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Table 5.

Main results of the analysis.

(1) (2) (3) (4) (5) (6) (7)
Target χ2 log[νpeak(Hz)] Class β fP(d) PN
1ES 0033+595 5.9 18.17  ±  0.14 HBL −1.34  ±  0.15 7 48.3
1ES 0120+340 2.4 17.66  ±  0.13 HBL −1.46  ±  0.30 61 44.0
RGB 0136+391 60.5 16.00  ±  0.30 HBL −1.57  ±  0.15 10 6.8
RGB 0214+517 2.4 16.08  ±  0.07 HBL −1.27  ±  0.23 130 99.1
3C 66A 899.0 14.15  ±  0.09 IBL −1.40  ±  0.11 15 77.5
1ES 0647+250 80.8 16.41  ±  0.23 HBL −1.86  ±  0.20 13 88.6
1ES 0806+524 185.2 15.84  ±  0.14 HBL −1.79  ±  0.19 38 54.0
OJ 287 1393.6 13.27  ±  0.07 LBL −1.30  ±  0.10 40 18.5
1ES 1011+496 155.0 15.63  ±  0.26 HBL −1.50  ±  0.14 16 30.6
1ES 1028+511 33.1 16.70  ±  0.26 HBL −1.57  ±  0.15 6 96.4
Mkn 421 355.2 17.03  ±  0.19 HBL −1.38  ±  0.09 477 0.1
RGB 1117+202 21.0 15.98  ±  0.12 HBL −1.36  ±  0.14 40 84.8
Mkn 180 48.2 16.47  ±  0.25 HBL −1.57  ±  0.15 29 99.9
RGB 1136+676 3.1 17.90  ±  0.29 HBL −1.81  ±  0.49 40 51.7
ON 325 137.2 14.85  ±  0.18 IBL/HBL −1.25  ±  0.12 28 99.5
1ES 1218+304 93.7 17.17  ±  0.23 HBL −1.72  ±  0.17 33 34.3
RGB 1417+257 2.7 17.62  ±  0.10 HBL −1.41  ±  0.31 20 88.8
1ES 1426+428 4.5 18.02  ±  0.26 HBL −1.25  ±  0.15 12 90.0
1ES 1544+820 16.04  ±  0.21 HBL
Mkn 501 8.3 16.47  ±  0.06 HBL −1.65  ±  0.16 15 97.9
OT 546 10.3 16.35  ±  0.20 HBL −1.40  ±  0.15 18 64.8
1ES 1959+650 249.1 16.70  ±  0.04 HBL −1.70  ±  0.17 1050 84.7
BL Lac 849.6 13.99  ±  0.12 LBL −1.27  ±  0.10 197 94.5
1ES 2344+514 5.7 16.35  ±  0.12 HBL −1.47  ±  0.17 14 10.0

S5 0716+714 2761.4 14.24  ±  0.13 IBL −1.18  ±  0.09 163 20.8
ON 231 354.6 14.32  ±  0.08 IBL −1.38  ±  0.15 18 98.8
3C 279 1597.3 12.69  ±  0.05 FSRQ −1.54  ±  0.14 202 80.0
PG 1424+240 162.5 15.14  ±  0.07 IBL/HBL −1.54  ±  0.19 17 88.8
PKS 1510−089 248.3 13.75  ±  0.15 FSRQ −0.97  ±  0.14 155 40.1
PG 1553+113 323.6 15.90  ±  0.16 HBL −1.49  ±  0.15 174 31.5
PKS 2155−304 1980.8 16.01  ±  0.28 HBL −1.55  ±  0.15 99 81.1

Notes. Columns: (1) target name, (2) reduced chi-squared from the variability analysis, (3) synchrotron peak frequency, (4) classification, (5) power spectral density slope, (6) most significant rest-frame period (days), and (7) probability in percent of finding such a period in the case of pure power-law noise input spectrum.

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