The Atacama Cosmology Telescope: CO(J = 3 - 2) mapping and lens modeling of an ACT-selected dusty star-forming galaxy
J. Rivera, A. J. Baker, P. A. Gallardo, M. Gralla, A. I. Harris, K. M., Huffenberger, J. P. Hughes, C. R. Keeton, C. H. Lopez-Caraballo, T. A., Marriage, B. Partridge, J. Sievers, A. S. Tagore, F. Walter, A. Weiss, E. J., Wollack

TL;DR
This study uses NOEMA observations to map a dusty star-forming galaxy at z=2.55, revealing its lensing properties, gas content, and possible disk-like structure, advancing understanding of high-redshift galaxy dynamics.
Contribution
It provides the first spatially resolved CO(3-2) mapping and lens modeling of an ACT-selected dusty galaxy, estimating its gas mass, lensing magnification, and dynamical state.
Findings
Lensing magnification factor $ imes$7-22, mean $ imes$13.
Derived cold gas mass of approximately 3.86 x 10^{10} M_sun.
Galaxy possibly exhibits a rotating disk structure.
Abstract
We report Northern Extended Millimeter Array (NOEMA) CO() observations of the dusty star-forming galaxy ACT-S\,J020941+001557 at , which was detected as an unresolved source in the Atacama Cosmology Telescope (ACT) equatorial survey. Our spatially resolved spectral line data support the derivation of a gravitational lens model from 37 independent velocity channel maps using a pixel-based algorithm, from which we infer a velocity-dependent magnification factor with a luminosity-weighted mean . The resulting source-plane reconstruction is consistent with a rotating disk, although other scenarios cannot be ruled out by our data. After correction for lensing, we derive a line luminosity , a cold gas mass $M_{{\rm gas}}= (3.86 \pm 0.33)…
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