Table 2.
Cross-correlation results derived by the DCF (top) and ICF (bottom) between the Fermi/LAT γ-ray and different radio light curves.
| Light curve | ν | rcorr | Significance | τγ, ν |
|---|---|---|---|---|
| [GHz] | [σ] | [days] | ||
| (1) | (2) | (3) | (4) | (5) |
| DCF: | ||||
| ALMA 7 | 341.9 ± 8.5 | 0.63 ± 0.13 | 2.73 | 84 ± 102 |
| SMA | 225.6 ± 4.8 | 0.57 ± 0.15 | 1.91 | 144 ± 224 |
| ALMA 3 | 97.0 ± 6.2 | 0.623 ± 0.079 | 2.39 | 220 ± 69 |
| OVRO | 15 | 0.45 ± 0.14 | 1.16 | 252 ± 219 |
| ICF: | ||||
| ALMA 7 | 341.9 ± 8.5 | 0.54 | 2.07 | 120 ± 46 |
| SMA | 225.6 ± 4.8 | 0.48 | 1.88 | 198 ± 82 |
| ALMA 3 | 97.0 ± 6.2 | 0.57 | 2.15 | 220 ± 34 |
| OVRO | 15 | 0.48 | 1.34 | 225 ± 153 |
Notes. Col.(1): Radio light curve; Col.(2): Mean frequency of the radio light curve; Col.(3): Peak cross-correlation coefficient; Col.(4): Significance of the peak cross-correlation coefficient in units of the Gaussian equivalent standard deviation; Col.(5): Time lag corresponding to the peak cross-correlation coefficient.
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