Comparison of methods to extract an asymmetry parameter from data

Several methods to extract an asymmetry parameter in an event distribution function are discussed and compared in terms of statistical precision and applicability. These methods are: simple counting rate asymmetries, event weighting procedures and th…

Authors: J"org Pretz

Comparison of methods to extract an asymmetry parameter from data
Comparison of metho ds to extract an asymmetry parameter from data J¨ org Pretz ∗ Physikalisches Institut, Universit¨ at Bonn, 5 3115 Bonn, German y Abstract Sev eral metho ds to extract an asymmetry parameter in an even t d istribution func- tion are d iscussed and compared in terms of statistical precision and applicabilit y . These metho ds are: simple counting rate asymmetries, ev ent w eighti ng pro cedures and the unbinned extended maxim um lik eliho o d metho d. I t is kno wn th at w eight- ing metho ds reac h the same figure of merit (FOM) as the likeli ho od metho d in the limit of v anishing asymmetries. T h is article pr e sen ts an improv ed we ighting pro ce- dure reac h i ng th e F O M of the lik eliho od metho d for arbitrary asymmetries. Cases where the maxim u m lik eliho o d metho d is not app lic able are also d iscussed. Key wor ds: ev ent w eighti ng, min ima l v ariance b ound, Cram ´ er-Rao inequalit y, asymmetry extraction, optimal observ ables, parameter d et ermination, maximum lik eliho od P ACS: 02.70.Rr, 13.88.+e 1 In tr o duction W e consider t w o differen tial ev ent distributions n ± ( x ) f o llo wing the functional form n ± ( x ) = α ( x )(1 ± β ( x ) A ) . (1) In a typical exp erime n tal situation encoun tered in pa rticle ph ysics α ( x ) in- cludes a flux and acceptance factor and β ( x ) is an analyzing p o w er. Both dep en d o n a set of kinematic v ariables here denoted by x . Concrete examples ∗ corresp onding author Email addr ess: j org.pretz@cern. ch (J¨ org Pretz). Preprint submitted to Elsevier 29 Octob er 2018 are spin cross section asymmetries and muon deca y . In the latter case the asymmetry corresp onds to the muon p olarization. The tw o data sets (+ and − ) are for example o bta ine d by c hanging the sign of a p o larization. The goal is to extract the parameter A by measuring t he eve nt distributions n ± ( x ). This w ould be an easy task if b oth α ( x ) and β ( x ) we re know n. Ho we v er in man y applications the factor α ( x ) is not kno wn, or not accurately enough kno wn and o nly β ( x ) is giv en. Section 2 presen ts v arious metho ds to extract the parameter A : The simplest metho d, based on coun ting rate asymmetries, the more efficien t extended un- binned maxim um lik eliho o d (EML) metho d and finally metho ds based on ev en t w eighting are discussed. While in Section 2 we assume that the fa c t o r α ( x ) is the same f or b oth data sets, Section 3 extends the discussion to the case where one has t wo different factors. Up to Section 3 w e a s sume that the n umber of observ ed ev en ts is large enough so that av erages can b e replaced b y the corresp onding exp ec t a tion v alues. Effects o ccurring at low statistics ev en t samples are discussed in Section 4. A summary and conclusions are give n in Section 5. 