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Burgon, Ross
(2012).
Abstract
Within the Gaia astrometry field all stars with magnitudes fainter than 13 will have their 2-D readout windows binned to 1-D image shapes. For some readout windows there many be additional sources present in the window that remain undetected due to the window creation and binning process performed on-board the spacecraft. This technical note describes procedures and preliminary results into assessing the probability that an image shape for a star fainter than 13th magnitude contains an undetected secondary source.