Table 7.
Properties of the associated OVRO sources.
| J2000 name | 4FGL name | Opt. | z | log(νs) | log(νFνs) | δvar | Mod. |
|---|---|---|---|---|---|---|---|
| class | (Hz) | (erg cm−2 s−1) | index | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| J0211+1051 | 4FGL J0211.2+1051 | BLL | 0.2 | 14.2 | −10.3 | 8.4 |
0.255 |
| J0336+3218 | 4FGL J0336.4+3224 | FSRQ | 1.259 | 13.2 | −11.0 | 5.5 |
0.275 |
| J0341+3352 | FSRQ | 0.725 | 12.9 | −12.6 | 5.1 |
0.227 | |
| J0502+1338 | 4FGL J0502.5+1340 | BLL | 0.35 | 13.0 | −11.7 | 15.8 |
0.301 |
| J0509+0541 | 4FGL J0509.4+0542 | BLL | 0.3365 | 14.6 | −10.7 | 14.7 |
0.167 |
| J0630−1323 | FSRQ | 1.021 | 13.6 | −12.1 | 32.3 |
0.125 | |
| J0631−1410 | FSRQ | 1.017 | 12.6 | −12.2 | 0.6 |
0.100 | |
| J1125+2610 | FSRQ | 2.341 | 12.3 | −12.1 | 56.8 |
0.140 | |
| J1256−0547 | 4FGL J1256.1−0547 | FSRQ | 0.5361 | 12.7 | −10.5 | 11.6 |
0.203 |
| J1310+3220 | 4FGL J1310.5+3221 | FSRQ | 0.997 | 12.7 | −11.2 | 26.4 |
0.244 |
| J1504+1029 | 4FGL J1504.4+1029 | FSRQ | 1.839 | 12.7 | −11.7 | 17.7 |
0.230 |
| J1743−0350 | 4FGL J1744.2−0353 | FSRQ | 1.057 | 12.7 | −11.2 | 6.4 |
0.056 |
| J1916−1519 | 4FGL J1916.7−1516 | BCU | ... | 12.8 | −12.0 | ... | 0.185 |
| J2148+0657 | 4FGL J2148.6+0652 | FSRQ | 0.99 | 12.5 | −10.7 | 1.2 |
0.201 |
| J2151+0709 | FSRQ | 1.364 | 12.8 | −12.1 | 13.1 |
0.115 | |
| J2151+0552 | FSRQ | 0.74 | 12.4 | −12.2 | 18.0 |
0.030 | |
| J2200+1030 | 4FGL J2200.3+1029 | BLL | 0.172 | 13.0 | −12.5 | 3.4 |
0.156 |
| J2200+0234 | FSRQ | 1.323 | 13.1 | −12.5 | 31.1 |
0.246 | |
| J2203+1007 | BCU (a) | 0.172 | 12.6 | −12.5 | 7.6 |
0.156 | |
| J2238+0724 | FSRQ | 1.011 | 12.9 | −12.0 | 16.8 |
0.347 |
Notes. Optical classifications in Col. (3) are taken from the 4LAC catalog (Ajello et al. 2020) for the sources included in there (ones with name given in Col. (2)), and from the 5BZCat catalog (Massaro et al. 2015) for the non-LAT sources unless otherwise stated. BCU stands for blazars of unknown optical class. Column (4) gives the redshift of the source. Columns (5) and (6) give the synchrotron peak frequency and peak luminosity, respectively, taken from 4LAC catalog or determined by ourselves for the non-LAT sources. Variability Doppler factors, given in Col. (7) are taken from Liodakis et al. (2018) or determined by ourselves using the same methods. Radio modulation index determined from OVRO data are given in Col. (8), and are taken from Liodakis et al. (2017) or determined by ourselves.
Classification taken from Sowards-Emmerd et al. (2005).
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