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Table 2.

QPO candidates identified by the CWT of the Fermi-LAT light curves in time bins of 30 days and 7 days.

Source Period (d) 30 d LC Significance (σ) Period (d) 7 d LC Significance (σ) Nr. fitted cycles
4C +01.02 268±55 > 5 268±54 > 5 4
123±26 4.7 122±26 > 5 5

PKS 0537−441 285±67 > 5 286±73 > 5 4

S5 1044+71 1133±229 4.9 1127±226 4.6 3
116±33 > 5 117±38 > 5 4

B2 1520+31 176±48 > 5 179±42 > 5 6
71±15 > 5 14
39±11 > 5 17

PKS 2247−131 217±38 > 5 214±43 > 5 6
34±13 > 5 10
4C +28.07 230±90 > 5 244±88 > 5 3

NGC 1275 282±84 3.3 247±63 > 5 3
92±33 > 5 4

PKS 0402−362 221±56 > 5 221±60 > 5 3
122±42 > 5 5

PKS 0426−380 85±26 > 5 8

PKS 0447−439 120±37 > 5 111±42 > 5 7

PKS 0454−234 69±21 > 5 4

S5 0716+714 325±75 2.4 324±77 3.2 5

263±52 > 5 264±59 4.9 4
1H 1013+498 100±25 > 5 4
52±15 > 5 12

Mrk 421 300±64 > 5 300±65 > 5 3

4C +21.35 66±17 > 5 6

3C 273 177±36 > 5 177±38 > 5 4
99±26 > 5 97±25 > 5 3

3C 279 102±26 > 5 101±27 > 5 6
40±8 > 5 4

PKS 1424−418 94±25 > 5 90±22 > 5 5

PKS 1510−089 119±31 > 5 120±36 > 5 3

Mrk 501 315±98 2.9 326±76 > 5 7 (a)

PKS 2155−304 334±107 2.2 341±106 3.5 4

CTA 102 370±85 > 5 366±81 > 5 3
179±40 > 5 178±40 > 5 5

3C 454.3 117±23 > 5 120±27 > 5 4

PMN J2345−1555 197±50 > 5 191±44 > 5 4

Notes.

(a)

Number fitted cycles observed only in the weekly binned light curve.

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