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Adding Two Secondary Datasets for JME POG #43534
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please test |
+code-checks Logs: https://cmssdt.cern.ch/SDT/code-checks/cms-sw-PR-43534/38116
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A new Pull Request was created by @jordan-martins (Jordan Martins) for master. It involves the following packages:
@AdrianoDee, @miquork, @sunilUIET can you please review it and eventually sign? Thanks. cms-bot commands are listed here |
+1 Summary: https://cmssdt.cern.ch/SDT/jenkins-artifacts/pull-request-integration/PR-1ec2c8/36394/summary.html Comparison SummarySummary:
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Hi @jordan-martins , following the full ReReco 2022/2023 based on CMSSW_14_0_X, is it necessary to backport to 13_3_X and 13_0_X? Or will JME POG have special production under those cmssw versions? On the other hand, the HLTs for some skims are different between 2022 and 2023. I will put both years' HLTs together for these skims to synchronize 2022 and 2023 full ReReco skim after this PR is merged. |
Hi @youyingli, We will have a special production for the JETMET for 2022 and 2023 plus the Muon and EGamma 22FG PDs. For that, we will use the 130X. At some point, it was unclear if we wanted to move to 133X, mainly because of the nanov13 (yet to be concluded at 133X), hence why the backport for that as well, and not 132X or 131X. Thanks for checking the HLTs skims, indeed, as you highlighted, we will do a full ReRECO of 2022 and 2023 in 140X that will require not only Skims but AlCa outputs to be available for those years based on the PDs (as some had naming changes :) ). Is it clear? Thanks, |
Thanks for the clarification. @sunilUIET, could you please sign it and its backports? Thanks! |
+pdmv |
This pull request is fully signed and it will be integrated in one of the next master IBs (tests are also fine). This pull request will now be reviewed by the release team before it's merged. @antoniovilela, @rappoccio, @sextonkennedy (and backports should be raised in the release meeting by the corresponding L2) |
+1 |
Hi,
This PR addresses the ongoing effort within JME POG to understand the highPt Jets tail highlighted by the dijet analysis. The idea is to provide two SDs from Muon (Z+jets) and EGamma (Photon+jets) PDs streamed by specific HLT paths.
In this PR we offer the following:
1- in the scope of this PR, 2022 has Muon and EGamma, and 2023 has EGamma[0,1] and Muon[0,1]
2- given that a full ReRECO of 2022 and 2023 is on the horizon, 2022 PDs have been allowed (removed the #) so that PdmV can ask for the Skims as a whole for all the PDs.
There will be a backport to 13_3_X and 13_0_X.
Thanks,
PPD