Next: Feature enhancement: local Up: No Title Previous: Feature enhancement: filtering . ... As a result, a common magnitude scale (contour lines on the maps above, or color scale on Fig.1) will poorly display the short-duration events in a signal. Normalizing each line of the map (fixed duration) so it has unit variance (in effect dividing the energy map by the mean energy spectrum) at each duration restores more details of small-scale activity (Fig. ...

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• ApSA courses
• Long description of how floats overlap with boxes in normal flow
• Long description for normal flow example

. This image shows a system where two massive galaxy clusters have collided and in doing so have forced the separation between dark and "normal" matter. X-rays from Chandra (pink) show where most of the normal, or baryonic, matter in the cluster resides. Optical data from Hubble (blue) is used to trace the mass. NASA/CXC/Stanford/S.Allen; Optical/Lensing: NASA/STSci/UC Santa Barbara/M.Bradac

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• If neutron stars don't produce energy from fusion, like normal stars, how can
• Age of mystery star cluster unknown | Astronomy.com
• Spectacularly bright object in Andromeda caused by "normal" black hole |

... Science User Portal . ... ESO, the European Southern Observatory . ... Travel and Contacts . Travel to ESO Headquarters . ... Survey Telescopes . ... Galaxies . ... ESO Science Newsletter . ... ESO 3.6-metre telescope . ... MPG/ESO 2.2-metre telescope . ... ESO 1-metre Schmidt telescope . ... ESO Science Outreach Network . ... This is an image of the most distant "normal'' galaxy known, G 0102 190, as seen on a CCD exposure obtained with the EFOSC II instrument at the ESO New Technology Telescope. ...

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• ESO - Thesis Topic: Dynamical models of multiple globular cluster populations
• Most distant "normal'' galaxy known, G 0102 190 | ESO Australia
• Most distant "normal'' galaxy known, G 0102 190 | ESO United States

Analysis of the Systematic Errors of CCD-observations of Asteroids Performed in 2007-2008 . ... Analysis of systematic errors based on CCD-observations taken with Normal Astrograph (D/F = 0.33 m/3.5 m, FOV = 18 16 arcmin, scale = 1 arcsec/pix) of Pulkovo observatory during 2007-2008 has been made. ... A statistical approach that used mean (O-C) values obtained for positions of reference stars within the field of view separated on square bins and magnitude ranges was applied. ...

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Atmospheric influence on the different radio-engineering system functioning . ESTIMATION OF ATMOSPHERIC OPTICAL CHARACTERISTICS AND REMOTELY SANSED IMAGE CORRECTION . ... Direct transmittance estimation results for 12 channels of the spectrometer CHRIS. ... We have managed to develop a direct method of estimating the discrete Normalized Atmospheric Point Spread Function (NAPSF) from available images alone, not using any external sources of information about the atmosphere. ... IRE RAS 1996-20 11 ...

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• Lab234 - Design, fabrication and experimental studies of a novel device: Cold

Although the background level of meteors from the Leonid stream is not especially high, within the stream are dense, narrow trails of meteoroids and dust, the debris of Comet 55P/Tempel-Tuttle. ... The number density of particles is much higher at the centre of these trails than elsewhere in the Leonid stream. ... Although the overall number densities of meteoroid particles in resonant trails are smaller than in normal trails, the resonant trails are rich in larger particles. ...

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• Armagh Observatory
• C.J. Butler, Research Astronomer
• IAJ: Publications

... We present a photometric and spectroscopic study of the unique isolated nearby galaxy KKR25. The isolated dwarf spheroidal (dSph) galaxy KKR25 was discovered by Karachentseva, Karachentsev Richter (1999, A , 135, 221) during the search of dwarf galaxies in the direction of the Local Void. In spite of its isolation KKR 25 has no gas and looks like a normal dwarf spheroidal system. ... This is the first known planetary nebula in a dwarf spheroidal galaxy outside the Local Group. ...

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• important11-15_en
• Detection of Radio Transients and Variable Radio Sources Using the Archive Data
• articles_lebedev_en

... Primordial theory review : Dick Bond . Defects and the CMB review : Andy Albrecht . ... Gravitational wave contribution to CMB anisotropies : V.B. Lukash and E.V. Mikheeva . C_l from cosmic strings : Lloyd Knox . Some aspects of CMB anisotropies induced from topological defects : Mairi Sakellariadou . ... CMB anisotropies from scaling sources : Ruth Durrer . ... SZ observations I : Sarah Church . ... Holes in the microwave sky? ... Detecting cosmic strings in the CMB : James Robinson . ...

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• Bojan Nikolic -- Simple smoothing of astronomical images in FITS format
• Samantha Thompson - Research
• Limits on Phase Correction Performance Due to Differences Between Astronomical

. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

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ATMoB "Open Cluster Observing Award " Guidelines Purpose: To promote observing among the membership of the Amateur Telescope Makers of Boston through participation in the Open Clusters Observing Awards program. Introduction: This awards program is oriented towards visually observing open clusters above magnitude 9.9. ... It turns out that a very unprejudiced and convenient method to dermine the limiting magnitude is to count the number of visible stars in certain areas on the sky. ...

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• http://www.atmob.org/about/observing/awards/files/globular_cluster_instructions_2011-02-01.pdf
• Amateur Telescope Makers of Boston
• Amateur Telescope Makers of Boston ATMoB Observing Awards Program

... Кресла . ... Размер: XS . ... Цвет: белый . ... Размер шлица: PZ2 ; . ... Цвет: Фиолетовый . ... Глубина: 90 . ... Цвет: черный . ... Цвет: серый . ... Размер INT: 54 . ... Глубина пропила: 90, . ... Макс. глубина пропила под углом 90њ: 90, . ... Размер площадки: 800x550, . ...

