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Basic pipeline

The basic pipeline shall operate on single pointings or ``well-defined'' observing sequences taken during a single night to produce instrument signature-free images and to derive object catalogues from them. The object catalogues will be used to provide the first pass astrometric and photometric calibration.

The two-dimensional image data products at this stage will be instrumental signature-corrected: single frames; lossless interleaved super frames; stacked dither (super)frames; tiled contiguous mosaics, combining four pointings with any of previous options; and confidence maps for all pipeline output products.

The catalogue data products will be lists of detected images with an agreed set of parameters summarising useful astronomical information and providing the necessary DQC information.

In more detail the requirements are:


next up previous
Next: Survey progess Database Up: PIPELINE PROCESSING REQUIREMENTS Previous: Summit Pipeline
Nigel Hambly 2002-10-02