Fig. 5
Two-dimensional completeness function deprojected along the orthogonal coordinate axis RA-Dec. The imprint of a single galaxy spectrum is visible in the plot as the almost zero rectangular region at small angular separation. This region corresponds to the typical area occupied by the projected spectrum of an observed source. The enhancement of clustering in the top left region of the plot is produced by the particular displacement along common columns of slits within a quadrant. The scale of the abscissa and the ordinates is very different.
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