Published March 12, 2025
| Version v1
Software
Open
Neural networks for quasar and galaxy continuum fitting
Description
The trained models are divided into quasars (qso) and galaxies (gal). For the qso's models, they are also divided if they are trained only on the red part of the spectrum (red, λ > 1216 Å) or the full spectrum (full, λ > 1020 Å) The highest wavelength is λ = 2000 Å for the autoencoders and λ = 2020 Å for the U-Net and CNNs.
Files
Files
(740.7 MB)
| Name | Size | Download all |
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md5:982c7827bcf18f739ec4130dcaf8a46a
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66.9 MB | Download |
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md5:7b43a27bec61223eedcb358d52caa2c9
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95.9 MB | Download |
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md5:9330af3f84b5ab7484487465b84e3d70
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31.3 MB | Download |
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md5:5c20fe0aba9e2315cdd26d9fcc5451d4
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92.8 MB | Download |
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md5:b93ebdd266f17a9f691cdc39b5f91300
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86.8 MB | Download |
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md5:8f6dc4c9e1f9b1ebc86e034bd76b2e9d
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160.9 MB | Download |
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md5:ffdbee033efd8d98825949fe2d37ab81
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198.9 MB | Download |
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md5:7bd7be46e2a1aa4d5a5fae8bdbbf8561
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7.2 MB | Download |
Additional details
Identifiers
- arXiv
- arXiv:2505.10976
- DOI
- 10.1051/0004-6361/202453377
Dates
- Submitted
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2024-12-10Astronomy & Astrophysics
- Accepted
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2025-05-16Astronomy & Astrophysics