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Table 3

Multiwavelength properties of the studied BL Lac objects.

Object Distance L Optical L Radio L Fermi ΓHE
[Mpc] [erg s-1] [erg s-1] [erg s-1]
(1) (2) (3) (4) (5) (6)

SHBL J001355.9–185406 413 (1.5 ± 0.3) × 1044
PKS 0048–097 3659 (1.0 ± 0.5) × 1046 (2.3 ± 0.5) × 1044 (6.9 ± 1.4) × 1046 2.14 ± 0.04
RGB J0152+017 660 (6.2 ± 1.3) × 1044 (5.0 ± 1.5) × 1044 1.79 ± 0.14
1ES 0229+200 632 (2.5 ± 0.5) × 1044 (2.5 ± 0.5) × 1040
AO 0235+16 5967 (2.2 ± 2.0) × 1046 (1.2 ± 0.2) × 1045 (7.7 ± 1.6) × 1047 2.02 ± 0.03
PKS 0301–243 1268 (3.0 ± 0.8) × 1045 (1.5 ± 0.3) × 1046 1.94 ± 0.03
HBL J032541.0–164618 1444 (1.1 ± 0.4) × 1045
1ES 0323+022 668 (1.8 ± 0.4) × 1044 (2.9 ± 0.6) × 1041 (7.7 ± 1.9) × 1044 2.06 ± 0.09
1ES 0347–121 788 (1.9 ± 0.5) × 1044 (1.0 ± 0.2) × 1041
1ES 0414+00.9 1260 (1.0 ± 0.2) × 1045 (1.7 ± 0.3) × 1042 (1.5 ± 0.4) × 1045 1.99 ± 0.16
PKS 0447–439 476 (1.1 ± 0.3) × 1045 (3.7 ± 0.8) × 1045 1.86 ± 0.02
PKS 0537–441 5613 (4.9 ± 3.3) × 1046 (1.4 ± 0.3) × 1048 2.01 ± 0.02
PKS 0548–322 299 (9.5 ± 1.9) × 1043
PKS B0735+178 2256 (4.0 ± 1.3) × 1045 (6.8 ± 1.4) × 1043 (3.5 ± 0.7) × 1046 2.05 ± 0.04
OJ 287 1537 (7.9 ± 3.6) × 1045 (2.0 ± 0.4) × 1044 (1.2 ± 0.2) × 1046 2.23 ± 0.04
HBL J101015.9–311908 655 (3.7 ± 0.8) × 1044
1ES 1101–232 877 (4.4 ± 0.9) × 1044
Mrk 421 85.15 ± 67.67 (0.9 ± 0.8) × 1044 (0.8 ± 0.6) × 1041 (3.3 ± 3.2) × 1044 1.771 ± 0.012
1ES 1218+304 594.00 ± 206.48 (3.8 ± 2.8) × 1044 (2.9 ± 2.0) × 1041 (1.6 ± 1.1) × 1045 1.71 ± 0.07
W Comae 517 (7.0 ± 2.6) × 1044 (2.0 ± 0.4) × 1042
1ES 1312–423 485 (1.1 ± 0.2) × 1044
PKS 1424+240 882 (4.0 ± 0.9) × 1045 (4.1 ± 0.8) × 1042 (1.4 ± 0.3) × 1046 1.78 ± 0.02
AP Lib 243 (2.0 ± 0.4) × 1044 (4.1 ± 0.9) × 1044 2.06 ± 0.04
PG 1553+113 1090.00 ± 127.28 (9.2 ± 3.0) × 1045 (3.8 ± 0.9) × 1042 (2.8 ± 0.7) × 1046 1.67 ± 0.02
Mrk 501 119 (1.0 ± 0.2) × 1044 (2.9 ± 0.6) × 1041 (1.9 ± 0.4) × 1044 1.74 ± 0.03
RGB J1725+118 74.6 (1.2 ± 0.3) × 1043 (6.0 ± 1.2) × 1039
PKS 2005–489 351.50 ± 51.62 (1.3 ± 0.5) × 1045 (7.1 ± 2.2) × 1044 1.78 ± 0.05
HBL J213135.4–091523 2405 (1.1 ± 0.3) × 1045
PKS 2155–304 492 (2.8 ± 1.3) × 1045 (8.2 ± 1.7) × 1045 1.838 ± 0.015
BL Lacertae 472.0 ± 59.4 (1.6 ± 0.7) × 1045 (2.2 ± 0.5) × 1043 (2.8 ± 0.7) × 1045 2.11 ± 0.04

Notes. (1) Source name; (2) source distance based on NED (if marked with the metric distance is used, otherwise the luminosity distance provided); (3) optical luminosity in R band; (4) radio luminosity at 15 GHz based on the OVRO monitoring (Richards et al. 2011); (5) HE γ-ray luminosity based on the 2FGL (Nolan et al. 2012); (6) HE γ-ray photon index from the 2FGL.

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