Table 4
Correlation coefficient and significance for gamma-ray vs. MWACS data.
| Sample | # objects | # redshift bins | r | ρ | p-value | |
| (1) | (2) | (3) | (4) | (5) | (6) | |
|
|
||||||
| All sources | 87 | – | 0.26 | 0.27 | – | |
| All sources, with z | 76 | 7 | 0.29 | 0.31 | 6.1 × 10-2 | |
| FSRQ | 52 | 5 | 0.21 | 0.25 | 0.15 | |
Notes. In each row, we indicate the sample considered in Col. (1), the number of objects included (Col. 2), and the redshift bins used for the statistical analysis (Col. 3), the Pearson r and Spearman ρ correlation coefficients and the statistical significance for the correlation between MWACS flux density and gamma-ray energy flux Sγ (Cols. 4–6) determined using the method of Pavlidou et al. (2012). The method does not consider sources without a measured redshift, therefore values in Cols. 3 and 6 are not determined for the entire sample.
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