8.3.6 Error model for Photometry

Author(s): Laurent Galluccio, Marco Delbó, Alberto Cellino

The uncertainty for the G-band photometric flux of the SSO, referred to as ${\mathrm{\Phi }}_{\mathrm{err}}$, was computed using error propagation for the weighted average photometry measured on the corresponding AF CCDs actually used (see Equation 8.14):

The information is given in the archive on the table gaiadr3.sso_observation in the field g_flux_error.