  We present the detection of 9 new planet candidates orbiting M dwarfs,
identified using an independent search and vetting pipeline applied to TESS
Full-Frame Image (FFI) data from Sectors 1 to 63. Our candidates include
planets as small as 1.4 $R_{\oplus}$, with orbital periods up to 20 days. Among
the 9 new candidates, we identified 5 gas giants, which represent a rare and
unexpected outcome of planet formation. Our findings add to the growing sample
of giant planets around M dwarfs found by TESS. We discuss their follow-up
potential for mass measurements through radial velocity observations and
atmospheric characterization through transmission spectroscopy. We highlight
TIC 12999193.01 as a particularly unique gas giant candidate in an eccentric
orbit and excellent potential for atmospheric characterisation.
