. 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

... The procedure of radiometer signal integration can be considered as a sort of reducing dimension of the initial sampling space, where the samples are the result of analog-to-digital conversion. ... The probability distribution of the signal and spikes is completely known. ... The quality of the considered algorithm could be also illustrated by Figure 2 . ... One could see the considered adaptive algorithm is preferable even by low degree of compression, because all spikes have been depressed. ...

... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. The Roche model is assumed. Proximity effects of components (reflection of radiation and surface gravity darkening) are taken into account. ... Figure 1: The surface temperature distribution for Algol A-B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation effect. ...

... Classes . ... casa::Geometric . ... Discrete geometric distribution. ... Geometric ( RNG *gen, Double probability=0.5) . Construct a random number generator for a geometric uniform distribution. virtual . ... probability () const . ... The second argument defines the range of possible return values for this distribution as described in the synopsis. virtual casa::Geometric::~Geometric . ... virtual Double casa::Geometric::operator() . ... virtual Vector < Double > casa::Geometric::parameters . ...

... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...

... 13-Aug-2014 12:13 106K lk_20140815_0905.tar.. 15-Aug-2014 09:06 106K lk_20140901_0823.tar.. 01-Sep-2014 08:23 103K lk_20141016_1324.tar.. 16-Oct-2014 13:25 103K lk_20141211_1708.tar.. 11-Dec-2014 17:08 103K lk_20150430_0315.tar.. 30-Apr-2015 03:15 103K lk_20150430_0420.tar.. 30-Apr-2015 04:20 103K lk_20150818_1511.tar.. 18-Aug-2015 15:11 104K lk_20151113_1903.tar.. 13-Nov-2015 19:04 105K lk_20160314_0610.tar.. 14-Mar-2016 06:11 105K . ...

... The low energy plasma composition spectrometer AMEI-2 is built to be able to find in the low energy range of the phase space (E, q, j) and separate the fluxes of the major ion species in the magnetotail - H+, He++, He+ and O+, and analyse their energy and angular distributions. ... Electrostatic angular scanning in one direction and the use of the spin of the satellite to sample the other angle give the ability to measure 2-D distributions for each ion specie several times per spin. ...

... A clear description of El Nino Southern Oscillation and of its consequence on climate in Australia and South America is available at El Nino or ENSO theme pages of the NOAA climate diagnosis center. ( historical comparison of previous elninos with soi indices ) . This image shows cold water upwelling near the coast of Peru (purple) and joining the South Equatorial Current, which flows westward across the Pacific Ocean. ... July 16, 1998 : Satellite image shows pacific stabilizing . ...

... It consists of two energy-angle analyzers EA-2 and EA-3 for low energy particles, and two identical oppositely directed time-of-flight (TOF) analyzers EM-1-1 and EM-1-2 for high energies. ... Analyzers of low energy charged particles (EA-2 and EA-3). ... The instruments allow to measure simultaneously in eight angular sectors evenly distributed in the angle 2 perpendicular to the satellite rotation axis, and sequentially in 7 energy intervals for each angular sector. ... Interval . ...

. Below are links to the theoretical energy distributions of WR stars included in the database of Leitherer et al. (1996; PASP, 108, 996). You can use the links below to read a description of the models (Readme file), and to download the files. Readme file . ftp directory with the individual files All data available for mass FTP at: . ftp ftp.stsci.edu login anonymous password your username cd science/starburst/Schmutz . Last update: December 15, 2001 - Claus Leitherer