Table 1
TeV sample sources and their variability properties.
Name | TeVCat name | 2FHL name | Redshifta | SED | Intrinsic mean | Intrinsic | Median | N | Host-corr | Mean | De-red. | Host-corr | Host gal. | Ref. | Jet PA | Ref. | |
classa | p fraction | mod. index | |dθ/dt| | obs | p fraction | R-mag.b | R-mag. | R-mag. | R-mag.c | host | (deg) | jet. PA | |||||
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J0136+3905 | RGB J0136+391 | 2FHL J0136.5+3906 | > 0.41 d | HSP |
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2.94 | 9 | − | 15.6 ± 0.02 | 15.5 | − | − | − | − | − | |
J0152+0146 | RGB J0152+017 | 2FHL J0152.8+0146 | 0.082 | HSP |
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0.26 | 9 | 0.049 | 15.3 ± 0.08 | 15.2 | 15.6 | 16.7 | 1 | − 135.6 | 8 | |
J0222+4302 | 3C 66A | 2FHL J0222.6+4301 | > 0.335 e | HSP |
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1.05 | 7 | − | 14.47 ± 0.07 | 14.29 | − | − | − | − | − | |
J0232+2017 | 1ES 0229+200 | − | 0.139 | HSP |
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0.41 | 3 | − | 16.1 ± 0.01∗ | 15.8 | 18.2 | 16.2 | 2 | − | − | |
J0319+1845 | RBS 0413 | 2FHL J0319.7+1849 | 0.192 | HSP | − | − | − | 3 | − | 17.5 ± 0.14 | 17.3 | − | − | − | − | − | |
J0416+0105 | 1ES 0414+009 | 2FHL J0416.9+0105 | 0.287 | HSP | − | − | − | 1 | − | 16.55 ± 0.04 | 16.2 | − | − | − | − | − | |
J0507+6737 | 1ES 0502+675 | 2FHL J0507.9+6737 | 0.341 | HSP | 0.045 ± 0.007 |
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0.80 | 5 | 0.062 | 16.6 ± 0.11 | 16.3 | 17.0 | 18.0 | 3 | − | − | |
J0521+2112 | VER J0521+211 | 2FHL J0521.7+2112 | 0.108 | ISP |
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< 0.435 | 0.30 | 6 | − | 15.4 ± 0.01 | 13.9 | − | − | − | − | − | |
J0648+1516 | RX J0648.7+1516 | 2FHL J0648.6+1516 | 0.179 | HSP | − | − | − | 1 | − | 17.25 ± 0.01 | 16.94 | − | − | − | − | − | |
J0650+2502 | 1ES 0647+250 | 2FHL J0650.7+2502 | 0.410f | HSP | − | − | − | 2 | − | 15.6 ± 0.04∗ | 15.4 | 15.4 | 19.9 | 4 | 157.9 | 8 | |
J0710+5908 | RGB J0710+591 | 2FHL J0710.5+5908 | 0.125 | HSP | 0.043 ± 0.004 | < 0.412 | 0.33 | 6 | 0.060 | 16.4 ± 0.03 | 16.3 | 16.7 | 17.8 | 1 | − 145.3 | 8 | |
J0809+5218 | 1ES 0806+524 | 2FHL J0809.7+5218 | 0.138 | HSP | 0.051 ± 0.002 | <0.205 | 0.25 | 4 | 0.054 | 15.1 ± 0.04 | 15.0 | 15.1 | 18.0 | 6 | − | − | |
J1136+7009 | Markarian 180 | 2FHL J1136.5+7009 | 0.045 | HSP |
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< 0.437 | 0.45 | 10 | 0.043 | 14.9 ± 0.03 | 14.9 | 15.2 | 16.6 | 1 | − | − | |
J1217+3007 | 1ES 1215+303 | 2FHL J1217.9+3006 | 0.130 | HSP |
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0.17 | 14 | 0.112 | 14.3 ± 0.05 | 14.2 | 14.3 | 18.1 | 1 | 143.6 | 9 | |
J1221+3010 | 1ES 1218+304 | 2FHL J1221.3+3009 | 0.182 | HSP |
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0.68 | 9 | 0.087 | 16.5 ± 0.04 | 16.5 | 17.2 | 17.4 | 3 | − | − | |
J1221+2813 | W Comae | − | 0.102 | ISP |
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< 0.192 | 0.47 | 6 | 0.188 | 15.6 ± 0.06 | 15.6 | 15.8 | 17.9 | 1 | 114.6 | 9 | |
J1224+2436 | MS 1221.8+2452 | 2FHL J1224.4+2435 | 0.218 | HSP |
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2.57 | 9 | 0.043 | 16.0 ± 0.06 | 15.9 | 16.0 | 19.5 | 2 | − | − | |
J1427+2348 | PKS 1424+240 | 2FHL J1427.0+2348 | 0.6035g | HSP |
