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Table 2
Results of the correlation analysis between 1FHL (10−500 GeV) energy fluxes and VLBI flux densities for various 1FHL-n sub-samples.
Source type | Catalog | Number of sources | Number of z-bins | r-Pearson | Significance |
|
|||||
All sources | 1FHL | 147 | 14 | −0.05 | 0.59 |
3FGL | 147 | 14 | 0.71 | < 10-6 | |
BL Lac | 1FHL | 100 | 9 | 0.12 | 0.55 |
3FGL | 100 | 9 | 0.70 | < 10-6 | |
FSRQ | 1FHL | 44 | 4 | −0.01 | 0.99 |
3FGL | 44 | 4 | 0.49 | < 10-6 | |
HSP | 1FHL | 60 | 5 | 0.57 | 1.0 × 10-6 |
3FGL | 60 | 5 | 0.77 | < 10-6 | |
ISP | 1FHL | 23 | 2 | 0.19 | 0.40 |
3FGL | 23 | 2 | 0.46 | 2.5 × 10-2 | |
LSP | 1FHL | 52 | 5 | 0.21 | 0.12 |
3FGL | 52 | 5 | 0.43 | 3.0 × 10-6 |
Notes. For comparison, the same analysis was performed by using 3FGL (0.1−300 GeV) energy fluxes.
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