activity
20072026
most citedKiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing

1k citations · 9.4k across the 114 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

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★ 207 cited

The SPTpol Extended Cluster Survey

L. E. Bleem, S. Bocquet, B. Stalder +135

We describe the observations and resultant galaxy cluster catalog from the 2770 deg SPTpol Extended Cluster Survey (SPT-ECS). Clusters are identified via the Sunyaev-Zel'dovich…

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.CO2019★ 173 cited

Modelling baryonic feedback for survey cosmology

Nora Elisa Chisari, Alexander J. Mead, Shahab Joudaki +10

Observational cosmology in the next decade will rely on probes of the distribution of matter in the redshift range between to elucidate the nature of dark matter and dark e…

astro-ph.CO2019★ 169 cited

KiDS+VIKING-450 and DES-Y1 combined: Cosmology with cosmic shear

S. Joudaki, H. Hildebrandt, D. Traykova +12

We present a combined tomographic weak gravitational lensing analysis of the Kilo Degree Survey (KV450) and the Dark Energy Survey (DES-Y1). We homogenize the analysis of these two…

astro-ph.CO2019★ 102 cited

Implications of a transition in the dark energy equation of state for the and tensions

Ryan E. Keeley, Shahab Joudaki, Manoj Kaplinghat +1

We explore the implications of a rapid appearance of dark energy between the redshifts () of one and two on the expansion rate and growth of perturbations. Using both Gaussian p…