2 Differen t Metho ds to extract A 2.1 Determining A fr om c ounting r ate a s ymm etry The exp ectation v alue of the nu m b er of eve nts for the tw o data sets reads D N ± E = Z n ± ( x )d x = (1 ± h β i A ) Z α ( x )d x (2) with h β i = R αβ d x/ R α d x . The in tegrals run o ver the kinematic range of x . The a s ymmetry A can b e extracted without the kno wledge of R α ( x )d x : A = 1 h β i h N + i − h N − i h N + i + h N − i . (3) Eq. (3) leads to fo llowing estimator for A : ˆ A cnt = N + + N − P + β i + P − β i N + − N − N + + N − = N + − N − P + β i + P − β i where β i ≡ β ( x i ), N + and N − are the num b ers of o bs erved ev en ts. The sums P + and P − run ov er all ev en ts in the corresp onding data set (+ o r − ). 2 As shown in Section 2.3 and App. A, the figure of merit (F OM), i.e. the inv erse of the v a r ianc e on ˆ A cnt , is F OM ˆ A cnt = N h β i 2 1 − A 2 h β 2 i (4) where N = N + + N − denotes t he total n umber o f ev ents. This figure of merit ma y b e increased if a cut is set to remov e some data with lo w v alues of β . How ev er, it will not reac h t he FOM o f the unb inned extended lik eliho o d metho d discussed now, unless β ( x ) is constan t. 2.2 Extende d Maximum Likeliho o d (EML) Metho d W e no w turn to the unbinne d extended maxim um lik eliho o d (EML) metho d[1,2] whic h is known to r each t he Cram ´ er-Ra o limit of the lo we st p ossible statistical error. The log- likelihoo d function derived from Eq. (1 ) reads l = X + ln ( α i (1 + β i A )) − h N + i ( A ) + X − ln ( α i (1 − β i A )) − h N − i ( A ) . Using the expression in Eq. (2) for the exp e ctation v alues h N ± i results in l = X + ln (1 + β i A ) + X − ln (1 − β i A ) − 2 Z α ( x )d x − X + , − ln α i . (5) The last t wo terms do not dep end on A and can b e ignored in the lik eliho o d maximization. The asymmetry A can thus b e determined without know ledge of α ( x ). F or small v alues of β A one can ev en deriv e an analytic expression for ˆ A LH whic h reads ˆ A LH = P + β i − P − β i P + β 2 i + P − β 2 i . (6) F or arbitrary asymmetries the maximization has to b e done num erically . Note, that this requires CPU intensiv e sums ov er all ev en ts in the maximization pro cedure. The fig ure o f merit (F O M ) is giv en by F OM ˆ A LH = − ∂ 2 l ∂ A 2 = X + β 2 i (1 + β i A ) 2 + X − β 2 i (1 − β i A ) 2 . 3 Replacing the sum ov er ev ents by in tegrals o ne finds F OM ˆ A LH = Z α (1 + β A ) β 2 (1 + β A ) 2 d x + Z α (1 − β A ) β 2 (1 − β A ) 2 d x = Z 2 αβ 2 1 − β 2 A 2 d x . (7) Noting, that for an ar bitrary function f ( x ) the av erage is defined b y h f i = R f ( x ) ( n + ( x ) + n − ( x ))d x R n + ( x ) + n − ( x )d x = R α ( x ) f ( x )d x R α ( x )d x , the figure of merit can b e written as F OM ˆ A LH = N * β 2 1 − β 2 A 2 + . (8) 2.3 Weighting Metho d Next, consider the follow ing estimator ˆ A w = P + w i − P − w i P + w i β i + P − w i β i (9) where w i ≡ w ( x i ) is a, for the moment arbitrary , w eight factor assigned to ev ery ev ent. The exp ectation v alue of ˆ A w equals A indep ende ntly of the w eigh t function w ( x ) used. App. A sho ws that F OM ˆ A w = N h w β i 2 h w 2 (1 − A 2 β 2 ) i . (10) Tw o cases a re o f intere st: 1.) Setting w = 1 corresp onds to the coun ting rate asymmetry discussed in Section 2.1 and pro ves Eq. (4) f or the FOM. 2.) In the case w = β the FOM is F OM ˆ A w = β = N h β 2 i 1 − A 2 h β 4 i h β 2 i . A comparison with Eq. (8) indicates tha t FOM ˆ A w = β coincides with the FOM of the likelihoo d metho d fo r v a nishing A . Actually , in this case, the t w o es- 4 timators ar e iden tical as can b e see n b y comparing Eq. (9) with w ≡ β and Eq. (6). Note tha t the estimator ˆ A w can b e applied for arbitrary asymmetries as w ell, accepting a decrease of t he F OM