The MUSE view of Lyman-α nebulae in high redshift radio galaxies

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Table 2.

Properties of the brightness profiles.

Object	log L_Lyα	r_h	r_Max,Lyα	r_Radio
	[erg s⁻¹]	[ckpc]	[ckpc]	[ckpc]
NVSS J151020-352803	43.35	^a	57.0	58
TXS 0952-217	43.63	33.6	21.3	^d
TN J1112-2948	43.47	31.8	28.1	83
NVSS J095751-213321	42.32	^b		129
MRC 0251-273	43.73	25.4	16.3	^d
NVSS J094724-210505	42.54	29.4	52.9	46
NVSS J095438-210425	42.77	16.7	15.1	^d
TN J1049-1258	42.98	28.3	10.1^c	92
TN J0924-2201	42.94	^b		10

Notes. Column description: Logarithm of the total Lyα luminosity in erg s⁻¹, scale length of the SBP, maximum extent of the Lyα emission, and maximum size of the radio emission all in ckpc.

^(a)

Due to the double lobe morphology of this source, the exponential fit radius was not derived.

^(b)

These are compact Lyα sources, and no estimate of their size can be derived.

^(c)

The size of the extended red emission region reported in Coloma Puga et al. (2023) is not included in this measurement, as its origin is yet to be clearly ascertained. As such, the size is limited to that traced by the host galaxy emission near the given redshift.

^(d)

Unresolved radio sources.

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