Table 5.
Rmol (log10(y)) scaling relations and correlation coefficients (ρ) for the discussed physical quantities Σgas, ΣSFR, Σ*, Z′(rgal), PDE, and ΣSFR/PDE (log10(x)) for each galaxy (see Figure 9).
log10(x) | NGC | ρ | ⟨ρ⟩ | β | α | p-value | Covariance | Scatter |
---|---|---|---|---|---|---|---|---|
or IC | correlation coeff. | slope | intercept | intrinsic | ||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | ||
1512 | 0.12 ± 0.19 | 0.16 ± 0.14 | −0.17 ± 0.11 | 0.43 | −0.01 | 0.23 | ||
4535 | 0.61 ± 6.50 × 10−10 | 0.91 ± 0.12 | −0.83 ± 0.14 | 2.89 ×10−11 | −8.60 × 10−3 | 0.08 | ||
7496 | 0.85 ± 3.60 × 10−16 | 1.80 ± 0.15 | −1.90 ± 0.16 | 2.93 ×10−19 | −0.59 | 0.09 | ||
Σgas | 1566 | 0.85 ± 1.60 × 10−38 | 0.67 | 1.50 ± 0.08 | −2.10 ± 0.10 | 9.55 × 10−44 | −0.03 | 0.08 |
1672 | 0.82 ± 2.90 × 10−29 | 1.20 ± 0.07 | −1.50 ± 0.09 | 7.02 × 10−34 | 0.37 | 0.07 | ||
3511 | 0.72 ± 2.20 × 10−6 | 1.60 ± 0.24 | −2.20 ± 0.23 | 1.41 × 10−7 | 0.69 | 0.10 | ||
5068 | 0.56 ± 7.00 × 10−3 | 0.97 ± 0.33 | −1.40 ± 0.41 | 8.69 × 10−4 | 0.90 | 0.08 | ||
1954 | 0.56 ± 0.01 | 0.83 ± 0.27 | −1.10 ± 0.28 | 7.13 × 10−3 | 0.75 | 0.12 | ||
1512 | 0.63 ± 1.70 × 10−4 | 0.92 ± 0.19 | 2.50 ± 0.51 | 5.70 × 10−5 | 4.20 | 0.14 | ||
4535 | 0.63 ± 2.90 × 10−4 | 0.89 ± 0.28 | 2.40 ± 0.63 | 1.90 × 10−3 | 4.90 | 0.12 | ||
7496 | 0.74 ± 1.50 × 10−9 | 0.87 ± 0.12 | 2.10 ± 0.29 | 4.98 × 10−10 | 5.00 | 0.20 | ||
ΣSFR | 1566 | 0.72 ± 3.70 × 10−17 | 0.72 | 0.84 ± 0.08 | 1.90 ± 0.18 | 1.51 × 10−17 | 5.10 | 0.14 |
1672 | 0.72 ± 1.00 × 10−13 | 0.71 ± 0.08 | 1.60 ± 0.17 | 4.58 × 10−14 | 2.50 | 0.10 | ||
3511 | 0.76 ± 2.50 × 10−6 | 1.10 ± 0.22 | 2.50 ± 0.58 | 1.14 × 10−5 | 2.90 | 0.06 | ||
5068 | −0.14 ± 0.11 | −0.13 ± 0.24 | −0.51 ± 0.62 | 0.59 | 2.20 | 0.12 | ||
1954 | 0.97 ± 1.10 × 10−11 | 0.94 ± 0.07 | 2.00 ± 0.17 | 8.89 × 10−13 | 2.30 | 0.01 | ||
1512 | 0.40 ± 6.90 × 10−4 | 0.46 ± 0.10 | −0.90 ± 0.19 | 4.92 × 10−5 | 2.10 | 0.20 | ||
4535 | 0.77 ± 4.00 × 10−14 | 0.93 ± 0.08 | −1.60 ± 0.15 | 4.44 × 10−19 | 0.73 | 0.05 | ||
7496 | 0.54 ± 6.50 × 10−5 | 0.79 ± 0.15 | −1.30 ± 0.25 | 2.03 × 10−6 | −0.77 | 0.24 | ||
Σ* | 1566 | 0.85 ± 3.40 × 10−31 | 0.52 | 1.00 ± 0.05 | −2.20 ± 0.10 | 1.48 × 10−40 | 1.50 | 0.08 |
1672 | 0.50 ± 9.50 × 10−7 | 0.60 ± 0.09 | −1.20 ± 0.17 | 2.52 × 10−9 | 1.20 | 0.15 | ||
3511 | 0.72 ± 2.60 × 10−6 | 0.59 ± 0.09 | −1.50 ± 0.13 | 8.92 × 10−8 | 2.30 | 0.10 | ||
5068 | −0.18 ± 0.10 | −0.13 ± 0.15 | −0.01 ± 0.21 | 0.37 | 2.70 | 0.11 | ||
1954 | 0.10 ± 0.18 | 0.07 ± 0.14 | −0.40 ± 0.22 | 0.72 | 2.30 | 0.17 | ||
