The timeline code is provided on ifarm via module load timeline.
Please report any issues to the software maintainers, such as warnings or error messages.
This step is integrated in the cooking workflow using the "qtl" model; see the Chefs' documentation wiki for details. Output files will appear in your chosen output directory, within hist/detectors/.
If you are not using the cooking workflow...
See the detailed procedure's Step 1 instead. The cooking workflow's "qtl" model just runs
qtl histogramwith the appropriate arguments.
For physics QA timelines...
Note: we are working on combining the procedure for physics timelines with that for detector timelines; until then, to get the full set of physics timelines, the procedure is separate. For Step 1, either:
- Use the
--physicsoption with the workflow "qtl" model- Use
qtl histograminstead of the workflow, with the option--focus-physics; this will run on SLURM directly (rather than through SWIF)
In general, run:
qtl analysis -i $out_dir/hist/detectors -p $publish_dirwhere $out_dir is the output directory from Step 1 and $publish_dir is the publishing directory to clas12mon.
Additional options may be needed for your specific dataset, so check the usage guide by running with no arguments:
qtl analysisA URL will be printed upon success, and a link will appear in clas12mon in your run group's area momentarily.
For physics QA timelines...
Run
qtl physicsinstead ofqtl analysis; its options are similar.
Tip
Step 2 runs on an interactive node and can take some time if there are a lot of data. We recommend using tools such as tmux terminal multiplexer or GNU Screen to keep the job running if you lose your SSH connection.
Tip
Step 2 produces temporary files, by default in a subdirectory of ./outfiles/. Consider making a symbolic link named outfiles pointing to somewhere on /volatile.
For more details, see other guides in the table of contents or reach out to the software maintainers.