Table 1

Galaxy sample global properties.

Field ID z F814W/F850LP R e i log10(M) log10(SFR) Morphology – Notes
(mag) (arcsec) (°) (M) (M yr-1)
(1) (2) (3) (4) (5) (6) (7) (8) (9)

HDFS 1 0.17 21.22 0.87 75.0 8.78±0.42 –1.01±0.67
HDFS 3 0.56 21.52 1.34 16.0 9.66±0.14 0.24±0.37 Spirals – clumpy
HDFS 4 0.56 21.78 1.38 75.0 9.86±0.17 0.54±0.35 Weak spirals
HDFS 5 0.58 21.97 0.37 68.0 9.82±0.17 0.59±0.38 Compact – Nucleus – weak spirals
HDFS 6 0.42 21.98 0.60 29.0 9.23±0.10 –0.61±0.50 Spirals – bar
HDFS 7 0.46 21.99 0.73 41.0 9.31±0.12 –0.51±0.54 Clumps – Spirals?
HDFS 8 0.58 22.08 0.30 61.0 9.88±0.23 1.38±0.58 Satellite
HDFS 9 0.56 22.08 0.42 61.0 9.31±0.20 0.8±0.41 Compact
HDFS 11 0.58 22.72 0.17 62.0 9.22±0.18 0.08±0.49 Compact
HDFS 12 0.67 22.79 0.09 37.0 9.02±0.27 0.82±0.67 Compact – “jet”
UDF-10 1 0.62 20.13 1.26 27.0 10.44 0.86 Grand design spiral
UDF-10 2 0.42 20.72 0.54 34.0 9.82 0.21 Asym. spiral – bar – merger?
UDF-10 3 0.62 21.42 0.75 61.0 9.92 0.29 Asym. spiral – merger?
UDF-10 4 0.76 21.48 0.72 50.0 9.97 0.83 Asym. spiral – Clump – merger?
UDF-10 5 0.62 21.25 0.36 49.0 10.66 0.06 Early-type disk-like
UDF-10 7 0.62 21.91 0.66 50.0 9.33 0.44 Asym. spiral – bar
UDF-10 10 0.27 22.49 0.45 57.0 8.3 –0.72 Stellar stream – satellite

Notes. Properties of the sample of galaxies with spatially resolved continuum: (1) MUSE data sets. (2)–(3) Galaxy ID number, and redshift, from Bacon et al. (2015) and I17–Paper II catalogues. (3)–(4) Apparent magnitude I814W (HDFS) and I850LP (udf-10). (5) Effective radii from Casertano et al. (2000, HDFS) and I17–Paper II (udf-10). (6) Galaxy inclination from C16 (HDFS) and I17–Paper II (udf-10). (7)–(8) Stellar mass and SFR measured in C16 (HDFS) and I17–Paper II (udf-10). (9) Morphological properties from HST images.

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