Virgo Filaments VIII: Characterizing the Structural Parameters of Virgo Galaxies with Machine Learning to Probe Environmental Quenching

arXiv:2609.01739 · astro-ph.GA, astro-ph.IM · Submitted 2026-09-01 · Read on arXiv

astro-ph.GA, astro-ph.IM

Submitted: 2026-09-01

Updated: 2026-09-01

Terminology

• Clustering — 28× in this paper · explained in 2 episodes
• AGN — 10× in this paper · explained in 1 episode
• Environmental Quenching — 5× in this paper · explained in 2 episodes
• Abundance — 4× in this paper · explained in 1 episode
• Robustness — 4× in this paper · explained in 5 episodes
• Trace — 4× in this paper · explained in 2 episodes
• Consistency — 3× in this paper · explained in 3 episodes
• Adjusted Rand Index — 2× in this paper
• Aperture — 2× in this paper · explained in 1 episode
• Dark Energy Survey — 2× in this paper
• Failure Modes — 2× in this paper · explained in 3 episodes
• AGN Feedback — 1× in this paper · explained in 1 episode
• Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
• Aperture Photometry — 1× in this paper · explained in 1 episode
• Beijing-Arizona Sky Survey — 1× in this paper
• Cooperation — 1× in this paper · explained in 2 episodes
• Decoupling — 1× in this paper · explained in 2 episodes
• Dust Attenuation — 1× in this paper · explained in 2 episodes
• Feature Selection — 1× in this paper · explained in 4 episodes
• Initial Mass Function (IMF) — 1× in this paper · explained in 2 episodes
• Metallicity — 1× in this paper · explained in 3 episodes
• NOIRLab and the Lawrence Berkeley National Laboratory — 1× in this paper
• Near-Earth Object Wide-field Infrared Survey Explorer — 1× in this paper
• Velocity Dispersion — 1× in this paper · explained in 2 episodes
• alpha — 1× in this paper · explained in 1 episode

Sources

• Data Release 1 of the Dark Energy Spectroscopic Instrument
• What is the True HI Gas Content in Massive Quiescent Galaxies in the Local Universe?
• Machine Learning-Based Classification of Active Galaxies and Estimation of Supermassive Black Hole Masses
• Galaxy Morphological Classification with Efficient Vision Transformer

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