Project Details
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Analysis of new WHT, VLT, and SOAR observations: Confirming new galaxy clusters from Planck & Calibrating the masses of high-redshift SPT clusters via weak gravitational lensing for cosmological investigations

Subject Area Astrophysics and Astronomy
Term from 2019 to 2023
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 415537506
 
Final Report Year 2024

Final Report Abstract

The project had the overall scientic objective to improve cosmological measurements with the help of galaxy cluster samples, primarily by analysing data sets that improve the calibration of cluster mass proxies using weak gravitational lensing. As one component of the project ground-based observations including deep VLT imaging were analysed to achieve an improved selection of background galaxies for the weak gravitational lensing analysis of distant galaxy clusters from the South Pole Telescope. Within the project we also contributed to an analysis of simulated data with the goal to reduce systematic uncertainties related to weak lensing mass modelling. Important ndings of this work include constraints on the dependence of mass modelling biases on assumptions regarding cluster concentrations, a demonstration how mass modelling biases can be quantied and corrected for independent of the level of shape noise, constraints on the actual distribution of mass modelling biases, and a demonstration that the standard assumption of isotropic miscentring in weak lensing shear proles can lead to a systematic overestimation of cluster masses. By participating in the analysis of weak lensing data from the VST Kilo Degree Survey we additionally contributed to the weak lensing mass calibration of the eROSITA survey. The achieved weak lensing constraints have been included in the latest cosmological analyses of the South Pole Telescope and eROSITA galaxy cluster samples under the lead of our collaboration partners, yielding improved constraints on the cosmological model.

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