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 Supernova catalog
• Contributions by amateurs: SN1996X.
• Contributions

documentstyle[paasms4,pptwocol,psfig]{preprint} \input pub.sty \hoffset=-.1in \begin{document} \def\sec{$^{\prime\prime}$} \def\min{$^{\prime}$} \hyphenation{a-ni-so-tro-pic flux---ca-li-bra-ted} \title{THE SPECTRAL ENERGY DISTRIBUTION OF NORMAL STARBURST\\ ~\\ AND ACTIVE GALAXIES} \author{Henrique R.\ Schmitt\/\thanks{Also Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218.}\morethanks{CNPq Fellow.} ...

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• ACS Instrument Handbook for Cycle 20
• Space Telescope Imaging Spectrograph Instrument Handbook
• CVZ Subscription Monitoring.

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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• Effect of sources evolution on
• Gravitational waves from supernova explosions
• Seminars

... Archives . ... Reduced and Processed Data . ... 2 distribution plays an incredibly important role in astronomical data analysis, but it is pretty much a black box to most astronomers. ... Comment ( RSS ) | ... I guess in the typical analysis we call chi2 a ?random variable? that follows the chi2 distribution: . ... where D(i) is the observed data, M(i) is the model predicted data and we ?silently? assume that D(i) is normally distributed and each i measurement is independent. ... Chandra Blog . ...

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• Comments on: [ArXiv] Pareto Distribution By: vlk By: hlee By: TomLoredo By:...
• The AstroStat Slog Blog Archive [ArXiv] Pareto Distribution
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Main Program Travel Where to go in Moscow Information . ... The 2014 year marks the 100th anniversary of Yakov Zeldovich . ... John Carlstrom (University of Chicago) . ... Lyman Page (Princeton University) . ... The conference will be held at the Space Research Institute (IKI) in Moscow, Russia, on June 16-20, 2014 . ... International Conference: Cosmology and High Energy Astrophysics (Zeldovich-90) 20-24 Dec 2004, Moscow, Russia . ... 2014 Space Research Institute, Moscow Русская версия ...

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... The Astronomical Data Analysis Software and Systems (ADASS) conference is held each year at a different hosting astronomical institution. The conference provides a forum for scientists and programmers concerned with algorithms, software and software systems employed in the acquisition, reduction, analysis, and dissemination of astronomical data. ... The 26th annual ADASS conference will be held from October 16th to 20th, 2016 at the Stazione Marittima Conference Centre , Trieste, Italy. ...

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• Distributed Software for Observations in the Near Infrared
• ADASS 2002 Conference Proceedings
• Object Oriented Near Real Time Packet Distribution as Part of the FIRST

Observation and modelling of main sequence star chromospheres. ... We compare our calculations to recent high res­ olution observations for selected stars in a narrow spectral range ((R­I) џ =0.875\Sigma0.05); we show that Hff line profiles behave as expected, with a tight correlation be­ tween the line width and equivalent width. ... We show that the hydrogen series dominate the radiative cooling in the spectral lines (form 40% to 90%) for Hff emission line stars. ...

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• How We Contribute to New TSN
• Armagh Observatory
• What We Do

... It is reasonable to expect that UV part of the irradiating spectrum is most influenced by the grain evolution (growth and sedimentation ) which marks the very initial stage of planet formation. 2 log J [erg s­1 cm­2] 1 0 -1 -2 -3 1000 BB 40 0 0 (A5 ) BB 20 0 00 (A5) Drai ne (A5 ) BP Ta u (A5) BB 40 0 0 (GS) BB 20 0 00 (GS) Drai ne (GS) BP Ta u (GS) Disk Model Density distribution is based on a 1+1D disk ... Green lines are used for a model with dust growth and sedimentation. ...

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• Podgorny

This service contributes to the International Service of Geomagnetic Indices (ISGI) of the IAGA . ... The Kp numbers of the previous month are available in tabular format . ... There are available also historical and current Kp and derived indices per anonoymos FTP (see below). ... U.S.A. FTP server: ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/ . monthly update) . ... contains the monthly Kp / ap tables in a simple text format readable for both humans and computers (*.tab). ...

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LIF Marseille and Institute for Information Transmission Problems, Moscow, Russia. E-mail: alexander.shen AT lif.univ-mrs.fr, sasha.shen AT gmail.com . ... Kolmogorov complexity, algorithmic information theory . Teaching (mathematics, computer science): Independent University of Moscow, Moscow State University, Moscow mathematical school No 57. ... Kolmogorov memorial conference, Moscow. IEEE Conference on Computational Complexity, Aarhus (Denmark), ("Kolmogorov day") . ...

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• Young researchers' seminar in statistical physics
• Number Theory Semester - Poncelet Laboratory

... Using the central limit theorem, the total noise can be approximated by a Gaussian or normal distribution which has the frequency function : . ... where is the mean intensity of the source. ... In the statistical analysis of the probability distribution of data several estimators based on moments are used. ... For a normal distribution, these moments are and while for a Poisson distribution are and . Besides these moments other estimators are used to describe a distribution e.g. median and mode . ...

