Difference between revisions of "May 10, 2019 - PrimEx-Eta Meeting"
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#* It would good to ask Sean to attend one of the meetings in the future to give a detailed explanation as to how the fcal and rf timing is calculated. | #* It would good to ask Sean to attend one of the meetings in the future to give a detailed explanation as to how the fcal and rf timing is calculated. | ||
#* Ilya pointed out that we will likely need to study each channel of the hadronic background individually with simulations. | #* Ilya pointed out that we will likely need to study each channel of the hadronic background individually with simulations. | ||
+ | #* For some reason, subtracting accidentals reduced the eta yields consistently over all angular bins. This likely indicates an issue with the fitting that needs to be corrected. | ||
# Compton Yields | # Compton Yields | ||
#* uncertainty below 2% over run periods over a week or so | #* uncertainty below 2% over run periods over a week or so |
Revision as of 09:40, 17 May 2019
Time and Place
- Time: Friday, May 10, 2019 2:00 pm EST.
- Room: CEBAF Center, Room F227
Meeting Connections
- If joining via web browser, go to [1] https://jlab.bluejeans.com/7572695553/
- If joining via phone, use one of the following numbers and the Conference ID: 7572695553.
- US or Canada: +1 408 740 7256 or
- US or Canada: +1 888 240 2560
- If joining via Polycom room system go to the IP Address: 199.48.152.152 (bjn.vc) and enter the meeting ID: 7572695553.
Slides
Minutes
- Drew showed some plots (see slides) showing the motivations for the cuts and vetos used in selecting eta -> 2gamma events, as well as highlighting some issues that will need to be studied in detail at a later point.
- These plots were all made using the default calibration constants with a time stamp from the middle of April, so they don't have any updates to the timing or energy calibrations applied.
- It would good to ask Sean to attend one of the meetings in the future to give a detailed explanation as to how the fcal and rf timing is calculated.
- Ilya pointed out that we will likely need to study each channel of the hadronic background individually with simulations.
- For some reason, subtracting accidentals reduced the eta yields consistently over all angular bins. This likely indicates an issue with the fitting that needs to be corrected.
- Compton Yields
- uncertainty below 2% over run periods over a week or so
- There is a several percent shift
- Overview of Ilya's physics talk at the collaboration meeting:
- what is primexd, statistics
- mention compton on different targets
- dNdTheta, constrained mass, elasticity
- Future Plans:
- analyze data
- ask for second run