compared the EML estimator as discusse d in Section 2.5. Suc h a weigh t ing pro cedure has b een used for example in Refs. [3,4] to extract spin asymmetries in the case where h β i A ≪ 1. In Ref. [5] a w eigh ting metho d is discussed to sim ultaneously extract signal and background asymmetries . The fact that a weigh ting pro cedure reac hes the same FOM as the EML metho d w as first discussed in Ref. [7] in the con text o f signal and bac kground extractions. The next section sho ws that one can find a w eigh t factor reac hing the FOM of the EML metho d ev en in the case of non- v anishing asymmetries. 2.4 Impr ove d Weighting Metho d V ariational calculus sho ws (s. App. B) that t he maxim um F OM is reache d using a we ig h t factor w = β 1 − β 2 A 2 0 . (11) Here, A 0 is a first estimate of t he a s ymmetry A obtained fo r ex ample from the w eigh ting metho d presen ted in Section 2 .3 . The w eighting factor defined in Eq. (11) leads to the fo llo wing estimator (the index iw stands for improv ed w eigh t ) ˆ A iw = P + β i 1 − β 2 i A 2 0 − P − β i 1 − β 2 i A 2 0 P + β 2 i 1 − β 2 i A 2 0 + P − β 2 i 1 − β 2 i A 2 0 . (12) Eq. (10) giv es F OM ˆ A iw = N D β 2 1 − β 2 A 2 0 E 2 D β 2 1 − β 2 A 2 (1 − β 2 A 2 0 ) 2 E . (13) Th us giv en a go o d estimate A 0 ≈ A , we get FOM ˆ A iw = FOM ˆ A LH , i.e. the impro ve d w eigh ting metho d reac hes the same F OM a s the EML method for arbitrary a symmetries as we ll with the adv an ta ge that no CPU consuming maximization pro cedure is needed. 5 Count in g rate w eight in g Lik eliho o d Impro ved w eighti ng asymmetry metho d metho d metho d Figure of merit N h β i 2 1 − A 2 h β 2 i h β 2 i 1 − A 2 h β 4 i h β 2 i D β 2 1 − β 2 A 2 E T able 1 The r atio F OM/ N for v arious metho ds d iscu ssed. Before w e mo ve to a comparison of the differen t metho ds, w e note that the estimator ˆ A = P + β + i − P − β − i P + ( β + i ) 2 + P − ( β − i ) 2 + A 0 with β ± = β 1 ± β A 0 (14) reac hes as w ell the FOM of the EML for A ≈ A 0 , In con trast to ˆ A iw its exp ectatio n v alue o nly equals A if A 0 ≈ A . F or τ deca ys the optimal w eight factor in Eq. (14) is discussed in Ref. [6]. 2.5 Comp arison of differ ent metho ds T ab. 1 summarizes the FOM of the v a r io us estimators prop osed. Fig . 1 sho ws the figure of merit o f the differen t estimators vs. A for the c ho ic e α ( x ) = const. = 2 500 and β ( x ) = x, 0 < x < 1 . (15) The curv es are a naly tic calculations. The p oin ts are results of sim ula t io ns . F or eac h v alue of the asymmetry 10000 configurations with α = 2500 , whic h corresp onds on av erage to 50 00 ev ents , w ere sim ulated. One configur a tion consists of a plus and min us data set used to ev aluate an asymmetry . F or each of the 1 0000 configuratio ns sim ulated, the asymmetries we re calculated using the estimators dis cussed abov e. The FOM w as dete rmined from the RMS of the asymmetry distributions. The results are in p erfect agreemen t with the analytic calculations. The sta- tistical errors of the sim ulat ions are of the order of the size of the p oin t s. Note, t ha t for all metho ds no bias w as found for the asymmetry . The question of bias and the range of v alidit y of the expressions for the F OM will be dis- cussed in more detail in Section 4. The weigh ting metho ds are sup erior to the 6 A 0 0.2 0.4 0.6 0.8 1 FOM 0 500 1000 1500 2000 2500 3000 3500 4000 4500 5000 counting rate weighting improved weighing Likelihood Fig. 1. Figure of mer it for different metho ds as