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Table 1
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.
D † | p-value‡ | |
|
||
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 |
Redshift | 0.22 | 0.16 |
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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0.30 | 0.034 |
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