Allow for sub-array when inverting.
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added the jcmt_chopper module
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create WCS in the cube
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initial addition
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use _GET_PLATE_SCALE_ to determine x and y pixelscales
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initial addition, UIST-specific version
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Original version for ESO AA..BB..BB..AA.. sequences. Starlink style.
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Augment prologue.
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Original version based upon generic code, but added smoothing to _EXTRACT_FIND_ROWS_ and more comments. Starlink style.
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Add note about NBEAMS=0, and clarified to which user header BEAMS is written.
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Steers pair-based spectroscopy recipes. Rewrite for ESO.
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remove duplicate declaration of $param
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Forgot a perldoc link to the primitive.
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Original version adapted from generic version to invoke _GET_ARC_NAME_.
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Original version based upon generic code converted to Starlink style, change from Figaro:ISHIFT to KAPPA:SLIDE, multiply negative beams by -1 before passing to SCROSS.
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restrict RA and Dec seconds to two decimal places
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Removed residual =cut.
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use quadratic interpolation instead of linear
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general tidyup
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do not use variance for mosaicking, update group headers
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update Group header
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large rewrite, growing cube, etc, etc, etc
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use group for standard division
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Set positive-intensity threshold. Make default binsize 5. Report binning boxsize.
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Use LAMP_FLAT recipe for imaging calibration-lamp flat template.
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Switch the sign of the telescope offsets as originally commented.
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Renamed from ISAAC/ with minor documentation changes.
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Moved to ESO tree as should be suitable for other infrared spectroscopes.
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Added LAMP ORAC_OBSERVATION_TYPE for calibration-lamp flats.
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Original version
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Correct documentation typo's.
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Original version
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Removed commented out code line.
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Create a list of distinct filters within the group stored by reference in Grp uhdr FILTER_LIST.
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Original version
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Allow obstype of LAMP.
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Switch calibration thingone and thingtwo to subgrp current frame for display.
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add atools_mon to list of algorithm engines for UIST
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Add POLARIMETRY argument. Pass it to _FIND_APPROX_OFFSETS_.
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Invoke _GENERATE_OFFSETS_ with new POLARIMETRY argument set to 1. Add exaplanatory comments.
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Separate the beam-separation from polarimetry. Former is just for messages when processing polarimetry mosaics. Latter is needed for all polarimetry to ignore the offsets for central-source, unless tying into other frames in the group registered using telescope offsets. Introduce POLARIMETRY argument for this.
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Set OFFSET_TYPE to beam-separation in _GENERATE_OFFSETS_.
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Revise angle based upon analysis by Tim Gledhill.
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