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Table C.2.

Star formation rate, Hα luminosity, BPT classification, and the radial velocity sub-sample.

(1) (2) (3) (4) (5)
Region SFR LHα BPT Vel
ID (×10−3 M⊙ yr−1) (×1038 erg s−1)
2 12.81 ± 0.69 16.21 ± 0.87 SF 1
3 11.08 ± 0.78 14.02 ± 0.99 SF 1
4 27.53 ± 0.70 34.84 ± 0.89 SF 1
5 – 0.63 ± 0.09 C 1
6 17.70 ± 1.35 22.40 ± 1.71 SF 1
8 31.37 ± 1.80 39.71 ± 2.27 SF 1
9 10.26 ± 0.46 12.99 ± 0.58 SF 1
10 39.85 ± 0.87 50.44 ± 1.10 SF 1
11 3.33 ± 0.24 4.21 ± 0.30 SF 1
12 1.66 ± 0.16 2.10 ± 0.21 SF 1
13 76.48 ± 1.61 96.82 ± 2.03 SF 1
14 94.95 ± 4.06 120.19 ± 5.14 SF 1
15 196.79 ± 5.31 249.10 ± 6.72 SF 1
24 29.67 ± 2.38 37.55 ± 3.01 SF 1
25 17.79 ± 1.51 22.52 ± 1.91 SF 1
26 – 2690.21 ± 192.90 AGN 1
27 – 552.11 ± 55.75 AGN 1
29 – 3.45 ± 0.53 AGN 1
30 – 23.05 ± 3.23 C 1
33 2.31 ± 0.27 2.93 ± 0.34 SF 0
35 23.79 ± 2.45 30.12 ± 3.10 SF 1
39 6.37 ± 0.58 8.06 ± 0.73 SF 0
40 – 11.44 ± 1.22 C 1
42 13.18 ± 0.81 16.68 ± 1.03 SF 0
43 – 3.63 ± 0.48 C 0
45 12.63 ± 1.32 15.99 ± 1.67 SF 0
46 12.23 ± 1.01 15.48 ± 1.28 SF 0
47 0.67 ± 0.10 0.85 ± 0.12 SF 0
48 6.19 ± 0.96 7.83 ± 1.22 SF 0
50 3.00 ± 0.42 3.79 ± 0.53 SF 0
51(b) 15.59 ± 2.35 19.73 ± 2.97 SF 1
52 41.39 ± 1.85 52.39 ± 2.34 SF 0
53 – 0.82 ± 0.15 C 0
54 – 2.28 ± 0.33 C 0
58(a) – 7.57 ± 1.26 AGN 0
59(a) – 10.63 ± 1.54 C 0
59(b) 36.96 ± 7.87 46.78 ± 9.96 SF 1
60(a) – 1.26 ± 0.19 C 0
60(b) 11.77 ± 2.09 14.90 ± 2.64 SF 1
64 6.14 ± 0.63 7.77 ± 0.80 SF 1
65 36.82 ± 2.38 46.60 ± 3.01 SF 0
66(a) – 17.69 ± 2.30 AGN 0
67 – 8.74 ± 1.23 C 0
68(a) – 16.09 ± 1.70 C 0
69(a) – 1.52 ± 0.23 C 0
70 14.75 ± 1.00 18.68 ± 1.27 SF 0
71 – 2.83 ± 0.32 C 0
74 14.51 ± 1.27 18.37 ± 1.61 SF 1
75 17.09 ± 1.11 21.63 ± 1.41 SF 0
76(a) 7.37 ± 0.99 9.33 ± 1.26 SF 0
76(b) 3.56 ± 0.67 4.51 ± 0.85 SF 1
77 8.81 ± 0.92 11.15 ± 1.16 SF 1
78 2.20 ± 0.31 2.78 ± 0.39 SF 0
81(a) – 2.45 ± 0.39 C 0
82 7.07 ± 0.39 8.95 ± 0.50 SF 0
83(b) 22.20 ± 3.06 28.10 ± 3.87 SF 1
86(a) – 15.92 ± 3.06 AGN 0
90 – 19.96 ± 1.45 C 0
91 4.29 ± 0.50 5.43 ± 0.64 SF 0
92 – 6.18 ± 0.48 AGN 0
96 19.53 ± 2.10 24.72 ± 2.66 SF 1
97 3.88 ± 0.24 4.92 ± 0.31 SF 0
98 – 15.75 ± 1.40 C 0
102(a) 3.40 ± 0.63 4.30 ± 0.80 SF 0
