. Documents latest versions (PS and Latex)

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• Jonathan's ASC/SDS documents
• The AstroStat Slog ICA
• The AstroStat Slog model

... The fitting procedure will only converge to a unique solution if the components are linearly independent. ... The task calculates for each pair of component images and fails with an error if any is greater than 0.99. ... Hence components may be linearly independent in masked pixels yet still fail the test within the task. ... Finally, since the Poisson image values are necessarily all , negative values are not allowed in the model components. ...

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• Description
• Memory Models

... HST . ... Lensing Models . ... In order to interpret many of the properties of background lensed galaxies, reliable models of the lensing maps for each cluster are required. Preliminary models for each of the six Frontier Fields clusters have been provided by five independent groups prior to the HST Frontier Fields observing campaign in order to facilitate rapid analysis of the FF data by all members of the community. ... The various groups model the cluster mass distribution in different ways. ...

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• HST Focus Model
• Starburst and Galaxy evolution
• Prior Models and the Richardson-Lucy Restoration Method

Next: Colophon Up: Contents Previous: Software Systems . Spectroscopic reduction and analysis programs at the DAO (invited talk) . ... H.-M. Adorf . Interpolation of Irregularly Sampled Data Series---A Survey . ... Robust Data Analysis Methods for Spectroscopy . ... Application of the Linear Quadtree to Astronomical Databases . ... Automated Globular Cluster Photometry with DASHA . ... A. W. Jones, J. Bland-Hawthorn, and P. L. Shopbell . ... J. Bland-Hawthorn, S. Serjeant, and P. L. Shopbell . ...

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• Modelling Spectro-photometric Characteristics of Eclipsing Binaries
• StarView II: A Customizable Query Generation Tool
• Spatial Structure of NGC 6822: An Example for Statistical Modeling of

... The axial support is provided by 78 air pistons. ... The transverse support is provided by 38 air pistons, supported by cantilevers from the mirror cell, that act on the mirror local center of gravity surface. ... The locations where the transverse mirror support forces should be applied to the mirror are listed in Table 1 and illustrated in Figure 1. ... Figure 1: CAD drawing showing the 2.5-m primary mirror and the locations of the transverse support posts (black) and axial pneumatic pistons (blue...

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• Drawing and Part Configuration Management Directive and Procedures:

Cost Estimating Web Site . ... 2005 NASA Cost Analysis Symposium Databases . ... World , European Communities , Other European Countries , Americas , Asia , Africa , General US , US Federal Government , US Department of Defense , Aerospace Industry , NASA , Science & Engineering Handbooks . NASA Cost Estimating Handbook 2004 , Parametric Estimating Handbook .. ... Consumer Price Index , Employment Cost Index , GDP Deflator , Import Price Index , NASA New Start Index , Producer Price Index . ...

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... The magnetic field of the Earth has been investigated by satellites for several decades now, and enough of it is known to model its average strength and shape during different levels of overall magnetic activity. Presently the most used empirical global magnetic field models are the Tsyganenko models (1987, 1989) , referred to as T87 and T89, respectively, although even these consist of several submodels. ... Earth's magnetic field from T89c model during Kp=2 for different seasons. ... Res. ...

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• Folding Paper Model of Magnetosphere

Direct Electron Imaging Using Back Thinned CCD's . ... where, Vim is the maximum radial emission energy of photoelectrons from the cathode (eV), Vs is the cathode to anode voltage (V), k is the spatial frequency (2 p lp/mm), L is the cathode to anode spacing of the proximity focused diode (mm), d is the field-free region thickness(mm), h is the backscattering coefficient, (G/G 0 .) is the ratio of the average EBS gain of the secondary electrons to the primary gain, and W is the CCD pixel pitch (mm). ...

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• Diffuse Model
• Signals and their models
• Fourier analysis: The sine model

Next: Stellar models Up: Introduction Previous: Photometry Contents . In a hierarchical stellar system, the separation between two neighboring stars is always much smaller than the separation of this pair from the next companion in the system, be it another pair or a single star. ... They are also numerically easier to handle than non-hierarchical systems, since each pair can be described with the standard orbital parameters, and each star with a small number of physical parameters. ... System . ...

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• Model manipulation
• Manipulation of a model
• ESO - Thesis Topic: Dynamical models of multiple globular cluster populations

On this page you can compute thermodynamics, opacity and nuclear reaction rates for conditions which exist inside the Sun. ... Logarithmic partial derivative dlogP/dlogT (hi_t) . Logarithmic partial derivative dlogP/dlogRHO (hi_rho) . Logarithmic partial derivative dlogP/dlogX (hi_x) . Logarithmic partial derivative dlogU/dlogT (ksi_t) . ... Input field size does not limit the amount of data entered; you can type or paste thousands of lines (10,000 lines tested with output size over 5MB). ...

