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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 every 14 years QED : -0.1964 (9) 5, 3039 (2009) Theory: J. Chem. ... Wave function is represented by a linear combination of basis functions Choice of the basis functions: · · Explicitly correlated basis set. ...

Peremennye Zvezdy", . ... Find.Chart . ... GSC 04516-02121 . ... The new variable star 2MASS J00511854+5022580 (indicated as V in the finding chart) is inside the field of view of the known variable star V364 Cas. ... The new variable star GSC 04516-02121 (indicated as V in the finding chart) is inside the field of view of the known variable star V405 Cep. ... The variable star 2MASS GSC 00770-00523 (indicated as V2 in the finding chart) is inside the field of view of the known variable star AV CMi. ...

We investigate models for main-sequence and horizontal-branch (HB) stars constructed using the Carson opacities and make comparisons with models based on the Cox-Stewart opacities. ... The drop in the hydrogen-shell luminosity due to the helium-core expansion during HB evolution is greater than that obtained with the Cox-Stewart opacities. ... Studies of main-sequence (MS) stars lead to agreement with Stothers' (1974a,b, 1976) results for homogeneous models constructed with Carson opacities. ...

This page provides explanatory text for the dials shown on the Rice Current Solar Wind Conditions and Current Solar Wind Conditions (Dials Only) webpage. These dials use the last good received set of measurements from the Real Time Solar Wind package on the Advanced Composition Explorer (ACE) spacecraft. ... Measured) This quantity is the number of solar wind protons per unit volume as measured by the ACE Solar Wind Electron Proton Alpha Monitor (SWEPAM) . ... It is measured by ACE/SWEPAM. ...

... Each DFS Department official document has to be issued according to the following internal procedure. Documents to be distributed outside DMD division must also be issued according to the Technical Archive procedure . ... Several documents are also available as complete templates defined internally for DFS Department documentation (e.g. template for Test Plan, for Test Report, .. ... Define the internal document number as: dfs-volxx-yyy-zzzz . ... Document title, . ... Issue number (e.g. 1). ...

Physica C 1 PHYSICA C C ELSEVIER CONDUCTIVITY and Antiferromagnetism of CaCuO2 Thin Films Doped by Sr Gennady A. Ovsyannikova,b*, Viktor V. Demidovb, Yuli V. Kislinskib, Philippe V. Komissinskia,b, Dag Winklera a Chalmers ... revised date here; accepted date here Abstract The results of electrical and magnetic investigations of epitaxial CaxSr1-xCuO2 ( CSCO ) thin films grown by pulsed laser deposition are presented ... Temperature dependence EPR amplitude for two CSCO films with =0.15 ...

... We have measured this "redshift" for the pink black holes, and allowed for it in our calculations. ... We see this effect in the emission from gas around these pink black holes, but it is far too small an effect to account for the pinkness. Thus the swirling motions of gas around or into the black holes cannot produc the colour. ... At first we thought that these things were normal blue black holes hidden behind clouds of interstellar dust, that absorbed the blue light and made them appear pink. ...

... April 26, 2006 4 Monte Carlo Integration Suppose we want to compute where f(x) is a probability density. ... As , the simulated draws will be more and more concentrated around the maximizer of p(x) =2 dens ity =1 0.0 0.1 0.2 0.3 0.4 dens ity -5 0 x 5 0.00 0.05 0.10 0.15 -5 0 x 5 dens ity =20 0.0 e+00 8.0 e-09 -5 0 x 5 April 26, 2006 6 Simulating from a Distribution What does it mean? ... N Step 1: Draw x Step 2: Draw x .. ... N} Discard the first N0 draws Use {(x1(t), x2(t),..., xk(t) ): t= N0+1,2,....

SLIDE 1 Coherent beam­beam e#ects study. ... He has shown that a finite length (in other words equal to # # ) of colliding bunches can lead to the coupling of synchro­betatron modes in the beam­beam system, and thus a head­tail type instability of colliding bunches may arise. ... These modes have been observed in di#erent machines. ... SLIDE 5 Figure shows the dependence of the measured and calculated synchro­betatron mode tunes on the beam current for equal electron and positron bunch intensities. ...