The resulting values of the prior parameters obtained by fitting (14) to a subset of 10 000 randomly selected galaxies from the BS and FS together. The three galaxy types t = 1, 2, 3 are the same that were defined in Section 3 for the LFs. f3 and k3 do not appear because Π(t = 3∣m0) is deduced by normalization.
| t . | f . | k . | α . | z0 . | km . |
|---|---|---|---|---|---|
| 1 | 0.565 | 0.186 | 2.456 | 0.312 | 0.122 |
| 2 | 0.430 | 0.000 | 1.877 | 0.184 | 0.130 |
| 3 | – | – | 1.404 | 0.047 | 0.148 |
| t . | f . | k . | α . | z0 . | km . |
|---|---|---|---|---|---|
| 1 | 0.565 | 0.186 | 2.456 | 0.312 | 0.122 |
| 2 | 0.430 | 0.000 | 1.877 | 0.184 | 0.130 |
| 3 | – | – | 1.404 | 0.047 | 0.148 |
The resulting values of the prior parameters obtained by fitting (14) to a subset of 10 000 randomly selected galaxies from the BS and FS together. The three galaxy types t = 1, 2, 3 are the same that were defined in Section 3 for the LFs. f3 and k3 do not appear because Π(t = 3∣m0) is deduced by normalization.
| t . | f . | k . | α . | z0 . | km . |
|---|---|---|---|---|---|
| 1 | 0.565 | 0.186 | 2.456 | 0.312 | 0.122 |
| 2 | 0.430 | 0.000 | 1.877 | 0.184 | 0.130 |
| 3 | – | – | 1.404 | 0.047 | 0.148 |
| t . | f . | k . | α . | z0 . | km . |
|---|---|---|---|---|---|
| 1 | 0.565 | 0.186 | 2.456 | 0.312 | 0.122 |
| 2 | 0.430 | 0.000 | 1.877 | 0.184 | 0.130 |
| 3 | – | – | 1.404 | 0.047 | 0.148 |
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