Workflow information system for QC

This plot shows the number of cosmic events detected by the pipeline in the science observations as a function of the total exposure time.

For the UVB and VIS arm, we offer correlations for the two values of detector gain (low gain = lg or high gain = hg) and for the two pixel binnings (1x1 or 2x2). Datasets split by the different observing techniques:

• red for STARE (single exposure),
• green for NODDING (exposure pairs)
• blue for OFFSET (OBJECT and SKY exposures)

In the NIR arm, the left box is for the STARE and OFFSET mode observations (including the mapping template observations). For the K-band supressing 0.9x11JH slit, the pipeline does not evaluate the K-band orders resulting in an effective smaller pixel region with respect to the 0.9x11 slit, and a smaller resulting number of cosmics. The right box displays the NODDING products, with the most frequently used values of PRO.DATANCOM (N, the total number of combined raw frames) highlighted.