Free Access

Table 1

Correlation between and FWHM for various samples.

Sample N Spearman’s coeff. p-value Kendall’s coeff. p-value Dispersion (km s-1)

All 195 0.55 1.7 × 10-16 0.39 < 1.0 × 10-16 187.

Submm galaxies 72 0.53 2.1 × 10-6 0.37 4.2 × 10-6 272.
QSO hosts 31 0.53 2.0 × 10-3 0.39 1.9 × 10-3 245.
Submm galaxies +QSO hosts 103 0.52 1.4 × 10-8 0.37 < 1.0 × 10-16 218.

CO(4–3) only 26 –0.34 9.2 × 10-2 –0.21 1.4 × 10-1 279.
CO(3–2) only 62 0.12 3.5 × 10-1 0.09 2.8 × 10-1 217.
CO(2–1) only 38 0.18 2.8 × 10-1 0.14 2.2 × 10-1 182.
CO(1–0) only 43 0.22 1.5 × 10-1 0.15 1.6 × 10-1 121.

All but CO(4–3) 143 0.52 4.0 × 10-11 0.37 < 1.0 × 10-16 206.
All but CO(3–2) 107 0.56 2.5 × 10-10 0.40 < 1.0 × 10-16 201.
All but CO(2–1) 131 0.58 5.9 × 10-13 0.42 < 1.0 × 10-16 231.
All but CO(1–0) 126 0.52 4.8 × 10-10 0.37 < 1.0 × 10-16 237.

μ known 85 0.42 7.3 × 10-5 0.30 5.3 × 10-5 156.
μ unknown 110 0.47 2.4 × 10-7 0.33 3.6 × 10-7 205.

24 μm sources 8 0.45 2.6 × 10-1 0.36 2.2 × 10-1 204.
BzK galaxies 4 0.80 2.0 × 10-1 0.67 1.7 × 10-1 156.

Notes. Dispersion is around the best-fit power law. The p value of <0.05 can be considered significant.

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.