Table 5
Confidence intervals for data obtained with the VLT by King et al. (2012).
| cosθ | n | Reported interval | Confidence interval | β for α = 0.05 |
| (1) | (2) | (3) | (4) | (5) |
|
|
||||
| 0.248 | 26 | (−0.37,0.77) | (−4.55 × 10-2,1.02) | 0.91 |
| 0.519 | 17 | (9.99 × 10-2,0.70) | (−0.26,1.21) | 0.75 |
| 0.368 | 18 | (−0.54,0.61) | (−0.47,0.27) | 0.74 |
| 0.330 | 30 | (−1.94,0.46) | (−0.23,0.42) | 0.77 |
| 0.552 | 9 | (−0.49,0.56) | (−0.55,1.69) | 0.82 |
| 0.567 | 11 | (−1.01,0.61) | (−0.75,1.25) | 0.79 |
| 0.266 | 31 | (−0.68,0.15) | (1.18 × 10-2,0.98) | 0.90 |
| 5.047 × 10-2 | 7 | (−5.87 × 10-2,0.62) | (−0.85,1.21) | 0.91 |
| 0.497 | 10 | (−2.30, − 0.70) | (−0.59,1.52) | 0.84 |
| 0.372 | 18 | (0.28,0.59) | (−0.47,0.27) | 0.74 |
Notes. Comparison with single quasar obtained with the VLT by Srianand (2013, priv. comm.). Data sets are selected according to angular position. Columns:
number of data reported by King et al. (2012) inside the interval;
calculated confidence interval from a group of data reported by King et al. (2012) in units of 10-5;
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