this multidisciplinary work provides an updated assessment of possible future eruptive scenarios for the city of Rome. Seven new 40 Ar/ 39 Ar ages from selected products of the Monti Sabatini and Vulsini volcanic districts, along with a compilation of all the literature ages on the colli Albani and Vico products, are used to reconstruct and compare the eruptive histories of the Monti Sabatini and colli Albani over the last 900 ka, in order to define their present state of activity. Petrographic analyses of the dated units characterize the crystal cargo, and Advanced-inSAR analysis highlights active deformation in the MS. We also review the historical and instrumental seismicity affecting this region. Based on the chronology of the most recent phases and the time elapsed between the last eruptions, we conclude that the waning/extinguishment of eruptive activity shifted progressively from nW to Se, from northern Latium toward the neapolitan area, crossing the city of Rome. Although Monti Sabatini is unaffected by the unrest indicators presently occurring at the Colli Albani, it should be regarded as a dormant volcanic district, as the time of 70 kyr elapsed since the last eruption is of the same order of the longest dormancies occurred in the past. The city of Rome was founded upon tuffaceous hills that are part of a thick pyroclastic plateau formed by the eruptions of two large volcanic districts: Monti Sabatini (MS) to the NW and Colli Albani (CA) to the SE (Fig. 1). A number of recent studies has ascertained the state of quiescence of the CA, given an average dormancy of 38.5 ± 1.5 kyr during the last 600 ka, and the occurrence of the most recent eruption at 36 ± 1 ka 1 (and references therein). Moreover, a 20 year-long InSAR data record revealed ongoing inflation with maximum uplift rates >2 mm/yr in the area hosting the most recent (<200 ka) eruptive vents, suggesting that magma recharge is possibly occurring at depth 2 (and references therein). In contrast, no similar studies have been undertaken in the MS so far, precluding a reliable assessment of its actual state. However, a recent geomorphologic study on the fluvial terraces of the Tiber Valley found evidence of ca. 50 m of differential uplift occurred along the MS eastern sector in the last 125 kyr, concurrent with the most recent phase of eruptive activity from multiple vents 1 (Fig. 1). For this reason, a dedicated research project has been conducted to refine the MS eruptive history through a set of new 40 Ar/ 39 Ar age determinations, and to assess possible active soil deformation, including seismotectonic processes and vertical movements, through InSAR analysis. The analysis of the regional seismicity, comparing instrumental and historical records for the four volcanic districts of Latium, is provided aiming at highlighting possible unrest indicators, as recently shown for the CA 2. Geologic setting The MS belongs to the highly potassic Roman Magmatic Province 3 , which originated in the area comprised between the Apennine orogen and the Tyrrhenian ...