Difference between revisions of "Elong-13-05-02"

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Rebinned ''x'' values so that they correspond to the ±''x'' error bars shown. For the highest two points, the SHMS and HMS data have been combined.
 
Rebinned ''x'' values so that they correspond to the ±''x'' error bars shown. For the highest two points, the SHMS and HMS data have been combined.
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'''[http://nuclear.unh.edu/~elong/analysis_files/2013-05-05/ The best plots in vector format can be found here.]'''
  
 
[[Image: 2013-05-02-current-best.png]]
 
[[Image: 2013-05-02-current-best.png]]

Latest revision as of 17:41, 5 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.

No x Cuts, W>2

Cuts: W>2

2013-05-02-100percent.png

No x Cuts, Loose W cut

Cuts: W>1.85

2013-05-02-loosew.png

Current Best Numbers

f_phys=f_calc*0.95

W>1.85

Rebinned x values so that they correspond to the ±x error bars shown. For the highest two points, the SHMS and HMS data have been combined.

The best plots in vector format can be found here.

2013-05-02-current-best.png


--E. Long 20:59, 3 May 2013 (UTC)