- Timestamp:
- 11/10/04 16:11:37 (20 years ago)
- Location:
- trunk/MagicSoft/TDAS-Extractor
- Files:
-
- 2 edited
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trunk/MagicSoft/TDAS-Extractor/Changelog
r5322 r5370 19 19 20 20 -*-*- END OF LINE -*-*- 21 22 2004/11/10: Markus Gaug 23 * Pedestal.tex: put a copy of Wolfgangs two emails with definitions 24 and explications 21 25 22 26 2004/10/27: Oscar Blanch Bigas -
trunk/MagicSoft/TDAS-Extractor/Pedestal.tex
r5244 r5370 15 15 } 16 16 17 \subsection{Copy of email by W. Wittek from 25 Oct 2004 and 10 Nov 2004} 18 19 20 \subsubsection{Pedestal RMS} 21 22 We all know how it is defined. It can be completely 23 described by the matrix 24 25 \begin{equation} 26 < (P_i - <P_i>) * (P_j - <P_j>) > 27 \end{equation} 28 29 where $i$ and $j$ denote the $i^{th}$ and $j^{th}$ FADC slice, 30 $P_i$ is the pedestal 31 value in slice $i$ for an event and the average $<>$ is over many events. 32 \par 33 34 By definition, the pedestal RMS is independent of the signal extractor. 35 Therefore no signal extractor is needed for the pedestals. 36 37 \subsubsection{Bias and Error} 38 39 Consider a large number of signals (FADC spectra), all with the same 40 integrated charge $ST$ (true signal). By applying some signal extractor 41 we obtain a distribution of extracted signals $SE$ (for fixed $ST$ and 42 fixed background fluctuations). The distribution of the quantity 43 44 \begin{equation} 45 X = SE-ST 46 \end{equation} 47 48 has the mean $B$ and the RMS $R$ 49 50 \begin{eqnarray} 51 B &=& <X> \\ 52 R^2 &=& <(X-B)^2> 53 \end{eqnarray} 54 55 One may also define 56 57 \begin{equation} 58 D^2 = <(SE-ST)^2> = <(SE-ST-B + B)^2> = B^2 + R^2 59 \end{equation} 60 61 $B$ is the bias, $R$ is the RMS of the distribution of $X$ and $D$ is something 62 like the (asymmetric) error of $SE$. It is the distribution of $X$ (or its 63 parameters $B$ and $R$) which we are eventually interested in. The distribution 64 of $X$, and thus the parameters $B$ and $R$, depend on $ST$ and the size of the 65 background fluctuations. 66 \par 67 68 By applying the signal extractor to pedestal events you want to 69 determine these parameters, I guess. 70 71 \par 72 By applying it with max. peak search you get information about the bias $B$ 73 for very low signals, not for high signals. By applying it to a fixed window, 74 without max.peak search, you may get something like $R$ for high signals (but 75 I am not sure). 76 77 \par 78 For the normal image cleaning, knowledge of $B$ is sufficient, because the 79 error $R$ is not used anyway. You only want to cut off the low signals. 80 81 \par 82 For the model analysis you need both, $B$ and $R$, because you want to keep small 83 signals. Unfortunately $B$ and $R$ depend on the size of the signal ($ST$) and on 84 the size of the background fluctuations (BG). However, applying the signal 85 extractor to pedestal events gives you only 1 number, dependent on BG but 86 independent of $ST$. 87 88 \par 89 90 Where do we get the missing information from ? I have no simple solution or 91 answer, but I would think 92 \begin{itemize} 93 \item that you have to determine the bias from MC 94 \item and you may gain information about $R$ from the fitted error of $SE$, which is 95 known for every pixel and event 96 \end{itemize} 97 98 The question is 'How do we determine the $R$ ?'. A proposal which 99 has been discussed in various messages is to apply the signal extractor to 100 pedestal events. One can do that, however, this will give you information 101 about the bias and the error of the extracted signal only for signals 102 whose size is in the order of the pedestal fluctuations. This is certainly 103 useful for defining the right level for the image cleaning. 104 \par 105 106 However, because the bias $B$ and the error of the extracted signal $R$ depend on 107 the size of the signal, applying the signal extractor to pedestal events 108 won't give you the right answer for larger signals, for example for the 109 calibration signals. 110 111 The basic relation of the F-method is 112 113 \begin{equation} 114 \frac{sig^2}{<Q>^2} = \frac{1}{<m_{pe}>} * F^2 115 \end{equation} 116 117 Here $sig$ is the fluctuation of the extracted signal $Q$ due to the 118 fluctuation of the number of photo electrons. $sig$ is obtained from the 119 measured fluctuations of $Q$ ($RMS_Q$) by subtracting the fluctuation of the 120 extracted signal ($R$) due to the fluctuation of the pedestal RMS : 121 122 \begin{equation} 123 sig^2 = RMS_Q^2 - R^2 124 \end{equation} 125 126 $R$ is in general different from the pedestal RMS. It cannot be 127 obtained by applying the signal extractor to pedestal events, because 128 the calibration signal is usually large. 129 130 In the case of the optimum filter, $R$ may be obtained from the 131 fitted error of the extracted signal ($dQ_{fitted}$), which one can calculate 132 for every event. Whether this statemebt is true should be checked by MC. 133 For large signals I would expect the bias of the extracted to be small and 134 negligible. 135 136 A way to check whether the right RMS has been subtracted is to make the 137 Razmick plot 138 139 \begin{equation} 140 \frac{sig^2}{<Q>^2} \quad \textit{vs.} \quad \frac{1}{<Q>} 141 \end{equation} 142 143 This should give a straight line passing through the origin. The slope of 144 the line is equal to 145 146 \begin{equation} 147 c * F^2 148 \end{equation} 149 150 where $c$ is the photon/ADC conversion factor $<Q>/<m_{pe}>$. 151 17 152 %%% Local Variables: 18 153 %%% mode: latex 19 154 %%% TeX-master: "MAGIC_signal_reco" 20 155 %%% TeX-master: "MAGIC_signal_reco" 156 %%% TeX-master: "MAGIC_signal_reco" 21 157 %%% End:
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