Region . | Galactocentric distance . | Area . | . | . | . | . |
---|---|---|---|---|---|---|
I.D. . | (kpc) . | (kpc2) . | IRX . | β . | 12 + log([O/H]) . | Dn(4000) . |
(1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . |
1.1 | 0.6 | 31.1 | 0.21 ± 0.3 | −1.26 ± 0.2 | 8.59 ± 0.1 | 1.31 ± 0.06 |
2.1 | 5.1 | 51.5 | 0.23 ± 0.3 | −1.09 ± 0.2 | 8.7 ± 0.1 | 1.23 ± 0.12 |
3.1 | 0.9 | 123.8 | 0.66 ± 0.3 | −1.13 ± 0.2 | 8.94 ± 0.1 | 1.27 ± 0.05 |
4.1 | 2.3 | 78.3 | 0.33 ± 0.3 | −1.29 ± 0.2 | 8.79 ± 0.1 | 1.3 ± 0.05 |
5.1 | 0.4 | 23.6 | 0.76 ± 0.3 | −0.9 ± 0.2 | 9.05 ± 0.1 | 1.55 ± 0.06 |
6.1 | 0.5 | 113.5 | 0.23 ± 0.3 | −1.15 ± 0.2 | 8.73 ± 0.1 | 1.33 ± 0.04 |
7.1 | 0.4 | 48.2 | 0.37 ± 0.3 | −1.43 ± 0.2 | 8.83 ± 0.1 | 1.32 ± 0.03 |
8.1 | 0.6 | 75.3 | 0.43 ± 0.3 | −1.07 ± 0.2 | 8.88 ± 0.1 | 1.28 ± 0.05 |
9.1 | 0.8 | 152.0 | 0.28 ± 0.3 | −1.37 ± 0.2 | 8.82 ± 0.1 | 1.26 ± 0.04 |
10.1 | 0.2 | 83.7 | 0.55 ± 0.3 | −1.03 ± 0.2 | 8.81 ± 0.1 | 1.26 ± 0.06 |
11.1 | 0.4 | 126.7 | 0.91 ± 0.3 | −0.7 ± 0.2 | 8.97 ± 0.1 | 1.4 ± 0.07 |
12.1 | 0.8 | 151.3 | 0.13 ± 0.3 | −1.43 ± 0.2 | 8.66 ± 0.1 | 1.13 ± 0.01 |
13.1 | 5.7 | 31.7 | 0.46 ± 0.3 | −1.26 ± 0.2 | 8.79 ± 0.1 | 1.21 ± 0.02 |
13.2 | 5.3 | 31.7 | 0.61 ± 0.3 | −1.29 ± 0.2 | 8.73 ± 0.1 | 1.23 ± 0.02 |
14.1 | 0.2 | 88.1 | 1.37 ± 0.3 | −0.48 ± 0.2 | 8.9 ± 0.1 | 1.46 ± 0.07 |
15.1 | 1.3 | 31.2 | 0.54 ± 0.3 | −1.3 ± 0.2 | 8.89 ± 0.1 | 1.22 ± 0.01 |
16.1 | 5.4 | 55.9 | 0.92 ± 0.3 | −0.97 ± 0.2 | 8.98 ± 0.1 | 1.47 ± 0.07 |
17.1 | 0.2 | 33.4 | 1.0 ± 0.3 | −1.03 ± 0.2 | 9.09 ± 0.1 | 1.46 ± 0.03 |
18.1 | 0.6 | 74.5 | 1.66 ± 0.3 | −0.96 ± 0.2 | 8.94 ± 0.1 | 1.45 ± 0.05 |
19.1 | 0.3 | 173.3 | 1.03 ± 0.3 | −0.67 ± 0.2 | 9.05 ± 0.1 | 1.28 ± 0.03 |
20.1 | 8.0 | 48.4 | 0.53 ± 0.3 | −1.42 ± 0.2 | 8.97 ± 0.1 | 1.33 ± 0.03 |
20.2 | 8.5 | 48.4 | 0.65 ± 0.3 | −1.14 ± 0.2 | 8.97 ± 0.1 | 1.33 ± 0.03 |
21.1 | 0.5 | 63.4 | 0.67 ± 0.3 | −1.25 ± 0.2 | 9.11 ± 0.1 | 1.59 ± 0.04 |
22.1 | 1.2 | 226.5 | 0.88 ± 0.3 | −0.68 ± 0.2 | 9.01 ± 0.1 | 1.3 ± 0.03 |
23.1 | 13.7 | 81.8 | 0.54 ± 0.3 | −1.37 ± 0.2 | 8.97 ± 0.1 | 1.26 ± 0.03 |