104(b) 11.35 ± 1.59 14.36 ± 2.01 SF 1
109 0.54 ± 0.13 0.69 ± 0.17 SF 1
112 23.20 ± 1.29 29.37 ± 1.63 SF 0
113 3.69 ± 0.55 4.68 ± 0.70 SF 1
117 119.16 ± 2.67 150.84 ± 3.38 SF 0
120 – 20.64 ± 1.11 C 0
121 139.98 ± 6.46 177.19 ± 8.18 SF 1
122 733.22 ± 13.18 928.12 ± 16.69 SF 1
123 0.57 ± 0.08 0.72 ± 0.10 SF 1
125 7.57 ± 0.98 9.58 ± 1.24 SF 0
127 14.95 ± 0.80 18.93 ± 1.01 SF 0
128 18.60 ± 1.03 23.54 ± 1.30 SF 0
129 59.93 ± 2.10 75.86 ± 2.65 SF 0
130 26.72 ± 1.25 33.82 ± 1.59 SF 0
132 38.31 ± 1.36 48.49 ± 1.72 SF 0
133 94.48 ± 1.55 119.59 ± 1.97 SF 0
134 13.96 ± 1.16 17.66 ± 1.46 SF 0
136 33.43 ± 1.69 42.32 ± 2.14 SF 0
137 43.84 ± 2.03 55.50 ± 2.57 SF 0
138 32.01 ± 1.18 40.52 ± 1.49 SF 0
139 19.86 ± 0.64 25.14 ± 0.81 SF 0
140 21.83 ± 1.51 27.63 ± 1.91 SF 0
141 42.05 ± 1.28 53.22 ± 1.62 SF 0
142 31.38 ± 1.33 39.73 ± 1.68 SF 0
143 29.21 ± 1.43 36.98 ± 1.81 SF 0
146 44.23 ± 1.39 55.99 ± 1.76 SF 0
147 8.64 ± 1.08 10.94 ± 1.37 SF 0
148 8.24 ± 0.74 10.43 ± 0.94 SF 0
149 2.93 ± 0.34 3.70 ± 0.43 SF 0
150 5.24 ± 0.49 6.63 ± 0.61 SF 0
151 – 2.43 ± 0.22 C 0
152 10.59 ± 0.81 13.41 ± 1.02 SF 0
153 25.37 ± 1.31 32.12 ± 1.65 SF 0
154 19.76 ± 0.86 25.01 ± 1.09 SF 0
155 15.12 ± 0.82 19.14 ± 1.04 SF 0
156 2.69 ± 0.23 3.40 ± 0.29 SF 0
157 19.74 ± 1.18 24.98 ± 1.49 SF 0
159 14.09 ± 1.04 17.84 ± 1.32 SF 0
160 6.16 ± 0.66 7.80 ± 0.84 SF 0
164 85.55 ± 1.73 108.29 ± 2.19 SF 0
165 93.67 ± 2.09 118.57 ± 2.65 SF 0
166 53.28 ± 1.53 67.44 ± 1.93 SF 0
167 34.23 ± 1.17 43.33 ± 1.48 SF 0
168 8.00 ± 0.30 10.12 ± 0.39 SF 0
169 7.31 ± 0.38 9.26 ± 0.48 SF 0
170 5.95 ± 0.32 7.54 ± 0.40 SF 0
171 10.65 ± 0.47 13.48 ± 0.60 SF 0
172 23.95 ± 0.84 30.32 ± 1.06 SF 0
173 21.09 ± 0.73 26.69 ± 0.92 SF 0
174 24.79 ± 0.76 31.38 ± 0.96 SF 0
176 90.27 ± 9.22 114.26 ± 11.66 SF 1

Notes. The columns correspond to: (1) identifier of the HII region; (2) star formation rate (×10−3 M⊙ yr−1); (3) Hα luminosity (×1038 erg s−1); (4) BPT classification; (5) velocity of the region belongs to the LV (0) or the HV (1) sub-samples. For regions with two velocity components we use “(a)” and “(b)” for low- and high-velocity components, respectively.

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