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.\"
.\" hdfsee man page
.\"
.\" Copyright © 2012 Thomas White <taw@physics.org>
.\"
.\" Part of CrystFEL - crystallography with a FEL
.\"
.TH HDFSEE 1
.SH NAME
hdfsee \- HDF5 image viewer
.SH SYNOPSIS
.PP
.B hdfsee \fIimage.h5\fR [\fIoptions\fR] \fB...\fR
.PP
\fBhdfsee --help\fR
.SH DESCRIPTION
hdfsee is a simple image viewer for images stored in HDF5 files.
.PP
Most of the options that can be set on the command line can be changed via the user interface once the program is running. The command line options are to help when running hdfsee from a script.
.SH OPTIONS
.PD 0
.IP "\fB-p\fR \fIfilename\fR"
.IP \fB--peak-overlay=\fR\fIfilename\fR
.PD
Peak locations will be read from \fIfilename\fR and displayed on the image. The peak location file can use the format used in CrystFEL stream files for lists of integrated reflections, i.e. including the Miller indices. If a line cannot be read using this format, it will be assumed to be a simple two-column list of fast scan and slow scan coordinates. Any text beyond the second column will be ignored. If the line cannot be read in either format, it will be ignored.
.PD 0
.IP \fB--ring-size=\fR\fIradius\fR
.PD
Set the radius of the rings used for displaying peak locations. The radius is given in pixels on the screen, i.e. the circles are drawn \fIafter\fR binning the image data.
.PD 0
.IP "\fB-b\fR \fIb\fR"
.IP \fB--binning=\fR\fIb\fR
.PD
Show the image after binning down by a factor of \fIb\fR.
.PD 0
.IP "\fB-e\fR \fIpath\fR"
.IP \fB--image=\fR\fIpath\fR
.PD
Get the image data to display from \fIpath\fR inside the HDF5 file. For example: \fI/data/rawdata\fR. If this is not specified, the default behaviour is to display the first two-dimensional dataset with both dimensions greater than 64.
.PD 0
.IP "\fB-g\fR \fIfilename\fR"
.IP \fB--geometry=\fR\fIfilename\fR
.PD
Display the image data according to the geometry description in \fIfilename\fR. Out of plane components of the geometry will be ignored. This is required, in addition to a beam file, to display resolution rings.
.PD 0
.IP "\fB-m\fR \fIfilename\fR"
.IP \fB--beam=\fR\fIfilename\fR
.PD
Get beam parameters from \fIfilename\fR. This is required, in addition to a geometry file, to display resolution rings. Note that the short version of this option is \fB-m\fR, not \fB-b\fR as for all other CrystFEL programs.
.PD 0
.IP "\fB-i\fR \fIn\fR"
.IP \fB--int-boost=\fR\fIn\fR
.PD
Multiply the intensity in the image by \fIn\fR before displaying. With n=1, the top of the colour scale will represent the maximum pixel intensity found in the image.
.PD 0
.IP \fB--show-rings\fR
.PD
Show resolution rings on the image at 1 Angstrom intervals. You must provide both a geometry and a beam file to use this option.
.PD 0
.IP \fB--simple-rings=\fR\fIradii\fR
.PD
Show rings on the image with the radii specified. \fIradii\fR can be a comma-deliminated list of several values, for example \fI100,200\fR. The radii have units of pixels on the detector before bininng. You must provide a geometry file to use this option.
.PD 0
.IP \fB-c\fR \fIscale\fR
.IP \fB--colscale=\fR\fIscale\fR
.PD
Use \fIscale\fR as the colour scale. Possible scales are: \fBmono\fR, \fBinvmono\fR and \fBcolour\fR.
.PD 0
.IP \fB--median-filter=\fR\fIn\fR
.PD
Apply a median filter with box "radius" \fIn\fR to the image. Each pixel will be set to the median of the values from a \fI(n+1)\fRx\fI(n+1)\fR square centered on the pixel. This might help with peak detection if the background is high and/or noisy. The \fIunfiltered\fR image will be used for the final integration of the peaks. If you also use \fB--noise-filter\fR, the median filter will be applied first.
.PD 0
.IP \fB--filter-noise\fR
.PD
Apply a noise filter to the image with checks 3x3 squares of pixels and sets all of them to zero if any of the nine pixels have a negative value. This filter may help with peak detection under certain circumstances. The \fIunfiltered\fR image will be used for the final integration of the peaks, because the filter is destroys a lot of information from the pattern. If you also use \fB--median-filter\fR, the median filter will be applied first.
.SH AUTHOR
This page was written by Thomas White.
.SH REPORTING BUGS
Report bugs to <taw@physics.org>, or visit <http://www.desy.de/~twhite/crystfel>.
.SH COPYRIGHT AND DISCLAIMER
Copyright © 2012 Deutsches Elektronen-Synchrotron DESY, a research centre of the Helmholtz Association.
.P
hdfsee, and this manual, are part of CrystFEL.
.P
CrystFEL is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version.
.P
CrystFEL is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details.
.P
You should have received a copy of the GNU General Public License along with CrystFEL. If not, see <http://www.gnu.org/licenses/>.
.SH SEE ALSO
.BR crystfel (7),
.BR pattern_sim (1),
.BR crystfel_geometry (5).
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