From 129ddd9f60ff61b3bd7ec87b9c5d108d1d54045d Mon Sep 17 00:00:00 2001 From: Thomas White Date: Wed, 8 Feb 2023 15:43:37 +0100 Subject: crystfel_geometry(5): Add missing documentation for 'bandwidth' --- doc/man/crystfel_geometry.5 | 7 ++++++- 1 file changed, 6 insertions(+), 1 deletion(-) (limited to 'doc/man') diff --git a/doc/man/crystfel_geometry.5 b/doc/man/crystfel_geometry.5 index 66a3d71b..6056c463 100644 --- a/doc/man/crystfel_geometry.5 +++ b/doc/man/crystfel_geometry.5 @@ -1,7 +1,7 @@ .\" .\" Geometry man page .\" -.\" Copyright © 2012-2021 Deutsches Elektronen-Synchrotron DESY, +.\" Copyright © 2012-2023 Deutsches Elektronen-Synchrotron DESY, .\" a research centre of the Helmholtz Association. .\" .\" Part of CrystFEL - crystallography with a FEL @@ -81,6 +81,11 @@ These statements specify the incident radiation wavelength. You must include on .IP Units should be specified after the value (or location). These can be \fBm\fR or \fBA\fR for \fBwavelength\fR, \fBeV\fR or \fBkeV\fR for \fBphoton_energy\fR, and \fBV\fR or \fBkV\fR for \fBelectron_voltage\fR. For \fBphoton_energy\fR, if no units are given then the value will be taken to be in eV. +.PD 0 +.IP "\fBbandwidth = \fIbw" +.PD +The bandwidth of the radiation, expressed as a fraction of the wavelength. The bandwidth will be interpreted as the standard deviation of a Gaussian spectrum, and used for calculating reflection positions. + .PD 0 .IP "\fBdetector_shift_x = \fInnn \fB[m|mm]" .IP "\fBdetector_shift_y = \fInnn \fB[m|mm]" -- cgit v1.2.3