ASC-FITS-2.0.1: ASC FITS File Designers' Guide (Rots and McDowell) (1999 Jun) . ASC-FITS-REGION-1.0: FITS region document (McDowell and Rots) (1998 Mar) . ... CXC-DM-001 Introduction: Data Analysis with the Chandra Data Model (2001 Oct) . ... 1998 Feb 26: SDS-1.0: Data Product List: obsolete . ... 1998 Mar 09: SDS-10.0: (ASC-FITS-REGION-1.0) FITS region document: see ASC-FITS-REGION-1.0 . 1998 Feb 09: SDS-11.0: FITS function document (superseded by ASC-FITS-FUNCTION-1.2) . ...

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• Jonathan's ASC documents
• The AstroStat Slog Blog Archive [ArXiv] Post Model Selection, Nov. 7, 2007
• The AstroStat Slog Blog Archive A Quote on Model

Next: Simulations Up: Maximum Likelihood Estimation of Previous: Introduction . The properties of an ensemble of faint galaxies can be defined by the distribution of the parameters of the models that best fit each individual object. ... The model also includes instrumental parameters, such as the sky background (estimated locally) and amplitude of the noise. ... The probability of the observed value is then computed for each pixel using the adopted error distribution. ...

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• The DIRTY Model. I. Monte Carlo Radiative Transfer through Dust
• Notation and Model
• Modeling Dust and Starlight in Galaxies Observed by Spitzer and Herschel: NGC

... 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...

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• LWN: Driver porting: Device model overview

... 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). ...

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• Informational system "Evolution of RG"

... CentralProcessor 0.11 documentation . Calibration and Imaging Documentation . The cmodel pipeline task is responsible for extracting a local sky model (LSM) from the global sky model (GSM) and building an image from the components and/or images resulting from the request. ... MPI wrapper> cmodel -c config.in . ... None . ... If Cmodel.gsm.database is set to asciitable then a row/column (space separated) file is used as the global sky model source. ... cmodel (Model Image Generator) . ...

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• Fitting a tilted ring model to a warped galactic disk
• Unified Radio Catalog: results for Version 1.1
• Multi-Plane Models

... Next: Cheating Poisson: A Up: Statistical Analysis Previous: Spatial Models and . ... The spatial distribution of stars in the Local Group dwarf irregular galaxy NGC 6822 has been studied, using recent positions and deep photometry for about 15,000 stars in the galaxy. Based on photometrical data, OB stars and red stars could be studied separately. Spatial statistical tools have been applied to the analysis of the spatial structure. ... Figure: Model selection by the aid of CAIC . ...

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• Modelling Spectro-photometric Characteristics of Nonradially Pulsating Stars
• Modelling Spectro-photometric Characteristics of Eclipsing Binaries
• Synthetic Images of the Solar Corona from Octree Representation of 3-D Electron

.

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• Modelling the Milky Way in the Era of Gaia - JD5 programme
• Model of clusters
• Model realization and some results

. Next: Frequency distribution of galactic Previous: Gravitational Wave Sky: An . Frequency distribution of galactic binaries . Structure of the Galaxy . Mike E. Prokhorov . Sat Feb 22 18:38:13 MSK 1997

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• The Model
• Frequency distribution of galactic binaries
• Structure of the Galaxy

... Abstract: We present Monte Carlo radiative transfer simulations for spiral galaxies modelled as a stellar disk and a two-phase clumpy dust distribution. ... As a general result, clumpy models are less opaque than the corresponding homogeneous models. ... 0.00 0.15 0.50 0.1 0.5 1.0 2.0 5.0 10.0 0.25 X . ... We have also produced several homogeneous models, to compare to the clumpy models. ... Homogeneous and clumpy models with the same tauV have the same dust mass. ...

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• Atlas of Monte Carlo Models of Dust Extinction in Galaxies
• HwB: SGI Mouse (Model 021-0004-002) Connector Connector (Offline)
• Francesco Tribioli - More about my hobbies

. This Directory contains Model of distribution of density, temperature and effective collision freguency of electrons. Yu.K.Chasovitin. 1998. This Directory contains The program RIM98 for calculating the parameters of the ionosphere to use the "Reference Ionospheric Model-98" (RIM-98).Yu.K.Chasovitin. 1998.

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• Catalogue 5 of WDC-B

... 08.04.2016 12 апреля состоится гала-концерт Студенческой весны СГАУ . 08.04.2016 Ученые СГАУ получат областную премию . ... 08.04.2016 В СГАУ состоялся День карьеры . Информация Новости Сегодня в СГАУ иностранные студенты области отметили Международный день студента . ... 17 ноября в Международный день студентов в рамках акции - Студенческий марафон по Самарской области на территории нашего университета встретились 135 лучших студентов-иностранцев из 12 вузов Самары и Тольятти. ...

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• Команда иностранных студентов СГАУ приняла участие в VI фестивале русской речи
• Встреча иностранных студентов с ректором
• СГАУ рассчитывает удвоить количество поступивших иностранных студентов

Next: Uncorrelated flux component Up: Introduction Previous: The Hierarchical Stellar Systems Contents . The type parameter allows to select from a range of stellar models, either analytical, or availbale as data files or FITS images. ... For all types from zero to 11, the flux distribution is computed as flat ( teff=0 ), a black body ( teff < 0 ), or a stellar atmosphere ( teff > 0 ). For all types, specifying an arbitrary SED will override stellar spectra or fluxes derived from the images. ...

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• Operations with DFOS: daily workflow, the simple model
• ESO - Thesis Topic: Dynamical models of multiple globular cluster populations
• The Hierarchical Stellar Systems Model Format

... Bojan Nikolic web pages (r. 329) . Understanding Infrared emission from galaxies . This page contains a description and links for download of software that may be used for modelling various aspect of absorption and emission of radiation by interstellar dust. ... Also, some basic modelling of radiation fields and similar supporting code . ... dust-1.0.1 . ... Modelling absorption and emission of radiation by interstellar dust . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• Modelling absorption and emission of radiation by interstellar dust
• Bojan Nikolic -- Fitting and Comparison of Models of Radio Spectra
• Bojan Nikolic -- Nested sampling modelling of Star-Formation History of the

15. The magnetosphere models

16. Distributions and Sobolev spaces (Fall 2005)

17. Астрономия в ГАИШ МГУ: учебники по астрономии, физике: курс астрономии

18. Lesson 1: Using Uncertainties

19. http://xmm.vilspa.esa.es/external/xmm_links/trainee/alumni/a_laruelo.pdf

20. Extinction and transformation models