Fig. A.2.
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RMS sensitivities (σ) of the CO(3 − 2) maps converted into molecular mass surface densities (in M⊙ pc−2) as a function of luminosity distance (in Mpc). For each galaxy we show two values, connected by a vertical bar: green squares correspond to the case r31 = 0.7 (average value in galaxy centers, Israel 2020) combined with the standard Milky Way disk conversion factor XCO = 2 × 1020 mol cm−2 (K km s−1)−1 (Bolatto et al. 2013); blue stars correspond to the case r31 = 2.9 (measured at the AGN position in NGC 1068, Viti et al. 2014) combined with the recommended conversion factor for the nuclear region of the Milky Way XCO = 0.5 × 1020 mol cm−2 (K km s−1)−1 (Bolatto et al. 2013).
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