Improving Photometric Redshifts by Merging Probability Density Functions from Template-Based and Machine Learning Algorithms*
Year: 2022
Type: article
Abstract: This study aims to improve the photometric redshifts (photo-zs) of galaxies by integrating two contemporary methods: template-fitting and machine learning. Finding the synergy between these two methods was not a high priority in the past, but now that our computer processing power and observational accuracy have increased, we deem it worth investigating. We compared two methods to improve galaxy photometric redshift estimations by using the algorithms ANNz2 and BPz on different photometric and spectroscopic samples from the Sloan Digital Sky Survey (SDSS). We find that the photometric redshift performance of ANNz2 (machine learning) is better than that of BPz (galactic templates), and with the utilization of the merging technique we introduced, we see that there is an improvement in photo-z when the two strategies are consolidated, providing improvements in $${\sigma}_{\mathrm{RMS}}$$ and $${\sigma}_{68}$$ up to [0] in LRG sample and [0] in the Stripe-82 sample. This simple demonstration can be used for photo-zs of galaxies in fainter and deeper sky surveys, and future work is required to prove its viability in these samples.
Source: Astronomy Letters
Institution: Universiti Sains Malaysia
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
Funders: National Science Foundation, U.S. Department of Energy, National Aeronautics and Space Administration, Alfred P. Sloan Foundation, Princeton University, Ohio State University, University of Washington, Johns Hopkins University, University of Pittsburgh, Case Western Reserve University, Drexel University, Universität Basel, University of Portsmouth, New Mexico State University, Chinese Academy of Sciences, Max-Planck-Gesellschaft, Universiti Sains Malaysia, Max-Planck-Institut für Astronomie, U.S. Naval Observatory, Fermilab, Los Alamos National Laboratory
Award: G1950212031
OpenAlex ID: W4328029211
