ProMage: fast galaxy magnitudes emulation combining SED forward-modelling and machine learning
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arXiv
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| Autori principali: | , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| _version_ | 1866911130421559296 |
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| author | Tortorelli, Luca Fischbacher, Silvan Robotham, Aaron S. G. Nussbaumer, Céline Refregier, Alexandre |
| author_facet | Tortorelli, Luca Fischbacher, Silvan Robotham, Aaron S. G. Nussbaumer, Céline Refregier, Alexandre |
| contents | We present ProMage, a feed-forward neural network that emulates the computation of observer- and rest-frame magnitudes from the generative galaxy SED package ProSpect. The network predicts magnitudes conditioned on input galaxy physical properties, including redshift, star formation history, gas and dust parameters. ProMage accelerates magnitude computation by a factor of $10^4$ compared to ProSpect, while achieving per-mille relative accuracy for $99\%$ of sources in the test set across the $g,r,i,z,y$ Hyper Suprime-Cam bands. This acceleration is key to enabling fast inference of galaxy physical properties in next-generation Stage IV surveys and to generating large catalogue realisations in forward-modelling frameworks such as GalSBI-SPS. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2509_00150 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | ProMage: fast galaxy magnitudes emulation combining SED forward-modelling and machine learning Tortorelli, Luca Fischbacher, Silvan Robotham, Aaron S. G. Nussbaumer, Céline Refregier, Alexandre Astrophysics of Galaxies Instrumentation and Methods for Astrophysics We present ProMage, a feed-forward neural network that emulates the computation of observer- and rest-frame magnitudes from the generative galaxy SED package ProSpect. The network predicts magnitudes conditioned on input galaxy physical properties, including redshift, star formation history, gas and dust parameters. ProMage accelerates magnitude computation by a factor of $10^4$ compared to ProSpect, while achieving per-mille relative accuracy for $99\%$ of sources in the test set across the $g,r,i,z,y$ Hyper Suprime-Cam bands. This acceleration is key to enabling fast inference of galaxy physical properties in next-generation Stage IV surveys and to generating large catalogue realisations in forward-modelling frameworks such as GalSBI-SPS. |
| title | ProMage: fast galaxy magnitudes emulation combining SED forward-modelling and machine learning |
| topic | Astrophysics of Galaxies Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2509.00150 |