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• Equation of state for solar modeling
• Scholarly Pursuits

... G.P.Panasenko (J.-V.Poncelet, Moscow) Multiscale problems: junction of models of different dimension, applications to hemodynamics. ... Gubkina , Moscow, Russia . ... The workshop is devoted to an important trend in mathematical modeling, the multiscale methods and its applications in biology and medicine. ... It was organized in the frame of the thematic year on the multiscale methods and modeling in biology and medicine organized by the Russian-French laboratory J.-V.Poncelet. ...

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. Next: Timing noise Up: Glitches and timing noise Previous: Adjustments in ellipticity: star . љ . Majority of I in crust . Fluid interior loosely coupled to crust . Crust slows down, interior keeps spinning fast . Sudden increase in coupling causes spin up . indicates this is the cause of most glitches . Jon Bell . Thu Dec 19 15:15:11 GMT 1996

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• imfit
• cmodel (Model Image Generator) CentralProcessor 0.11 documentation
• uvmodel

... Numerical Modeling of RadioAstron SRT Temperature Deformations M. Yu. Arkhipov, I. S. Vinogradov, S. B. Novikov, and S. D. Fedorchuk Astro Space Center, Lebedev Physical Institute of the Russian Academy of Sciences, Moscow, Russia e mail: rusengineer@mail.ru Received December 16, 2013 Abstract--The results of modeling the thermal deformations of a space radio telescope's reflecting surface are presented in the paper. ...

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• RadioAstron meeting
• ОТЧЕТ
• Description of the RadioAstron project, english version

... G., Filippova A.S. Presented by: Filippova A.S Achievements · Refined model based on the celestial-mechanics methods is presented that is a generalized version of the previously developed basic model · Subtle effects are qualitatively explained based on the amplitude-frequency analysis and the computer numerical modelling of the oscillatory pole motion, where the key feature is the Chandler wobble 2 Basic Model of the Polar Oscillations ...

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• Pulkovo EOP and Reference Systems Analysis Center (PERSAC)
• Phase light curves of young binary systems

Next: J.E. Chambers, Research Astronomer Up: Research Previous: Research Contents . ... Solar Variability and Climate . Other Activities . ... Applied to data of flares on Gliese866 he was able to estimate the area of hydrogen emitting flare regions as 1-13% of the stellar surface. ... As partners in the project, Armagh Observatory has been asked to contribute to the selection process in exchange for priority access to the data which will eventually flow from the satellite. ...

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• M. de Groot, Senior Research Associate
• lte-codes: sterne model atmospheres
• A Blinker Model

... Classes . ... Class List . Class Hierarchy . Class Members . include < dustmodel.h > . Collaboration diagram for dust_model: . ... List of all members. dust_pahenhancements . ... dust_carbprops . ... dust_nmoded . ... Represents the entire dust model . The documentation for this struct was generated from the following file: . dustmodel.h . Generated on Fri Jul 11 07:32:08 2008 for DUST by 1.5.5 ...

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• Inference of Coefficients for Use in Phase Correction Bojan Nikolic web pages
• Inference of Coefficients for Use in Phase Correction
• Paper II: Spinning dust in galaxies Bojan Nikolic web pages (r. 329)

... SADT CASE- Bpwin (AllFusion Process Modeler) Erwin (AllFusion Erwin Data Modeler) Computer Associates, , . ... SADT IDEF0, CASE- BPWin. 34.003-90 ". " (automated system, ) ­ , , . ... 8 Tools/Reports/Model Report. ... ERwin , « » : · Column Reports ­ ; · Attribute Reports ­ ; · Entity Reports ­ , ; · Domain Reports ­ ; · Table Reports ­ ; · Subject Area Reports ­ ; · Model Validation Reports ­ ; 33 · Stored Procedure Reports ­ ; · Relationship Reports ­ ; · View Reports ­ ; · ERWin Volume Reports ­ ...

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• Mathematical Modeling and Informational Technologies in Photonics

home education > activities . ... Quick math activity that asks students to calculate scale models of a binary star system with a black hole in it. [h] . ... Students use a radiometer and a light bulb with a dimmer switch to make connections between the temperature, color, and radiation output of a star. ... This demonstration, similar to the above, from the Exploratorium Snack-book of science activities, lets students demonstrate how molecules scatter light and change the colors of the beam. [m,h] . ...

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• ASP: Black Holes
• ASP: Sharing the Universe
• ASP: The Universe At Your Fingertips Activities TOC

Next: Initial binary parameters Up: Population synthesis of Previous: Introduction . Monte-Carlo method for statistical simulation of binary evolution was originally proposed by Kornilov & Lipunov (1983a,b) for massive binaries and developed later by Lipunov & Postnov (1987) for low-massive binaries. ... Recently Leitherer & Heckman (1995) have modelled star formation for elliptical and spiral galaxies, taking into consideration only the single stars. ... Initial binary parameters . ...

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• Cosmion-99
• Structure of the Galaxy
• Normal star evolution

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Although their determination is based on the scattering process model, independent check-ups by rocket experiments have shown their correctness in experimental applications. ... Ionospheric data analysis, especially during strong disturbances, cannot be without some other kinds of diagnostic tools. ... The lack of data has always been a challange in this case. ...

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