23.2 | 8.4 | 81.8 | 0.8 ± 0.3 | −1.16 ± 0.2 | 9.13 ± 0.1 | 1.41 ± 0.03 |
24.1 | 3.7 | 133.1 | 0.76 ± 0.3 | −0.79 ± 0.2 | 9.04 ± 0.1 | 1.27 ± 0.03 |
25.1 | 8.6 | 42.0 | 0.86 ± 0.3 | −1.36 ± 0.2 | 8.93 ± 0.1 | 1.31 ± 0.02 |
25.2 | 10.0 | 47.2 | 0.83 ± 0.3 | −1.33 ± 0.2 | 8.99 ± 0.1 | 1.3 ± 0.03 |
25.3 | 11.6 | 47.2 | 0.84 ± 0.3 | −1.33 ± 0.2 | 8.99 ± 0.1 | 1.31 ± 0.03 |
26.1a | 13.4 | 56.4 | – | – | 8.87 ± 0.1 | 1.2 ± 0.01 |
26.2a | 12.1 | 62.7 | – | – | 8.91 ± 0.1 | 1.24 ± 0.02 |
27.1 | 6.1 | 336.9 | 1.16 ± 0.3 | −0.22 ± 0.2 | 8.97 ± 0.1 | 1.72 ± 0.08 |
28.1 | 3.1 | 242.5 | 1.29 ± 0.3 | −0.84 ± 0.2 | 9.0 ± 0.1 | 1.27 ± 0.01 |
29.1 | 0.4 | 386.5 | 0.74 ± 0.3 | −1.38 ± 0.2 | 9.08 ± 0.1 | 1.4 ± 0.03 |
Region . | Galactocentric distance . | Area . | . | . | . | . |
---|---|---|---|---|---|---|
I.D. . | (kpc) . | (kpc2) . | IRX . | β . | 12 + log([O/H]) . | Dn(4000) . |
(1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . |
1.1 | 0.6 | 31.1 | 0.21 ± 0.3 | −1.26 ± 0.2 | 8.59 ± 0.1 | 1.31 ± 0.06 |
2.1 | 5.1 | 51.5 | 0.23 ± 0.3 | −1.09 ± 0.2 | 8.7 ± 0.1 | 1.23 ± 0.12 |
3.1 | 0.9 | 123.8 | 0.66 ± 0.3 | −1.13 ± 0.2 | 8.94 ± 0.1 | 1.27 ± 0.05 |
4.1 | 2.3 | 78.3 | 0.33 ± 0.3 | −1.29 ± 0.2 | 8.79 ± 0.1 | 1.3 ± 0.05 |
5.1 | 0.4 | 23.6 | 0.76 ± 0.3 | −0.9 ± 0.2 | 9.05 ± 0.1 | 1.55 ± 0.06 |
6.1 | 0.5 | 113.5 | 0.23 ± 0.3 | −1.15 ± 0.2 | 8.73 ± 0.1 | 1.33 ± 0.04 |
7.1 | 0.4 | 48.2 | 0.37 ± 0.3 | −1.43 ± 0.2 | 8.83 ± 0.1 | 1.32 ± 0.03 |
8.1 | 0.6 | 75.3 | 0.43 ± 0.3 | −1.07 ± 0.2 | 8.88 ± 0.1 | 1.28 ± 0.05 |
9.1 | 0.8 | 152.0 | 0.28 ± 0.3 | −1.37 ± 0.2 | 8.82 ± 0.1 | 1.26 ± 0.04 |
10.1 | 0.2 | 83.7 | 0.55 ± 0.3 | −1.03 ± 0.2 | 8.81 ± 0.1 | 1.26 ± 0.06 |
11.1 | 0.4 | 126.7 | 0.91 ± 0.3 | −0.7 ± 0.2 | 8.97 ± 0.1 | 1.4 ± 0.07 |
12.1 | 0.8 | 151.3 | 0.13 ± 0.3 | −1.43 ± 0.2 | 8.66 ± 0.1 | 1.13 ± 0.01 |
13.1 | 5.7 | 31.7 | 0.46 ± 0.3 | −1.26 ± 0.2 | 8.79 ± 0.1 | 1.21 ± 0.02 |
13.2 | 5.3 | 31.7 | 0.61 ± 0.3 | −1.29 ± 0.2 | 8.73 ± 0.1 | 1.23 ± 0.02 |
14.1 | 0.2 | 88.1 | 1.37 ± 0.3 | −0.48 ± 0.2 | 8.9 ± 0.1 | 1.46 ± 0.07 |
