The Chandra Local Volume Survey: The X-ray Point Source Catalog of NGC 300
Breanna Binder, Benjamin F. Williams, Michael Eracleous, Terrance J., Gaetz, Paul P. Plucinsky, Evan D. Skillman, Julianne J. Dalcanton, Scott F., Anderson, Daniel R. Weisz, Albert K. H. Kong

TL;DR
This paper catalogs X-ray point sources in NGC 300 using Chandra data, analyzes their properties, and classifies their likely origins, providing insights into the galaxy's stellar populations and X-ray source characteristics.
Contribution
It presents a new X-ray source catalog for NGC 300, introduces a novel classification scheme, and compares XLFs across different stellar populations.
Findings
95 X-ray sources detected with high significance
XLF slopes differ between young and old stellar populations
X-ray source population aligns with properties of late-type galaxies
Abstract
We present the source catalog of a new Chandra ACIS-I observation of NGC 300 obtained as part of the Chandra Local Volume Survey. Our 63 ks exposure covers ~88% of the D25 isophote (R~6.3 kpc) and yields a catalog of 95 X-ray point sources detected at high significance to a limiting unabsorbed 0.35-8 keV luminosity of ~10^36 erg s^-1. Sources were cross-correlated with a previous XMM-Newton catalog, and we find 75 "X-ray transient candidate" sources that were detected by one observatory, but not the other. We derive an X-ray scale length of 1.7+/-0.2 kpc and a recent star formation rate of 0.12 Msun yr^-1, in excellent agreement with optical observations. Deep, multi-color imaging from the Hubble Space Telescope, covering ~32% of our Chandra field, was used to search for optical counterparts to the X-ray sources, and we have developed a new source classification scheme to determine…
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