... Posts tagged ?flare distribution? ... In 2002ApJ?580.1118K , we dealt with modeling the photon arrival time differences as due to flares occuring at random times but with a power-law intensity distribution with index alpha. physics/0706.1758 deals with time-between-touches and tries to characterize that distribution itself in terms of a number of ?phases? beta. ... Tags: arXiv , flare distribution , football , soccer , stochastic process . ... 1 Comment . ... vlk on [MADS] Parallel Coordinates . ...

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• The AstroStat Slog background
• The AstroStat Slog Blog Archive tests of fit for the Poisson distribution
• The AstroStat Slog distribution

Find Similar Abstracts . ... Intergalactic gas in galactic clusters, the microwave background radiation and cosmology . ... The types of information that can be obtained from astrophysical studies of the microwave background in the direction of galactic clusters and from radio observations of clusters are examined. ... Use: Authors Title Abstract Text Text Query with Keywords Return: Query Results Query Form Database: Astronomy Instrumentation Physics and Geophysics ABSTRACT QUERY USER FEEDBACK HELP ...

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Proceedings of the Particle Physics and Early Universe Conference (PPEUC). For this paper: postscript PPEUC CMB index 1 Introduction.. ... Nuffield Radio Astronomy Laboratories , University of Manchester, Jodrell Bank, Cheshire SK11 9DL, U.K. We use radiation emitted by the galaxy to probe the amplitude and spatial distribution of galactic free-free radiation. ... 2 Using to Trace Free--free Emission . ... Acknowledgements . ... PPEUC Proceedings . Fri Jul 25 11:50:21 BST 1997 ...

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... It is found that the metallisity distribution of disk stars has a gap which subdivide the disk population into two groups. The distribution may be described by the sum of two normal curves which are centered at [Fe/H]=-0.22 and +0.08. The curves can be interpreted as distributions of random errors in metallisity of sample stars. This leads to the conclusion that all stars in each group have actually the same value of [Fe/H]. ... Рассмотрен вопрос о происхождении подсистем Галактики. ...

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... P2720 Date Received: 2012-Mar-02 00:09:27 Technical Page Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT: Regular Pulsars Galactic 6 Hours 2 hours Resolving Pulsar Emission Regions with Arecibo We propose to measure the distribution of flux density for three distant and strongly scattered pulsars. ... We will export baseband voltage data directly to disk with PUPPI for analysis off-site. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/ZhoutagT3002tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/GwinntagP2720tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/DuhautagT1057tp.ps

... Abstract . ... A Survey for Supernovae in Massive High-Redshift Clusters . ... Combined optical and x-ray image of the "Bullet" galaxy cluster: the red outlines the distribution of hot, baryonic gas (from X-rays); the blue maps the underlying (dark matter) mass distribution. ... Galaxy-galaxy lenses, however, offer a distinct advantage, since the background source is extended, and therefore imposes a stronger constraints on the mass distribution of the lensing galaxy than a point-source QSO. ...

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• SODRM Statistical Summary 2012
• HST this week: 335
• HST this week: 275

... ATNF Home . About ATNF . ... About ATNF overview . ... Governance overview . Australia Telescope Steering Committee . ... Our people overview . ... Universe@CSIRO blog . ... Mapping the Hidden Universe: . The Galaxy Distribution in the Zone of Avoidance . ... Due to the foreground extinction of the Milky Way, galaxies become increasingly faint as they approach the Galactic Equator creating a ``zone of avoidance'' (ZOA) in the distribution of optically visible galaxies of about 25%. ...

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• Star formation and gas distribution in the Magellanic Spiral NGC 4214
• The H I Column Density Distribution Function at z=0: the Connection to Damped
• Finding the Bivariate Brightness Distribution of galaxies from an HI selected

... Previous: Accessing Astronomical Data over the WWW using datOZ . ... Robust, distributed searching of networked-based astronomical databases requires an investment not only by individual data providers, but also by the astronomical community as a whole. ... Designing a distributed, networked-based astronomical information system requires a four-step approach including original data source analysis, modeling the system, profiling the system, and implementation of the system. ...

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• Starlink's Software Distribution System
• Modelling Spectro-photometric Characteristics of Eclipsing Binaries
• Modelling Spectro-photometric Characteristics of Nonradially Pulsating Stars

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... AIA 304 ? ... bottom) images (colour table reversed) of a coronal hole region at the South Pole taken on 14 May 2010. ... In the present work we derive a Differential Emission Measure (DEM) distribution from a region dominated by spicules. ... This distribution is then used to study the thermal properties of the emission contributing to the 171 ? ... From our off-limb DEM we found that the radiance in the AIA 171 ? ...

