activity
20242026
collaborators

7 papers

astro-ph.CO2026

The PAU Survey and Euclid: Analysing photometric redshifts from realistically simulated narrow-band photometry with Flagship 2

A. Wittje, H. Hildebrandt, D. Navarro-Gironés +154

The study of the large-scale structure of the Universe and the distribution of galaxies has been greatly advanced by the application of various types of photometric redshift estima…

astro-ph.IM2026

Redshift Assessment Infrastructure Layers (RAIL): Rubin-era photometric redshift stress-testing and at-scale production

The RAIL Team, Jan Luca van den Busch, Eric Charles +30

Virtually all extragalactic use cases of the Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST) require the use of galaxy redshift information, yet the vast majorit…

astro-ph.CO2025

KiDS-Legacy: Redshift distributions and their calibration

Angus H. Wright, Hendrik Hildebrandt, Jan Luca van den Busch +30

We present the redshift calibration methodology and bias estimates for the cosmic shear analysis of the fifth and final data release (DR5) of the Kilo-Degree Survey (KiDS). KiDS-DR…

astro-ph.CO2025

KiDS-1000 cosmic shear reanalysis using MetaCalibration

Mijin Yoon, Henk Hoekstra, Shun-Sheng Li +10

A number of cosmic shear studies have reported results that are in mild tension with the Planck cosmic microwave measurement. To explore if this can be caused by biases in the shea…

astro-ph.CO2025

KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables

Robert Reischke, Sandra Unruh, Marika Asgari +24

We introduce OneCovariance, an open-source software designed to accurately compute covariance matrices for an arbitrary set of two-point summary statistics across a variety of larg…

astro-ph.GA2024

Enhancing Photometric Redshift Catalogs Through Color-Space Analysis: Application to KiDS-Bright Galaxies

Priyanka Jalan, Maciej Bilicki, Wojciech A. Hellwing +11

We present a method to refine photometric redshift galaxy catalogs by comparing their color-space matching with overlapping spectroscopic calibration data. We focus on cases where…