  We present 370 candidate eclipsing binaries (EBs), identified from ~510,000
short cadence TESS light curves. Our statistical criteria identify 5,105 light
curves with features consistent with eclipses (~1% of the initial sample).
After visual confirmation of the light curves, we have a final sample of 2,288
EB candidates. Among these, we find 370 sources that were not included in the
catalog recently published by Prsa et al. We publish our full sample of 370 new
EB candidates, and statistical features used for their identification, reported
per observation sector.
