Difference between revisions of "Elong-13-05-02"
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Rates code now matches what Patricia gets. The issue was in the spectrometer acceptance -- I was using a larger acceptance based on old calculations of what the SHMS could do. This has been fixed, the points on Azz and b1d have been moved to the central x value that the range is over, and the dark points on the kinematics plots show where the spectrometers will sit. This is using [[Elong-13-05-01-Azz-Method-2#Azz_Formalism_-_Method_2|what I've called Azz method 2]] to calculate the uncertainties. | Rates code now matches what Patricia gets. The issue was in the spectrometer acceptance -- I was using a larger acceptance based on old calculations of what the SHMS could do. This has been fixed, the points on Azz and b1d have been moved to the central x value that the range is over, and the dark points on the kinematics plots show where the spectrometers will sit. This is using [[Elong-13-05-01-Azz-Method-2#Azz_Formalism_-_Method_2|what I've called Azz method 2]] to calculate the uncertainties. | ||
| − | == | + | ==Current Good Estimate, No x Cuts== |
| − | [[Image: 2013-05-02- | + | Cuts: W>2 |
| + | [[Image: 2013-05-02-100percent.png]] | ||
| + | ==No x Cuts, Loose W cut== | ||
| − | + | Cuts: W>1.85 | |
| + | [[Image: 2013-05-02-loosew.png]] | ||
| − | + | == == | |
Revision as of 15:04, 3 May 2013
Rates Update
Rates code now matches what Patricia gets. The issue was in the spectrometer acceptance -- I was using a larger acceptance based on old calculations of what the SHMS could do. This has been fixed, the points on Azz and b1d have been moved to the central x value that the range is over, and the dark points on the kinematics plots show where the spectrometers will sit. This is using what I've called Azz method 2 to calculate the uncertainties.
Current Good Estimate, No x Cuts
Cuts: W>2
No x Cuts, Loose W cut
Cuts: W>1.85
