... Big ellipse: the region of the photometric analysis Smaller ellipses: the adopted inner boundaries of the Main Body and the C component Small circles: diffuse background objects, manually selected and removed from the photometry Uncleaned CMDs [V-I, I] of I Zw 18, obtained using Aloisi et al. (left) and Izotov & Thuan (right) datasets. ... Where is the 'halo'? Blue compact dwarf galaxy SBS 1415+435 Hubble Space Telescope / Advanced Camera for Surveys NASA, ESA A. Aloisi (STScI, ESA) et al. ...

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• Galaxy sector, archive 2009
• The Present and Future of Small and Medium Size Telescopes
• C/2010 S1 (LINEAR), C/2010 R1 (LINEAR)

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Flights Chronology . ... ISS Russian Segment . ... Rocket Space Complexes . Sea Launch . ... Bus Module . ... Brief History of Rocket Space Technology Development . ... Flight of the Zvezda Service Module as the key component of the ISS was initiated. ... Contribution of RSC Energia to the Russian Rocket-Space Technology . ...

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• S.P. Korolev RSC Energia - International Space Station
• INTERNATIONAL SPACE STATION
• General Designer

... Cooling and thermal control system (CTCS):an angle between normal of thermal radiator plane (Z-axis) and vector "SC-Sun" must exceed 90 deg.. ... The axes of the first two sensors are in the plane YOZ; they have an angle of 35 degrees with Y and -Y axis being inclined to the direction of -Z axis. ... 30 degrees for Sun; . ... An angle between +Z-axis and direction to the Sun center must exceed 90 degrees. ... An angle between direction "SA-Sun(center)" and XOZ plane must not exceed 30 degrees. ...

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• Description of the RadioAstron project, english version
• RadioAstron main page, english version
• Список литературы и документации

... F. Rodionova and E. A. Kozlova . ... Sternberg State Astronomical Institute, 119899, Moscow, Russia; jeanna@sai.msu ru. ... Brown University - Vernadsky Institute Microsymposium 34, October 8-9, 2001, Moscow, Russia . ... Brown University - Vernadsky Institute Microsymposium 38, October 27-29, 2003, Moscow, Russia . ... Brown University - Vernadsky Institute Microsymposium 40, 2004, Moscow, Russia . ... 1 Sternberg State Astronomical Institute Lomonosov Moscow University, Russia; marss8@mail.ru . ...

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• Родионова Жанна Федоровна
• Morphological Catalogue Of The Craters Of Moon
• Morphological Catalogue Of The Craters Of Mars

The direct detection of gravitational waves is one of those events long-expected by physicists that are nevertheless a significant occurrence which excites the world scientific community as if something unexpected has happened. ... Many rumors leaked ahead of the conference, and the fact that something (that is, a signal corresponding to gravitational waves) was discovered by LIGO (Laser Interferometer Gravitational-Wave Observatory) was discussed on the sidelines. ... arXiv:1602.03868 . ...

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XmTel ----- XmTel is a Motif-based telescope control program based on INDI, the Instrument-Neutral Distributed Interface. ... See the files LICENSE and COPYRIGHT for the details. ... About Epoch ----------- XmTel assumes that the telescope is set to "Epoch of Date", which means that it is using ideal celestial coordinates precisely aligned today. ... XmTel assumes that target coordinates entered from the keyboard are in the Epoch that the telescope coordinates are currently displayed in. ...

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• http://www.astro.louisville.edu/software/xmtel/archive/xmtel-5.1/DOCUMENTATION
• http://www.astro.louisville.edu/software/xmtel/xmtel-7.1/DOCUMENTATION
• Line (ImageJ API)

... 3, 2006 OBSERVATIONS OF THE BINARY STAR 61 Cyg ON THE 26 INCH REFRACTOR AT THE PULKOVO OBSERVATORY D. L. Gorshanov, N. A. Shakht, and A. A. Kisselev UDC: 524.38 Results from an analysis of a forty year series of photographic observations of the binary star 61 Cyg on the 26 inch refractor at the Pulkovo Observatory are presented. The orbit is constructed and the sum of the masses of the components is determined from the relative positions of the components. ...