a function of the asymmetry A . metho d using simply the coun ting rates. As exp ec t e d the improv ed weigh ting or the EML metho d reac h a higher FOM than the simple we ig h ting method the la rger the asymmetry A . The results dep end of course o n the shap e of α ( x ) and β ( x ). The gain in F OM using w eigh t ed ev en ts compared to coun ting rates dep ends o n the spread of β ( x ). F or A = 0 for example it is h β 2 i / h β i 2 as can b e deriv ed from Eq. (10). Fig. 2 sho ws the influence of the choic e of A 0 on the FOM in the impro ved w eigh t ing metho d for the factor s α and β as given in Eq. ( 15 ) and an a sym- metry A = 0 . 8. Cho osing A 0 in a range 0.7– 0.86, one reache s a t least 99% of F OM ˆ A LH . The normal w eighting metho d cor r esp onds to A 0 = 0. 3 Differen t acceptance/flux factor in t he t wo data sets W e now turn to the case where the acceptance and flux factor α is not the same in the t wo data se ts. W e ass ume that they differ by a known factor c whic h is indep end en t of x . In this case the differen tial eve nt distributions are giv en by n + ( x ) = 2 c 1 + c α ( x )(1 + β ( x ) A ) and (16) n − ( x ) = 2 1 + c α ( x )(1 − β ( x ) A ) . (17) 7 0 A 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 iw A /FOM LH A FOM 0.9 0.92 0.94 0.96 0.98 1 Fig. 2. FOM ˆ A iw / F OM ˆ A LH for A = 0 . 8 as a fu nctio n of A 0 . The factor 2 / (1+ c ) has been in tro duced in order to normalize the distributions to the same num b er of ev en ts for all v alues of c at A = 0. The log lik eliho o d function reads l = X + ln  2 c 1 + c α i (1 + β i A )  − D N + E ( A ) + X − ln  2 1 + c α i (1 − β i A )  − h N − i ( A ) = X + ln (1 + β i A ) + X − ln (1 − β i A ) + X + ln 2 c 1 + c α i + X − ln 2 1 + c α i − 2 Z α d x − 2 A c − 1 1 + c Z αβ d x . (18) Here the last term cannot b e ignored b ecause it con ta ins the parameter A and th us the lik eliho o d metho d cannot b e applied without kno wledge of the factor R αβ d x . The w eighting metho d on the other hand can b e applied with a small mo dification: ˆ A w ,c = P + w i − c P − w i P + w i β i + c P − w i β i . (19) The exp ec tation v alue of ˆ A w ,c equals again A . The figure o f merit reads (deriv a- 8 A 0 0.2 0.4 0.6 0.8 1 FOM 0 500 1000 1500 2000 2500 3000 3500 4000 4500 5000 c=1 c=2 c=3 Fig. 3. Figure of merit for three different v alues of c as a f unction of the asymmetry A , assu ming the same num b er of ev ents in the case A = 0. tion see s. App. C) F OM ˆ A w,c = N 4 c (1 + c ) 2 h w β i 2 D w 2 (1 − β 2 A 2 )  1 − β A 1 − c 1+ c E . (20) The F OM is show n in Fig. 3 for differen t v alues of c for the improv ed we ig h ting metho d. As in Fig. 1 the lines corresp ond to an analytic calculation using Eq. (20), the points are results of sim ulations. Note, t ha t for arbitrary c the w eigh t reac hing the highest FOM is w = β (1 − β 2 A 2 )  1 − β A 1 − c 1+ c  . The EML method could b e used for c 6 = 1, if one uses an estimate for R αβ d x ≈ P + β ( x i ) + c P − β ( x i ) from data. Sim ulations sho wed that the F O M of this mo dified EML metho d equals the one of the improv ed w eighting metho d. 4 V alidit y at low n um b er of eve n ts In this section w e discuss the v alidity o f t he equations derive d fo r the v arious F OMs and p ossible biases of the estimators. The form ula s w ere deriv ed us- 9 time + - + - + - + - + - + - + - + - + - + - + - + - + - small config. asymmetry larger configuration asymmetry Fig. 4. C ombining data in d iffe r e n t