  We developed, tested and validated a new Fast, Robust and Automated (FRA)
tool to detect solar-like oscillations. FRA is based on the detection and
measurement of the frequency of maximum oscillation power $\nu_{max}$, without
relying on the detection of a regular frequency spacing to guide the search. We
applied the FRA pipeline to 254 synthetic power spectra representative of TESS
red giants, as well as 1689 red giants observed by Kepler and 2344 red giants
observed by TESS. We obtain a consistency rate for $\nu_{max}$ compared with
existing measurements of $\sim$ 99% for Kepler red giants and of $\sim$ 98% for
TESS red giants. We find that using $\nu_{max}$ as an input parameter to guide
the search for the large frequency separation $\Delta\nu$ through the existing
Envelope AutoCorrelation Function (EACF) method significantly improves the
consistency of the measured $\Delta\nu$ in the case of TESS stars, allowing to
reach a consistency rate above 99%. Our analysis reveals that we can expect to
get consistent $\nu_{max}$ and $\Delta\nu$ measurements while minimizing both
the false positive measurements and the non-detections for stars with a minimum
of four observed sectors and a maximum G magnitude of 9.5.
