TOPz: Photometric redshifts using template fitting applied to the GAMA survey

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Table 1

Flux and flux uncertainty corrections applied to the GAMA data for nine passbands.

Passband	$f_{bias}^{α}$ $f_{{\rm{bias}}}^\alpha$	$f_{σ,rel}^{α}$ $f_{\sigma {\rm{,rel}}}^\alpha$	$f_{σ,scaling}^{α}$ $f_{\sigma {\rm{,scaling}}}^\alpha$
u	1.0585	0.0500	1.3221
g	0.9935	0.0000	1.3246
r	1.0098	0.0000	1.0000
i	0.9890	0.0000	1.0599
Z	0.9566	0.0000	1.1819
Y	0.9702	0.0000	1.2295
J	1.0493	0.0000	1.2112
H	1.0083	0.0000	1.4387
Ks	1.0198	0.0000	1.6254

Notes. $f_{bias}^{α}$ $f_{{\rm{bias}}}^\alpha$ is linear flux bias correction, $f_{σ,rel}^{α}$ $f_{\sigma {\rm{,rel}}}^\alpha$ is relative uncertainty added to the observed flux uncertainty and $f_{σ,scaling}^{α}$ $f_{\sigma {\rm{,scaling}}}^\alpha$ defines the scaling parameter for flux uncertainty. See Sect. 4 for more details.

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