  The recently proposed Swampland Criteria aim to evade any (meta-)stable de
Sitter constructions within String landscapes, making it difficult to
accommodate accelerating phases, like dark energy domination and inflationary
epoch, in cosmology. In this note, we analyse the status of various models of
single field slow-roll inflation given the old as well as the refined Swampland
conjectures, which constrain the form of scalar potentials in any low energy
effective field theory residing in the landscapes. In particular, we note that
Warm Inflation turns out to be the most befitting scenario as long as lifting
the tensions with Swampland Criteria are concerned.
