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Table 1.

Physical properties of the detected CEN.

Lyα CIV
λCEN [Å] (a) 5543.8 ± 1.8 7064.7 ± 1.8
zCEN(b) 3.560 ± 0.002 3.559 ± 0.001
Size [kpc] (c) 150 75
Spectral width [Å] (d) 95 42
[kpc] (e) 10.4 ± 3.7 ( ⋆ ) 15.1 ± 3.7 ( ⋆ )
[kpc] (f) 5.7 ± 3.7 ( ⋆ ) 13.7 ± 3.7 ( ⋆ )
α(g) 0.72 0.62
ϕ [degree] (h) 62 11
Flux [×10−16 erg s−1 cm−2] (i) 17.8 ± 0.1 0.77 ± 0.03
Luminosity [×1043 erg s−1] (j) 20.55 ± 0.16 1.00 ± 0.03
[km s−1] (k) 770 ± 2 352 ± 7
[km s−1] (l) 560 ± 15 455 ± 55

Notes.

(a)

Line peak wavelength from the Gaussian modelling of Lyα- and CIV-CEN spectrum.

(b)

Redshift of the CEN corresponding to λCEN. We used as Lyα and CIV λ rest-frame 1215.67 Å and 1549.48 Å, respectively.

(c)

Maximum projected physical size derived from the 3D-mask.

(d)

Spectral width within which the CEN was detected (from 3D-mask).

(e)

Distance from the quasar position to the SB peak of the CEN.

(f)

Distance from the quasar position to the flux weighted centroid of the CEN.

(g)

Asymmetry parameter, i.e. the ratio between the semi-minor and semi-major axis of the SB map.

(h)

Position angle east of north of the major axis of the SB map.

(i)

Total flux derived from the SB maps (Figs. 1 and 4).

(j)

Total CEN luminosity.

(k)

Averaged velocity dispersion measured from the S/N ≥ 3 velocity dispersion maps (see Sect. 4.3) of the Lyα and CIV.

(l)

Velocity dispersions derived from the Gaussian fit of the total Lyα- and CIV-CEN spectrum.

( ⋆ )Errors according to the spatial resolution of MUSE data.

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