Open Access

Table D.1.

Sample of high-z candidate blazars.

Object RA DEC Date E(B-V) Ref(z)
4FGLJ0038.1+0012 00:38:08.48 00:13:36.5 2017-12-28 0.02 1,2
4FGLJ0047.0+5657 00:47:00.40 56:57:42.0 2022-09-20 0.3 3
4FGLJ0050.7-0929 00:50:41.3 -09:29:05.0 2022-09-20 0.03 3
4FGLJ0124.8-0625 01:24:50.48 -06:25:00.9 2018-12-05 0.04 3
4FGLJ0148.6+0127 01:48:33.8 01:29:01.0 2018-12-14 0.02 3
4FGLJ0153.9+0823 01:54:02.77 08:23:51.1 2022-11-24 0.07 3
4FGLJ0303.6+4716 03:03:35.24 47:16:16.3 2022-11-03 0.22 3
5BZBJ0407+0742 04:07:29.09 07:42:07.5 2017-12-20 0.23 4
4FGLJ0434.1-2014 04:34:07.91 -20:15:17.1 2018-11-04 0.04 3
4FGLJ0501.0+2424 05:01:06.86 24:23:16.4 2022-11-28 0.44 5
5BZBJ0508+8432 05:08:42.36 84:32:04.5 2017-12-20 0.09 6,7
4FGLJ0525.8-0052 05:25:54.63 -00:51:40.4 2023-12-10 0.15 8
4FGLJ0629.3-1959 06:29:23.76 -19:59:19.7 2018-11-10 0.21 3
4FGLJ0706.8+7742 07:06:51.33 77:41:37.0 2022-11-28 0.04 3
5BZBJ0726+3734 07:26:59.52 37:34:23.0 2018-11-04 0.05 2,9
4FGLJ0733.7+4110 07:33:46.8 41:11:20.0 2019-03-09 0.05 2,10
4FGLJ0753.0+5353 07:53:01.38 53:52:59.6 2022-11-30 0.04 3
4FGLJ0754.4-1148 07:54:26.4 -11:47:16.9 2022-12-01 0.17 3
4FGLJ0800.9+4401 08:01:08.28 44:01:10.2 2023-03-22 0.04 2,3
5BZBJ0801+1336 08:01:15.05 13:36:42.6 2017-12-20 0.03 2,6
5BZBJ0823+2223 08:23:24.76 22:23:03.4 2017-12-13 0.04 11
5BZBJ0839+0319 08:39:49.25 03:19:54.2 2017-12-19/20 0.02 12
4FGLJ0849.5+0456 08:49:32.55 04:55:07.9 2023-12-10 0.06 2
4FGLJ0902.4+2051 09:02:26.91 20:50:46.4 2024-01-18 0.03 2
4FGLJ0921.7+2336 09:21:45.38 23:35:48.2 2023-03-22 0.03 2
5BZBJ0926+5411 09:26:38.8 54:11:26.5 2017-12-18 0.02 2
4FGLJ1007.0+3455 10:06:56.47 34:54:45.1 2019-04-09 0.01 2,6
4FGLJ1054.5+2211 10:54:30.56 22:10:55.5 2023-01-25 0.01 2,3
5BZBJ1107+5010 11:07:04.8 50:10:38.0 2019-03-27 0.02 2
4FGLJ1110.5-1836 11:10:27.69 -18:35:51.2 2024-01-16 0.04 3,13
5BZBJ1132+0034 11:32:45.61 00:34:27.8 2018-01-16 0.02 2
4FGLJ1151.5-1347 11:51:30.00 -13:47:51.0 2019-04-02 0.04 2
4FGLJ1155.8+6137 11:55:48.40 61:35:54.0 2023-01-27 0.03 2,8
4FGLJ1215.1+5002 12:15:00.80 50:02:16.0 2023-02-20 0.02 3, 8
4FGLJ1302.8+5748 13:02:52.47 57:48:37.6 2023-03-27 0.01 14
4FGLJ1303.0+2434 13:03:03.21 24:33:55.7 2018-03-16 0.02 15
5BZBJ1312-2156 13:12:31.55 -21:56:23.4 2023-03-24 0.10 3,16
5BZBJ1423+1412 14:23:30.66 14:12:47.8 2018-03-26 0.02 2
5BZBJ1437+4717 14:37:16.14 47:17:26.3 2018-03-26 0.02 2
5BZBJ1438+1204 14:38:25.55 12:04:18.9 2018-04-29 0.02 2
4FGLJ1500.7+4752 15:00:48.65 47:51:15.5 2023-03-28 0.02 14
4FGLJ1503.3+1651 15:03:16.60 16:51:17.0 2020-05-11 0.04 2
4FGLJ1509.7+5556 15:09:48.00 55:56:17.0 2023-07-19 0.01 3
4FGLJ1529.2+3812 15:29:13.60 38:12:18.0 2023-07-21 0.01 2
4FGLJ1530.9+5736 15:30:58.20 57:36:25.0 2023-02-20 0.01 2
4FGLJ1549.6+1710 15:49:29.30 17:08:28.0 2020-05-10 0.03 2
5BZBJ1555+2141 15:55:00.50 21:41:59.7 2018-04-29 0.05 2
4FGLJ1559.9+2319 15:59:52.20 23:16:56.8 2023-04-25 0.05 2
4FGLJ1630.7+5221 16:30:43.10 52:21:38.0 2022-10-01 0.02 3
4FGLJ1824.1+5651 18:24:07.06 56:51:01.5 2018-08-07 0.05 18
5BZBJ2134-0153 21:34:10.31 -01:53:17.2 2018-10-18 0.05 19
4FGLJ2145.5+1006 21:45:30.20 10:06:05.0 2022-10-03 0.06 2
4FGLJ2152.5+1737 21:52:24.81 17:34:37.7 2018-08-30 0.09 3
4FGLJ2206.8-0032 22:06:43.28 -00:31:02.4 2018-11-26 0.10 3
5BZBJ2339+0534 23:39:07.39 05:34:26.2 2018-09-29 0.07 17

Notes. Column 1: Object name; Column 2: Right ascension; Column 3: Declination; Column 4: Date of observation; Column 5 : UT of the start of the observation ;Column 6: E(B-V) from the NASA/IPAC Infrared Science Archive (https://irsa.ipac.caltech.edu/applications/DUST/); Column 7: Reference of the redshift reported in literature : (1) Sandrinelli et al. (2013); (2) Sloan Digital Sky Survey (SDSS-DR7 or DR16); (3) Shaw et al. (2013); (4) Sowards-Emmerd et al. (2003); (5) Sheng et al. (2024); (6) Roma-BZCAT Massaro et al. (2015); (7) Stocke & Rector (1997); (8) 4LAC Ajello et al. (2020); (9) Landoni et al. (2018); (10) Plotkin et al. (2010, 2011); (11) Stickel et al. (1993); (12) Drinkwater et al. (1997); (13) Rajagopal et al. (2020); (14) NASA/IPAC Extragalactic Database (NED); (15) Glikman et al. (2007); (16) Blades et al. (1980); (17) Rector et al. (2000); (18) Lawrence et al. (1996); (19) Sbarufatti et al. (2006).

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