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Finding calibration frames

When a frame is reduced and files as a calibration, it is added to an index file located in ORAC_DATA_OUT named after the type of calibration, e.g., dark frames are filed in index.dark. When the pipeline is run up and needs a calibration frame but has not been asked to reduce one in that session it will look in the index files for one that may have been reduced at a previous time.

If the pipeline is unable to find a suitable calibration it will complain vociferously and exit. This may seem extreme, but remember that ORAC-DR is designed for online use at an observatory. If an observer has not taken appropriate calibrations, we wish to point it out to them in the strongest terms because we do not want them to end up with un-reduceable data.



next up previous 98
Next: Overriding defaults
Up: The ORAC-DR Calibration Selection
Previous: What happens

ORAC-DR: Overview and General Introduction
Starlink User Note 230
Frossie Economou, Tim Jenness,
Malcolm Currie, Andy Adamson, Alasdair Allan, Brad Cavanagh
Joint Astronomy Centre, Hilo, Hawaii
June 2004
E-mail:ussc@star.rl.ac.uk

Copyright © 1997-2004 Particle Physics and Astronomy Research Council