15.1 | 1.3 | 31.2 | 0.54 ± 0.3 | −1.3 ± 0.2 | 8.89 ± 0.1 | 1.22 ± 0.01 |
16.1 | 5.4 | 55.9 | 0.92 ± 0.3 | −0.97 ± 0.2 | 8.98 ± 0.1 | 1.47 ± 0.07 |
17.1 | 0.2 | 33.4 | 1.0 ± 0.3 | −1.03 ± 0.2 | 9.09 ± 0.1 | 1.46 ± 0.03 |
18.1 | 0.6 | 74.5 | 1.66 ± 0.3 | −0.96 ± 0.2 | 8.94 ± 0.1 | 1.45 ± 0.05 |
19.1 | 0.3 | 173.3 | 1.03 ± 0.3 | −0.67 ± 0.2 | 9.05 ± 0.1 | 1.28 ± 0.03 |
20.1 | 8.0 | 48.4 | 0.53 ± 0.3 | −1.42 ± 0.2 | 8.97 ± 0.1 | 1.33 ± 0.03 |
20.2 | 8.5 | 48.4 | 0.65 ± 0.3 | −1.14 ± 0.2 | 8.97 ± 0.1 | 1.33 ± 0.03 |
21.1 | 0.5 | 63.4 | 0.67 ± 0.3 | −1.25 ± 0.2 | 9.11 ± 0.1 | 1.59 ± 0.04 |
22.1 | 1.2 | 226.5 | 0.88 ± 0.3 | −0.68 ± 0.2 | 9.01 ± 0.1 | 1.3 ± 0.03 |
23.1 | 13.7 | 81.8 | 0.54 ± 0.3 | −1.37 ± 0.2 | 8.97 ± 0.1 | 1.26 ± 0.03 |
23.2 | 8.4 | 81.8 | 0.8 ± 0.3 | −1.16 ± 0.2 | 9.13 ± 0.1 | 1.41 ± 0.03 |
24.1 | 3.7 | 133.1 | 0.76 ± 0.3 | −0.79 ± 0.2 | 9.04 ± 0.1 | 1.27 ± 0.03 |
25.1 | 8.6 | 42.0 | 0.86 ± 0.3 | −1.36 ± 0.2 | 8.93 ± 0.1 | 1.31 ± 0.02 |
25.2 | 10.0 | 47.2 | 0.83 ± 0.3 | −1.33 ± 0.2 | 8.99 ± 0.1 | 1.3 ± 0.03 |
25.3 | 11.6 | 47.2 | 0.84 ± 0.3 | −1.33 ± 0.2 | 8.99 ± 0.1 | 1.31 ± 0.03 |
26.1a | 13.4 | 56.4 | – | – | 8.87 ± 0.1 | 1.2 ± 0.01 |
26.2a | 12.1 | 62.7 | – | – | 8.91 ± 0.1 | 1.24 ± 0.02 |
27.1 | 6.1 | 336.9 | 1.16 ± 0.3 | −0.22 ± 0.2 | 8.97 ± 0.1 | 1.72 ± 0.08 |
28.1 | 3.1 | 242.5 | 1.29 ± 0.3 | −0.84 ± 0.2 | 9.0 ± 0.1 | 1.27 ± 0.01 |
29.1 | 0.4 | 386.5 | 0.74 ± 0.3 | −1.38 ± 0.2 | 9.08 ± 0.1 | 1.4 ± 0.03 |
Notes. Column 1: Region I.D. Column 2: Distance of region from the nominal centre of the galaxy in kpc. Column 3: Area of the region in kpc2. Column 4: Calculated value of IRX. Column 5: Calculated value of β. Column 6: Gas-phase metallicity. We calculate this using the [N ii]/[O ii] ratio, as described by Kewley & Dopita (2002). Column 7: The systematic uncertainty in Dn(4000) as reported by Westfall et al. (2019) is included in the reported error.
aWe do not calculate values for galaxy 26 that rely on Swift/UVOT measurements due to the supernova light that contaminates the image.
