Power-law shot noise

1990 ◽  
Vol 36 (6) ◽  
pp. 1302-1318 ◽  
Author(s):  
S.B. Lowen ◽  
M.C. Teich
Keyword(s):  
2003 ◽  
Vol 24 (4-5) ◽  
pp. 741-756 ◽  
Author(s):  
M.Alper Kutay ◽  
Athina P Petropulu ◽  
Catherine W Piccoli

2015 ◽  
Vol 31 (2) ◽  
pp. 187-207 ◽  
Author(s):  
François Baccelli ◽  
Anup Biswas
Keyword(s):  

2000 ◽  
Vol 48 (7) ◽  
pp. 1883-1892 ◽  
Author(s):  
A.P. Petropulu ◽  
J.-C. Pesquet ◽  
Xueshi Yang

2006 ◽  
Vol 42 (21) ◽  
pp. 1237 ◽  
Author(s):  
H. Koskinen ◽  
T. Tirronen ◽  
J. Virtamo

1999 ◽  
Vol 173 ◽  
pp. 289-293 ◽  
Author(s):  
J.R. Donnison ◽  
L.I. Pettit

AbstractA Pareto distribution was used to model the magnitude data for short-period comets up to 1988. It was found using exponential probability plots that the brightness did not vary with period and that the cut-off point previously adopted can be supported statistically. Examination of the diameters of Trans-Neptunian bodies showed that a power law does not adequately fit the limited data available.


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