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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