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HFEGammaSLCorrector.cc
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#include "
HFEGammaSLCorrector.h
"
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#include "CLHEP/Vector/LorentzVector.h"
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namespace
hf_egamma
{
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double
eSeLCorrected
(
double
es,
double
el,
double
pc,
double
px,
double
py){
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double
x =
log
(el/100) ;
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double
y = es / el ;
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return
pc + px*x + py*y ;
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}
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double
eSeLCorrected
(
double
es,
double
el,
int
era
){
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double
pc=0.0,px=0.0,py=0.0;
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switch
(era) {
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case
(0):
//Data 41
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pc = -1.02388e-1 ;
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px = -1.51130e-1 ;
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py = 9.88514e-1 ;
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break
;
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case
(1):
//Fall 10 MC
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pc = -4.06012e-2 ;
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px = -1.34769e-1 ;
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py = 9.90877e-1 ;
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break
;
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case
(2):
//Spring 11 MC
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pc = 5.98732e-3 ;
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px = -1.74767e-1 ;
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py = 9.84610e-1 ;
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break
;
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case
(3):
//Summer 11 MC
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pc = -0.036416 ;
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px = -0.195854 ;
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py = 0.980633 ;
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break
;
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case
(4):
//July 5 Data
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pc = -0.008077 ;
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px = -0.216002 ;
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py = 0.976393 ;
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break
;
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}
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//After fitting the 2D histogram, we find a y-intercept b, a slope m,
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//and a point x0 around which we choose to rotate the data points. We
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//will map (x,y) --> (x,y') where y' = pc + px*x + py*y, with
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//pc = sin(atan(m))*x0 - cos(atan(m))*(m*x0+b), px = -sin(atan(m)),
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//and py = cos(atan(m)). This transformation preserves the x-value of the
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//data point and takes y' to be the y-value of the original point after it
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//is rotated through angle atan(m) (to flatten the line of best fit) and
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//transposed vertically downward by b (to make the line of best fit coincide with the x-axis).
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return
eSeLCorrected
(es, el, pc, px, py) ;
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}
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}
hf_egamma
Definition:
HFEGammaSLCorrector.cc:4
year_2016_cff.era
era
Definition:
year_2016_cff.py:7
cmsBatch.log
log
Definition:
cmsBatch.py:343
hf_egamma::eSeLCorrected
double eSeLCorrected(double es, double el, double pc, double px, double py)
Definition:
HFEGammaSLCorrector.cc:6
HFEGammaSLCorrector.h
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