  In the search for life in the cosmos, NASA's Transiting Exoplanet Survey
Satellite (TESS) mission has already monitored about 74% of the sky for
transiting extrasolar planets, including potentially habitable worlds. However,
TESS only observed a fraction of the stars long enough to be able to find
planets like Earth. We use the primary mission data - the first two years of
observations - and identify 4,239 stars within 210pc that TESS observed long
enough to see 3 transits of an exoplanet that receives similar irradiation to
Earth: 738 of these stars are located within 30pc. We provide reliable stellar
parameters from the TESS Input Catalog that incorporates Gaia DR2 and also
calculate the transit depth and radial velocity semi-amplitude for an
Earth-analog planet. Of the 4,239 stars in the Revised TESS HZ Catalog, 9 are
known exoplanet hosts - GJ 1061, GJ 1132, GJ 3512, GJ 685, Kepler-42, LHS 1815,
L98-59, RR Cae, TOI 700 - around which TESS could identify additional
Earth-like planetary companions. 37 additional stars host yet unconfirmed TESS
Objects of Interest: three of these orbit in the habitable zone - TOI 203, TOI
715, and TOI 2298. For a subset of 614 of the 4,239 stars, TESS has observed
the star long enough to be able to observe planets throughout the full
temperate, habitable zone out to the equivalent of Mars' orbit. Thus, the
Revised TESS Habitable Zone Catalog provides a tool for observers to prioritize
stars for follow-up observation to discover life in the cosmos. These stars are
the best path towards the discovery of habitable planets using the TESS mission
data.
