Table 1.
Properties of the SFGss selected in the MXDF.
ID | z | texp | S/Nmax | log M⋆/M⊙ | SFR | mF775W | n⋆ | i⋆ | B/T | Re⋆ | RAFID |
---|---|---|---|---|---|---|---|---|---|---|---|
(h) | (M⊙ yr−1) | (mag) | (deg) | (kpc) | |||||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
3 | 0.62 | 42 | 15 | 10.08![]() |
2.62![]() |
21.68 | 0.87/0.81 ± 0.06 | 64 ± 5 | 0.04 | 5.61 ± 0.04 | 24 353 |
15 | 0.67 | 136 | 9 | 10.23![]() |
0.99![]() |
23.30 | 0.86/0.74 ± 0.06 | 86 ± 5 | < 0.01 | 5.75 ± 0.03 | 10 345 |
37 | 0.98 | 136 | 61 | 8.87![]() |
0.80![]() |
24.65 | 1.15/0.97 ± 0.08 | 56 ± 5 | < 0.01 | 3.54 ± 0.06 | 9791 |
912 | 0.62 | 136 | 124 | 9.19![]() |
1.29![]() |
22.99 | 0.97/0.93 ± 0.06 | 27 ± 5 | < 0.01 | 1.87 ± 0.01 | 5082 |
919 | 1.10 | 136 | 98 | 9.83![]() |
4.28![]() |
23.23 | 1.54/1.20 ± 0.06 | 28 ± 5 | 0.21 | 3.28 ± 0.03 | 23 037 |
937 | 0.73 | 44 | 18 | 9.35![]() |
1.50![]() |
23.49 | 1.13/0.96 ± 0.06 | 82 ± 5 | 0.16 | 5.39 ± 0.06 | 7734 |
943 | 0.66 | 136 | 32 | 9.28![]() |
1.00![]() |
23.63 | 0.86/0.59 ± 0.06 | 77 ± 5 | < 0.01 | 5.09 ± 0.07 | 22 950 |
982 | 1.10 | 92 | 22 | 9.75![]() |
3.25![]() |
23.95 | 1.47/1.02 ± 0.06 | 70 ± 5 | 0.43 | 4.79 ± 0.05 | 22 509 |
1002 | 0.99 | 47 | 35 | 9.43![]() |
1.18![]() |
24.15 | 1.29/1.05 ± 0.06 | 73 ± 5 | 0.21 | 4.15 ± 0.03 | 25 458 |
Notes. (1) Galaxy MUSE ID from Inami et al. (2017); (2) Redshift; (3) Exposure time (h); (4) Maximum S/N in the brightest [O II] spaxel; (5) Stellar mass M⋆ from SED fitting with MAGPHYS; (6) SFR from SED fitting; (7) F775W magnitude; (8) Sérsic n⋆ from van der Wel et al. (2014) and from our GALF IT fits both on HST/F160W WFC3; (9) Inclination i⋆ from HST/F160W WFC3; (10) B/T ratio at 2 Re from a two component GALF IT fit to HST/F160W; (11) Re in kpc measured from HST/F160W from a single component GALF IT fit to the HST/F160W data; (12) ID in the Rafelski et al. (2015) catalog. The quoted erros are 1σ (68%).
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