  The transit method is biased toward short orbital period planets that are
interior to their host star's Habitable Zone (HZ). These planets are
particularly interesting from the perspective of exploring runaway greenhouse
scenarios and the possibility of potential Venus analogs. Here, we conduct an
analysis of predicted TESS planet yield estimates produced by Huang et al.
(2018), as well as the TESS Object of Interest (TOI) list resulting from the
observations of sectors 1 - 13 during Cycle 1 of the TESS primary mission. In
our analysis we consider potential terrestrial planets that lie within their
host star's Venus Zone (Kane et al. 2014). These requirements are then applied
to a predicted planetary yield from the TESS primary mission (Huang et al.
2018) and the TOI list, which results in an estimated 259 Venus analogs by the
end of the TESS primary mission, and 46 Venus analogs in the TOI list for
sectors 1 - 13. We also calculate the estimated transmission spectroscopy
signal-to-noise ratio (S/N) for Venus analogs from the predicted yield and TOI
list if they were to be observed by the Near-Infrared Imager and Slitless
Spectrograph (NIRISS) on the James Webb Space Telescope (JWST), as well as
update the S/N cutoff values determined by Kempton et al. (2018). Our findings
show that the best estimated Venus analogs and TOI Venus analogs with $R_{p} <
1.5 \, R_\odot$ have an estimated transmission spectroscopy S/N $> 40$ while
planets with radii $2 \, R_\oplus < R_p < 4 \, R_\oplus$ can achieve S/N $>
100$
