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We present comprehensive X-ray point source catalogs of NGC~55, NGC~2403, andNGC~4214 as part of the Chandra Local Volume Survey. The combined archivalobservations have effective exposure times of 56.5 ks, 190 ks, and 79 ks forNGC~55, NGC~2403, and NGC~4214, respectively. When combined with our publishedcatalogs for NGC 300 and NGC 404, our survey contains 629 X-ray sources totaldown to a limiting unabsorbed luminosity of $\sim5\times10^{35}$ erg s$^{-1}$in the 0.35-8 keV band in each of the five galaxies. We present X-ray hardnessratios, spectral analysis, radial source distributions, and an analysis of thetemporal variability for the X-ray sources detected at high significance. Toconstrain the nature of each X-ray source, we carried out cross-correlationswith multi-wavelength data sets. We searched overlapping Hubble Space Telescopeobservations for optical counterparts to our X-ray detections to providepreliminary classifications for each X-ray source as a likely X-ray binary,background AGN, supernova remnant, or foreground star.

The Chandra Local Volume Survey I: The X-ray Point Source Populations of NGC 55, NGC 2403, and NGC 4214