The final data release of ALLSMOG: a survey of CO in typical local low-M∗ star-forming galaxies

C. Cicone; M. Bothwell; J. Wagg; P. Møller; C. De Breuck; Z. Zhang; S. Martín; R. Maiolino; P. Severgnini; M. Aravena; F. Belfiore; D. Espada; A. Flütsch; V. Impellizzeri; Y. Peng; M. A. Raj; N. Ramírez-Olivencia; D. Riechers; K. Schawinski

doi:10.1051/0004-6361/201730605

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Volume 604 (August 2017)

A&A, 604 (2017) A53

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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
A_V [mag] (CCM89)	0.51	4.1E-6
A_V [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
	0.30	0.034

Notes.

^(†)

Value of the K-S statistic.

^(‡)

The associated probability of the null hypothesis, that is the hypothesis according to which the two samples of detections and non-detections come from the same distribution. We reject the null hypothesis if the p-values <0.05.

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