  We present the discovery of two new 10-day period giant planets from the
Transiting Exoplanet Survey Satellite ($TESS$) mission, whose masses were
precisely determined using a wide diversity of ground-based facilities. TOI-481
b and TOI-892 b have similar radii ($0.99\pm0.01$ $\rm R_{J}$ and $1.07\pm0.02$
$\rm R_{J}$, respectively), and orbital periods (10.3311 days and 10.6266 days,
respectively), but significantly different masses ($1.53\pm0.03$ $\rm M_{J}$
versus $0.95\pm0.07$ $\rm M_{J}$, respectively). Both planets orbit metal-rich
stars ([Fe/H]= $+0.26\pm 0.05$ dex and [Fe/H] = $+0.24 \pm 0.05$ dex, for
TOI-481 and TOI-892, respectively) but at different evolutionary stages.
TOI-481 is a $\rm M_{\star}$ = $1.14\pm0.02$ $\rm M_{\odot}$, $\rm R_{\star}$ =
$1.66\pm0.02$ $\rm R_{\odot}$ G-type star ($T_{\rm eff}$ = $5735 \pm 72$ K),
that with an age of 6.7 Gyr, is in the turn-off point of the main sequence.
TOI-892, on the other hand, is a F-type dwarf star ($T_{\rm eff}$ = $6261 \pm
80$ K), which has a mass of $\rm M_{\star}$ = $1.28\pm0.03$ $\rm M_{\odot}$,
and a radius of $\rm R_{\star}$ = $1.39\pm0.02$ $\rm R_{\odot}$. TOI-481 b and
TOI-892 b join the scarcely populated region of transiting gas giants with
orbital periods longer than 10 days, which is important to constrain theories
of the formation and structure of hot Jupiters.