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• http://www.puldb.ru/nikolaev_2011/PUB_NIKOLAEV_2011/mu.pdf
• http://www.puldb.ru/laza_gao/PUB/aj_1.pdf
• http://www.puldb.ru/laza_gao/FOR_page_11/old_plates.pdf

Curriculum vitФ Evgeny Smirnov Personal Details Date and Place of Birth: Nationality: Address: November 9, 1982, Moscow , Russia Russian Laboratoire J.-V. Poncelet Bolshoi Vlassievskii pereulok, 11 119002 Moscow Russia +7 499 795 11 27 +7 499 795 10 15 smirnoff@mccme.ru http://www.mccme.ru/~smirnoff Phone: Fax: E-mail: Webpage: Current p osition 09. 2009 ­present Researcher, Laboratoire franco-russe J.-V. Poncelet (UMI 2615); 09 ... 2007 Algebra seminar, University of Lyon 1, France; Nov. ...

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• http://www.mccme.ru/dfc/2013/Program2/Khoroshkin_publications_2013.pdf
• IUM10 conference: A.Rudakov
• MCCME: Moscow Center for Continuous Mathematical Education

. This artist's illustration represents the variety of planets being detected by NASA's Kepler spacecraft. A new analysis has determined the frequencies of planets of all sizes, from Earths up to gas giants. Key findings include the fact that one in six stars hosts an Earth-sized planet in an orbit of 85 days or less, and that almost all Sun-like stars have a planetary system of some sort. // Credit: C. Pulliam D. Aguilar (CfA)

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBC6C94F8-FCF7-4C13-8903-2AB6E698CA48%7D
• Spacecraft capture an Earth-directed coronal mass ejection | Astronomy.com
• Gravitational waves remain elusive, according to Planck | Astronomy.com

SPECTRUM ANALYZER OF MAGNETIC PHENOMENA SAMW . Spectrum analyzer allows onboard computation of electromagnetic waves spectra registered (observed) in the ionosphere and magnetosphere in the ELF/VLF frequency band. ... It consists of magnetic antenna, preamplifier, 16 bit sigma delta AD converter, DSP processor and telemetry interface. ... The channels of lower frequencies are averaged and transmitted with lower repetition rate so the telemetry volume is reduced. ... Dynamic range: 90 dB . ...

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• HIGH RESOLUTION IONOSPHERIC MASS SPECTROMETER P-11

Russian . ... text in Russian) . ... The Behaviour of the Bz Component of the Magnetic Field in Coronal Mass Ejections . ... Cooperation of IZMIRAN and Sternberg Astronomical Institute in the Study of the Sublimational Component of the Solar Coronal Radiation . ... Solar Wind and Magnetic Storms in the 24th Solar Activity Cycle . ... text in English) . ... The Solar Corona in the Light of TRACE Observations . ... Expeditions of Irkutsk Astronomers to Total Solar Eclipses in 1981--2012 . ...

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• Glossary of Terms
• UNIXhelp Glossary - "A"
• Remote telescopes

... The bright supernova (hereafter SN) in the galaxy NGC 4527 was first sighted by S. Knight (USA) on April 13.17UT at magnitude ~14.0v. The report of the sighting was subsequently forwarded by phone to the AAVSO. ... SN 1991T. The galaxy NGC 4527 is an Sb(s)II type galaxy with an apparent Blue magnitude of 11.32 (Shapley-Ames, 1981). ... An analysis of this event utilizing visual observations by amateurs, plus a light curve is presented.. ... THE LIGHT CURVE: . ... ISN SN 1991T web page . ...

