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Table 4.

Discrete cross-correlation function between the low (3–10 keV) and high energy (10–79 keV) emission of the NuSTAR blazars.

Source Obs. ID Lag (ks) ZDCF Likelihood
S5 0014+81 60001098002 0.22
60001098004 0.62
B0222+185 60001101002 0.29
60001101004 0.42
HB 0836+710 60002045002 0.35
60002045004 0.33
3C 273 10202020002 0.44
10302020002 0.45
3C 279 60002020002 0.43
60002020004 0.45
PKS 1441+25 90101004002 0.08
PKS 2149–306 60001099002 0.72
60001099004 0.19
S5 0716+714 90002003002 0.13
Mrk 501 60002024002 0.13
60002024004 0.57
60002024006 0.40
60002024008 0.72
1ES 1959+650 60002055002 0.41
60002055004 0.54
PKS 2155–304 10002010001 0.61
60002022002 0.37
60002022004 0.38
60002022006 0.15
60002022008 0.53
60002022010 0.36
60002022012 0.37
60002022014 0.30
60002022016 0.20
BL Lac 60001001002 0.35

Notes. The +ve lag indicates hard lag.

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