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 |
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30 ± 6 |
2 | hiz_z1_195 | COSMOS | 10 00 34.63 | +02 14 29.5 | 0.856 | 9.75 ± 0.09 | 8.0 | 49 |
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26 ± 5 |
3 | hiz_z1_258 | COSMOS | 10 01 05.65 | +01 52 57.6 | 0.838 | 10.41 ± 0.11 | 1.61 | 54 |
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19 ± 7 |
4 | u3_5138† | UDS | 02 16 59.89 | –05 15 07.6 | 0.809 | 9.74 ± 0.12 | 3.3 | 62 |
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26 ± 6 |
5 | u3_14150† | UDS | 02 16 58.00 | –05 12 42.6 | 0.896 | 10.11 ± 0.14 | 21.8 | 50 |
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27 ± 5 |
6 | u3_25160† | UDS | 02 17 04.69 | –05 09 46.4 | 0.897 | 10.05 ± 0.15 | 9.3 | 53 |
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23 ± 3 |
7 | zcos_z1_192 | COSMOS | 10 01 03.45 | +01 54 00.4 | 0.917 | 10.17 ± 0.05 | 5.31 | 45 |
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35 ± 5 |
8 | zcos_z1_202 | COSMOS | 10 00 53.39 | +01 52 40.8 | 0.841 | 10.54 ± 0.06 | 8.21 | 45 |
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39 ± 6 |
9 | zcos_z1_690 | COSMOS | 10 00 36.54 | +02 13 09.5 | 0.927 | 10.59 ± 0.25 | 45.6 | 50 |
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38 ± 6 |
10 | zcos_z1_692 | COSMOS | 10 00 36.42 | +02 11 19.2 | 0.930 | 10.61 ± 0.18 | 58.4 | 42 |
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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 |
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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 |
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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 |
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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 |
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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 |
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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 |
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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 |
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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 |
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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.
SFR from Hα integrated flux (Kennicutt 1998).
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