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| author | Thomas White <taw@physics.org> | 2013-11-06 17:07:55 +0100 |
|---|---|---|
| committer | Thomas White <taw@physics.org> | 2013-11-06 17:07:55 +0100 |
| commit | a92b6fa6ebc393c6943637f7a69a46b4ffe722e5 (patch) | |
| tree | 1c1d4859ff7bd9e33e8e1ff02931b37cb770c204 | |
| parent | 1958c15d63555cc5c17f26a586e39d6d00dbcaca (diff) | |
Update docs
| -rw-r--r-- | doc/man/compare_hkl.1 | 6 |
1 files changed, 6 insertions, 0 deletions
diff --git a/doc/man/compare_hkl.1 b/doc/man/compare_hkl.1 index 825dbd09..8ae7574c 100644 --- a/doc/man/compare_hkl.1 +++ b/doc/man/compare_hkl.1 @@ -108,6 +108,12 @@ Use intensity shells instead of resolution shells. The range of shells will sta .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. +.PD 0 +.IP \fB--shell-file=\fR\fIfilename\fR +.PD +Write the statistics in resolution shells to \fIfilename\fR. + + .SH AUTHOR This page was written by Thomas White. |