Results of the two-sample Kolmogorov–Smirnov test performed on the distribution of detections and non-detections as a function of the galaxy physical parameters explored in this work.
|log M∗ [M⊙]||0.60||1.75E-8|
|log SFR [M⊙ yr-1]||0.56||1.82E-7|
|log SSFR [yr-1]||0.21||0.19|
|AV [mag] (CCM89)||0.51||4.1E-6|
|AV [mag] (Calzetti)||0.51||4.1E-6|
|12 + log (O/H) (Tremonti+04)||0.70||1.9E-11|
|12 + log (O/H) N2 PP04||0.67||2.2E-10|
|12 + log (O/H) N2 M13||0.67||2.2E-10|
|12 + log (O/H) O3N2 PP04||0.67||2.5E-10|
|12 + log (O/H) O3N2 M13||0.67||2.5E-10|
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