CGM CASBaH: The Mass Dependence of H~I Ly-Galaxy Clustering and the Extent of the CGM
arXiv:2301.02718 · doi:10.3847/1538-4357/acc85b
Abstract
We combine datasets from the CGM and CASBaH surveys to model a transition point, , between circumgalactic and intergalactic media (CGM and IGM, respectively). In total, our data consist of 7244 galaxies at z < 0.5 with precisely measured spectroscopic redshifts, all having impact parameters of 0.01 - 20 comoving Mpc from 28 QSO sightlines with high-resolution UV spectra that cover H I Ly. Our best-fitting model is an exclusionary two-component model that combines a 3D absorber-galaxy cross correlation function with a simple Gaussian profile at inner radii to represent the CGM. By design, this model gives rise to a determination of as a function of galaxy stellar mass, which can be interpreted as the boundary between the CGM and IGM. For galaxies with , we find that . Additionally, we find excellent agreement between and the theoretically-determined splashback radius for galaxies in this mass range. Overall, our results favor models of galaxy evolution at z < 0.5 that distribute K gas to distances beyond the virial radius.
arXiv commentSubmitted to ApJ, 17 pages, 8 figures
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