Region . | Galactocentric distance . | Area . | . | . | . | . |
---|---|---|---|---|---|---|
I.D. . | (kpc) . | (kpc2) . | IRX . | β . | 12 + log([O/H]) . | Dn(4000) . |
(1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . |
1.1 | 0.6 | 31.1 | 0.21 ± 0.3 | −1.26 ± 0.2 | 8.59 ± 0.1 | 1.31 ± 0.06 |
2.1 | 5.1 | 51.5 | 0.23 ± 0.3 | −1.09 ± 0.2 | 8.7 ± 0.1 | 1.23 ± 0.12 |
3.1 | 0.9 | 123.8 | 0.66 ± 0.3 | −1.13 ± 0.2 | 8.94 ± 0.1 | 1.27 ± 0.05 |
4.1 | 2.3 | 78.3 | 0.33 ± 0.3 | −1.29 ± 0.2 | 8.79 ± 0.1 | 1.3 ± 0.05 |
5.1 | 0.4 | 23.6 | 0.76 ± 0.3 | −0.9 ± 0.2 | 9.05 ± 0.1 | 1.55 ± 0.06 |
6.1 | 0.5 | 113.5 | 0.23 ± 0.3 | −1.15 ± 0.2 | 8.73 ± 0.1 | 1.33 ± 0.04 |
7.1 | 0.4 | 48.2 | 0.37 ± 0.3 | −1.43 ± 0.2 | 8.83 ± 0.1 | 1.32 ± 0.03 |
8.1 | 0.6 | 75.3 | 0.43 ± 0.3 | −1.07 ± 0.2 | 8.88 ± 0.1 | 1.28 ± 0.05 |
9.1 | 0.8 | 152.0 | 0.28 ± 0.3 | −1.37 ± 0.2 | 8.82 ± 0.1 | 1.26 ± 0.04 |
10.1 | 0.2 | 83.7 | 0.55 ± 0.3 | −1.03 ± 0.2 | 8.81 ± 0.1 | 1.26 ± 0.06 |
11.1 | 0.4 | 126.7 | 0.91 ± 0.3 | −0.7 ± 0.2 | 8.97 ± 0.1 | 1.4 ± 0.07 |
12.1 | 0.8 | 151.3 | 0.13 ± 0.3 | −1.43 ± 0.2 | 8.66 ± 0.1 | 1.13 ± 0.01 |
13.1 | 5.7 | 31.7 | 0.46 ± 0.3 | −1.26 ± 0.2 | 8.79 ± 0.1 | 1.21 ± 0.02 |
13.2 | 5.3 | 31.7 | 0.61 ± 0.3 | −1.29 ± 0.2 | 8.73 ± 0.1 | 1.23 ± 0.02 |
14.1 | 0.2 | 88.1 | 1.37 ± 0.3 | −0.48 ± 0.2 | 8.9 ± 0.1 | 1.46 ± 0.07 |
15.1 | 1.3 | 31.2 | 0.54 ± 0.3 | −1.3 ± 0.2 | 8.89 ± 0.1 | 1.22 ± 0.01 |
16.1 | 5.4 | 55.9 | 0.92 ± 0.3 | −0.97 ± 0.2 | 8.98 ± 0.1 | 1.47 ± 0.07 |
17.1 | 0.2 | 33.4 | 1.0 ± 0.3 | −1.03 ± 0.2 | 9.09 ± 0.1 | 1.46 ± 0.03 |
18.1 | 0.6 | 74.5 | 1.66 ± 0.3 | −0.96 ± 0.2 | 8.94 ± 0.1 | 1.45 ± 0.05 |
19.1 | 0.3 | 173.3 | 1.03 ± 0.3 | −0.67 ± 0.2 | 9.05 ± 0.1 | 1.28 ± 0.03 |
20.1 | 8.0 | 48.4 | 0.53 ± 0.3 | −1.42 ± 0.2 | 8.97 ± 0.1 | 1.33 ± 0.03 |
20.2 | 8.5 | 48.4 | 0.65 ± 0.3 | −1.14 ± 0.2 | 8.97 ± 0.1 | 1.33 ± 0.03 |
21.1 | 0.5 | 63.4 | 0.67 ± 0.3 | −1.25 ± 0.2 | 9.11 ± 0.1 | 1.59 ± 0.04 |
22.1 | 1.2 | 226.5 | 0.88 ± 0.3 | −0.68 ± 0.2 | 9.01 ± 0.1 | 1.3 ± 0.03 |
23.1 | 13.7 | 81.8 | 0.54 ± 0.3 | −1.37 ± 0.2 | 8.97 ± 0.1 | 1.26 ± 0.03 |
