There is no SIDIS-like train, so let's use DST files for the QA.
Similarly to RG-C, there are several targets that we'll need to combine; let's also combine torus polarities.
The DSTs are found in:
/cache/clas12/rg-e/production/spring2024/pass1/*/*/dst/recon
TODO:
- check if needed; see Fall 2018 RG-K notes
- if reheating is needed, fix
qtl histogrampaths below
Important
Check any run-dependent settings in qa-physics/monitorRead.groovy, such as beam energy.
Note
Using --rundir and --fast-ls here rather than --flatdir, since we're using a directory of DST files.
check cache:
bin/qtl histogram -d rge_sp24 --check-cache --rundir --fast-ls --focus-physics $(ls -d /cache/clas12/rg-e/production/spring2024/pass1/*/*/dst/recon)run:
bin/qtl histogram -d rge_sp24 --rundir --fast-ls --focus-physics $(ls -d /cache/clas12/rg-e/production/spring2024/pass1/*/*/dst/recon)Important
In case any runs disappeared from /cache while running monitoring or reheating, be sure to cross check the output runs with those from /mss
TODO:
- populate
/data/metadatafor RG-E's target types
Make the timelines:
bin/qtl physics -d rge_sp24 -p rge/qa_pass1_sp24Warning
You may not have permission to publish to this directory; if not, publish to another place and ask the chef to copy the files