Table 2
Non-TeV sample sources and their variability properties.
| Name | Other name | 2FHL name | Redshifta | SED | Intrinsic mean | Intrinsic | Median | N | Host-corr | Mean | De-red. | Host-corr | Host gal. |
| Classa | p fraction | mod. index | |dθ/dt| | obs. | p fraction | R-mag.b | R-mag. | R-mag. | R-mag.c | ||||
|
|
|||||||||||||
| J0114+1325 | GB6J0114+1325 | − | > 0.26 d | HSP | 0.072 ± |
0.497 ± |
2.43 | 8 | − | 16.3 ± 0.10 | 16.2 | − | − |
| J0848+6606 | GB6J0848+6605 | − | − | ISP | 0.063 ± |
< 0.820 | 0.73 | 4 | − | 17.8 ± 0.08 | 17.6 | − | − |
| J1037+5711 | GB6J1037+5711 | 2FHL J1037.6+5710 | > 0.175 d | ISP | 0.023 ± 0.005 | 0.499 ± |
4.25 | 11 | − | 15.6 ± 0.05 | 15.6 | − | − |
| J1203+6031 | SBS1200+608 | − | 0.065 | ISP | − | − | − | 9 | − | 15.7 ± 0.04 | 15.7 | − | − |
| J1542+6129 | GB6J1542+6129 | 2FHL J1542.9+6129 | − | ISP | 0.049 ± |
0.401 ± |
1.93 | 18 | − | 15.3 ± 0.02 | 15.3 | − | − |
| J1558+5625 | TXS1557+565 | − | 0.300 | ISP | 0.067 ± 0.008 | 0.447 ± |
2.74 | 19 | − | 17.3 ± 0.05 | 17.2 | − | − |
| J1649+5235 | 87GB164812.2+524023 | − | − | ISP | 0.028 ± |
< 0.500 | 0.27 | 16 | − | 16.4 ± 0.09 | 16.3 | − | − |
| J1754+3212 | RXJ1754.1+3212 | 2FHL J1754.2+3211 | > 0.54 e | ISP | 0.047 ± |
0.448 ± |
0.24 | 13 | − | 16.7 ± 0.07 | 16.6 | − | − |
| J1809+2041 | RXJ1809.3+2041 | − | > 0.28 f | HSP | 0.038 ± |
< 0.663 | 1.42 | 12 | − | 18.0 ± 0.12 | 17.8 | − | − |
| J1813+3144 | B21811+31 | − | 0.117 | ISP | 0.058 ± |
0.545 ± |
0.61 | 8 | 0.066 | 16.3 ± 0.06 | 16.2 | 16.5 | 18.6 |
| J1836+3136 | RXJ1836.2+3136 | − | − | ISP | 0.069 ± |
0.472 ± |
1.09 | 10 | − | 17.5 ± 0.05 | 17.2 | − | − |
| J1838+4802 | GB6J1838+4802 | 2FHL J1838.9+4802 | 0.3g | HSP | 0.093 ± 0.006 | 0.212 ± |
0.41 | 11 | 0.095 | 15.2 ± 0.06 | 15.1 | 15.2 | 19.4 |
| J1841+3218 | RXJ1841.7+3218 | − | − | HSP | − | − | − | 8 | − | 18.1 ± 0.06 | 17.9 | − | − |
| J1903+5540 | TXS1902+556 | 2FHL J1903.2+5540 | > 0.727 f | ISP | 0.08 ± |
0.341 ± |
1.31 | 9 | − | 15.7 ± 0.07 | 15.6 | − | − |
| J2015−0137 | PKS2012-017 | − | − | ISP | 0.164 ± 0.006 | < 0.184 | 0.27 | 10 | − | 17.5 ± 0.04 | 17.2 | − | − |
| J2022+7611 | S52023+760 | − | 0.594 | ISP | 0.113 ± |
0.302 ± |
3.96 | 11 | − | 16.5 ± 0.16 | 16.0 | − | − |
| J2131−0915 | RBS1752 | 2FHL J2131.4-0914 | 0.449 | HSP | 0.103 ± |
< 0.168 | 0 | 6 | − | 17.0 ± 0.02 | 17.0 | − | − |
| J2149+0322 | PKSB2147+031 | − | > 0.724 f | ISP | 0.131 ± |
0.287 ± |
0.24 | 7 | − | 16.2 ± 0.15 | 16.0 | − | − |
| J2340+8015 | 1RXSJ234051.4+801513 | 2FHL J2340.8+8014 | 0.274 | HSP | 0.041 ± |
0.600 ± |
0.28 | 11 | − | 17.0 ± 0.13 | 16.5 | − | − |
Notes.
Taken from the 3rd Fermi AGN catalog (Ackermann et al. 2015) unless otherwise stated.
Host galaxy magnitude used in this work, using the correct aperture size of 5.2′′ for RoboPol observations. The original R-band values are taken from Nilsson et al. (2003).
Lower limit based on non-detection of the host galaxy (Plotkin et al. 2010).
Lower limit based on non-detection of the host galaxy (Shaw et al. 2013a).
Lower limit based on intervening absorbers in the spectrum(Shaw et al. 2013b).
Based on a host galaxy detection (Nilsson et al. 2003).
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