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Hi,

I found my old talk with the proof-of-principle energy estimator.  It was in Dec. 2021 (!!):

https://indico.fnal.gov/event/52371/

On the slides (p. 11) it looks like I claim 3% muon energy resolution around Emu=1 GeV, though the plot there suggests 4% is maybe a fairer number to quote.  It's also worth recognizing that this number is a fairly strong function of the true neutrino energy because of track reconstruction/PID inefficiency (at the low end) and containment issues (at the high end).  (The slides also reminded me that at the time I didn't make any effort to use the actual PID GNN, but rather just used track length as a muon PID, which worked ~ok.  Using the actual PID algorithm should recover many of the ones I lost at low Emu due to my very crude muon selection.)

-Jeremy

On 4/4/23 11:58 PM, Drielsma, Francois wrote:
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Hi everyone,

 

We'll hold our ML meeting tomorrow, Wed. Apr. 5th at 2 PM CT on the usual zoom:

 

https://stanford.zoom.us/my/drielsma?pwd=WU16RGJtWGtKZ0I2N04xSlN6Y2lXdz09 (ID: 973 985 8922, PW: 105658)

 

If you have any slides you'd like to share, please make sure to upload them to this page:

 

https://indico.slac.stanford.edu/event/7988/

 

All the best,
Francois and Kazu



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