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Table 4.

LF properties of H II region subsamples in the PHANGS–MUSE galaxies.

Galaxy αa na αi ni αr< nr< αr> nr> αq< nq< αq> nq>
NGC 5068 1.57 ± 0.09 607 1.60 ± 0.08 598 2.01 ± 0.17 525 1.39 ± 0.00 587
IC 5332 1.87 ± 0.14 199 1.76 ± 0.11 158 2.39 ± 0.25 134 1.58 ± 0.09 189
NGC 1087 1.66 ± 0.09 303 1.84 ± 0.13 135 2.31 ± 0.23 170 1.55 ± 0.08 268
NGC 1385 1.59 ± 0.08 197 1.49 ± 0.08 359 1.46 ± 0.08 389 1.80 ± 0.12 167 1.85 ± 0.13 224 1.42 ± 0.00 331
NGC 7496 1.73 ± 0.11 174 1.65 ± 0.09 127 2.14 ± 0.20 136 1.52 ± 0.08 164
NGC 2835 1.65 ± 0.09 186 1.87 ± 0.14 229 1.70 ± 0.10 238 1.83 ± 0.13 194 2.86 ± 0.31 119 1.62 ± 0.08 311
NGC 0628 1.66 ± 0.09 883 1.85 ± 0.13 389 1.76 ± 0.11 572 1.66 ± 0.09 700 2.17 ± 0.20 510 1.48 ± 0.09 633
NGC 3351 2.03 ± 0.17 204 1.93 ± 0.15 165 2.07 ± 0.18 158 1.74 ± 0.11 152
NGC 4254 1.58 ± 0.09 792 1.65 ± 0.09 637 1.57 ± 0.09 921 1.72 ± 0.10 508 1.74 ± 0.11 583 1.55 ± 0.08 846
NGC 4303 1.49 ± 0.08 864 1.68 ± 0.10 668 1.52 ± 0.08 937 1.65 ± 0.09 630 1.83 ± 0.13 731 1.44 ± 0.00 823
NGC 4535 1.54 ± 0.08 341 1.71 ± 0.10 545 1.64 ± 0.09 455 1.62 ± 0.09 479 1.70 ± 0.10 459 1.50 ± 0.08 393
NGC 1300 1.67 ± 0.10 397 2.13 ± 0.19 184 1.79 ± 0.12 344 1.75 ± 0.11 289 1.87 ± 0.14 337 1.67 ± 0.10 289
NGC 1512 1.96 ± 0.16 125 2.18 ± 0.20 77 2.18 ± 0.21 108 1.92 ± 0.15 101 2.83 ± 0.31 78 1.81 ± 0.13 128
NGC 1672 1.57 ± 0.09 145 1.79 ± 0.12 265 1.67 ± 0.10 307 1.67 ± 0.10 263 1.97 ± 0.16 228 1.55 ± 0.08 337
NGC 4321 1.84 ± 0.13 217 2.15 ± 0.20 134 1.91 ± 0.14 233 2.02 ± 0.17 150 2.00 ± 0.17 213 1.89 ± 0.14 168
NGC 1566 1.47 ± 0.09 586 1.86 ± 0.14 407 1.52 ± 0.08 644 1.71 ± 0.10 383 1.70 ± 0.10 506 1.48 ± 0.09 513
NGC 3627 1.48 ± 0.09 320 1.70 ± 0.10 282 1.51 ± 0.08 350 1.65 ± 0.09 307 1.80 ± 0.12 259 1.45 ± 0.08 371
NGC 1433 2.01 ± 0.17 203 1.92 ± 0.15 204 2.40 ± 0.25 182 1.74 ± 0.11 217
NGC 1365 1.60 ± 0.08 111 1.89 ± 0.14 182 1.77 ± 0.12 146 1.71 ± 0.10 200 2.17 ± 0.20 119 1.61 ± 0.08 226

Notes. The table reports the galaxy name (Col. 1) and the LF slope and the number of H II regions involved in the LF fit for the H II region subsamples in spiral arms areas (Cols. 2–3), in inter-arms areas (Cols. 4–5), in the inner star-forming disk (Cols. 6–7), in the outer star-forming disk (Cols. 8–9), with low ionization parameter (Cols. 10–11), and with high ionization parameter (Cols. 12–13).

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