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

Home

All issues

Volume 604 (August 2017)

A&A, 604 (2017) A53

Full HTML

Press Release

Free Access

Table A.1

Analysis of the dependencies of the quantity on A_V, O/H and M_HI.

Model: y = α + βx, with

Total sample
x	α	β	σ _intr	ρ

A_V [mag]^† (CCM89)	−2.65 ± 0.15	0.09 ± 0.10	0.10 ± 0.10	0.5 ± 0.4
A_V [mag]^† (Calzetti)	−2.67 ± 0.16	0.10 ± 0.10	0.09 ± 0.10	0.5 ± 0.4
12 + log (O/H) (Tremonti+04)	−9 ± 2	0.7 ± 0.2	0.07 ± 0.10	0.88 ± 0.13
12 + log (O/H) N2 PP04	−10 ± 5	0.9 ± 0.5	0.06 ± 0.10	0.8 ± 0.3
12 + log (O/H) N2 M13	−12 ± 5	1.1 ± 0.6	0.08 ± 0.09	0.8 ± 0.2
12 + log (O/H) O3N2 PP04	−8 ± 2	0.6 ± 0.3	0.08 ± 0.09	0.8 ± 0.2
12 + log (O/H) O3N2 M13	−10 ± 3	0.9 ± 0.4	0.07 ± 0.10	0.8 ± 0.2
^‡	−5.2 ± 1.2	0.27 ± 0.12	0.09 ± 0.07	0.8 ± 0.2

Low-M_∗ sample (log M_∗ [M_⊙] < 10.0)
x	α	β	σ _intr	ρ

A_V [mag]^† (CCM89)	−2.62 ± 0.17	0.07 ± 0.11	0.10 ± 0.10	0.4 ± 0.5
A_V [mag]^† (Calzetti)	−2.66 ± 0.15	0.09 ± 0.09	0.10 ± 0.10	0.5 ± 0.4
12 + log (O/H) (Tremonti+04)	−9 ± 3	0.7 ± 0.3	0.07 ± 0.09	0.90 ± 0.11
12 + log (O/H) N2 PP04	−10 ± 4	0.8 ± 0.4	0.07 ± 0.04	0.8 ± 0.2
12 + log (O/H) N2 M13	−11 ± 5	1.0 ± 0.6	0.06 ± 0.05	0.8 ± 0.2
12 + log (O/H) O3N2 PP04	−7 ± 3	0.5 ± 0.3	0.06 ± 0.04	0.81 ± 0.19
12 + log (O/H) O3N2 M13	−11 ± 3	1.0 ± 0.4	0.07 ± 0.05	0.83 ± 0.19
^‡	−4 ± 2	0.1 ± 0.2	0.16 ± 0.10	0.3 ± 0.4

High-M_∗ sample (log M_∗ [M_⊙] ≥ 10.0)
x	α	β	σ _intr	ρ

A_V [mag]^† (CCM89)	−2.55 ± 0.19	0.03 ± 0.12	0.08 ± 0.10	0.2 ± 0.5
A_V [mag]^† (Calzetti)	−2.57 ± 0.19	0.04 ± 0.11	0.10 ± 0.06	0.2 ± 0.5
12 + log (O/H) (Tremonti+04)	−3 ± 8	0.0 ± 0.9	0.09 ± 0.10	0.0 ± 0.5
12 + log (O/H) N2 PP04	22 ± 17	−3 ± 2	0.06 ± 0.03	−0.8 ± 0.3
12 + log (O/H) N2 M13	27 ± 17	−3 ± 2	0.09 ± 0.05	−0.7 ± 0.2
12 + log (O/H) O3N2 PP04	5 ± 9	−0.9 ± 1.0	0.07 ± 0.05	−0.5 ± 0.4
12 + log (O/H) O3N2 M13	11 ± 14	−1.6 ± 1.7	0.09 ± 0.06	−0.5 ± 0.4
^‡	−6.4 ± 1.9	0.4 ± 0.2	0.10 ± 0.05	0.8 ± 0.2

Notes. (α,β) are the best-fit linear regression coefficients, σ_intr is the intrinsic scatter about the best-fit regression line, and ρ is the correlation coefficient. We refer to Sect. 7 and to Table 2 for additional details on the regression analysis method.

^(†)

Because of the large measurement errors on A_V, of the order of ~ 0.5 mag, the regression analysis for the vs. A_V relationships was performed without taking into account the errors on x, in order not to bias the results.

^(‡)

In this case the regression analysis was performed by considering only the sources with an Hi line detection.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.