The Population of Type 1 Active Galactic Nuclei in Dark Energy Spectroscopic Instrument. I. Profile-dependent Measurements of the Low-redshift Sample
astro-ph.GA
Submitted: 2026-10-09
Updated: 2026-10-09
Comments: 24 pages, 14 figures; Accepted for publication in ApJS
Code: https://github.com/PuDu-Astro/DASpec
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Sources
- QuasarNET: Human-level spectral classification and redshifting with Deep Neural Networks
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- Data Release 1 of the Dark Energy Spectroscopic Instrument
- The Narrow-Line Seyfert 1 Phenomenon: Accretion State Versus Host Galaxy Properties
- Narrow-Line Seyfert 1 Galaxies
- PyTorch: An Imperative Style, High-Performance Deep Learning Library
- Scikit-learn: Machine Learning in Python
- The Mass of Quasars
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