Imdad Mahmud Pathi
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
John Y.H. Soo
Mao Jie Wee
Sazatul Nadhilah Zakaria
Nur Azwin Ismail
Professor Carlton Baugh c.m.baugh@durham.ac.uk
Professor
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 |
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