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Fig. 1.

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Example of the data products used for each galaxy in the VERTICO survey. Left: SFR surface density measured for NGC 4501 using GALEX NUV and WISE3 photometry. Right: Molecular gas surface density map derived from the VERTICO CO (2–1) data products. Molecular gas surface brightness contours at 3, 5, 10, 20 and 40-σ detection are overlaid on both panels. The illustrated beam in the lower left corner of each panel is 9″ in diameter and represents the working angular resolution. This beam corresponds to 720 pc at the distance of Virgo (16.5 Mpc). The complete figure set for the VERTICO subsample used in this paper is available online.

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