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• Брюки Saint Tropez Модель: 26474651 - Saint Tropez - Saint Tropez Юбка Motion
• Одеяло Сонный гномик Сердечко 90 х 90 см голубой хлопок 588 - Сонный гномик -
• Настенный светильник Favourite Espresso 1503-1W Панно "Буква 'O'

... 1st Announcement IAU Symposium 312 Star Clusters and Black Holes Across Cosmic Time, Beijing, China, Aug. 25-29, 2014 . ... SUBJECT: 1st Announcement IAU Symposium 312 Star Clusters and Black Holes Across Cosmic Time, Beijing, China, Aug. 25-29, 2014 . ... which will be held in Beijing, P.R. China, from August 25-29, 2014, hosted by Chinese Academy of Sciences . ... China), . ... 1st Announcement IAU Symposium 312 Star Clusters and Black Holes Across Cosmic Time, Beijing, China, Aug. ...

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• The Laboratory of Astrometry
• MAO NASU :: Topic: The DRAGON globular cluster simulations: a million stars,
• Optical systems and devices

EVIDENCE FOR AGE DELAY BETWEEN THE FORMATION OF THE OLD HALO AND THE THICK DISK. ... The metallicity function of globular clusters of thick disk and old halo is shown on Fig.1Ю There are a two approximately the same normal distribution with well-defined gap between them with width [Fe/H] 0.2 dex. ... Metallicity function (left panel), and age distribution (right panel) for the old halo and thick disk globular clusters. ... Plots of V S against cos for the thick disk and the old halo samples. ...

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• Population of Galactic globular clusters, figures
• Vladimir Marsakov Abstracts
• Subsystems of the Galactic halo, figures

... astro-ph . ... Statistical Characterization of the Chandra Source Catalog . ... The first release of the Chandra Source Catalog (CSC) contains ~95,000 X-ray sources in a total area of ~0.75% of the entire sky, using data from ~3,900 separate ACIS observations of a multitude of different types of X-ray sources. ... In addition to these traditional catalog elements, for each X-ray source the CSC includes an extensive set of file-based data products that can be manipulated interactively. ...

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• people:sergeykarpov:paper-arxiv-2007-adass [SAI Virtual Observatory - Wiki]
• SAI CAS: About the SAI CAS project

J/AstL/vol/page SAI Open Clusters Catalog (Glushkova+, 2009) ================================================================================ Automated search for star clusters in large multiband surveys. ... Color excesses E(B-V), distance moduli and ages were determined for 141 new and 27 known, but poorly studied clusters. We present the Sternberg Astronomical Institute Open Clusters Catalog (SAI OCL Catalog) of coordinates, diameters and main physical parameters of these clusters. ...

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• SAI OCL Catalog Description
• SAI Open Star Clusters (SAI OCL) Catalog
• SAI OCL Catalog Virtual Observatory

... Future seminars . P a s t seminars . Seminar council . Collective processes and structures in spiral galaxies " . ... A new approach to studying global structures in thin stellar disks, which allows to describe universally both bar and spiral modes, is presented. ... Study of line-of sight velocity maps of gaseous disk in spiral galaxies allows, under some conditions, to reconstruct 3 components of gas velocity in the galactic plane. ...

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• DOK-2 Results Page
• Main results of the experimental and theoretical research completed in 2010

Determination of short-term proper motions of fast stars with Pulkovo Normal Astrograph. ... Khovritchev Laboratory of Astrometry and Stellar Astronomy of the Pulkovo Observatory, RAS, Saint-Petersburg Observations Normal Astrograph (D/F=33 cm/3.5m), CCD camera: S2C, FOV = 18x16 arcmin, Pixel size 900x900 mas Determination of the new proper motions of 413 LSPM stars 1 epoch : CCD-surveys and catalogs -- M2000, CMC14, 2MASS, SDSS DR7 2 epoch : CCD-observations with the ...

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• Pulkovo Astrometrical Plate Database
• Pulkovo Databases
• plut_pub

Title , Contents , Index . Nested lists can be made from an RTF document by using a different style for each level of indentation. The styles "bullet list 1" "numbered list 2" ... represent different levels of nesting. The only rule for use is that no levels of nesting are skipped. For example, a "ol 3" paragraph must not appear immediately after a "Normal" paragraph. It must follow a paragraph with a nesting level of 2 or higher. ...

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• Font Style Elements
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Stellarium 0.12.3 . ... Renderer . FileљStructure . ... core . ... StelVertexAttribute.hpp . ... 53 љ inline int attributeDimensions( const AttributeType type) . ... 122 љ qDebug() << "Unknown vertex attribute type: \"" << typeStr . ... 179 љ // Ensure that every kind of vertex attribute is present at most once. 180 љ foreach ( const StelVertexAttribute & attribute, attributes) . ... 186 љ "Vertex type has more than one vertex position attribute" ); . ... 239 љ #define VERTEX_ATTRIBUTES(...)\ . ...

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• Stellarium: StelTextureBackend Class Reference
• Stellarium: BooleanFader Class Reference
• Ключевое слово ?Cluster?

... overview of instrument and science (15) 11:10 Mikhail Gubarev: Development of mirror modules for ART XC (15) 11:25 -- 11:55 Coffee break 11:55 -- 12:50 X ray missions 11:55 Joachim Truemper: Lessons learned from the ROSAT all sky survey (30) 12:25 Naomi Ota: ASTRO H (25) 12:50 -- 14:20 Lunch 1 14:20 -- 15:40 Galaxy clusters and cosmology 14:20 Eugene Churazov: Galaxy clusters in X rays: plasma physics, AGN feedback and ...

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• http://hea.iki.rssi.ru/Z-90/arc/Program.doc
• SIXA acceptance tests, 2000
• z90-program