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David Thomas Hill PhD Thesis - Research@StAndrews:FullText ...

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5.8 The covariance matrix for the deeper rKron sample. . . . . . . . . . . . . . . 168<br />

5.9 Best-fitting Choloniewski function parameters from other surveys. In the<br />

case of de Jong & Lacey, where the BBD is generated in M-re, the re,∗<br />

parameter is quoted. Parameters from v1 of Ball et al. are shown, as the<br />

parameters they have published may result from a local minima (Ball &<br />

Loveday, priv. comm). Parameters have not been converted onto the AB<br />

magnitude system. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 175<br />

5.10 Thebestfittingmodified-modelfunctionparametersfortheBivariatebrightness<br />

distributions. These datapoints are for samples that will suffer from<br />

colour incompleteness, but use varying magnitude limits for each object<br />

within the SWML algorithm to correct for this bias. The dataset fit to the<br />

model is the same dataset fit to the unmodified function, so sample sizes<br />

are shown in Table 5.4. χ 2 parameters for this dataset are shown in Table<br />

5.6. Uncertainties are calculated from the 90% confidence intervals for a<br />

system with 7 degrees of freedom, when all other parameters are fixed to<br />

the best-fitting solution. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 182<br />

5.11 Thebestfittingmodified-modelfunctionparametersfortheBivariatebrightness<br />

distributions. These parameters are for samples that have been cut to<br />

a brighter apparent magnitude in order to guarantee that they are colour<br />

complete. The dataset fit to the model is the same dataset fit to the unmodified<br />

function, so sample sizes are shown in Table 5.5. The rSDSS Petro<br />

sampleisthesameasthesampledetailedinTable5.10, andsoisnot shown.<br />

χ 2 parameters for this dataset are shown in Table 5.6. Uncertainties are<br />

calculated from the 90% confidence intervals for a system with 7 degrees of<br />

freedom, when all other parameters are fixed to the best-fitting solution. . . 185<br />

5.12 j and νf(ν) statistics from the deepest cut sample Bivariate brightness distributions,<br />

derived from the best-fitting Choloniewski and modified model<br />

parameters. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 188<br />

5.13 j and νf(ν) statistics from the GAMA CSED paper (Driver et al, in prep),<br />

and a combined MGC-SDSS-UKIDSS sample detailed in Chapter 3. . . . . 189

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