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• Distribution Policy
• Background Estimates
• Contributing

... SteMaGE is a research program aimed at improving the way we measure stellar mass in galaxies, map its distribution and understand how it affects galaxy evolution. ... At each position in a galaxy the stellar mass density is computed by comparing the observed optical/NIR emission with a library of models that reproduce different SFHs and dust attenuation. ... This new standard will be used to estimate the local SMF, providing a new unbiased reference for galaxy evolution models. ...

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• Selected articles from the K20 survey
• The Apache License, Version 2.0 - Apache HTTP Server
• research field

... 30, 2006 . ... If you retrieve these files via a Web browser, please note that you need to use the browser's "Save As..." facility. ... Figures must be provided as Encapsulated PostScript files and should be incorporated in your contribution using the standard Latex2e "graphicx" package as demonstrated in the demo file author.tex. ... Please submit the LaTeX source file of your contribution, and PostScript/PDF files of any figures, via email (!!!) to Iris Bronnert ( ibronner@eso.org ). ...

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Hallerstrasse 6 · CH-3012 Bern · Switzerland ISSI Call for Proposals 2015 for Johannes Geiss Fellowship The International Space Science Institute is an Institute of Advanced Studies located in Switzerland. ... Purpose ISSI has approved the introduction of the Johannes Geiss Fellowships (JGF). ... ISSI has a visitor programme, funds post-doctoral fellows, and encourages the participation of young scientists in the International Teams. ... Financial support requested from ISSI. ...

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• http://www.mao.kiev.ua/lao/presentation/staehelin_Is%20Ozone%20Recovering_Kiev%20SSch08.pdf
• MAO NASU :: Topic: Newsletter : January 2015 : International Space Science

Since I started teaching at Syracuse, it has been obvious to me that no faculty member works in a vacuum: administrative and support services contribute important elements of our working environment. Faculty members can contribute to the quality of this environment through a wide range of Committees and other voluntary activities. ... Member, Engineering Co-op Advisory Committee (since 1992) . ... Chair, Departmental Committee on Graduate Affairs (for 8 years) . ...

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• Lecturing list

THE CHEMICAL COMPOSITION OF REGOLITH AT THE MOON'S SOUTH POLE, ACCORDING TO DATA OF LUNAR PROSPECTOR AND LUNAR RECONNAISSANCE ORBITER MISSIONS. ... Introduction: The article tells about the results of integrated study of the craters at the Moon's South Pole with permanently shadowed region of craters. ... We have compared the ultimate composition of the soil matters in the craters with "cold traps" in the Moon's South Pole with regard to thorium, ferric oxide and hydrogen contents (Fig. ...

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• http://selena.sai.msu.ru/Rod/Publications/ms40/78_Sitnikov_etal.pdf
• http://selena.sai.msu.ru/Rod/Publications/ms34/MS059.pdf
• http://selena.sai.msu.ru/Shev/Publications/ms38/ms084.pdf

... Published by the Bureau of Astronomical Communications . ... TITLE OF THE ARTICLE IN RUSSIAN . ... This text contains Instructions for our Authors; at the same time, it shows the general layout of a contribution to the Astronomicheskii Tsirkulyar as it will appear published in the electronic form or printed on paper. ... The text of your article starts here. We accept articles in all branches of astronomy. ... 1543-1548, Information for Authors), text taped and figures drawn on paper. ...

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• Acknowledgments
• Rudnitskij Georgij M. Home Page

Since the light from galaxies represents the integrated contribution of its consitutient stars, then we can learn about stellar populations in galaxies by modelling their light by summing up individual stellar spectra for different kinds of stars. ... The data cover the wavelength range 3500 - 9000 angstroms. ... Retrieve Digital Stellar Spectra Click on the appropriate spectral type. ... Note that the designation V means main sequence, IV means subgiants, III means giants, I means supergiant. ...

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• Evidence for Dark Matter

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Flights Chronology . ... Acquiring new scientific information about the role of the right and the left heart in adaptation of the blood circulation system to long-term space flight conditions. ... Investigation of relations between hemodynamic and energetic characteristics of the heart in different phases of a long-term space flight. ... Data carrier "Cardiovector - Data". ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

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• S.P Korolev Rocket and Space Corporation "Energia"
• S.P. Korolev RSC Energia - Important Anniversaries of the Corporation
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... A. M. Neminsky, D. V. Shovkun, and O. T. Vyaselev . ... Received 18 January 1996 . The temperature dependence of ac susceptibility chi ( T ) has been measured at different values of dc magnetic field for Rb 3 C 60 fine powder. ... The chi ( T ) measurements at different dc magnetic fields allow us to distinguish between these two contributions and to obtain precisely the temperature dependence of the London penetration depth lambda ( T ). ...

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• Department of Solid State Physics MIPT
• About ISSP
• XVIII International Astronomy Olympiad: Important Notes for interested