Table 1.
Statistic | 1 | 2 | 3 | 4 | 5 | 6 | 7 |
---|---|---|---|---|---|---|---|
sm | 0.95 | 1.54 ± 0.06 | 1.54 ± 0.08 | 0.95 ± 0.04 | 9.7 | 0.1 | 0.1 |
〈m〉 | 21.28 | 20.93 ± 0.07 | 20.92 ± 0.07 | 21.43 ± 0.05 | −4.9 | −0.1 | −1.0 |
β | 1.56 | 3.46 ± 0.28 | 3.47 ± 0.38 | 1.58 ± 0.19 | 6.7 | 0.0 | 0.1 |
ρ1 | −0.79 | −0.40 ± 0.05 | −0.44 ± 0.06 | −0.78 ± 0.02 | 9.1 | −0.8 | 0.1 |
ρ2 | −0.10 | 0.36 ± 0.06 | 0.36 ± 0.08 | −0.09 ± 0.06 | 7.8 | 0.0 | 0.1 |
σ1 | 1.36 | 1.29 ± 0.06 | 1.29 ± 0.06 | 1.35 ± 0.05 | 1.0 | 0.0 | 0.1 |
σ2 | 0.84 | 1.27 ± 0.05 | 1.27 ± 0.06 | 0.84 ± 0.04 | 8.1 | 0.0 | 0.0 |
Here and in Tables 2–6, column 1 gives the observed value of the statistic in question. Column 2 is the predicted value according to C1, as determined from SLF1, where SLFp denotes the sample LF according to NPMLE, as given in closed form in ref. 11, for cosmology p. Column 3 is the predicted value, according to C2, of the predicted value according to C1, as determined from SLF2. Column 4 is the predicted value according to C2, as determined from SLF2. Columns 5, 6, and 7 are the corresponding prediction errors in units of standard deviations.