configur ations. T he b o xes denote the plus and min u s data sets. ing usu al error propagation and can th us only be appro ximations whic h are the b etter the higher N . In the simulations presen ted in Section 2.5 for ev ery v alue of the asymmetry 100 0 0 configurations we r e sim ulated with on a verage 5000 even ts (corresp onding to α = 2500 in Eq. (15)). In eac h of these config- urations t he asymmetry was determined using the v ario us estimators. In this section w e discuss effects o ccurring if the asymmetries are extracted in smaller configurations, as indicated in Fig. 4. F o r lo w er n umber of eve n ts in o ne configuration one reac hes a p oin t where due to statistical fluctuations the estimated asymmetry in a giv en configuration can b e larger than 1 or smaller than − 1. In this case the EML metho d is no more applicable since the term (1 ± β A ) can get negative. F or α = 250 this happ ens in ab out 1% of the configurations for an asymmetry of A = 0 . 8. Dividing the sample f ur t her in many smaller configurations one reac hes a p oin t where one ha s o nly 0 or 1 ev en t in one configura t ion. This limit can also b e obt a ine d b y dividing the sample in man y narrow bins of β ha ving a t most one ev en t in a bin. In this case the remaining estimators are iden tical: ˆ A cnt ≡ ˆ A w = β ≡ ˆ A iw = ± 1 /β i . The sign dep end s whether the ev en t o ccurred in the plus or the m in us data set. One finds D ˆ A iw E = A a nd D ˆ A 2 iw E = 1 /β 2 i , th us the FOM for this ev en t reads F OM i = 1 D ˆ A iw E 2 − D ˆ A 2 iw E = β 2 i 1 − β 2 i A 2 . Note that A is not the estimated asymmetry from a s ing le ev ent but rather tak en fr o m a larger ev en t sample. Combining all the asymmetries determined on single ev ents leads to P i ± 1 β i · F OM i P i F OM i = P + 1 β i β 2 i 1 − β 2 i A 2 − P − 1 β i β 2 i 1 − β 2 i A 2 P + β 2 i 1 − β 2 i A 2 + P − β 2 i 1 − β 2 i A 2 . (21) 10 Assuming A = A 0 , Eq. (21) is nothing but the estimator of the impro ve d w eigh t ing metho d, ˆ A iw , defined in Eq. (12). In other words, for the impro ve d w eigh t ing metho d it mak es no differences whether the da t a ar e analyz ed in one large configuratio n or in many small o ne s. The impro ved we ig h ting is also equiv alen t to using a n infinite n umber of bins in β and ev alua t ing the asymmetries in eve ry bin and then com bining the results. The adv an tag e of the impro ved w eighting metho d is that this binning has not t o b e p erformed. The obse rv ations discusse d ab o v e are c onfirmed b y sim ula t ions . In tota l 1 0 9 configurations with α = 0 . 025 w ere sim ulated. The sim ulated data w ere a na- lyzed as fo llo ws. First the asymmetries were calculated in the appro ximately 5% of the configurations actually con taining at least one ev ent. Then the w eigh t e d a verage of these asymmetries is calculated. The same data w ere an- alyzed in a differen t w a y by com bining 10 configurations and calculating the asymmetries in these la rger configurations corresp onding to α = 0 . 2 5 . This pro cedure w as rep eated un t il r e a c hing 10 4 configurations with α = 25 0 0. Fig . 4 illustrates the pr o cedure. Thes e simulations w ere p erformed for an asymmetry of 0.8 generating ev en ts in the range 0 . 01 < β ( x ) < 0 . 