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Hi everyone, sorry for the repeated emails but due to issues with the workflows/networks the final three 10 GeV inbending runs are in an additional directory, /volatile/clas12/rg-a/production/pass0/Spring18/dst/rga_sp18_inb_10GeV_physics_2/dst/train, instead
of the first one I listed.
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<div>Best regards,</div>
<div>Timothy<br id="lineBreakAtBeginningOfMessage">
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<div>On Feb 6, 2025, at 10:38 PM, Timothy Hayward <haywardt@mit.edu> wrote:</div>
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Dear RGA,
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<div>Although many of the workflows seem to be stuck at around 95% (if you stick to using the trains that won’t be a problem as they only appear in the train outputs when completed), I wanted to send out this email now to give you as much time as possible to
have a look at the Spring 2018 physics validation runs before next Wednesday. Unfortunately, the previous runs that I sent out were cooked with the wrong AI network (they used the Fall 2018 versions which should amount to about a 1% difference at most) and
were critically missing the helicity information. The new directories should be the final versions.</div>
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<div><b>10 GeV inbending </b>(currently only 4/7 runs with completed trains but the rest could appear at any moment)</div>
<div>/volatile/clas12/rg-a/production/pass0/Spring18/dst/rga_sp18_inb_10GeV_physics_1/dst/train/</div>
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<div><b>10 GeV outbending </b></div>
<div>/volatile/clas12/rg-a/production/pass0/Spring18/dst/rga_sp18_outb_10GeV_physics/dst/train/</div>
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<div><b>6 GeV inbending</b></div>
<div>/volatile/clas12/rg-a/production/pass0/Spring18/dst/rga_sp18_inb_6GeV_physics/dst/train/</div>
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<div><b>6 GeV outbending</b> (currently no runs with completed trains but they could appear at any moment)</div>
<div>/volatile/clas12/rg-a/production/pass0/Spring18/dst/rga_sp18_outb_6GeV_physics/dst/train/</div>
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<div><b>inbending luminosity scan</b> (4302 - 10 nA, 4303 - 30 nA, 4180 - 50 nA, 4177 - 75 nA)</div>
<div>/volatile/clas12/rg-a/production/pass0/Spring18/dst/rga_sp18_inb_10GeV_luminosity_scan/dst/train/</div>
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<div><b>outbending luminosity scan</b> (3210 - 25 nA, 3970 - 45 nA, 3987 - 45 nA)</div>
<div>/volatile/clas12/rg-a/production/pass0/Spring18/dst/rga_sp18_outb_10GeV_luminosity_scan_1/dst/train/</div>
<div>/volatile/clas12/rg-a/production/pass0/Spring18/dst/rga_sp18_outb_10GeV_luminosity_scan_2/dst/train/</div>
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<div>Where possible, comparisons to Fall 2018 results (without using developed post-processing algorithms like momentum corrections) would be particularly useful. There have already been a few analyses and so far things look very promising. Please let me know
if you have any questions. </div>
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<div>Best,</div>
<div>Timothy</div>
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