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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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