99 . Fig. 5 shows the mean v alue of the asymmetries and the stat istical error f or the v a rious estimators for the different v alues of α . As expected the estimator ˆ A iw giv es the same result indep e nden t of α . No bias is observ ed within the statistical error whic h is of the order of 10 − 4 . The asymmetry for the EML metho d is o nly sho wn for α = 2 5 00 since at low er v alues, as explained ab o v e, the EML metho d is no more a pplicable. Fig. 6 sho ws the distribution of the asymmetry ˆ A iw for differen t v alues of α . The en tries in the histograms in Fig. 6 are w eighted b y their correspo nd ing F OM. In the case α = 2500 this w o uld not b e nece ssary b ecause all entries ha ve essen tially the same F OM for a giv en metho d since t he relativ e v aria t ion of the num b er of ev en ts N a nd t he av erages lik e P ± β 2 i / N entering the FOM v ary only v ery little from configuratio n to configuration. At lo w er v alues of α , ho we ver, this is no more the case. T aking ag ain t he extreme case where the asymmetries is calculated from single ev ents , the FOM dep ends on the v alue of β for this even t. This explains wh y the n umber of en tries is smaller tha n 1 in some bins of the histogra m s. At α = 0 . 025 the num b er of configurations is 10 9 . The corresp onding histogram has o nly appro ximately 4 . 9 · 10 7 en tries reflecting the fact that in most of the configuratio n there is no ev en t. Finally , Fig . 7 sho ws the FOM/ N calculated fr o m the RMS of the asymmetry distributions presen ted in Fig. 6 for differen t v a lue s of α . The three lines corresp ond to F OM ˆ A iw / N , FOM ˆ A w = β / N and FOM ˆ A cnt / N calculated using the expressions g iv en in T ab. 1. F or α ≥ 25 there is go od agreemen t with the F OM deriv ed in Section 2 since the p oin ts coincide with the corresp onding lines. A t low er v alues of α the F OM of the w eigh ting and the coun ting rate 11 α -2 10 -1 10 1 10 2 10 3 10 asym metry A 0.7995 0.7996 0.7997 0.7998 0.7999 0.8 0.8001 0.8002 0.8003 0.8004 0.8005 counting rate weighting improved weighing Likelihood Fig. 5. Results for the asymmetry of the simulatio n s as a function of the a ve r a ge n u m b er of eve nts in one configuration. The p oin ts are at α = 0 . 025 , 0 . 25 , 2 . 5 , 25 , 250 , 2500, resp ectiv ely . F or a giv en v alue of α they are sligh tly disp l aced on the horizonta l axis for b etter r e ad ab ility . Note, that v alues at different v alues of α are correlated since the same data were used. metho d start to increase and finally reach as exp ected FOM ˆ A iw at α = 0 . 0 2 5, where the three estimators are practically identical. 5 Summary & Conclusions W e presen ted sev eral estimators to extract an a symmetry parameter A in a num b er densit y function. These estimators w ere based on coun ting ra tes , ev en t w eighting and the un binned extended maximum lik eliho od method. A w eigh t ing pro cedure w as deriv ed tha t reaches the same figure of merit as the un binned maxim um lik eliho o d metho d, kno wn to reach t he minimal v ar ianc e b ound. This w eighting estimator is giv en as an analytic expression, whereas in the EML metho d the maximization of the lik eliho o d function has to b e do ne n umerically . Moreo ve r t his estimator can b e used (with a small mo dification) 12 β w= A -100 -50 0 50 100 nb. of entries 10 4 10 7 10 =0.025 α Entries = 4.88e+07 Mean = 0.7999 RMS = 1.31 11 β w= A -100 -50 0 50 100 nb. of entries -1 10 10 3 10 5 10 7 10 =0.25 α Entries = 3.93e+07 Mean = 0.7999 RMS = 1.1776 β w= A -100 -50 0 50 100 nb. of entries -2 10 10 4 10 7 10 =2.5 α Entries = 9.93e+06 Mean = 0.7999 RMS = 0.5915 β w= A -1 -0.5 0 0.5 1 1.5 2 2.5 3 nb. of entries 2 10 