... 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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• HST this week: 066
• HST this week: 275
• HST this week: 015

SAI 175 anniversary . ... Moscow University . Search for in SAI Moscow University Search for in Russian astronomical resources . ... SAI Astronomical Databases . ... Browse SAI Software archive(ftp.sai.msu.su) . ASTRONET.RU - Russian Astronomical Network (available in translit also) . ... SAI Supernovae Research Group . ... Department of the Galaxy and Variable Stars (in Russian) . Sternberg Astronomical Institute Seminars . ... All-Russian Astronomical Olympiad (in Russian) . ...

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• SAI SN RESEARCH GROUP

... About ATNF overview . ... Governance overview . Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Our people overview . ... Publications overview . ... Careers overview . ... I present new high-resolution observations of the HI in NGCб 4214 made as part of a study of the small-scale kinematics and star formation regions of the galaxy. Keywords: galaxies; individual (NGC 4214) - galaxies: kinematics and dynamics - radio lines: galaxies . ...

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• Distribution of Young Stars
• ATNF Colloquium
• Archive of VLBI Observations Majordomo List

Twilight observations with MASS/DIMM B. Safonov Sternberg Astronomical Institute Moscow State University Comprehensive Characterization of Astronomical Sites, 2010 B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 1 / 17 Why observe in twilight with MASS/DIMM? ... ASM includes 3 devices sensitive to background: guider, DIMM and MASS. B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 2 / 17 Background in guider. ...

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Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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• Amplitude Distribution
• Old neutron star distribution in the Galaxy
• Vladimir Mikhaylovich Lipunov

... 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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• U of O High Energy Physics Seminars
• Physics 410/510 Observational Cosmology
• Evidence for Dark Matter

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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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• David Nicholls: CV and publications
• The SMS Survey
• COALA - Computational Astrophysics Laboratory

... The technology needed to implement a Distributed Astronomical Data Archive (DADA) is available today (e.g., Fullton 1993). Query interface standards are needed, however, before the DADA information will be discoverable. ... These parameters would be used to index each dataset in each catalog. ... The technology is available today to perform cross-catalog queries, to fetch the data at the click of a mouse, quickly to add new observation catalogs, and to distribute the load across multiple machines. ...

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• DASH--Distributed Analysis System Hierarchy
• Distributed Software for Observations in the Near Infrared
• A Distributed System for ``Phase II'' Proposal Preparation

. Field of research interest . Telecommication networks and systems , Programming. Scientific Degree . Student of MIPT. Position . Laboratory assistant of IKI. Department Number . 902 (Space Monitoring Information Support) . Postal Address . Space Research Institute . Russian Academy of Sciences . Profsoyuznaya St. 84/32 . Moscow, RUSSIA . Postal Code . 117810 . Telephone Number . +7(095) 333-53-13 . E-mail . andrew@d902.iki.rssi.ru . If you want to get more information click here

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• Matyushkin Evgeny, Space Research Institute (SRI)

... Interdisciplinary seminar "Satellite methods and systems for Earth research" (chairman - corresponding member of Russian Academy of Sciences G.M.Chernyavsky) . ... SMIS Information System for Acquisition, Processing, Storage and Distribution of Satellite Data . ... Provides operational access to satellite data and derived products. ... Provides automatic collection, processing and cataloging of satellite data and remote access to information. ... Provides remote access to information. ...

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• Space Research Institute (IKI) Seminar
• Институт космических исследований РАН (ИКИ РАН)

... Institutes of Chernogolovka . The largest of all the scientific institutions of the center is the Institute of Chemical Physics in Chernogolovka , where fundamental problems of chemical physics are studied: kinetics and mechanisms of chemical and biological processes; processes of combustion, explosion, and polymerization; and mechanisms of elementary reactions involving high energy particles. ... Developments and Technologies . ...

