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Table 1.
TELAMON sample of TeV-emitting AGN.
| ID | Alternative | Class (a) | Synchr. Peak (b) | Redshift (c) | Synchr. Peak | Redshift |
|---|---|---|---|---|---|---|
| (J2000) | Name | log |
Reference | Reference | ||
| J0035+5950 | 1ES 0033+595 | EHBL | 18.4 | 0.467 | Chang et al. (2019) | Paiano et al. (2017) |
| J0112+2244 | S2 0109+22 | IBL | 14.41 | 0.265 | Zhou et al. (2021a) | Healey et al. (2008) |
| J0136+3906 | RGB J0136+391 | HBL | 16.27 | – | Fan et al. (2016) | – |
| J0152+0146 ( * ) | RGB J0152+017 | HBL | 16.25 | 0.080 | Zhou et al. (2021a) | Laurent-Muehleisen et al. (1998) |
| J0214+5144 ( * ) | TXS 0210+515 | HBL | 17.3 | 0.049 | Chang et al. (2019) | Laurent-Muehleisen et al. (1999) |
| J0221+3556 | S3 0218+35 | FSRQ | 13.98 | 0.954 | Zhou et al. (2021a) | Cohen et al. (2003) |
| J0222+4302 | 3C 66A | HBL | 15.76 | 0.340 | Nieppola et al. (2006) | Torres-Zafra et al. (2018) |
| J0232+2017 ( * ) | 1ES 0229+200 | EHBL | 18.6 | 0.140 | Chang et al. (2019) | Schachter et al. (1993) |
| J0303−2407 | PKS 0301−243 | HBL | 15.8 | 0.263 | Chang et al. (2019) | Pesce et al. (1995) |
| J0316+4119 | IC 310 | RG or HBL | 17 | 0.0190 | Ahnen et al. (2017) | Arp (1968) |
| J0319+1845 | RBS 0413 | HBL | 16.37 | 0.190 | Zhou et al. (2021a) | Gioia et al. (1984) |
| J0416+0105 ( * ) | 1ES 0414+009 | HBL | 16.6 | 0.287 | Chang et al. (2019) | Halpern et al. (1991) |
| J0507+6737 | 1ES 0502+675 | EHBL | 18.0 | 0.340 | Chang et al. (2019) | Shaw et al. (2013) |
| J0509+0541 | TXS 0506+056 | HBL | 15.47 | 0.3365 | Nieppola et al. (2006) | Paiano et al. (2018) |
| J0521+2112 | RGB J0521+212 | HBL | > 15.2 | > 0.18 | Chang et al. (2019) | Paiano et al. (2017) |
| J0648+1516 | RX J0648.7+1516 | HBL | 16.71 | 0.179 | Zhou et al. (2021a) | Aliu et al. (2011) |
| J0650+2502 | 1ES 0647+250 | HBL | 16.8 | 0.41 | Chang et al. (2019) | Kotilainen et al. (2011) |
| J0710+5909 ( * ) | RGB J0710+591 | EHBL | 18.2 | 0.125 | Chang et al. (2019) | Giommi et al. (1991) |
| J0721+7120 | S5 0716+714 | IBL | 14.95 | 0.2304 ( ‡ ) | Zhou et al. (2021a) | Pichel et al. (2023) |
| J0733+5153 ( * ) | PGC 2402248 | EHBL | 17.9 | 0.0650 | Chang et al. (2019) | Becerra González et al. (2020) |
| J0739+0136 | [HB89] 0736+017 | FSRQ | 13.97 | 0.18941 | Zhou et al. (2021a) | Grasha et al. (2019) |
| J0809+5219 | 1ES 0806+524 | HBL | 15.95 | 0.138 | Zhou et al. (2021a) | Bade et al. (1998) |
| J0812+0237 | 1RXS J081201.8+023735 | EHBL | > 17.5 | 0.173 | Ventura et al. (2021) | Paiano et al. (2020) |
| J0847+1133 ( * ) | RBS 0723 | EHBL | 17.9 | 0.198 | Chang et al. (2019) | Cao et al. (1999) |
| J0854+2006 ( † ) | OJ287 | LBL | 13.29 | 0.306 | Zhou et al. (2021a) | Miller et al. (1978) |
| J0913−2103 | MRC 0910−208 | HBL | 17.2 | 0.198 | Chang et al. (2019) | Jones et al. (2009) |
| J0958+6533 | S4 0954+658 | FSRQ | 12.98 | 0.3694 | Zhou et al. (2021a) | Becerra González et al. (2021) |
| J1015+4926 | 1ES 1011+496 | HBL | 16.5 | 0.212 | Chang et al. (2019) | Albert et al. (2007) |
| J1058+2817 | GB6 J1058+2817 | EHBL | 18.47 | 0.254 | Nieppola et al. (2006) | DiPompeo et al. (2015) |
| J1104+3812 ( * ) | Mrk 421 | HBL | 16.3 | 0.0308 | Chang et al. (2019) | Ulrich et al. (1975) |
| J1136+7009 | Mrk 180 | HBL | 16.8 | 0.0458 | Chang et al. (2019) | Ulrich (1978) |
| J1136+6737 ( * ) | RX J1136.5+6737 | EHBL | 18.2 | 0.134 | Chang et al. (2019) | Bade et al. (1994) |
| J1145+1936 | 3C 264 | RG | ∼17 | 0.0216 | Archer et al. (2020) | Ahn et al. (2012) |
| J1159+2914 | 4C+29.45 | FSRQ | 13.05 | 0.724745 | Zhou et al. (2021a) | Albareti et al. (2017) |
| J1217+3007 | ON 325 | HBL | 15.63 | 0.129 | Nieppola et al. (2006) | Paiano et al. (2017) |
| J1221+3010 ( * ) | 1ES 1218+304 | HBL | 16.9 | 0.184 | Chang et al. (2019) | Bade et al. (1998) |
