shrink "white light" image by 3% on either end to avoid bringing in erroneous data from shifted slices
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*** empty log message ***
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removed
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testing removal
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small grammatical tidy-ups, added NOD_SKY_THERMAL to recipe list
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Do not compare the slit angles.
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Use observation type matching ARC.
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initial uist version
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update with correct wavelength values
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updated with correct wavelength values
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Added POL_JITTER to available recipes.
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More accurate dispersions, mostly low resolution. Added ARC observation type translation, and REDUCE_ARC to available recipes.
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Use the slit name in the sub-group selection and in the group name and filenames. Added note why the names are so long. Use the correct Notes in the podule.
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Use the slit name in the sub-group selection. Added messages before creating each flat detailing the subset attributes. Explicit flat display instead of DISPLAY_FLAT_IMAGE which compares with the current frame. Fixed typo's.
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No need to restrict the stored declination to nearest deciarcsecon. Improve related comments.
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Cope with negative declinations correctly.
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Correct the information message to the intended meaning.
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Limit to KAPPA gt 1.1-1 for working WCSADD.
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Store first approximation grating dispersion values of early April.
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Restrict to target and OBJECT obstype frames.
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Add distortion correction before registration.
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Move isaac2oracdr.csh to bin/.
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Original version.
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Original version
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Third main version
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Original version
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added module xmlDir
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Use ISAAC_DISTORTION as the domain name.
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Original version
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quick description of this dir
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make admin directory and move nongeneric_imaging.csh there from etc
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Add _to_EQUINOX subroutine, and check for dark sequence/template to assign ORAC_RECIPE to REDUCE_DARK.
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Remove commas from the WCSREG command line.
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Added ISAAC notes and output data names. Call _BIAS_CORRECT_GROUP_ after flat fielding.
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Added INGRID and ISAAC notes, and output data names. Call _BIAS_CORRECT_GROUP_ after flat fielding.
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Added INGRID and ISAAC notes, and output data names. Call _BIAS_CORRECT_GROUP_ and _FORM_SKY_LEVELS_ after flat fielding.
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Original version
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Original version
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Can now flat field the sky frames via a new argument FLATSKY, which defaults to true. Added some section headings.
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Record the template sky frame for the current cycle after masking deviant pixels, and restore that template for all the sky frames in the cycle after the flat has been made. This permits the sky frames to be flat-fielded before sky subtraction.
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Remove SKY_LEVELS storage. Now use _FORM_SKY_LEVELS_ on the prenormalised _flat-fielded_ sky frames for this purpose. No reporting of the modes now they're for internal use. Improved final report.
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Original version.
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Add _REMOVE_ELECTRONIC_GHOSTING_.
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Made default PERCENTILE 98 to bring it into line with other _GENERATE_OFFSETS_ primitives. Also works better for galaxies.
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Allow for some old data where the CTYPE1 was Detector Rows.
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Original dummy version for most instruments.
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Original CVS version.
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Add alias for isaac2oracdr C-shell script until the infrastructure can handle ISO dates and times in filenames automatically.
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Original null version.
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Allow for _bc registration files.
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Use broadened median to combine frames.
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Correct typo' in prologue.
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Allow for _bc registration files.
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fix tt mode error
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Up-to-date FCFs from Vicki
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Add possible cause to negative mode error message. Some tidying of number formatting.
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Return the number of good pixels in NUMBER argument.
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Combine my changes (including documentation) to warn against negative signals after dark subtraction with Brad's.
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comment out STANDARD == 1 line
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Added wvm_html
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Unwrap c1-c4 entries
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decrease detection threshhold to 1.0 sigmas
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update to version 4.0
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