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• Extragalactic Novae
• SN1989B in M66

Direct measurements of laser light aberration from the ARTEMIS geostationary satellite through thin clouds 1. ... During the experiments, the time propagation of laser signal from the satellite and the pointahead angle for the laser beam were calculated. ... 15,16 Fig. ... In our observations of propagation of laser light from the satellite to MAO OGS through clouds, we directly observed the positions of ARTEMIS that were equivalent to the calculated pointahead angle for the satellite. ...

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• MAO-2014: Astronomy in Ukraine ? Past, Present, and Future
• MAO NASU :: Topic: Open access submissions and content now available (1/1)
• MAO NASU :: Topic: Astronomy in Ukraine: Past, Present and Future (1/1)

... Torgashina, Gert de Lange, Leo de Jongb, Pavel A Yagoubovb a The Kotel'nikov Institute of Radio Engineering and Electronics, Moscow, Russia b SRON Netherlands Institute for Space Research, Groningen, the Netherlands Abstract--A Superconducting Integrated Receiver (SIR) developed for balloon borne instrument TELIS covers frequency range 450-650 GHz. The DSB noise temperature was measured as low as 120 K. The SIR application for high resolution spectroscopy of breathed out air has been proven. ...

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• SETI League Guest Editorial -- Past - Present - Future
• Basic Principles of Direct Chaotic Communications - NDCS-03
• Getting Started in Actor Prolog. Component-Oriented Programming.

Альтернативный форум . Scientific.ru Все форумы . ... Михалыч - 09.10.2006 13:10 . ИМХО вне формата опроса . ... Fermion Interactions and Mass Generation in the Nilpotent Formalism . ... Keywords: nilpotent, mass gap, baryon, Higgs mechanism, vacuum . ... Strong, weak and electric interactions and the acquisition of nonzero mass by fermions and bosons can all be related to the nilpotent structure. ... Time, 09.10.2006 00:02 . ... ИМХО вне формата опроса Михалыч, 09.10.2006 13:10 . ...

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• Новости науки

... There are a lot of computer codes simulating this scattering and freely available in the Internet (see e.g. links on our JPDOC page ). ... The code and input file are available in the directory . ... A slightly modified code of Barber Hill with a C-shell and input files is available in the directory . ... The code, input and test output files are available in the directory . ... See also readme file. file. ... The code, input file and their description (a TeX file) are available in the directory . ...

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• Kholtygin et al., Astron. Astroph. Trans., (2003)
• Kholtygin et al., "Stochastic Data in Astronomy. II.", Astrophysics (2007)
• Extinction properties (transmitted radiation)

... ACCESSORIES . ... OEM COMPONENTS . ... ABOUT LOMO . ... MICROSCOPES . ... OEM OPTICAL COMPONENTS . ... MICROSCOPE APPLICATION GUIDE AND MODEL SELECTOR . ... LOMO stereo microscopes deliver crisp images for such demanding applications as industrial inspection, electronic component manufacturing, biological and botanical studies, classroom teaching, etc. ... LOMO manufactures the widest range of microscope accessories and components such as objectives, eyepieces, condensers, illuminators, stages, etc....

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• OEM Components
• SF-Series
• OEM Optical Components

Authors: V.A. Marsakov , Yu.G. Shevelev , . Journal: 1988, Astron Zh. ... Absolute magnitudes, metallicities, effective temperatures, surface gravities, distances, and tangential velocities are calculated for 5498 F stars with homogeneous data on uvby photometry and proper motion, and placed within 80 pc from the Sun. Components of space velocities, eccentricities of galactic orbits, perigalactic and apogalactic distances, and maximal remotness from galactic plane are presented for 1787 stars. ...

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• Anomalous Absorption Theory
• Mid Scales Role
• Vertical Structure, figures

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

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... The Science Operation Department is composed of Astronomers, Telescope Instruments Operators(TIOs) and Data Handling Administrators(DHAs). ... Astronomers have proposed several methods to quantitatively measure the amount of turbulence above the telescope, which the most common ones is Differential Image Motion Monitor (DIMM). In optical testing, the Hartmann test is the common method to test the quality of optical components. ... Hartmann mask consists of 48 lenses. ...

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