. XMM-Newton Science Analysis System . calmosalgo (calmosalgo-2.7.2) [xmmsas_20080701_1801-8.0.0] . Meta Index / Home Page / Description This algorithm computes the ideal unperturbed response of the detector to a single photon with a given input energy. Add detailed description of employed model. XMM-Newton SOC/SSC -- 2008-07-01

... Classes . ... casa . casa::HyperGeometric . ... Hypergeometric distribution. ... HyperGeometric ( RNG *gen, Double mean=0.5, Double variance=1.0) . Construct a random number generator for an hypergeometric distribution. virtual . ... These function allow you to manipulate the parameters (mean & variance) described above through the base class. virtual Vector < Double > . ... virtual Double casa::HyperGeometric::operator() . ... virtual Vector < Double > casa::HyperGeometric::parameters . ...

... Archives . ... Clauset, Shalizi, & Newman (2007, arXiv/0706.1062 ) have a very detailed description of what power-law distributions are, how to recognize them, how to fit them, etc. ... Though it may not be a complete answer, I wanted to say that I learned applying the K-S test for the first time to test a homogeneous Poisson process from a spatial statistics class in a similar manner as this paper describes. ... Raoul LePage on From Terence?s stuff: You want proof? . ... Chandra Blog . ...

... Files . include <stdio.h> . ... Include dependency graph for tmsolve.c: . dust_tmatrix . dust_mkBmatrix ( dust_tmatrix *tm) . ... dust_TMSolve ( dust_tmatrix *tm) . Calculate the energy bin probability distribution of a grain by solving transition matrix. void . ... dust_tmatrix dust_mkBmatrix . ... References dust_tmatrix::data , and dust_tmatrix::M . Referenced by dust_TMSolve() . ... References dust_tmatrix::data , dust_mkBmatrix() , dust_normalisepvect() , and dust_tmatrix::M . ...

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

... The absolute flux calibration of NICMOS will be calculated from observations of standard stars with known flux distributions F( ). ... In order to expand the set of IR standard stars in the appropriate flux range for NICMOS, M. Rieke, R. Thompson, and collaborators at the University of Arizona are making photometric observations of solar-analog stars, which will be used to normalize the solar spectrum to the observed IR magnitudes. ... Relative flux references accurate to 1.5% for standard...

Планета Земля и Луна . ... Космическая защита . Луна . Фотографии . ... Строение Луны . ... Страница: Начало одиссеи , Экспедиции , Море Кризисов , "Аполлон-8" , "Аполлон-9" , "Аполлон-10" , "Аполлон - 11" , E-8 "Луноход" , Испытания Л-1 , Луноход - 1,2 , КА "Луна 1-24" , КА "Луна-9" , Луна от КА СССР ; . Луна - наш космический спутник . ... Снимки Луны от аппаратов серии Луна и Зонд (СССР) . Фотографии космических аппаратов серии "Луна" (также Луноходы) и "Зонд" - СССР . ... Зонд 3 . ...

... A response matrix is a discrete representation of a given instrument's response to incoming photons. ... This presentation is a preliminary report on MKRMF, a new tool developed by the Chandra X-ray Science Center (CXC), to calculate RMFs appropriate for the variety of science instruments on-board Chandra (Wise 1998). ... These external redistribution functions are stored using a new FITS format developed by the CXC for encapsulating functions. ... axes file : . ... list file : . ... CXC RMF Format ...