2000
DOI: 10.1016/s0010-4655(00)00086-2
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Particle tracks fitted on the Riemann sphere

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Cited by 31 publications
(20 citation statements)
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“…There are many other approaches to the circle fitting problem in the modern literature [4,10,35,28,29,31,33,36,38], but most of them are either quite slow or can be reduced to one of the algebraic fits [14, Chapter 8].…”
Section: Algebraic Circle Fitsmentioning
confidence: 99%
“…There are many other approaches to the circle fitting problem in the modern literature [4,10,35,28,29,31,33,36,38], but most of them are either quite slow or can be reduced to one of the algebraic fits [14, Chapter 8].…”
Section: Algebraic Circle Fitsmentioning
confidence: 99%
“…Since points close to the inversion point end up far away in inversive space (see Materials and Methods), a weighting dependent on the distance in “real” space is needed. Our weighting of d 4 is by analogy to Strandlie et al36 For 25,000 randomly selected surface patches of 2–6 Å radius covering the protein PTP‐1B, we found that the residual sum of squares from the plane fit in inverted space follows that of the sphere fit in “real” space with a correlation coefficient of r 2 = 0.93 ( r = 0.97). While the weighting scheme is not perfect, the correlation is nevertheless quite good, and for smaller patches the correlation is higher.…”
Section: Resultsmentioning
confidence: 91%
“…Data with cosmic tracks were taken for several different detector parameters: The track finding and noise suppression was done with a Riemann [6] pattern recognition after clustering. The found tracks were fitted with GENFIT [7], a generic fitting tool based on a Kalman [8] filter.…”
Section: Results From Cosmics Tracksmentioning
confidence: 99%