XMM-Newton Science Analysis System . omfchain (omfchain-1.22.13) [xmmsas_20030110_1802-5.4.1] . Meta Index / Home Page Mod-8 noise may affect the estimation of background and the output light-curves of very bright source. An algorithm to account for this pattern around bright objects needs to be developed. ... XMM-Newton SOC/SSC -- 2003-01-10 ...

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• Background: motivation for developing this procedure

Find Similar Abstracts . ... The velocity of clusters of galaxies relative to the microwave background - The possibility of its measurement . ... 02/1980 . ... BACKGROUND RADIATION, GALACTIC CLUSTERS, MICROWAVE EMISSION, POLARIZED RADIATION, VELOCITY MEASUREMENT, BACKGROUND NOISE, COSMIC GASES, COSMOLOGY . ... Use: Authors Title Abstract Text Text Query with Keywords Return: Query Results Query Form Database: Astronomy Instrumentation Physics and Geophysics ABSTRACT QUERY USER FEEDBACK HELP ...

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• Starobinsky
• Seminars
• Be/X-ray binaries and candidates

Proposer's Guide VLBI Space Observatory Programme Prepared by the VSOP Science Operations Group Institute of Space and Astronautical Science 10 August 1995 Proposals Due: Friday, 17 November 1995 Abstract This guide provides the technical information necessary to write a proposal for scientific observations with the VSOP space VLBI mission. ... 2 VSOP Spacecraft Antenna The main antenna of the VSOP spacecraft is of a Cassegrain design with a three­waveband coaxial feed at the focus. ...

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• The UKST H Survey - Scientific Background
• Overview of ATNF Engineering
• AstroGrid

... In addition, IZMIRAN comprises the St.Petersburg branch and magnetic ionospheric observatory in Kaliningrad. The history of IZMIRAN is largely that of investigating magnetic storms and sub-storms on the Earth surface, in circum-terrestrial and interplanetary space, initially by means of a network of ground stations of the Soviet Union (1930s - 1940s) and the nonmagnetic skunner "Zarja", then through the extensive use of magnetic measurements on artificial Earth satellites and automatic stations. ...

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• Soft X-ray Class of Far-Side Flares
• Magnetic Flux of EUV Arcades and Dimmings
• Spectra of raduo bursts and SEPs

... Астронет | ... Astronomy search engine . ... PhysicsWeb Home Page . ... Sternberg Astronomical Institute . ... Astro Space Center Home Page . ... Landau Institute for Theoretical Physics . ... Astronomy and Space Physics Dept of Kiev University . ... NATIONAL RADIO ASTRONOMY OBSERVATORY Home Page . ... Space Telescope Science Institute Home Page . ... The Next Generation Space Telescope Home Page . ... Sky & Telescope: The Essential Magazine of Astronomy . ... Springer LINK - Physics Online Library ...

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• Астронет > Deep Impact Spacecraft Hurtles Toward Comet
• Deep Impact Spacecraft Hurtles Toward Comet
• Journal "Peremennye Zvezdy"

... Институт прикладной математики им. М.В.Келдыша . БАЛЛИСТИЧЕСКИЙ ЦЕНТР . О Центре . ... Баллистический Центр Института прикладной математики им. М.В.Келдыша РАН . Баллистический центр (БЦ) ИПМ им. М.В. Келдыша создан по предложению С.П. Королева и М.В. Келдыша в 1965 году. На него были возложены работы по баллистико-навигационному обеспечению (БНО) управления полетом пилотируемых кораблей и автоматических космических аппаратов научного и народно-хозяйственного назначения. ...

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. Dedicated to 40th anniversary of the . first artificial Earth satellite launch . Russian (Win) .

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... The TESIS is a set of solar imaging instruments developed by the Lebedev Physical Institute of the Russian Academy of Science, and launched aboard the Russian spacecraft CORONAS-PHOTON on January 30, 2009. The main goal of the TESIS is to provide complex observations of solar active phenomena from the transition region to the inner and outer solar corona with high spatial, spectral and temporal resolution in the EUV and Soft X-ray spectral bands. ... Solar activity hits a new low . ...

