  In this work, we investigate the Higgs-Starobinsky (HS) model in the context
of warm inflation scenario. The dissipative parameter as a linear form of
temperature of warm inflation is considered with strong and weak regimes. We
study the HS model in the Einstein frame with the slow-roll inflation
framework. We compute the inflationary observables and then compare with the
Plank 2018 data. With the sizeable number of e-folds and proper choices of
parameters, we discover that the predictions of warm HS model present in this
work are in very good agreement with the latest Planck 2018 results. More
importantly, the parameters of the HS model are also constrained by using the
data in order to make warm HS inflation successful.
