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Table 5

Example illustrating the structure of tables provided in https://unidgamma.in2p3.fr as an output of the case A study.

3FGL name l () b () Flags HR23 HR34 HR23 − HR34 λ ζ BDT ζ MLP Type
J0032.35522 308.619 61.549 0 1.12 1.45 0.24 0.21 0.03 1.00 0.8563 0.9955 fsrq
J0537.0+0957 195.285 11.578 0 0.42 1.20 0.50 0.69 0.18 0.89 0.5999 0.9299 fsrq
J0940.67609 292.247 17.425 0 0.95 0.68 0.08 0.48 0.56 1.00 0.6433 0.6872 unc
J1050.4+0435 245.550 53.413 0 0.80 1.34 0.22 0.45 0.23 1.00 0.8447 1.2406 fsrq
J1221.50632 289.713 55.552 0 0.75 0.66 0.04 0.07 0.10 1.00 0.5249 0.6722 bll
J1315.70732 313.448 54.825 0 1.82 0.75 0.05 0.24 0.29 1.00 0.6916 1.0256 bll
J1335.24056 311.784 21.182 0 0.77 0.85 0.49 0.27 0.22 1.00 0.5341 0.8333 fsrq
J1417.54402 318.864 16.150 0 0.93 0.64 0.10 0.09 0.01 1.00 0.7065 0.8152 unc
J1417.75026 316.692 10.113 0 1.19 0.82 0.03 0.36 0.33 1.00 0.6654 0.9688 fsrq
J1548.4+1455 25.633 47.175 0 1.05 0.59 0.01 0.13 0.11 1.00 0.6562 0.8915 bll
J1625.62058 355.668 19.288 0 0.68 0.78 0.65 0.08 0.57 1.00 0.6440 0.7777 fsrq
J1704.1+1234 32.465 29.424 0 1.30 0.70 0.42 0.13 0.30 1.00 0.7970 0.9701 unc
J1704.40528 14.913 20.797 0 1.34 0.72 0.53 0.34 0.86 1.00 0.8318 0.9764 bll
J1747.3+0324 28.606 15.797 0 0.74 0.81 0.05 0.04 0.01 1.00 0.6598 0.8106 bll
J1801.57825 315.325 24.088 0 1.31 1.01 0.32 0.28 0.05 1.00 0.8304 0.9857 fsrq
J1816.06407 330.337 20.519 0 0.70 0.71 0.27 0.32 0.04 1.00 0.4172 0.4639 fsrq
J1845.52524 9.441 10.079 0 0.69 0.64 0.35 0.20 0.55 1.00 0.4874 0.7558 bll
J1917.13024 7.551 18.469 0 1.38 0.68 0.09 0.04 0.13 1.00 0.8109 1.0398 bll
J2109.4+1437 63.689 21.881 0 2.28 1.00 0.70 0.08 0.62 1.00 0.8806 0.8886 fsrq
J2250.3+1747 86.354 36.331 0 1.02 1.08 0.28 0.90 0.62 1.00 0.8135 1.2062 fsrq

Notes. Here we show the sample of the twenty brightest blazar candidates with no flag in the high galactic latitude region (|b| > 10 ). The columns correspond respectively to the 3FGL source name, the galactic coordinates of the source (l, b), the 3FGL caution flag, the values of the six discriminant parameters, and the values of the output parameters ζ built with the BDT and MLP classifiers. We added in the last column the assignation from the case B study for the BL Lac or FSRQ nature of the source (bll for BL Lac, fsrq for FSRQ and unc for uncertain). The superscripts correspond to a blazar candidate previously proposed by other authors: for Saz Parkinson et al. (2016), for Doert & Errando (2014), for Mirabal et al. (2012), ° for Massaro et al. (2013a) and for Ackermann et al. (2012). The full table is available at the CDS.

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