23.2 | 8.4 | 81.8 | 0.8 ± 0.3 | −1.16 ± 0.2 | 9.13 ± 0.1 | 1.41 ± 0.03 |
24.1 | 3.7 | 133.1 | 0.76 ± 0.3 | −0.79 ± 0.2 | 9.04 ± 0.1 | 1.27 ± 0.03 |
25.1 | 8.6 | 42.0 | 0.86 ± 0.3 | −1.36 ± 0.2 | 8.93 ± 0.1 | 1.31 ± 0.02 |
25.2 | 10.0 | 47.2 | 0.83 ± 0.3 | −1.33 ± 0.2 | 8.99 ± 0.1 | 1.3 ± 0.03 |
25.3 | 11.6 | 47.2 | 0.84 ± 0.3 | −1.33 ± 0.2 | 8.99 ± 0.1 | 1.31 ± 0.03 |
26.1a | 13.4 | 56.4 | – | – | 8.87 ± 0.1 | 1.2 ± 0.01 |
26.2a | 12.1 | 62.7 | – | – | 8.91 ± 0.1 | 1.24 ± 0.02 |
27.1 | 6.1 | 336.9 | 1.16 ± 0.3 | −0.22 ± 0.2 | 8.97 ± 0.1 | 1.72 ± 0.08 |
28.1 | 3.1 | 242.5 | 1.29 ± 0.3 | −0.84 ± 0.2 | 9.0 ± 0.1 | 1.27 ± 0.01 |
29.1 | 0.4 | 386.5 | 0.74 ± 0.3 | −1.38 ± 0.2 | 9.08 ± 0.1 | 1.4 ± 0.03 |
Region . | Galactocentric distance . | Area . | . | . | . | . |
---|---|---|---|---|---|---|
I.D. . | (kpc) . | (kpc2) . | IRX . | β . | 12 + log([O/H]) . | Dn(4000) . |
(1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . |
1.1 | 0.6 | 31.1 | 0.21 ± 0.3 | −1.26 ± 0.2 | 8.59 ± 0.1 | 1.31 ± 0.06 |
2.1 | 5.1 | 51.5 | 0.23 ± 0.3 | −1.09 ± 0.2 | 8.7 ± 0.1 | 1.23 ± 0.12 |
3.1 | 0.9 | 123.8 | 0.66 ± 0.3 | −1.13 ± 0.2 | 8.94 ± 0.1 | 1.27 ± 0.05 |
4.1 | 2.3 | 78.3 | 0.33 ± 0.3 | −1.29 ± 0.2 | 8.79 ± 0.1 | 1.3 ± 0.05 |
5.1 | 0.4 | 23.6 | 0.76 ± 0.3 | −0.9 ± 0.2 | 9.05 ± 0.1 | 1.55 ± 0.06 |
6.1 | 0.5 | 113.5 | 0.23 ± 0.3 | −1.15 ± 0.2 | 8.73 ± 0.1 | 1.33 ± 0.04 |
7.1 | 0.4 | 48.2 | 0.37 ± 0.3 | −1.43 ± 0.2 | 8.83 ± 0.1 | 1.32 ± 0.03 |
8.1 | 0.6 | 75.3 | 0.43 ± 0.3 | −1.07 ± 0.2 | 8.88 ± 0.1 | 1.28 ± 0.05 |
9.1 | 0.8 | 152.0 | 0.28 ± 0.3 | −1.37 ± 0.2 | 8.82 ± 0.1 | 1.26 ± 0.04 |
10.1 | 0.2 | 83.7 | 0.55 ± 0.3 | −1.03 ± 0.2 | 8.81 ± 0.1 | 1.26 ± 0.06 |
11.1 | 0.4 | 126.7 | 0.91 ± 0.3 | −0.7 ± 0.2 | 8.97 ± 0.1 | 1.4 ± 0.07 |
12.1 | 0.8 | 151.3 | 0.13 ± 0.3 | −1.43 ± 0.2 | 8.66 ± 0.1 | 1.13 ± 0.01 |
13.1 | 5.7 | 31.7 | 0.46 ± 0.3 | −1.26 ± 0.2 | 8.79 ± 0.1 | 1.21 ± 0.02 |
13.2 | 5.3 | 31.7 | 0.61 ± 0.3 | −1.29 ± 0.2 | 8.73 ± 0.1 | 1.23 ± 0.02 |
14.1 | 0.2 | 88.1 | 1.37 ± 0.3 | −0.48 ± 0.2 | 8.9 ± 0.1 | 1.46 ± 0.07 |
