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Fig. C.1.

image

Diversity of CO SLEDs for main-sequence and starburst galaxies. Blue filled circles and open squares indicate the main-sequence and starburst galaxies with detected CO (5 − 4) and CO (2 − 1) lines from our ALMA follow-up, normalized to the mean CO (2 − 1) flux for the main-sequence sample. The open red circles and squares indicate the mean fluxes for main-sequence, starburst (ΔMS ≥ 3.5), and extreme starburst (ΔMS ≥ 7) objects. The solid line shows the line ratios for a fully thermalized case. The gray shaded area marks the model by Narayanan & Krumholz (2014) for unresolved observations within ΣSFR = 1−10 M yr−1 kpc−2. The long dashed line indicates the simulations from Bournaud et al. (2015). The dotted line traces the empirical model by Papadopoulos et al. (2012). The dashed-dotted line points at the analytical model by Vollmer et al. (2017).

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