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... В НПО им. С.А. Лавочкина завершается подготовка и испытания астрофизической обсерватории "Спектр- РГ". Аппарат будет исследовать Вселенную в гамма- и рентгеновском жестком диапазоне энергий. 21-24 декабря 2015 г. в ИКИ РАН прошла всероссийская конференция "Астрофизика высоких энергий сегодня и завтра" . ... Спутник строится в НПО им. Лавочкина, а научная программа разрабатывается в Институте космических исследований РАН. ... 2016 ИКИ РАН ...

... 314, 2004 F. Ochsenbein, M. Al len, and D. Egret, eds. Images analysis in Asteroid and Satellites Astrometry Alvaro Lopez Garcґ ґ ia Astronomical Observatory and Astronomy Department, University of Valencia Jose A. Morano ~ Astronomical Observatory. ... At Astronomical Observatory of Valencia University (OAUV), CCD observations of asteroids and big planets satellites are obtained since 2001 with a big format camera and several telescopes. ... CCD field size allows this kind of observations every day...

RADIOASTROPHYSICAL DEPARTMENT  INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . ... Radioastrophysical Department , Institute of Solar-Terrestrial Physics, Siberian Division, Russian Academy of Science. ... Head of Laboratory dr. Gubin A.V. LABORATORY of INFORMATION SUPPLY and METHODOLOGY of RESEARCH . ... Head of Observatory Kitsanov S.V. SIBERIAN SOLAR RADIO TELESCOPE . Siberian solar radio telescope data at 5.7 GHz in I SOHO EIT 171 SOHO EIT 195 SOHO EIT 304 MDI Continuum MDI Magnetogram . ...

... Cambridge . ... Bojan Nikolic web pages home . ... Welcome to the web-log (AKA, blog) about my astronomical research. ... Some of the articles are simply commentary or pointers on others people work in astronomy and contain no original research . ... Simple smoothing of astronomical images in FITS format (April 29, 2012) . ... Talk at the University of Cambridge (November 3, 2010) . ... Introductory talk at the Kavli Institute for Cosmology, Cambridge (March 22, 2010) . ...

NATIONAL ASTRONOMY AND IONOSPHERE CENTER . ... Astronomy . ... Visitor Center . ... Kick-Off Ceremony of the Arecibo Observatory 50th Anniversary . ... UW - Madison Astronomy Department Board of Visitors€а ( one day meeting ) . ... 27, Arecibo Observatory . 1:30 - Visitor Center WELCOME - Bob Mathieu . 1:45 - History of Arecibo Observatory and Intro to Telescope - Ed Churchwell . 2:05 - Surfing Galactic Radio Waves with the Arecibo radiotelescope - Snezana Stanimirovic . ...

PERFORMANCE COMPARISION OF KODAK DCS460 DIGITAL CAMERA AND PIXELVISION BACK-ILLUMINATED CCD . ... ABSTRACT : A Kodak DCS460 digital camera (with 1300 x 1000, 9-micron square pixels) and a PixelVision, back-illuminated digital CCD camera (with 1024 x 1024 elements, 12-micron square pixels) were tested at calibrated light levels ranging from 10 -2 footcandles to 10 -5 footcandles. The PixelVision back-illuminated CCD was shown to be 10,000 more sensitive than the Kodak DCS460 CCD camera. ...

... Dept. for Astrometry & Space Geodynamics . ... Dept. for Physics of Stars&Galaxies . ... Dept. for Physics of Planetary Systems . Dept. for Solar Physics . ... Collaborators of our Department research Solar system planets and their satellites, planetary systems around stars of Milky Way and stars having disc structures. ... Researches of Solar system bodies, variations in planetary atmospheres and on their satellites, remote methods of researches the vertical structures of planetary atmospheres. ...

... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... An Analytic Approximation to the Bounce-Average Drift Angle for Gyrosynchrotron-Emitting Electrons in the Magnetosphere of V471 Tauri . ... To calculate how far the electrons drift before they have lost sufficient energy to be indistinguishable from the ambient population of mildly relativistic electrons we integrate . ...

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... Meta Index / Home Page / Description / Specifying source region shapes . When radiusstyle =`contour', the task calculates the source region shape as an elliptical locus which approximates the contour of the PSF at a given flux value. ... Clearly, in order to calculate the shape of such a flux contour, it is necessary firstly to normalize the PSF to the source brightness and secondly to determine the flux level (in `brightness' units per pixel) at which to find the contour. ...

QED calculations of H2 molecule Vladimir A. Yerokhin St. Petersburg State Polytechnical University in collaboration with Krzysztof Pachucki Warsaw University FFK 2013, Pulkovo, St. Petersburg, October 7-11 Do we need QED for H2? ... 150, 51 (2011) An order of magnitude in precision