Statistical Detection of Neutral Gas Outflows in z = 2.0–5.0 Quenching Galaxies with JWST
Overview
How do galaxies stop forming stars?
I use JWST data to trace neutral gas outflows and uncover their role in shutting down star formation in the early Universe.
Methods
- Constructed a quiescent galaxy sample at 2.0 < z < 5.0 from the JWST NIRSpec catalog using Hα equivalent width, separating quiescent, green-valley, and star-forming populations.
- Built matched spectroscopic–photometric datasets and performed SED fitting with Prospector to derive stellar continua and physical parameters.
- Subtracted stellar continua and performed spectral stacking of residual spectra to enhance Na I D absorption features.
- Measured equivalent widths and velocity offsets of stacked absorption lines to probe neutral-gas outflows.
Results
Results and figures to be added
Context & Motivation
Discussion of broader significance to be added