Bayesian Background Estimation
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1 Bayesian Background Estimation
2 mum knot spacing was determined by the width of the signal structure that one wishes to exclude from the background curve. This paper extends the earlier work in two important directions; first by employing adaptive splines
3 BAYESIAN APPROACH TO BACKGROUND ESTIMATION
4 we shall see, the evidence plays a central role in determining the number of spline knots,
5 In this paper we allow the positions of spline knots v to vary, except for 1 and #, which are fixed at x m i n and x max, respectively. The objective is to allow a variable degree of smoothing for the background. Since the are now parameters that are subject to a probabilistic treatment, we need a prior for them. We pick a general noncommittal prior by assuming it is uniform over the phase space available to the ^ [4]. For the interval from 1 = x m i n to ^ = x max, taking into account the minimum spacing Ax and the required ordering of the knot positions, that is 1 + Ax < 2; 2 + Ax < 3; E-I + Ax
6 When
7 10 U -5" 10 ~o 10" (drb,)/o, FIGURE 2. The likelihood functions for the cases that there is no signal present, and for positive and negative signals
8 Determining auxiliary parameters There are numerous parameters, Aa:, 0% E, (3 and A's, that have so far been assumed to be fixed. These must be specified to perform the data analysis. It is our view that as many of these parameters as possible should be determined from information about the experiment. Other parameters
9 called the evidence. We define the scalar )], (14) which is the minus-logarithm of the integrand in the previous equation. We approximate ty by expanding it to second order in c around its maximum value at c yielding a Gaussian for its exponential. Because the Gaussian is restricted to a narrow region,
10 Variance in background The expectation value of the second moment matrix of 6 is obtained by integrating over the posterior probability of the parameters c and, 6
11 depend on c. What is actually done is to minimize i/j, defined in Eq. (14), with respect
12 vector is the one that had the smallest value for i/j. In probability theory, Marginalization over number of knots
13
14 ln[p(e D)]... Likelihood ---- ln[volume(c) P(c)] LU Number
15 10 10' Energy (arb. units) FIGURE 4. The same PIXE spectrum as in Fig. 1, showing the most probable background estimate obtained using adaptive splines in which the optimal number of knots is found to be 14. In the energy region above 0.25, the estimated background is now smooth, indicating a lack of evidence in the data for the oscillations visible in Fig :* background data with signal o data without signal 10 U Energy (arb. units) FIGURE 5. Data points classified with a background probability greater than 50% as background-only points are depicted by open circles while data points carrying a signal contribution are marked by solid circles. semi-log plot, the curve varies somewhat more rapidly in the linear space in which it is modeled. These adaptive background estimates are very plausible.
16 background uncertainty... contribution
17 $> "w ci o transformed data
18 ing the logarithm of the measured spectrum, the nearly exponential rise of the spectrum is transformed into an approximately linear dependence that is more easily accommodated by the background model. Furthermore, such a transformation of the ordinate does not change the width of the signal structure, leaving unchanged the minimum knot separation criterion. As a general principle for applying our model to a specific spectrum, it may be transformed to bring the background into conformance with the background model, provided the signal contributions do not lose their assumed rapid and localized characteristics. For example, we find that taking the square root of the horizontal scale, after a suitable offset, yields a data record that also provided reasonable estimates of the background. Figure 7b shows the Auger spectrum after the transformation z(k) = log[a y(k)], where y(k)
19 We have developed SUMMARY
20
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