| J1221+2813 | W Comae | IBL | 14.88 | 0.102 | Nieppola et al. (2006) | Weistrop et al. (1985) |
| J1224+2436 | MS 1221.8+2452 | HBL | 15.68 | 0.219 | Zhou et al. (2021a) | Stocke et al. (1991) |
| J1224+2122 | PKS 1222+21 | FSRQ | 13.87 | 0.433826 | Zhou et al. (2021a) | Albareti et al. (2017) |
| J1230+2518 | ON 246 | IBL | 14.75 | 0.555 | Zhou et al. (2021a) | Kunsági-Máté et al. (2022) |
| J1415+1320 | PKS 1413+135 | LBL | 12.96 | 0.334 | Nieppola et al. (2006) | Bilicki et al. (2016) |
| J1422+3223 | OQ 334 | FSRQ | < 15 | 0.682 | MAGIC Collaboration (2021) | Wills & Wills (1974) |
| J1427+2348 | OQ 240 | HBL | 15.9 | 0.605 | Nieppola et al. (2006) | Paiano et al. (2017) |
| J1428+4240 ( * ) | 1ES 1426+428 | EHBL | 18.2 | 0.129 | Chang et al. (2019) | Remillard et al. (1989) |
| J1443+1200 ( * ) | 1ES 1440+122 | EHBL | 17.8 | 0.163 | Chang et al. (2019) | Schachter et al. (1993) |
| J1443+2501 | PKS 1441+25 | FSRQ | 13.39 | 0.939 | Zhou et al. (2021a) | Shaw et al. (2012) |
| J1518−2731 | TXS 1515−273 | HBL | 15.4 | 0.128 | Chang et al. (2019) | Becerra González et al. (2021) |
| J1555+1111 | PG 1553+113 | HBL | 15.6 | 0.028 | Chang et al. (2019) | Zhou et al. (2021b) |
| J1653+3945 ( * ) | Mrk 501 | EHBL | 17.9 | 0.0335 | Chang et al. (2019) | Wills & Wills (1974) |
| J1725+1152 | H 1722+119 | HBL | 16.46 | 0.028 | Zhou et al. (2021a) | Zhou et al. (2021b) |
| J1728+5013 ( * ) | I Zw 187 | HBL | 17.0 | 0.0554 | Chang et al. (2019) | Oke (1978) |
| J1743+1935 ( * ) | 1ES 1741+196 | EHBL | 17.8 | 0.084 | Chang et al. (2019) | Heidt et al. (1999) |
| J1751+0938 | PKS 1749+096 | LBL | 13.23 | 0.32 | Zhou et al. (2021a) | Stickel et al. (1988) |
| J1813+3144 | B2 1811+31 | FSRQ | 15.0 | 0.117 | Chang et al. (2019) | Giommi et al. (1991) |
| J1943+2118 | HESS J1943+213 | EHBL | 18.2 | 0.2 | Chang et al. (2019) | Malik et al. (2022) |
| J1958−3011 | 1RXS J195815.6−301119 | HBL | 17.0 | 0.119 | Chang et al. (2019) | Mauch & Sadler (2007) |
| J1959+6508 ( * ) | 1ES 1959+650 | HBL | 16.9 | 0.0470 | Chang et al. (2019) | Schachter et al. (1993) |
| J2001+4352 | MAGIC J2001+435 | HBL | ∼16 | 0.18 | Aleksić et al. (2014b) | Aleksić et al. (2014b) |
| J2039+5219 ( * ) | 1ES 2037+521 | HBL | 16.2 | 0.053 | Zhou et al. (2021a) | Nilsson et al. (2003) |
| J2056+4940 | RGB J2056+496 | EHBL | 17.6 | – | Chang et al. (2019) | – |
| J2158−3013 | PKS 2155−304 | HBL | 15.4 | 0.116 | Chang et al. (2019) | Falomo et al. (1993) |
| J2202+4216 | BL Lac | LBL | 12.95 | 0.0686 | Zhou et al. (2021a) | Oke & Gunn (1974) |
| J2243+2021 | RGB J2243+203 | HBL | 15.3 | 0.53 | Chang et al. (2019) | Rosa González et al. (2019) |
| J2250+3825 | B3 2247+381 | HBL | 16.33 | 0.119 | Zhou et al. (2021a) | Laurent-Muehleisen et al. (1998) |
| J2347+5142 ( * ) | 1ES 2344+514 | EHBL | 17.7 | 0.044 | Chang et al. (2019) | Perlman et al. (1996) |
Notes.
(a)
The classification into EHBL, HBL, IBL and LBL is performed according to the synchrotron peak frequency found in the literature.
(b)
Synchrotron peak frequency in the source rest frame, i.e., νpeak, rest = νpeak, obs(1 + z). Already corrected values from the literature were adjusted to the redshift values in this work.
(c)
For some sources no conclusive redshift value is available in the literature. See also Foschini et al. (2022) for a more detailed collection of redshifts for most sources including information about their reliability.
( * )Sources overlapping with Biteau et al. (2020).
( † )Observations are coordinated with the MOMO program (Komossa et al. 2023).
( ‡ )The adopted redshift is a statistical estimate, which may deviate from the z = 0.31, previously suggested based on marginal detection of the host galaxy by Nilsson et al. (2008).
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