Open Access

Table A.1.

Summary of the MUSE observations of the 59 additional faint quasars sample, which is first presented in this work.

ID Name RA Dec Mi (z = 2)(a) SeeingLyα SB limit(b) Sky Av(c)
[J2000] [J2000] [mag] [arcsec] [10−18 cgs] Conditions(d) [mag]
62 J0203-0443 02:03:57.00 -04:43:10.2 -24.6 0.69 2.28 PH 0.08
63 J0229-0029 02:29:56.55 -00:29:53.9 -26.1 2.02 2.26 CL 0.10
64 J0159-0032 01:59:45.45 -00:32:28.4 -24.7 0.77 2.28 CL 0.08
65 J0829+1426 08:29:39.91 +14:26:25.7 -25.0 1.08 2.33 PH 0.14
66 J0200-0606 02:00:12.60 -06:06:15 -27.0 0.58 1.81 CL 0.09
67 J0247-0023 02:47:46.86 -00:23:53.4 -26.9 0.71 1.94 PH 0.13
68 J0809+0643 08:09:49.16 +06:43:10.8 -24.5 0.93 1.85 CL 0.08
69 J0834+1012 08:34:15.33 +10:12:31.2 -25.4 0.83 2.06 PH 0.11
70 J0923+0011 09:23:00.29 +00:11:56.7 -24.8 0.86 1.89 PH 0.08
71 J0823+0531 08:23:07.22 +05:31:35.4 -26.2 0.97 1.97 CL 0.08
72 J0227-0113 02:27:21.91 -01:13:24.6 -24.1 0.93 2.04 PH 0.11
73 J1038+0919 10:38:40.81 +09:19:14.3 -25.0 1.40 2.17 CL 0.08
74 J0203-0153 02:03:33.76 -01:53:08.4 -25.6 1.52 1.92 PH 0.09
75 J0210-0945 02:10:03.52 -09:45:20.5 -26.0 0.79 2.37 TN 0.08
76 J0155-0732 01:55:25.44 -07:32:16.3 -26.6 1.08 1.97 PH 0.07
77 J0151+0023 01:51:25.83 +00:23:32.7 -24.4 0.77 2.00 PH 0.10
78 J0030+0047 00:30:42.91 +00:47:43.3 -24.0 0.91 2.82 TN 0.08
79 J0148-0055 01:48:09.00 -00:55:08.8 -24.4 0.78 1.87 PH 0.11
80 J0017+0316 00:17:44.80 +03:16:06.1 -26.9 0.87 2.31 CL 0.09
81 J0925+0344 09:25:41.80 +03:44:37.0 -25.2 0.96 2.26 CL 0.10
82 J0125-0005 01:25:29.50 -00:05:13.5 -24.1 1.23 4.75 TN 0.10
83 J0843+1916 08:43:19.90 +19:16:28.8 -24.8 1.15 2.29 CL 0.09
84 J0752+1244 07:52:54.22 +12:44:51.5 -25.1 0.94 2.26 PH 0.09
85 J0018-0026 00:18:17.73 -00:26:59.0 -26.2 0.88 2.00 TN 0.08
86 J0747+1429 07:47:14.29 +14:29:54.3 -26.5 1.59 1.93 CL 0.11
87 J0245-0036 02:45:23.32 -00:36:19.0 -24.9 1.00 1.82 CL 0.09
88 J0801+0534 08:01:30.16 +05:34:37.0 -25.7 1.15 2.07 CL 0.07
89 J0840+0141 08:40:58.35 +01:41:45.0 -26.0 1.15 1.73 CL 0.17
90 J1016+0833 10:16:25.72 +08:33:09.8 -25.2 0.97 2.50 CL 0.11
91 J0159+0025 01:59:22.99 +00:25:30.8 -24.3 0.69 2.28 PH 0.09
92 J0234-0044 02:34:41.17 -00:44:43.7 -24.4 1.00 2.10 PH 0.08
93 J0243-0038 02:43:00.58 -00:38:18.0 -24.5 0.86 1.98 PH 0.09
94 J0140-0202 01:40:20.33 -02:02:43.0 -25.5 0.78 1.94 PH 0.09
95 J0252-0333 02:52:42.99 -03:33:39.4 -25.8 0.95 2.27 PH 0.11
96 J0939+0451 09:39:29.36 +04:51:47.4 -25.1 0.74 2.13 PH 0.15
97 J0208-0922 02:08:02.86 -09:22:43.0 -26.8 1.00 1.92 PH 0.07
98 J0212-0602 02:12:48.13 -06:02:16.9 -25.7 1.00 2.15 CL 0.07
99 J1205+1059 12:05:12.55 +10:59:34.6 -24.5 2.11 2.22 CL 0.07
100 J1001-0007 10:01:22.20 -00:07:52.7 -25.3 0.80 2.41 TN 0.11
101 J1145-0209 11:45:19.45 -02:09:43.9 -25.9 0.98 2.05 CL 0.06
102 J1057+0804 10:57:37.23 +08:04:11.2 -26.1 0.79 2.20 CL 0.09
103 J1244-0027 12:44:08.39 -00:27:26.1 -26.0 1.31 2.27 CL 0.07
104 J1216+0454 12:16:29.25 +04:54:34.8 -25.7 1.67 1.93 CL 0.06
105 J1048+0449 10:48:04.72 +04:49:00.3 -24.8 1.34 2.03 CL 0.09
106 J0920-0048 09:20:56.50 -00:48:07.0 -25.8 0.86 1.65 PH 0.10
107 J0223-0309 02:23:04.27 -03:09:51.5 -25.3 0.97 1.91 PH 0.08
108 J1301-0020 13:01:12.26 -00:20:48.9 -26.5 1.00 2.10 PH 0.07
109 J0823+0340 08:23:25.59 +03:40:59.4 -26.7 1.00 2.03 CL 0.10
110 J0832+0450 08:32:20.15 +04:50:28.3 -25.5 0.95 2.00 CL 0.09
111 J1022+0418 10:22:25.90 +04:18:24.2 -26.4 1.01 2.11 PH 0.08
112 J1101+0314 11:01:05.12 +03:14:03.9 -26.3 1.67 2.09 CL 0.17
113 J0207-0306 02:07:16.83 -03:06:48.4 -25.9 1.02 2.43 CL 0.08
114 J1200+1528 12:00:26.16 +15:28:16.1 -25.4 0.96 1.87 CL 0.16
115 J0252-0057 02:52:53.28 -00:57:28.0 -24.4 0.67 2.07 PH 0.20
116 J0840+0636 08:40:26.81 +06:36:32.8 -26.3 1.06 2.08 CL 0.09
117 J1244+0327 12:44:06.42 +03:27:43.2 -24.7 1.27 1.86 CL 0.11
118 J1153-0141 11:53:02.24 -01:41:13.2 -26.4 1.11 1.94 CL 0.07
119 J1019+0845 10:19:17.81 +08:45:50.0 -26.1 0.81 2.03 CL 0.10
120 UM670-field 01:17:22.24 -08:41:43.5 -23.6 0.80 2.22 CL 0.12

Notes.

(a)

Absolute i−band magnitude normalized to z = 2 following Ross et al. (2013).

(b)

1σ SB limit within 1 arcsec2 and a 30 Å narrow band centered at the observed Lyα wavelength in units of 10−18 erg s−1 cm−2 arcsec−2.

(c)

Galactic v-band extinction from Schlegel et al. (1998).

(d)

Sky conditions during the observations as described in the ESO observational log: PH-photometric; CL-clear; TN-thin cirrus.

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