  The evolutionary status of 24 post-AGB stars is presented based on Gaia DR3
data. All 24 stars have parallaxes accurate to better than 3 X sigma and have
RUWE values less than 1.4. Based on the Gaia DR3 distances the absolute
luminosities are derived. For 14 of the stars, the luminosities confirm their
post-AGB evolutionary stage. However, V1027 Cyg, which was previously
classified as a post-AGB star, is found to have a higher luminosity; thus it
may be an evolved, massive, pulsating semi-regular variable star of type G7Ia.
For 9 of the stars, the luminosities are lower than 1000 L (sun), indicating
that some are post-RGB stars and some are post-HB stars.This paper was
completed more than four months ago but there was delay in getting it
published.
