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ANNZ+: an enhanced photometric redshift estimation algorithm with applications on the PAU survey

Pathi, Imdad Mahmud; Soo, John Y.H.; Wee, Mao Jie; Zakaria, Sazatul Nadhilah; Ismail, Nur Azwin; Baugh, Carlton M.; Manzoni, Giorgio; Gaztanaga, Enrique; Castander, Francisco J.; Eriksen, Martin; Carretero, Jorge; Fernandez, Enrique; Garcia-Bellido, Juan; Miquel, Ramon; Padilla, Cristobal; Renard, Pablo; Sanchez, Eusebio; Sevilla-Noarbe, Ignacio; Tallada-Crespí, Pau

Authors

Imdad Mahmud Pathi

John Y.H. Soo

Mao Jie Wee

Sazatul Nadhilah Zakaria

Nur Azwin Ismail

Giorgio Manzoni

Enrique Gaztanaga

Francisco J. Castander

Martin Eriksen

Jorge Carretero

Enrique Fernandez

Juan Garcia-Bellido

Ramon Miquel

Cristobal Padilla

Pablo Renard

Eusebio Sanchez

Ignacio Sevilla-Noarbe

Pau Tallada-Crespí



Abstract

annz is a fast and simple algorithm which utilises artificial neural networks (ANNs), it was known as one of the pioneers of machine learning approaches to photometric redshift estimation decades ago. We enhanced the algorithm by introducing new activation functions like tanh, softplus, SiLU, Mish and ReLU variants; its new performance is then vigorously tested on legacy samples like the Luminous Red Galaxy (LRG) and Stripe-82 samples from SDSS, as well as modern galaxy samples like the Physics of the Accelerating Universe Survey (PAUS). This work focuses on testing the robustness of activation functions with respect to the choice of ANN architectures, particularly on its depth and width, in the context of galaxy photometric redshift estimation. Our upgraded algorithm, which we named annz+, shows that the tanh and Leaky ReLU activation functions provide more consistent and stable results across deeper and wider architectures with > 1 per cent improvement in root-mean-square error (σ RMS) and 68th percentile error (σ 68) when tested on SDSS data sets. While assessing its capabilities in handling high dimensional inputs, we achieved an improvement of 11 per cent in σ RMS and 6 per cent in σ 68 with the tanh activation function when tested on the 40-narrowband PAUS dataset; it even outperformed annz2, its supposed successor, by 44 per cent in σ RMS. This justifies the effort to upgrade the 20-year-old annz, allowing it to remain viable and competitive within the photo-z community today. The updated algorithm annz+ is publicly available at https://github.com/imdadmpt/ANNzPlus.

Citation

Pathi, I. M., Soo, J. Y., Wee, M. J., Zakaria, S. N., Ismail, N. A., Baugh, C. M., Manzoni, G., Gaztanaga, E., Castander, F. J., Eriksen, M., Carretero, J., Fernandez, E., Garcia-Bellido, J., Miquel, R., Padilla, C., Renard, P., Sanchez, E., Sevilla-Noarbe, I., & Tallada-Crespí, P. (2025). ANNZ+: an enhanced photometric redshift estimation algorithm with applications on the PAU survey. Journal of Cosmology and Astroparticle Physics, 2025(1), Article 097. https://doi.org/10.1088/1475-7516/2025/01/097

Journal Article Type Article
Acceptance Date Dec 19, 2024
Online Publication Date Jan 22, 2025
Publication Date Jan 22, 2025
Deposit Date May 5, 2025
Journal Journal of Cosmology and Astroparticle Physics
Electronic ISSN 1475-7516
Publisher IOP Publishing
Peer Reviewed Peer Reviewed
Volume 2025
Issue 1
Article Number 097
DOI https://doi.org/10.1088/1475-7516/2025/01/097
Public URL https://durham-repository.worktribe.com/output/3931972
Other Repo URL https://arxiv.org/abs/2409.09981