therefore a promising complem…

astro-ph.CO2016★ 32 cited

A new model to predict weak-lensing peak counts III. Filtering technique comparisons

Chieh-An Lin, Martin Kilbinger, Sandrine Pires

This is the third in a series of papers that develop a new and flexible model to predict weak-lensing (WL) peak counts, which have been shown to be a very valuable non-Gaussian pro…

astro-ph.CO2015★ 71 cited

A new model to predict weak-lensing peak counts II. Parameter constraint strategies

Chieh-An Lin, Martin Kilbinger

Peak counts have been shown to be an excellent tool to extract the non-Gaussian part of the weak lensing signal. Recently, we developped a fast stochastic forward model to predict…

astro-ph.CO2014★ 71 cited

A new model to predict weak-lensing peak counts I. Comparison with -body Simulations

Chieh-An Lin, Martin Kilbinger

Weak-lensing peak counts has been shown to be a powerful tool for cosmology. It provides non-Gaussian information of large scale structures, complementary to second order statistic…