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Table B.1.

Mass–luminosity relation from the NOM25 model.

M/M Teff [K] mF150W2 mF322W2 m F 150 W 2 reddened $ m_{\mathrm{F150W2}}^{\mathrm{reddened}} $ m F 322 W 2 reddened $ m_{\mathrm{F322W2}}^{\mathrm{reddened}} $ M/M Teff [K] mF150W2 mF322W2 m F 150 W 2 reddened $ m_{\mathrm{F150W2}}^{\mathrm{reddened}} $ m F 322 W 2 reddened $ m_{\mathrm{F322W2}}^{\mathrm{reddened}} $
0.0835 1326 28.5716 26.6109 28.6539 26.6285 0.1277 3618 22.6685 22.0451 22.7410 22.0663
0.0836 1343 28.5085 26.5738 28.5909 26.5916 0.1372 3674 22.4687 21.8517 22.5412 21.8729
0.0839 1406 28.2747 26.4414 28.3575 26.4592 0.1484 3739 22.2525 21.6417 22.3249 21.6630
0.0839 1428 28.1914 26.3977 28.2745 26.4156 0.1604 3813 22.0333 21.4287 22.1058 21.4501
0.0842 1503 27.9088 26.2544 27.9930 26.2724 0.1729 3874 21.8317 21.2317 21.9042 21.2531
0.0844 1579 27.6186 26.0950 27.7035 26.1132 0.1871 3904 21.6542 21.0575 21.7267 21.0789
0.0844 1609 27.5086 26.0312 27.5937 26.0494 0.2062 3933 21.4502 20.8591 21.5227 20.8806
0.0846 1693 27.2394 25.8559 27.3244 25.8742 0.2284 3961 21.2432 20.6572 21.3157 20.6787
0.0847 1780 26.9732 25.6822 27.0580 25.7007 0.2539 3990 21.0370 20.4557 21.1095 20.4772
0.0849 1864 26.7293 25.5259 26.8141 25.5446 0.2831 4017 20.8320 20.2569 20.9046 20.2784
0.0850 1944 26.5138 25.3814 26.5983 25.4002 0.3170 4047 20.6235 20.0574 20.6961 20.0790
0.0852 2036 26.2801 25.2189 26.3642 25.2378 0.3559 4089 20.3942 19.8395 20.4668 19.8611
0.0854 2108 26.0932 25.0886 26.1770 25.1076 0.3968 4162 20.1166 19.5763 20.1893 19.5979
0.0857 2184 25.9133 24.9337 25.9960 24.9529 0.4309 4258 19.8574 19.3369 19.9303 19.3585
0.0861 2288 25.6578 24.7009 25.7390 24.7205 0.4604 4376 19.6168 19.1223 19.6900 19.1440
0.0864 2357 25.5094 24.5908 25.5903 24.6104 0.4797 4474 19.4566 18.9837 19.5300 19.0053
0.0870 2451 25.3086 24.4470 25.3890 24.4666 0.4853 4506 19.4092 18.9430 19.4827 18.9646
0.0875 2541 25.1170 24.2954 25.1967 24.3151 0.5036 4619 19.2596 18.8168 19.3334 18.8384
0.0881 2622 24.9556 24.1539 25.0344 24.1738 0.5200 4734 19.1294 18.7090 19.2036 18.7307
0.0889 2712 24.7795 23.9945 24.8574 24.0145 0.5350 4845 19.0128 18.6131 19.0873 18.6348
0.0897 2798 24.6034 23.8373 24.6804 23.8575 0.5491 4955 18.9047 18.5244 18.9796 18.5462
0.0907 2882 24.4436 23.6943 24.5199 23.7146 0.5545 4998 18.8643 18.4914 18.9393 18.5131
0.0919 2968 24.2908 23.5560 24.3664 23.5764 0.5677 5107 18.7650 18.4103 18.8403 18.4320
0.0930 3036 24.1605 23.4381 24.2356 23.4586 0.5804 5213 18.6702 18.3326 18.7459 18.3543
0.0946 3116 23.9920 23.2858 24.0665 23.3064 0.5928 5318 18.5765 18.2553 18.6524 18.2770
0.0966 3192 23.8194 23.1285 23.8934 23.1492 0.6052 5422 18.4819 18.1764 18.5581 18.1981
0.0993 3268 23.6395 22.9628 23.7130 22.9837 0.6176 5522 18.3850 18.0942 18.4614 18.1159
0.1028 3344 23.4515 22.7879 23.5247 22.8088 0.6299 5621 18.2853 18.0086 18.3619 18.0304
0.1073 3418 23.2567 22.6049 23.3296 22.6259 0.6425 5720 18.1813 17.9185 18.2582 17.9402
0.1129 3490 23.0610 22.4192 23.1338 22.4403 0.6551 5818 18.0719 17.8223 18.1490 17.8441
0.1196 3556 22.8667 22.2345 22.9393 22.2557 0.6680 5915 17.9547 17.7177 18.0319 17.7395

Notes. The table lists stellar masses, effective temperatures, and magnitudes in the F150W2 and F322W2 filters, both with and without reddening corrections.

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