Photometric Redshift Estimation with Hybrid Quantum Neural Network

A Hybrid Quantum Neural Network (HQNN) is applied to recover the photometric redshift of a galaxy dataset built using data from two astronomical surveys, the Kilo-Degree Survey (KIDS) and the VISTA Kilo-Degree Infrared Galaxy (VIKING), which provide data with coverage from the optical to the near-infrared electromagnetic spectrum. The results are then compared with those obtained by a classical neural network. We see that HQNN consistently recovers the reference photometric redshift with a high statistical fidelity. Furthermore, both the $R^2$ and the MSE found by the HQNN are consistently better than those found by the classical counterpart (albeit consistent in the error range), proving the worth of further investigating these novel technologies for this particular astrophysical application.

Authors

Publication Details

Journal
arXiv (Cornell University)
Published
2026-10-26
DOI
https://doi.org/10.48550/arxiv.2610.35196
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
preprint
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
preprint

Photometric Redshift Estimation with Hybrid Quantum Neural Network

V. F. Cardone, Farida Farsian, R. Scaramella, Giuseppe Sarracino et al.
arXiv (Cornell University)
Galaxies: Formation, Evolution, Phenomena
preprint

Photometric Redshift Estimation with Hybrid Quantum Neural Network

V. F. Cardone, Farida Farsian, R. Scaramella, Giuseppe Sarracino, C. Burigana, Fabio Roberto Vitello, C. Tortora, Francesco Schillirò, V. Testa, Giuseppe Murante, Andrea A. Bulgarelli, T. Trombetti, Irene Graziotti, Alessandro Rizzo, Niccolò Parmiggiani, Massimo Meneghetti
preprint en

Abstract

A Hybrid Quantum Neural Network (HQNN) is applied to recover the photometric redshift of a galaxy dataset built using data from two astronomical surveys, the Kilo-Degree Survey (KIDS) and the VISTA Kilo-Degree Infrared Galaxy (VIKING), which provide data with coverage from the optical to the near-infrared electromagnetic spectrum. The results are then compared with those obtained by a classical neural network. We see that HQNN consistently recovers the reference photometric redshift with a high statistical fidelity. Furthermore, both the $R^2$ and the MSE found by the HQNN are consistently better than those found by the classical counterpart (albeit consistent in the error range), proving the worth of further investigating these novel technologies for this particular astrophysical application.

arXiv (Cornell University)
Galaxies: Formation, Evolution, Phenomena
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

Laika access coming soon
Photometric Redshift Estimation with Hybrid Quantum Neural Network — V. F. Cardone, Farida Farsian, et al. · arXiv (Cornell University) (2026) | TGRS Research Map | TGRS