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• Astronomy: Olympiad of Scientific Centres: Institutes of Chernogolovka
• Laboratory of materials for electrochemical technologies ISSP RAS
• Multipurpose technology for crystal growth of zinc and cadmium chalcogenides

Peremennye Zvezdy", . ... Star Name: . GSC 4487-00399, . ... During observations of GSC 4487-00347, a new eclipsing binary star with an eccentric orbit (Otero et al. 2006), we discovered variability of GSC 4487-00399. ... We suggest that the star is a close-binary EW-type variable with the ephemeris: . ... Light Curve . The spectral window (1a), the power spectrum (1b), and the phase diagram (1c) of the variable star GSC 4487-00399. ... The finding chart for the variable star GSC 4487-00399. ...

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• Астронет > Archive of Astronomical and Astrophysical Transactions
• XWare > APOD

... Visible Distribution of Galaxies. ... Features of Elliptical, Lens-Shaped, Spiral and Irregular Galaxies. Galaxies with Bar. ... Distribution of Surface Brightness of Surface and Spiral Galaxies. ... Color Characteristics of Galaxies. ... Methods of Galaxies' Mass Determination. ... Hidden Mass of Spiral Galaxies. ... Features of Dark Matter Distribution in E and SO Galaxies. ... The Whole Number of Galaxies and Their Density by the Results of Observation on the 'Hubble' Space Telescope. ...

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... A GLAST-related opportunity: A Summer Science Institute at SLAC on Cosmic Accelerators is scheduled for August 4-15 in anticipation of GLAST science, and the co-directors welcome participation by students, postdocs, and researchers (even those with no background in astrophysics). ... Invitation to SLAC Summer Institute 2008 . ... We are writing to you about the 36th SLAC Summer Institute to be held Aug 4-15 this year on ?Cosmic Accelerators?. ... Tags: 2008 , GLAST , SLAC , SSI , Summer Institute . ...

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• The AstroStat Slog Blog Archive chi-square distribution [Eqn]
• Brad Wargelin CV
• Spectral Energy Distribution: Microquasar LS 5039

... The MIDAS system is available, free of charge, to all non--profit research institutes, whereas other organisations or companies may be charged a nominal fee to cover distribution. Institutes interested in using MIDAS must sign a User Agreement before they receive MIDAS. The necessary forms can be obtained by contacting the Data Analysis Group at ESO/Munich. ... The current system at ESO/Munich is frozen several months prior to the official release. ...

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• Footnotes
• "Structure" publications in 1996 year
• RMT_HOME_PAGE

NASA JOHNSON SPACE CENTER ORAL HISTORY PROJECT BIOGRAPHICAL DATA SHEET NAME: William R. Muehlberger O RAL H ISTORY: 9 November 1999 EDUCATIONAL BACKGROUND: University of California , Berkley, Berkley, California (no degree, Civil Engineering 1943-1944) B.S. in Geology , California Institute of Technology, Pasadena, California , 1949 M.S. in Geology , California Institute of Technology, Pasadena, California , 1949 Ph.D. in ... California Institute of Technology, 1954. ...

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• http://www.jsc.nasa.gov/history/oral_histories/GibsonEG/GibsonEG_Bio.pdf
• http://www.jsc.nasa.gov/history/oral_histories/ErbRB/RBE_BIO.pdf
• http://www.jsc.nasa.gov/history/oral_histories/BattinRH/RHB_Bio.pdf

... Effects of meteor ablation and the chemistry and physics of the upper atmosphere . ... Ablation and Ionization Modeling: Implications for Trail Instabilitiesand Head Echoes . Radar Observations of Meteors at a Polar Latitude . ... Radar meteor shower observations: processing and some results . ... Parameter estimation of meteors from radar head echoes combined with optical observations . ... Observations of meteor-head echoes using the Jicamarca 50 MHz radar in interferometer mode . ...

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• HISA Poster for the 197th Meeting of the AAS, January, 2001
• Project Description

... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/gross.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/medvedev.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/skurikhina.pdf

... 2006: . The distributions of radial ages and chemical compositions of the stellar population for several elliptical galaxies were measured from the BTA observations down to the record (to date) distances from the nucleus. ... Photometric distances were measured and peculiar radial velocities were determined for 3000 spiral galaxies from the 2MFGC catalog, compiled at the SAO RAS based on the 2MASS infrared sky survey. ... Archive . ...

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• Measurement of the dark halo shape in polar ring galaxies
• Solar system sector, archive 2006
• Galaxy sector, archive 2014