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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 1012Lv, ⊙ −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) 1011Lv, ⊙ −3.9 ± 0.8 0.17 −12.4 −3.1 ± 1.6 0.16 49.7 −7.2 ± 7.1 0.20
1010Lv, ⊙ −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 1012Lv, ⊙ 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) 1011Lv, ⊙ 24.3 ± 6.3 0.20 6.2 19.9 ± 8.0 0.20 12.4 20.8 ± 10.8 0.26
1010Lv, ⊙ 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 1012Lv, ⊙ 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) 1011Lv, ⊙ 132.6 ± 14.7 0.17 136.5 123.9 ± 8.5 0.24
1010Lv, ⊙

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 1011Lv, ⊙ 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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