VIEW: Difference between revisions

No change in size ,  7 February 2008
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If the integration has worked as it should, the following should be true:
If the integration has worked as it should, the following should be true:
- most (if not all) observed reflections are encircled by thin lines (corresponding to integration areas)
* most (if not all) observed reflections are encircled by thin lines (corresponding to integration areas)
- empty integration areas belong to weak reflections
* empty integration areas belong to weak reflections
- reflections without integration area are partial reflections, whose center is on an adjacent frame
* reflections without integration area are partial reflections, whose center is on an adjacent frame


Note: the pixel numbering in VIEW goes from 0 to NX-1 (similar for y), whereas XDS using a numbering of 1 to NX (NY). Thus, if you find out a position on the detector (e.g. the direct beam) by using VIEW, you should add 1 in both x and y if you want to put the numbers into [[XDS.INP]].
Note: the pixel numbering in VIEW goes from 0 to NX-1 (similar for y), whereas XDS using a numbering of 1 to NX (NY). Thus, if you find out a position on the detector (e.g. the direct beam) by using VIEW, you should add 1 in both x and y if you want to put the numbers into [[XDS.INP]].


VIEW -h  gives a short help output with options, VIEW -hv shows a short manual.
VIEW -h  gives a short help output with options, VIEW -hv shows a short manual.
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