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authorThomas White <taw@physics.org>2021-01-22 17:06:34 +0100
committerThomas White <taw@physics.org>2021-01-22 17:06:34 +0100
commit1ea31bb393d7f39fd19ea1f34de12de02a32f1b8 (patch)
treefb8f650eb0e0bfb7277e102c7653e0cb3adad476 /doc/man
parent28253276c24cc129047b4435c58d2bd600a1354c (diff)
compare_hkl: Remove --intensity-shells
No-one uses it, it doubles the complexity of the code, and the manual even warns not to use it.
Diffstat (limited to 'doc/man')
-rw-r--r--doc/man/compare_hkl.17
1 files changed, 0 insertions, 7 deletions
diff --git a/doc/man/compare_hkl.1 b/doc/man/compare_hkl.1
index 8c54b4c9..22de7df7 100644
--- a/doc/man/compare_hkl.1
+++ b/doc/man/compare_hkl.1
@@ -125,13 +125,6 @@ High resolution cutoff, as 1/d in m<sup>-1</sup>. Use this or \fB--highres\fR,
.IP \fB--highres=\fR\fId\fR
High resolution cutoff in Angstroms. Use this or \fB--rmax\fR, but not both.
-.PD 0
-.IP \fB--intensity-shells\fR
-.PD
-Use intensity shells instead of resolution shells. The range of shells will start at the intensity of the least intense reflection, and extend from there by 1/5000th of the intensity of the difference between the strongest and weakest reflection in the first reflection list. The pairs of reflections will also be assigned their bins according to the intensity of the reflection in the first list.
-.sp
-Because of the hardcoded factor of 1/5000, needed to avoid a very uneven distribution of the number of reflection pairs in each bin, you are advised not to draw strong conclusions from the results of using this option.
-
.SH AUTHOR
This page was written by Thomas White.