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3.59 | 12 | 0.039 | 14.1 ± 0.05 | 14.0 | 14.1 | > 21.0 | 5 | − | − | |
J1428+4240 | H 1426+428 | 2FHL J1428.5+4239 | 0.129 | HSP | 0.024 ± 0.002 | < 0.409 | 0 | 7 | 0.038 | 16.5 ± 0.02 | 16.5 | 17.0 | 17.6 | 6 | − 11.9 | 10 | |
J1442+1200 | 1ES 1440+122 | 2FHL J1442.9+1159 | 0.163 | HSP | 0.028 ± 0.003 |
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0.54 | 7 | − | 16.2 ± 0.02∗ | 16.2 | 16.5 | 17.5 | 1 | − | − | |
J1555+1111 | PG 1553+113 | 2FHL J1555.7+1111 | > 0.395 h | HSP |
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2.91 | 32 | 0.033 | 14.0 ± 0.01 | 13.9 | 14.00 | > 21.6 | 5 | − | − | |
J1725+1152 | H 1722+119 | 2FHL J1725.1+1154 | 0.34i | HSP |
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0.84 | 16 | 0.108 | 14.8 ± 0.05 | 14.5 | 14.8 | > 21.4 | 5 | − | − | |
J1728+5013 | 1ES 1727+502 | 2FHL J1728.2+5013 | 0.055 | HSP |
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2.40 | 17 | 0.027 | 15.7 ± 0.02 | 15.6 | 15.9 | 17.5 | 6 | − | − | |
J1743+1935 | 1ES 1741+196 | 2FHL J1743.9+1933 | 0.084 | HSP | 0.048 ± 0.005 |
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0.24 | 6 | − | 15.0 ± 0.01∗ | 14.8 | 16.1 | 15.4 | 1 | 70.0 | 8 | |
J1943+2118 | HESS J1943+213 | 2FHL J1944.1+2117 | > 0.03 j | HSP |
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< 0.417 | 0 | 6 | − | 17.15 ± 0.01 | 11.18l | − | − | − | − 149.2 | 11 | |
J1959+6508 | 1ES 1959+650 | 2FHL J2000.1+6508 | 0.048 | HSP | 0.058 ± 0.002 | < 0.160 | 0.51 | 13 | 0.067 | 14.9 ± 0.06 | 14.5 | 15.0 | 17.0 | 5 | 152.7 | 10 | |
J2001+4352 | MAGIC J2001+435 | 2FHL J2001.2+4352 | 0.190k | ISP | 0.167 ± 0.008 |
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0.58 | 12 | 0.190 | 16.8 ± 0.04 | 15.5 | 16.9 | 19.2 | 7 | − | − | |
J2250+3825 | B3 2247+381 | 2FHL J2249.9+3826 | 0.119 | HSP | 0.020 ± 0.002 |
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1.73 | 10 | 0.025 | 16.4 ± 0.04 | 16.1 | 16.6 | 18.2 | 1 | − | − | |
J2347+5142 | 1ES 2344+514 | 2FHL J2347.1+5142 | 0.044 | HSP | 0.026 ± 0.004 |
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0 | 5 | 0.080 | 15.8 ± 0.03 | 15.3 | 17.0 | 16.2 | 6 | − | − |
Notes.
Taken from the 3rd Fermi AGN catalog (Ackermann et al. 2015) unless otherwise stated.
Mean from RoboPol observations, except for sources with an asterisk for which this is from Tuorla monitoring program and 1ES 2344+514 for which this is from NOT observations. The quoted uncertainty is the standard error of the mean, unless N obs is one, in which case the uncertainty is the rms error of the measurement.
Host galaxy magnitude used in this work, converted to R-band magnitude where needed and with correct aperture radius of 3′′ used in the estimation.
Lower limit based on non-detection of the host galaxy (Nilsson et al. 2012).
Lower limit based on Lyα (Furniss et al. 2013a).
Based on a host galaxy detection (Kotilainen et al. 2011).
Based on a lower limit on Lyα (Furniss et al. 2013b), and a detection of a group of galaxies at the same redshift (Rovero et al. 2016).
Lower limit based on a confirmed Lyα + Oiv absorber (Danforth et al. 2010).
Lower limit based on a featureless spectrum (Landoni et al. 2014).
Lower limit based on a host galaxy association (Peter et al. 2014)
Based on a host galaxy detection (Aleksić et al. 2014).
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