1512 | 0.48 ± 0.19 | 3.60 ± 0.63 | −4.10 ± 0.72 | 1.86 × 10−7 | −0.06 | 0.18 | ||
4535 | 0.65 ± 5.20 × 10−5 | 2.40 ± 0.28 | −2.30 ± 0.29 | 3.70 × 10−13 | −0.12 | 0.07 | ||
7496 | 0.48 ± 0.01 | 2.00 ± 0.44 | −1.60 ± 0.35 | 2.13 × 10−5 | −0.74 | 0.26 | ||
Z′(rgal) | 1566 | 0.71 ± 5.90 × 10−10 | 0.48 | 3.60 ± 0.29 | −3.90 ± 0.31 | 4.32 × 10−24 | −0.35 | 0.14 |
1672 | 0.44 ± 6.70 × 10−3 | 2.00 ± 0.35 | −2.30 ± 0.39 | 1.68 × 10−7 | −0.10 | 0.16 | ||
3511 | 0.74 ± 8.30 × 10−3 | 2.00 ± 0.28 | −2.30 ± 0.23 | 1.98 × 10−8 | 0.45 | 0.09 | ||
5068 | −0.12 ± 0.28 | −0.34 ± 0.60 | 0.05 ± 0.42 | 0.55 | 0.61 | 0.11 | ||
1954 | 0.25 ± 0.29 | 0.84 ± 0.66 | −0.94 ± 0.52 | 0.25 | 0.33 | 0.16 | ||
1512 | 0.68 ± 0.25 | 0.65 ± 0.10 | −2.40 ± 0.36 | 3.50 × 10−9 | 6.90 | 0.10 | ||
4535 | 0.70 ± 0.28 | 0.61 ± 0.07 | −2.30 ± 0.30 | 1.04 × 10−12 | 5.90 | 0.06 | ||
7496 | 0.91 ± 0.25 | 1.30 ± 0.10 | −5.60 ± 0.43 | 6.32 × 10−19 | 4.50 | 0.08 | ||
PDE | 1566 | 0.91 ± 0.24 | 0.89 | 0.90 ± 0.04 | −4.10 ± 0.17 | 1.25 ×10−48 | 9.00 | 0.04 |
1672 | 0.89 ± 0.12 | 0.68 ± 0.04 | −3.00 ± 0.17 | 2.09 × 10−31 | 13.00 | 0.04 | ||
3511 | 0.89 ± 0.32 | 1.20 ± 0.12 | −5.60 ± 0.51 | 1.48 × 10−12 | 10.00 | 0.04 | ||
5068 | 0.33 ± 0.25 | 0.30 ± 0.26 | −1.60 ± 1.10 | 0.12 | 11.00 | 0.05 | ||
1954 | 0.95 ± 0.30 | 0.95 ± 0.10 | −4.40 ± 0.41 | 1.28 × 10−7 | 11.00 | 0.02 | ||
1512 | 0.31 ± 0.07 | 0.55 ± 0.29 | −3.60 ± 1.90 | 0.06 | 16.00 | 0.19 | ||
4535 | 0.72 ± 1.10 × 10−3 | 1.30 ± 0.35 | −8.70 ± 2.40 | 3.82 × 10−4 | 18.00 | 0.11 | ||
7496 | −0.01 ± 0.06 | −0.02 ± 0.28 | 0.17 ± 1.90 | 0.97 | 7.80 | 0.45 | ||
PDE/ΣSFR | 1566 | 0.55 ± 1.40 × 10−8 | 0.40 | 0.97 ± 0.15 | −6.70 ± 1.10 | 3.41 × 10−9 | 18.00 | 0.20 |
1672 | 0.50 ± 3.20 × 10−6 | 0.71 ± 0.15 | −4.70 ± 0.98 | 2.41 × 10−6 | 16.00 | 0.16 | ||
3511 | 0.34 ± 0.07 | 0.69 ± 0.45 | −5.20 ± 3.10 | 0.10 | 23.00 | 0.13 | ||
5068 | 0.46 ± 0.05 | 0.50 ± 0.26 | −3.70 ± 1.80 | 0.03 | 25.00 | 0.09 | ||
1954 | −0.29 ± 0.08 | −1.00 ± 0.90 | 6.60 ± 6.20 | 0.21 | 22.00 | 0.16 |
Notes. (1): The IC only applies for IC 1954. (2): The correlation coefficient ρ for individual fits for each galaxy using linmix, see Section 4.9. We perform a Monte Carlo analysis perturbing the x and y data points to get the uncertainty of ρ. (3): The median ρ for all galaxies for each log(x). (4): The slope β of the fit, and (5): The intercept α of the fit. (6): The covariance in the form of Cov(log10(x), log10(y)). (7): The regression intrinsic scatter.
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