Peering down the barrel with DESI DR2: 10 000+ inflows at $z$ < 0.6 reveal how galaxies accrete cold gas
S. Weng, A. Saintonge, Matthew M. Pieri, J. Moustakas, H. Zou, D. Mu\~noz Santos, J. Yu, J. Aguilar, S. Ahlen, D. Bianchi, D. Brooks, T. Claybaugh, A. Cuceu, A. de la Macorra, P. Doel, A. Font-Ribera, J. E. Forero-Romero, E. Gazta\~naga, Satya Gontcho A. Gontcho, G. Gutierrez

TL;DR
This study analyzes over 50,000 galaxies at redshift less than 0.6 using DESI DR2 data to observe how galaxies acquire cold gas, revealing multiple accretion pathways including radial inflows and satellite accretion.
Contribution
First large-scale observational evidence of diverse gas accretion pathways in galaxies at low redshift, using Bayesian analysis of NaI D absorption.
Findings
Approximately 50% of absorbers show inflow velocities less than -50 km/s.
Detected low-velocity inflows (~20 km/s) in edge-on galaxies.
Correlation between inflow velocity and stellar velocity dispersion suggests satellite accretion involvement.
Abstract
Direct observational constraints on how galaxies acquire their gas remain remarkably limited, hindering our understanding of the baryon cycle. We present a search for down-the-barrel NaI D absorption towards 15.6 million galaxies at in DESI Data Release 2. We use Bayesian evidence ratios to assess whether the absorption requires additional components tracing interstellar gas distinct from the systemic component of the galaxy. We construct a catalogue of 50 088 (27 420) galaxies with moderate (strong) evidence for down-the-barrel absorption. The inferred absorption components are broadly distributed in velocity, with approximately 50% at km/s, 30% within 50 km/s of the systemic velocity and the remaining 20% at km/s. We find strong evidence for a large population of low-velocity, infalling absorbers with velocities 20 km/s in…
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