Statistical analysis of probability density functions for photometric redshifts through the KiDS-ESO-DR3 galaxies
Valeria Amaro, Stefano Cavuoti, Massimo Brescia, Civita Vellucci,, Giuseppe Longo, Maciej Bilicki, Jelte T. A. de Jong, Crescenzo Tortora, Mario, Radovich, Nicola R. Napolitano, Hugo Buddelmeijer

TL;DR
This paper compares different methods for estimating probability density functions of photometric redshifts in galaxy surveys, highlighting the importance of multiple statistical estimators for assessing PDF reliability.
Contribution
It introduces a comprehensive comparison of three PDF estimation methods on KiDS-ESO-DR3 data, emphasizing the need for combined statistical estimators for validation.
Findings
Different PDF methods show varying reliability in redshift estimation.
A combined set of statistical estimators effectively assesses PDF quality.
Spectroscopic data from GAMA enhances the evaluation of photometric redshift PDFs.
Abstract
Despite the high accuracy of photometric redshifts (zphot) derived using Machine Learning (ML) methods, the quantification of errors through reliable and accurate Probability Density Functions (PDFs) is still an open problem. First, because it is difficult to accurately assess the contribution from different sources of errors, namely internal to the method itself and from the photometric features defining the available parameter space. Second, because the problem of defining a robust statistical method, always able to quantify and qualify the PDF estimation validity, is still an open issue. We present a comparison among PDFs obtained using three different methods on the same data set: two ML techniques, METAPHOR (Machine-learning Estimation Tool for Accurate PHOtometric Redshifts) and ANNz2, plus the spectral energy distribution template fitting method, BPZ. The photometric data were…
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