15.1 | 1.3 | 31.2 | 0.54 ± 0.3 | −1.3 ± 0.2 | 8.89 ± 0.1 | 1.22 ± 0.01 |
16.1 | 5.4 | 55.9 | 0.92 ± 0.3 | −0.97 ± 0.2 | 8.98 ± 0.1 | 1.47 ± 0.07 |
17.1 | 0.2 | 33.4 | 1.0 ± 0.3 | −1.03 ± 0.2 | 9.09 ± 0.1 | 1.46 ± 0.03 |
18.1 | 0.6 | 74.5 | 1.66 ± 0.3 | −0.96 ± 0.2 | 8.94 ± 0.1 | 1.45 ± 0.05 |
19.1 | 0.3 | 173.3 | 1.03 ± 0.3 | −0.67 ± 0.2 | 9.05 ± 0.1 | 1.28 ± 0.03 |
20.1 | 8.0 | 48.4 | 0.53 ± 0.3 | −1.42 ± 0.2 | 8.97 ± 0.1 | 1.33 ± 0.03 |
20.2 | 8.5 | 48.4 | 0.65 ± 0.3 | −1.14 ± 0.2 | 8.97 ± 0.1 | 1.33 ± 0.03 |
21.1 | 0.5 | 63.4 | 0.67 ± 0.3 | −1.25 ± 0.2 | 9.11 ± 0.1 | 1.59 ± 0.04 |
22.1 | 1.2 | 226.5 | 0.88 ± 0.3 | −0.68 ± 0.2 | 9.01 ± 0.1 | 1.3 ± 0.03 |
23.1 | 13.7 | 81.8 | 0.54 ± 0.3 | −1.37 ± 0.2 | 8.97 ± 0.1 | 1.26 ± 0.03 |
23.2 | 8.4 | 81.8 | 0.8 ± 0.3 | −1.16 ± 0.2 | 9.13 ± 0.1 | 1.41 ± 0.03 |
24.1 | 3.7 | 133.1 | 0.76 ± 0.3 | −0.79 ± 0.2 | 9.04 ± 0.1 | 1.27 ± 0.03 |
25.1 | 8.6 | 42.0 | 0.86 ± 0.3 | −1.36 ± 0.2 | 8.93 ± 0.1 | 1.31 ± 0.02 |
25.2 | 10.0 | 47.2 | 0.83 ± 0.3 | −1.33 ± 0.2 | 8.99 ± 0.1 | 1.3 ± 0.03 |
25.3 | 11.6 | 47.2 | 0.84 ± 0.3 | −1.33 ± 0.2 | 8.99 ± 0.1 | 1.31 ± 0.03 |
26.1a | 13.4 | 56.4 | – | – | 8.87 ± 0.1 | 1.2 ± 0.01 |
26.2a | 12.1 | 62.7 | – | – | 8.91 ± 0.1 | 1.24 ± 0.02 |
27.1 | 6.1 | 336.9 | 1.16 ± 0.3 | −0.22 ± 0.2 | 8.97 ± 0.1 | 1.72 ± 0.08 |
28.1 | 3.1 | 242.5 | 1.29 ± 0.3 | −0.84 ± 0.2 | 9.0 ± 0.1 | 1.27 ± 0.01 |
29.1 | 0.4 | 386.5 | 0.74 ± 0.3 | −1.38 ± 0.2 | 9.08 ± 0.1 | 1.4 ± 0.03 |
Notes. Column 1: Region I.D. Column 2: Distance of region from the nominal centre of the galaxy in kpc. Column 3: Area of the region in kpc2. Column 4: Calculated value of IRX. Column 5: Calculated value of β. Column 6: Gas-phase metallicity. We calculate this using the [N ii]/[O ii] ratio, as described by Kewley & Dopita (2002). Column 7: The systematic uncertainty in Dn(4000) as reported by Westfall et al. (2019) is included in the reported error.
aWe do not calculate values for galaxy 26 that rely on Swift/UVOT measurements due to the supernova light that contaminates the image.
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