...
I've run a few streams of diagnostic muons and all gamma with the CR track finder turned on. It appears that the all of the Acd2CR variables are being filled. I look at a few variables in a bit more detail. Specifically I show comparisons between the distance to active tiles and the energy deposited in active tiles between the cosmic-ray tracks , and the tree-based tracks, and the MC truth. All plots are made requiring at least one cosmic-ray track.tracking. To compare on equal footing, I apply the cut:
Code Block |
---|
"TkrNumTracks > 0 && TkrCRNumTracks > 0" |
The distributions look very similar for both photons and muons.
Diagnostic Muons
Acd2CRActiveDist3D | Acd2CRActDistTileEnergy |
---|---|
|
|
Acd2CR1ActiveDist | Acd2CR1ActDistTileEnergy |
|
|
...
Acd2CRActiveDist3D | Acd2CRActDistTileEnergy |
---|---|
|
|
Acd2CR1ActiveDist | Acd2CR1ActDistTileEnergy |
|
|
CR-Only Tracks
To get a very precursory look at what we can gain from the CR tracking, I look at events in the muon sample where the CR tracker finds a track but the tree-based tracking does not:
Code Block |
---|
TkrNumTracks==0 && TkrCRNumTracks > 0 |