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

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

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(ASC-FITS-REGION-1.0) FITS region document: see ASC-FITS-REGION-1.0 . 1998 Feb 09: SDS-11.0: FITS function document (superseded by ASC-FITS-FUNCTION-1.2) .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 A Quote on Model
• The AstroStat Slog Blog Archive [ArXiv] Post Model Selection, Nov. 7, 2007

The Earth's magnetosphere global structure is conditioned by the interaction of the Solar wind and Earth's magnetic field. ... Solar wind (SW) - the region outside BS; . ... Auroral field lines (AUR) region - the funnel-shape cavity restricted by the geocentric distance of the order of 6 RE, between surfaces formed by magnetic field lines emerged from the polar and equatorial OVAL borders; . ... Fairfield D.H., Average and unusual location of the Earth's magnetopause and bow shock, J. Geophys. ...

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lte-codes . Sterne . ... In 2006, Behara and Jeffery introduced a new file format for the model atmospheres produced by STERNE and used by SPECTRUM and SFIT. ... allow depth-dependent descriptions of composition, and . ... model.lambda_ref <lambda ref > . ... abundance < elem > < abund > . ... structure.abundance < elem > : ( needs N depth ) . ab elem,1 , ab elem,2 , ..., ab elem,Ndepth > . ... structure.tau_ref : ( needs N depth ) . ... structure.opac_ref : ( needs N depth ) . ...

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• ffit help file
• Abstract
• Armagh Observatory

... This article is part of the LWN Porting Drivers to 2.6 series . One of the more significant changes in the 2.5 development series is the creation of the integrated device model. The device model was originally intended to make power management tasks easier through the maintenance of a representation of the host system's hardware structure. ... Which devices exist in the system, what power state they are in, what bus they are attached to, and which driver is responsible for them. ...

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• Spectral energy distribution
• Search for distant radio galaxies in SAO
• Laboratory of spectroscopy and photometry of extragalactic objects : Vortex

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

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Information & tools for observers . ... Observers archives tools & information . ... Next Section: Fitting Rotation Curves: Mass . ... Although the approximately flat rotation curves of gas in the outskirts of spirals is generally taken as strong evidence for spherical, isothermal dark matter halos, this conclusion is often incorrect and always model-dependent. ... Fitting Rotation Curves: Mass Models Kinematics ....

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• cmodel (Model Image Generator) CentralProcessor 0.11 documentation
• Current redistribution model for flares
• Evolutionary Paths in Galaxy Morphology

motions, metallicities and Annie Robin (France) ages Large-scale non-equlibrium structures Vasily Belokurov (UK) Non-equlibrium dynamics and radial migration in the disc Alice Quillen ( USA ) Star-formation histories, metallicity distributions and luminosity Rosie Wyse ( USA ) functions of disk, bulge halo Measures of ISM density (absorption, emission at various frequen- ?? cies, polarization, Faraday rotation, dust to gas ratio) Gas ... How do we fit such a model to a catalogue? ...

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• Model realization and some results
• Vladimir P. Reshetnikov's Home Page
• Modelling the Milky Way in the Era of Gaia - JD5 Rationale

... 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"

... 2.3 Establishing the Extragalactic Distance Scale . ... 2.3.2 The Second Rung: Distances to stellar clusters . ... 2.3.4 Distances to Local Group Galaxies . ... The Luminosity Function of Planetary Nebulae . ... 3.2.2 Clusters of Galaxies . ... 4.2 Evidence for Dark Matter as a Function of Scale Size . ... 4.3 Other Dark Matter Indicators for Galaxies . ... What is the nature of the large-scale distribution of matter in the universe as traced by the three-dimensional galaxy distribution? ...

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• Physics 410/510 Observational Cosmology

... Research . ... Laboratory . ... The software developed in the laboratory allows to carry out the whole cycle of the satellite information processing: the initial treatment of the data, coordinate relation, topside ionogram deduction, Ne(h) profiles calculation, global mapping the ionospheric parameters, ionospheric modeling and investigations of the mechanisms of the ionospheric parameters variations with local time, season, magnetic activity level, longitude, latitude, and altitude. ...

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• SMF2 Ionosphere model Title
• Empirical Model of the Nighttime Winter Ionospheric Trough

... Spectral energy distributions (SED) for starburst galaxies and ULIRGs are made public available using self-consistent radiative transfer computations assuming dust for the diffuse ISM ( Siebenmorgen et al, 2014). ... In the library of SED models we consider three basic model paramters and use: . ... the radiative transfer model: Kr gel and Siebenmorgen, 1994, AA 282, 407 . ... The starburst model and the SED library is described by Siebenmorgen and Kr gel, 2007, AA 462, 445 . ...

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• http://www.eso.org/~rsiebenm/agn_models/
• Operations with DFOS: daily workflow, the simple model
• Stellar models

... 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
• research field
• HwB: SGI Mouse (Model 021-0004-002) Connector Connector (Offline)

. 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
• "STP Data" STP Data

... 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
• DUST: dust_model Struct Reference
• Atmospheric Modelling for ALMA Bojan Nikolic web pages (r. 329)

Scale-heights of the Galactic disk subsytems with different ages and metallicities . V.Marsakov & Yu. ... It is based on the fact, that all stars cross the disk plane several times during their Galactic orbital period. ... We have used our representative sample of nearby disk F2-G2 stars Marsakov & Shevelev (1995) in which fundamental stellar parameters was determined on the basis of published date on uvby-photometry, proper motion and radial velocities. ... Marsakov V.A., Shevelev Yu.G. Bull. ...

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• MONTE-CARLO

... TEXAS SURVEY: THE PRELIMINARY -35 and stronger than 0.25 Jy is intended to provide accurate (one arc-second rms error) positions, flux densities and structure models for each of the ~70000 sources expected to be listed. ... Average rms position accuracy for point sources is 1" in RA and 0.5" in DEC. ... 1 is the source name in IAU format. ... Thus, (+1,+1) means the second most likely lobe is 51.8" LATER in RA, and 51.8"*sec(z) HIGHER in DEC than the position listed. ...

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• Extinction and transformation models
• Direct electron imaging-model
• Signal detection

These lesson introduces you to the use of uncertainties. In particular how to interpret them, and how to factor them in when working out if a theory or prediction is good. It introduces probability distribution functions, the Gaussian Distribution, hypothesis testing and model fitting. Back Main Uncertainties Page .

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• Index of /~akarakas/model_data
• Pre-Lab 1
• COALA - Computational Astrophysics Laboratory

The multiscale analysis of heterogeneous structures is actually an important and effective tool of mathematical modeling in physics, technique and biology. ... The special year will extend the existing cooperation between French and Russian researchers in the multiscale analysis and in mathematical modeling in hemodynamics, taking into consideration the mass transport, coagulation, fluid-structure interaction and other aspects. ...

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• Young researchers' seminar in statistical physics
• Conference "Combinatorial Methods in Physics and Knot Theory" (February 2005)
• The Navier-Stokes-alpha model...