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Table 2.

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

Galaxy Slope α log Lmin log Lcompl O7V eq log Lmax log Ltot Ntot NLFfit NDB FWHMseeing
(erg s−1) (erg s−1) (erg s−1) (erg s−1) (pc)
NGC 5068 1.58 ± 0.09 35.92 ± 0.06 35.86 0.06 39.26 40.38 1465 1206 9 26.18
IC 5332 1.82 ± 0.13 36.25 ± 0.19 35.71 0.12 38.62 39.71 612 357 1 37.91
NGC 1087 1.71 ± 0.10 37.49 ± 0.10 36.88 2.04 40.01 41.24 891 439 101 70.38
NGC 1385 1.52 ± 0.08 37.29 ± 0.17 36.68 1.29 40.11 41.47 914 556 157 55.67
NGC 7496 1.69 ± 0.10 37.16 ± 0.09 36.64 0.95 39.70 40.75 547 300 39 80.35
NGC 2835 1.76 ± 0.11 37.08 ± 0.10 36.67 0.78 39.56 40.72 819 432 35 67.90
NGC 0628 1.71 ± 0.10 36.63 ± 0.08 36.24 0.28 39.34 40.87 2230 1273 42 43.77
NGC 3351 1.98 ± 0.16 36.84 ± 0.13 36.06 0.45 38.77 40.14 784 369 3 50.56
NGC 4254 1.61 ± 0.08 37.36 ± 0.12 36.77 1.49 39.93 41.62 2536 1430 333 56.32
NGC 4303 1.56 ± 0.09 37.26 ± 0.15 36.92 1.18 40.03 41.75 2208 1567 353 63.94
NGC 4535 1.63 ± 0.09 36.79 ± 0.09 36.13 0.40 39.87 41.00 1444 934 65 42.63
NGC 1300 1.77 ± 0.12 37.08 ± 0.25 36.26 0.79 39.42 40.84 1169 632 49 81.50
NGC 1512 2.04 ± 0.17 37.41 ± 0.10 36.48 1.71 39.07 40.43 472 209 15 113.51
NGC 1672 1.67 ± 0.10 37.55 ± 0.12 37.03 2.32 40.03 41.40 1051 570 152 89.80
NGC 4321 1.95 ± 0.15 37.95 ± 0.27 36.93 5.82 39.78 41.31 1385 382 111 85.17
NGC 1566 1.57 ± 0.09 37.14 ± 0.14 36.77 0.91 40.53 41.58 1655 1026 186 68.27
NGC 3627 1.57 ± 0.09 37.43 ± 0.23 36.84 1.78 40.10 41.56 1007 657 188 57.44
NGC 1433 1.96 ± 0.16 37.32 ± 0.14 36.20 1.37 39.41 40.69 1258 407 28 81.76
NGC 1365 1.74 ± 0.11 37.82 ± 0.20 37.04 4.31 40.76 41.44 854 347 119 108.51

Notes. The table reports the galaxy name (Col. 1), the LF slope (Col. 2) and Lmin (Col. 3), the LF completeness limit (Col. 4), the number of equivalent O7 V stars corresponding to Lmin (Col. 5), the luminosity of the brightest H II region (Col. 6), the integrated H II regions luminosity (Col. 7), the total number of H II regions (Col. 8), the number of H II regions used to fit the LF slope (Col. 9), the number of “density bounded” H II regions with LHα >  1038.6 erg s−1 (Col. 10), and the physical resolution of the Hα maps used to detect H II regions in parsecs (Col. 11).

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