Table 5.
Photometric position angle (PAp in degrees) and ellipticity (ϵ) measured at 0.6 arcsec from the peak of the full-band images in Figs. 8, B.3, and B.8.
| Z = 0.76 |
Z = 1.50 |
Z = 2.30 |
||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| Host | Host | PAp | ϵ | PAk | PAp | ϵ | PAk | PAp | ϵ | PAk |
| morph. | lum. | (deg) | (deg) | (deg) | (deg) | (deg) | (deg) | |||
HSIM |
−4.3 ± 0.8 | 0.29 | −6.2 | −4.1 ± 0.6 | 0.28 | −6.2 | −4.1 ± 0.6 | 0.29 | −6.2 | |
| Lenticular | 1012 Lv, ⊙ | −4.2 ± 0.2 | 0.17 | −6.2 | −4.3 ± 0.3 | 0.16 | 0.0 | −4.2 ± 0.3 | 0.21 | −6.2 |
| (NGC 809) | 1011 Lv, ⊙ | −3.9 ± 0.8 | 0.17 | −12.4 | −3.1 ± 1.6 | 0.16 | 49.7 | −7.2 ± 7.1 | 0.20 | – |
| 1010 Lv, ⊙ | −5.6 ± 4.4 | 0.19 | – | – | – | – | – | – | – | |
HSIM |
24.4 ± 9.8 | 0.29 | 12.4 | 19.7 ± 10.4 | 0.26 | 12.4 | 20.6 ± 9.7 | 0.27 | 12.4 | |
| Spiral | 1012 Lv, ⊙ | 24.5 ± 6.8 | 0.20 | 12.4 | 20.2 ± 6.5 | 0.20 | 18.6 | 21.1 ± 8.1 | 0.23 | 18.6 |
| (PGC 055442) | 1011 Lv, ⊙ | 24.3 ± 6.3 | 0.20 | 6.2 | 19.9 ± 8.0 | 0.20 | 12.4 | 20.8 ± 10.8 | 0.26 | – |
| 1010 Lv, ⊙ | 22.3 ± 7.4 | 0.19 | – | – | – | – | – | – | – | |
HSIM |
121.1 ± 0.1 | 0.50 | 130.3 | 119.9 ± 1.7 | 0.58 | 130.3 | 121.1 ± 1.1 | 0.54 | 130.3 | |
| Interaction | 1012 Lv, ⊙ | 132.4 ± 11.9 | 0.14 | 124.4 | 119.4 ± 4.7 | 0.25 | 136.5 | 118.1 ± 3.4 | 0.34 | 120.8 |
| (NGC 7119A) | 1011 Lv, ⊙ | 132.6 ± 14.7 | 0.17 | 136.5 | 123.9 ± 8.5 | 0.24 | – | – | – | – |
| 1010 Lv, ⊙ | – | – | – | – | – | – | – | – | – | |
Notes. Uncertainties correspond to the standard deviation of the PAp between 0.5 and 0.7 arcsec from the object centre. In the case of the spiral host, there is a significant variation of the PAp between these two radial distances due to the transition from the bar (PAbar ∼ 45 deg) to the disc (PAdisk ∼ 15 deg; see Appendix A). Uncertainties in ϵ are always less than 0.1. The third column at each redshift corresponds to the estimation of the kinematic position angle (PAk in degrees), with errors always < 6.5°. HSIM
corresponds to the HSIMInput data cube for the host scaled to 1011 Lv, ⊙ in each case. Same results are obtained for the other two host luminosities. For comparison, the photometric and kinematics parameters for the galaxies at z ∼ 0 are in Appendix A.
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