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• Abstract
• Galactic distribution and absolute magnitudes

... 2006 . ... Comparison of total ozone distribution in the high latitudes of both hemispheres SCAR XXIX Open Science Conference, 2006, 12-14 July, Hobart, Australia - Abstract Volume. ... Analyses of spectra, stability and eigenmode transverse small-scale oscillations in the inner Earth magnetosphere. 6th Open Conference of Space Projects Evpatoriya, September 2006, Abstracts . ... Ps6 pulsations in the Earth magnetosphere. 5th Open Conference of Space Projects Evpatoriya, September 2005, Abstracts . ...

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• Extragalactic Astronomy
• Theoretical Astrophysics

... Bisnovatyi-Kogan, Gennady S.; Merafina , Marco; Vaccarelli , Maria Rosaria; Spherically Symmetric Stellar Clusters with Anisotropy and Cutoff Energy in Momentum Distribution. ... We construct numerical models of spherically symmetric Newtonian stellar clusters with anisotropic distribution functions. ... Models of spherically symmetric relativistic stellar clusters with anisotropic distribution functions in relativistic regime are described by using Maxwellian distribution function with energy...

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• The summary plot of time distribution of the multisatellites magnetic
• Nonequilibrium distributions
• Space Research Institute (IKI) Seminar

... OGIP spectrum for selected source region . OGIP spectrum for selected background region . ... The primary input to especget is an image data set and two spatial selection expressions which need to mark an extraction region around a point source and a source-free background region. ... All regions will be deleted from the image - new initial selections for source and background regions must be made In the first and second case especget is eventually invoked with the appropriate input. ...

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... 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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• The peculiar post-AGB supergiant IRAS04296+3429: optical spectroscopy and its
• Results scientific researchs LRS
• A Method of Integrating

... 1Becker A catalog of 53522 4.85 GHz sources between 0 and 75^o declination has been generated from observation taken with the NRAO Green Bank 300 foot (91m) telescope. The flux limit of the catalog is dependent on confidence radius of ~50". Spectral indices have been calculated for 29051 sources which have counterpart in the Texas 365 MHz northern sky survey. ... The rms noise in the images varied from 5 to 8 mJy. The images has an angular resolution of ~3.5'. ...

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• "Structure" publications in 2001 year
• Noise distributions
• IRAS IDS

T he Siding Spring Survey (SSS) is a Near-Earth Object search program that utilises the 0.5-m Uppsala Schmidt Telescope at Siding Spring Observatory, N.S.W., Australia. ... The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. ... Based on the CSS Mission page . ... Siding Spring Survey Main Page . ...

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• Lecture 19: Probability Distribution Functions
• The GMRT Array Distribution
• Lesson 1: Using Uncertainties

POROUS GRAINS IN THE SHELLS OF HERBIG Ae/Be STARS V.B. Il'in and N.A. Krivova Abstract.- We simulate the polarized radiation transfer in the shells with a spheroidal spatial distribution of fluffy dust grains. The circumstellar dust is represented by MRN mixture of silicate and graphite particles. The optical properties of porous grains are calculated using the EMT approximation and Mie theory. ... Effects of the porosity of grains on these data are considered. ...

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• Polarization properties (transmitted radiation)
• Linear polarization: wavelength dependence
• Fractal Matter Distribution

... Public . Science . ... Science Users Information Science Software ESO-MIDAS jump to navigation jump to content . ... Publications with ESO Data . ... ESO-MIDAS . ... The short statement of the GNU license is included in every MIDAS file; the full text is included as a separate file in the ESO-MIDAS Release. ... Manual pages,installation guides and other documentation are generally released together with the source code and can also be obtained from the ESO-MIDAS ftp account (see below). ...

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• ESO - Thesis Topic: Foreground emission and Cosmic Microwave background
• Velocity Distribution of the XLSS-03 Cluster | ESO
• Distribution of Exoplanet Distances | ESO

... 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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• Serpens FCRAO (Abstract)
• BD_disks (Abstract)
• LASG - Distribution specific information

Organisers: Michel Balazard (CNRS, Laboratoire Poncelet) , Michael Tsfasman (CNRS, Laboratoire Poncelet, Institute for Information Transmission Problems) , Alexey Zykin (Laboratoire Poncelet, State University Higher School of Economics) . ... Number theory semester web page . Alexey Zaytsev (Dublin) . ... One of the big questions in the area of curves over finite fields concerns the distribution of the numbers of points: Which numbers are possible as the number of points on a curve of genus $g$? ...

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• Moscow Mathematical Journal
• IUM10 conference: abstracts of some talks
• Distributions and Sobolev spaces (Spring 2003)

Trudy GAISH, vol. LXV, 1996 . Abstracts . The global distribution of average (5 O x 5 O ) depths . of Mohorovicic discontinuity on the Earth . ... Such analysis allows detecting whether the sources of the largest anomalies reside within the Earth's core. This is possible if the limit depths of the sources exceed the depths of the core-mantle boundary. ... by Pasinok S.L. Influence of the Earth’s cover on the polar free oscillation of the Earth’s inner core is considered. ...

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