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Table 1

VHE BL Lac sample.

Source name RA Dec Dataa F( > 200 GeV) / 10-11 b Ref. z Ref. SED typec
[years] [Ph / cm2/ s]
1ES 0033+595 0:35:53 59:50:05 5 0.32 Alek15a > 0.24 d Sbaru05 HSP
RGB 0136+391 1:36:33 39:06:03 5 ? > 0.41 d Nil12 HSP
3C 66A 2:22:40 43:02:08 6 2.50 Abdo11 > 0.335 e Furn13A ISP
1ES 0229+200 2:32:49 20:17:18 6 0.46 Aha07 0.139 FK99 (HSP)
HB89 0317+185 3:19:52 18:45:34 5 0.24 Aliu12b 0.190 2LAC HSP
1ES 0414+009 4:16:52 1:05:24 5 0.19 Abram12 0.287 2LAC HSP
1ES 0502+675 5:07:56 67:37:24 5 2.55 Majum11 0.340 Shaw13 HSP
VER J0521+211 5:21:55 21:11:24 2.1 7.08 Archam13 0.108 Shaw13 ISP
VER J0648+151 6:48:48 15:16:25 2.1 0.75 Aliu11 0.179 Aliu11 HSP
1ES 0647+250 6:50:46 25:03:00 6 ? 0.410 Kot11 HSP
S5 0716+714 7:21:53 71:20:36 6 4.10 Ander09 0.31 Nil08 ISP
1ES 0806+524 8:09:49 52:18:58 6 2.45 Alek15b 0.137 2LAC HSP
RGB 0847+115 8:47:13 11:33:50 3.2 0.57 Mirz14a 0.198 Plot10 HSP
1ES 1011+496 10:15:04 49:26:01 5.4 23.0 Ahnen16a 0.212 Alb07b HSP
Mkn 421 11:04:27 38:12:32 6 232.65 Cort13 0.031 2LAC HSP
Mkn 180 11:36:26 70:09:27 6 2.25 Alb06a 0.046 2LAC HSP
RGB 1136+676 11:36:30 67:37:04 3.8 0.34 Mirz14c 0.134 Plot10 HSP
ON 325 12:17:52 30:07:01 6 0.77 Alek12a 0.130 2LAC HSP
1ES 1218+304 12:21:22 30:10:37 5 5.52 Accia10 0.184 2LAC HSP
ON 231 12:21:32 28:13:59 6 6.22 Accia09 0.103 2LAC ISP
PG 1424+240 14:27:00 23:48:00 5 0.53 Alek14a > 0.604 e Furn13b HSP
1ES 1426+428 14:28:33 42:40:21 6 66.21 Horan02 0.129 Laur98 HSP
PG 1553+113 15:55:43 11:11:24 5 4.44 Aliu15 > 0.395 f Danf10 HSP
Mkn 501 16:53:52 39:45:37 5 98.06 Aha99 0.034 2LAC HSP
H 1722+119 17:25:04 11:52:15 6 0.33 Ahnen16b >0.17 d Sbaru06 HSP
1ES 1727+502 17:28:19 50:13:10 6 0.26 Archam15 0.055 oke HSP
1ES 1741+196 17:43:58 19:35:09 6 0.19 Berg11 0.083 heidt HSP
1ES 1959+650 20:00:00 65:08:55 6 48.89 Krawc04 0.047 2LAC HSP
MAGIC J2001+439 20:01:14 43:53:03 3.4 1.80 Alek14b 0.190 Alek14b ISP
BL Lacertae 22:02:43 42:16:40 5 34.00 Arlen13 0.069 2LAC ISP∗
B3 2247+381 22:50:06 38:24:37 5 0.50 Alek12b 0.119 Laur98 HSP
1ES 2344+514 23:47:05 51:42:18 6 13.91 Accia11 0.044 2LAC HSP

Notes.

(a)

The length of the period of optical and radio data used for the analysis.

(b)

Highest flux reported in the literature, the fluxes have been converted to >200 GeV for easier comparison.

(c)

HSP = High synchrotron peak frequency source, ISP = Intermediate synchrotron peak frequency source. From Ackermann et al. (2011) except for 1ES 0229+200, which is not included in 2LAC.

(d)

Lower limit based on non-detection of the host.

(e)

Lower limit based on Lyα.

(f)

Lower limit based on a confirmed Lyα + Ovi absorber.

(*)

In many other catalogues classified as LSP = Low synchrotron peak frequency source.

(?)

The flux density has not been reported even if the detection has been announced.

Reference. Aleksić et al. (2015a); Abdo et al. (2011); Aharonian et al. (2007b); Aliu et al. (2012b); Abramowski et al. (2012); Majumdar (2011); Archambault et al. (2013); Aliu et al. (2011); Anderhub et al. (2009); Aleksić et al. (2015b); Mirzoyan (2014a); Ahnen et al. (2016a); Cortina & Holder (2014); Albert et al. (2006); Mirzoyan (2014b); Aleksić et al. (2012a); Acciari et al. (2010); Acciari et al. (2009); Aleksić et al. (2014a); Horan et al. (2002); Aliu et al. (2015)Aharonian et al. (1999); Ahnen et al. (2016b)Archambault et al. (2015); Berger et al. (2011); Krawczynski et al. (2004); Aleksić et al. (2014b); Arlen et al. (2013); Aleksić et al. (2012b); Acciari et al. (2011) (Sbaru05) Sbarufatti et al. (2005); (Nil12) Nilsson et al. (2012); (Furn13A) Furniss et al. (2013a); (FK99) Falomo & Kotilainen (1999); 2LAC Ackermann et al. (2011); (Shaw13) Shaw et al. (2013); (Aliu11) Aliu et al. (2011); (Kot11) Kotilainen et al. (2011); (Nil08) Nilsson et al. (2008); (Plot10) Plotkin et al. (2010); (Alb07b) Albert et al. (2007b); (Furn13b) Furniss et al. (2013b); (Laur98) Laurent-Muehleisen et al. (1998); (Danf10) Danforth et al. (2010); (Sbaru06) Sbarufatti et al. (2006); (oke) Oke (1978); (heidt) Heidt et al. (1999); (Alek14b) Aleksić et al. (2014b).

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