4 10 6 10 =25 α Entries = 1000000 Mean = 0.7999 RMS = 0.1877 β w= A 0.2 0.4 0.6 0.8 1 1.2 1.4 nb. of entries 3 10 4 10 5 10 6 10 =250 α Entries = 100000 Mean = 0.7999 RMS = 0.0595 β w= A 0.7 0.75 0.8 0.85 0.9 nb. of entries 4 10 5 10 6 10 =2500 α Entries = 10000 Mean = 0.7999 RMS = 0.0187 Fig. 6. Distributions of the estimated asymmetries ˆ A iw for different v alues of α . α -2 10 -1 10 1 10 2 10 3 10 FOM/N 0.3 0.35 0.4 0.45 0.5 0.55 0.6 counting rate weighting improved weighing Likelihood Fig. 7. Figur e of merit p er eve nt for differen t metho ds a s a function of α f or an asymmetry A = 0 . 8. The lines sh o w the exp ect ation calcula ted from the exp r essio n s giv en in T ab. 1 . 13 in cases where the EML metho d cannot b e applied b ecause of an incomplete kno wledge o f ev ent distribution function. Ac kno wledgmen t s : I am g rateful to Jean- Marc Le Goff fo r n umerous dis cus- sions on the sub ject, v erifying the calculations and for carefully reading the man uscript. 14 A Figure of merit of ˆ A w T o calculate the F OM o f ˆ A w defined in Eq. (9), o ne needs σ 2 ( P w i ), σ 2 ( P w i β i ) and co v ( P w i , P w i β i ). F or t wo arbit r a ry quan tities f and g the co v ariance b et w een P f i and P g i is co v( X i f i , X j g j ) (A.1) = * X i = j f i g i + X i 6 = j f i g j + − * X i f i + * X j g j + (A.2) = h N i h f g i + h N ( N − 1) i h f i h g i − h N i 2 h f i h g i (A.3 ) = h N i h f g i + D N 2 E − h N i − h N i 2  h f i h g i . (A.4) If the n umber of ev ents N is P oisson distributed, i.e. h N 2 i − h N i − h N i 2 = 0, one finds co v( X i f i , X j g j ) = h N i h f g i ≈ X i f i g i . (A.5) Setting f = g = w , f = g = w β and f = w , g = w β results in σ 2 ( X w i ) = h N i D w 2 E , (A.6) σ 2 ( X w i β i ) = h N i D ( w β ) 2 E , (A.7) co v( X w i , X w i β i ) = h N i D w 2 β E . (A.8) Simple erro r propa g ation in Eq. (9 ) finally leads to Eq. (1 0 ) for the figure of merit. B Optimal weigh t Denoting the w eight factor whic h maximizes the FOM by w 0 , w e consider small deviation f r o m this optim um b y w ( x ) = w 0 ( x ) + ǫ η ( x ) (B.1) where η ( x ) is arbitr a ry a nd ǫ ≪ 1. 15 Inserting Eq. (B.1) in Eq. ( 1 0 ) ke eping terms of 1st order in ǫ one finds F OM = ( h w 0 β i + ǫ h η β i ) 2 h ( w 2 0 + 2 ǫw 0 η ) (1 − β 2 A 2 ) i . (B.2) The conditio n ∂ FOM /∂ ǫ = 0 giv es w 0 = β 1 − β 2 A 2 . C F OM for the case c 6 = 1 The error for the estimator defined in Eq. ( 19) is obtained by simple error propagation taking in to accoun t t he correlatio ns b et we en P w β and P w .  F OM ˆ A w,c  − 1 = ~ v T C ~ v with ~ v T = ∂ ˆ A w ,c ∂ ( P + w i ) , ∂ ˆ A w ,c ∂ ( P − w i ) , ∂ ˆ A w ,c ∂ ( P + w i β i ) , ∂ ˆ A w ,c ∂ ( P − w i β i ) , ! = 1 P + w i β i + c P − w i β i (1 , − c, − A, − cA ) (C.1) and C =           P + w 2 i 0 P + w 2 i β i 0 0 P − w 2 i 0 P − w 2 i β i P + w 2 i β i 0 P + ( w i β i ) 2 0 0 P − w 2 i β i 0 P − ( w i β i ) 2           . (C.2) This leads to Eq. (20). References [1] R. J. Barlow, Statistics, Wiley 1989 [2] R. J. Barlow, Nucl. Instru m. Meth. A 297 (1990) 496. 16 [3] D. Adams et al. [S p in Muon Collaboration (SMC)], Ph ys. Rev. D 56 (1997 ) 5330 [4] E. S. Ageev et al. [COMP AS S Collab o ration], Ph ys. Lett. B 612 (2005) 154 [5] J. Pretz and J. M. Le Goff, Nucl. Instrum. Meth. A 602 (2009 ) 594 [6] M. Da vier, L. Duflot, F. Le Dib erder and A. Rouge, Phys. Lett. B 306 (1993) 411. [7] R. J. Barlow, J. Comput. Ph y s . 72 (1987) 202. 17

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