Open vvolkl opened 5 years ago
Indeed, one of the tests is currently failing (RecCalorimeter.recTopoClustersBarrelCaloSystemElecNoise
) since it is trying to access to:
/afs/cern.ch/user/a/azaborow/public/FCCSW/elecNoise_ecalBarrel_50Ohm_traces2_2shieldWidth_noise.root
which may not exist anymore.
we really need to invest some time on some simple condition database as well. Javier do you have some expertise with this?
Le 5 mars 2019 à 09:57, Javier Cervantes notifications@github.com<mailto:notifications@github.com> a écrit :
Indeed, one of the tests is currently failing (RecCalorimeter.recTopoClustersBarrelCaloSystemElecNoise) since it is trying to access to:
/afs/cern.ch/user/a/azaborow/public/FCCSW/elecNoise_ecalBarrel_50Ohm_traces2_2shieldWidth_noise.roothttp://cern.ch/user/a/azaborow/public/FCCSW/elecNoise_ecalBarrel_50Ohm_traces2_2shieldWidth_noise.root
which may not exist anymore.
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we really need to invest some time on some simple condition database as well.
@clementhelsens what do you mean with simple condition database?
I mean instead of having files stored on afs or cvmfs that can be used for calibrations, or event unit tests, we can have them in a database to keep track
Le 5 mars 2019 à 10:01, Javier Cervantes notifications@github.com<mailto:notifications@github.com> a écrit :
we really need to invest some time on some simple condition database as well.
@clementhelsenshttps://github.com/clementhelsens what do you mean with simple condition database?
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Hi Clement, for actual detector conditions such as alignment we should investigate also DD4hep https://github.com/AIDASoft/DD4hep/tree/master/DDCond For now I don't see a problem with keeping a few root files with noise maps etc. on eos, but it's true, at one point a database will be a better solution
Hi Valentin, last time I talked about DDCond with Markus Frank, it was not usable, but maybe things have changed. I don’t like much having too root many files on eos, as it really hard to keep track once people leaves. Clement
Le 5 mars 2019 à 11:00, vvolkl notifications@github.com<mailto:notifications@github.com> a écrit :
Hi Clement, for actual detector conditions such as alignment we should investigate also DD4hep https://github.com/AIDASoft/DD4hep/tree/master/DDCond For now I don't see a problem with keeping a few root files with noise maps etc. on eos, but it's true, at one point a database will be a better solution
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A quick search of FCCSW configs turns up the following files on eos:
All the hepmc files can be easily produced on the fly. In addition, there are the following files not in
testsamples
on eos, which should be moved there: