Table 2.
HzRGs MUSE sample properties.
| HzRG | RA (J2000) (†) | Dec (J2000) (†) | SB limit (*) | LLyα, int(‡) | LLyα, obs(§) |
|---|---|---|---|---|---|
| hh:mm:ss | dd:mm:ss | 10−19 cgs | 1044 erg s−1 | 1044 erg s−1 | |
| MRC 0943-242 | 09:45:32.73 | −24:28:49.65 (a) | 17.0 | 4.7±0.1 | 2.39±0.03 |
| MRC 0316-257 | 03:18:12.07 | −25:35:10.22 (b) | 2.62 | 7.3±1.2 | 1.04±0.04 |
| TN J0205+2242 | 02:05:10.69 | +22:42:50.4 (a)(c) | 13.3 | 8.3±0.4 | 3.82±0.06 |
| TN J0121+1320 | 01:21:42.73 | +13:20:58.0 (a) | 5.64 | 2.0±0.1 | 0.55±0.01 |
| 4C+03.24 | 12:45:38.37 | +03:23:21.0 (d) | 11.5 | 28.8±0.8 | 5.43±0.20 |
| 4C+19.71 | 21:44:07.56 | +19:29:14.6 (a) | 4.77 | 4.3±0.3 | 1.48±0.22 |
| TN J1338–1942 | 13:38:26.10 | −19:42:31.1 (e) | 4.34 | 12.3±0.3 | 5.89±0.10 |
| 4C+04.11 | 03:11:47.97 | +05:08:03.74 (f) | 9.84 | 20.0±0.7 | 2.89±0.07 |
Notes.
The surface brightness limit is the 2σ limit extracted from continuum-source- and Lyα-free regions in a narrow band image. The narrow band image is collapsed from v05 to v95 (see Sect. 4.1). The cgs unit is erg s−1 cm−2 arcsec−2.
Intrinsic Lyα luminosity (i.e. corrected for absorption) of the nebula. It is integrated over the entire area selected in Sect. 3.1 and multiplied with the luminosity distance using the cosmological parameters (Sect. 1).
Observed Lyα luminosity of the nebula integrated over the entire area from v05 to v95 (see text).
References.
Spitzer (Seymour et al. 2007; De Breuck et al. 2010).
Chandra Obs. ID 5734 (PI:Pentericci). Chandra Source Catalogue (Evans et al. 2010).
Radio (De Breuck et al. 2002).
Radio (van Ojik et al. 1996).
Radio (De Breuck et al. 1999).
Radio (Parijskij et al. 2014).
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