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Table 1

Sample of 18 disc galaxies at z ~ 1 analysed in this work.

# Name Field RA (J2000) Dec (J2000) z Log M/M SFR i V flat σHα
hms ° ′′ M/ yr ° km s-1 km s-1
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)

1 gs3_22005 GOODS-S 03 32 29.85 –27 45 20.5 0.954 10.72 ± 0.12 33.4 47 30 ± 6
2 hiz_z1_195 COSMOS 10 00 34.63 +02 14 29.5 0.856 9.75 ± 0.09 8.0 49 26 ± 5
3 hiz_z1_258 COSMOS 10 01 05.65 +01 52 57.6 0.838 10.41 ± 0.11 1.61 54 19 ± 7
4 u3_5138 UDS 02 16 59.89 –05 15 07.6 0.809 9.74 ± 0.12 3.3 62 26 ± 6
5 u3_14150 UDS 02 16 58.00 –05 12 42.6 0.896 10.11 ± 0.14 21.8 50 27 ± 5
6 u3_25160 UDS 02 17 04.69 –05 09 46.4 0.897 10.05 ± 0.15 9.3 53 23 ± 3
7 zcos_z1_192 COSMOS 10 01 03.45 +01 54 00.4 0.917 10.17 ± 0.05 5.31 45 35 ± 5
8 zcos_z1_202 COSMOS 10 00 53.39 +01 52 40.8 0.841 10.54 ± 0.06 8.21 45 39 ± 6
9 zcos_z1_690 COSMOS 10 00 36.54 +02 13 09.5 0.927 10.59 ± 0.25 45.6 50 38 ± 6
10 zcos_z1_692 COSMOS 10 00 36.42 +02 11 19.2 0.930 10.61 ± 0.18 58.4 42 22 ± 5
11 zmus_z1_21 GOODS-S 03 32 48.48 –27 54 16.0 0.839 10.40 ± 0.14 23.8 32 25 ± 4
12 zmus_z1_86 GOODS-S 03 32 25.19 –27 51 00.1 0.841 9.55 ± 0.08 10.3 51 24 ± 4
13 zmus_z1_119 GOODS-S 03 32 08.20 –27 47 52.1 0.840 10.34 ± 0.07 30.3 62 31 ± 6
14 zmus_z1_125 GOODS-S 03 32 21.76 –27 47 24.6 0.998 9.95 ± 0.06 17.8 58 36 ± 7
15 zmus_z1_129 GOODS-S 03 32 21.76 –27 47 24.6 0.995 9.83 ± 0.07 14.2 34 38 ± 6
16 zmus_z1_166 GOODS-S 03 32 16.49 –27 44 49.1 0.975 10.11 ± 0.15 36.9 51 39 ± 6
17 zmus_z1_217 GOODS-S 03 32 20.51 –27 40 58.9 0.895 10.02 ± 0.08 17.9 70 21 ± 4
18 zmvvd_z1_87 GOODS-S 03 32 05.66 –27 47 49.1 0.896 9.52 ± 0.08 5.6 52 24 ± 4

Notes. (1) Name adopted in the main survey (KROSS or KMOS3D); (2) field; (3)(4) celestial coordinates in J2000; (5) spectroscopic redshift; (6) stellar masses from CANDELS (Santini et al. 2015) or COSMOS/3D-HST (see text); (7) star formation rates from 3D-HST (Whitaker et al. 2014, SFRUV + SFRIR) or derived from integrated Hα flux (lower limits); (8) estimated inclination angle; (9) velocity of the flat part of the rotation curve, defined as specified in Sect. 4, derived in this work; (10) intrinsic Hα velocity dispersion averaged over the entire galaxy disc as derived in this work.

(†)

Galaxies belonging to the KMOS3D survey. Unmarked galaxies belong to the KROSS survey.

(1)

SFR from Hα integrated flux (Kennicutt 1998).

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