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All abstracts are due on 1 June 1998, these should be on one A4 page. A simple LaTeX template is given below. Please email LaTeX file to ambn@star.arm.ac.uk . ... Here comes the author(s) of the paper, please indicate within $^...$ %% the number which corresponds to the institute of each author. {\bf{ W. Me$^1$, A.N Other$^{2,3}$ \ N. Another$^2$}} %% Here write your institute name(s) and address(es), %% the number in $^..$ indicates your author number, for example: $^1$ {Here .. ...

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• Abstract 200
• Lindsay Centennial Symposium
• Abstract

... By the time Isaac Newton entered college, the scientific revolution of the 17th century was well underway. ... Men like Copernicus, Kepler, Galileo, and Descartes had all helped develop a new view of nature. ... Plato is my friend, Aristotle is my friend, but my best friend is truth." ... Isaac Newton was born on Christmas Day, 1642, the same year Galileo died. ... He was one of the most creative geniuses the world has ever seen and to many people the greatest scientist who ever lived. ...

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• http://zebu.uoregon.edu/disted/ph121/l3.html
• U of O High Energy Physics Seminars
• The Galaxy Gallery: Messier Objects

... The performance of a detector can be characterized by its efficiency for measuring individual x-rays or for measuring Bragg peak intensities. The performance for detecting individual x-rays is well modeled by the DQE. The performance for measuring Bragg peak intensities in the presence of an x-ray background can be modeled by an expanded definition of the DQE which allows inclusion of experimental constraints, the XDCE. ... The x-ray background per pixel has decreased. ...

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• http://www.sao.ru/cats/~satr/RFSymp/abs/38_Verkhodanov2.ps
• http://www.sao.ru/cats/~satr/RFSymp/abs/38_Verkhodanov2.pdf
• Abstract

... We present centimeter and millimeter interferometric continuum and molecular line images of the massive star-forming region AFGL 5142. ... The emission peak coincides with a 1.5 mJy centimeter continuum source. ... CH3CN (14-13) and (12-11) spectra indicate a gas temperature ~65 K in the innermost core. While the millimeter continuum emission is probably mostly due to optically thin thermal emission from dust grains, the centimeter continuum source is consistent with an ionized wind. ...

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• IG45VLA (Abstract)
• Automated Spacecraft
• G35.20-1.74 (Abstract)

... Astronomy search engine . ... PhysicsWeb Home Page . ... Sternberg Astronomical Institute . ... Astro Space Center Home Page . ... Landau Institute for Theoretical Physics . ... Astronomy and Space Physics Dept of Kiev University . ... NATIONAL RADIO ASTRONOMY OBSERVATORY Home Page . University of Hawaii - Institute for Astronomy . ... Space Telescope Science Institute Home Page . ... Sky & Telescope: The Essential Magazine of Astronomy . ... Springer LINK - Physics Online Library . ... Home . ...

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... Annual Meeting . ... Galileo Teacher Training Program Workshop . ... Co-sponsored by the Astronomical Society of the Pacific, Fiske Planetarium, and the Lunar Science Institute . In this hands-on workshop, teachers in grades 3 - 12 will learn how to do age-appropriate, inquiry-based activities in astronomy and physical science. ... The Galileo Teacher Training Program is a new model for teacher professional development established during the 2009 International Year of Astronomy. ...

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• ASP: The Astronomical Society of the Pacific: Your Partner in Education
• ASP: 2009 Award Winners Press Release
• ASP: Family ASTRO FAQ

Weaving together Astronomy+Statistics+Computer Science+Engineering+Intrumentation, far beyond the growing borders . ... Posts tagged ?GLAST? ... Category: Astro , gamma-ray , High-Energy , News , Optical , X-ray | ... Posted by chasc . ... and intends to post status reports and related information on it. ... This week, instead of only filtering AstroStatistics related papers from arxiv, I chose additional arxiv/astro-ph papers related to CHASC folks? astrophysical projects. ... Category: arXiv | ...

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• Statistics 310 2005-2006
• The AstroStat Slog Summer Institute
• The AstroStat Slog Blog Archive SLAC Summer Institute

... There are preliminary series of photometric and radio spectral observations of the above-mentioned stars, archival data on the light curves of the stars, results of the search for OH and H 2 O maser emission in IRAS point sources that possess the IR parameters similar to Miras. ... The aim is a detailed study of the maser emission variability. ... In 1996-1997, astronomical observations of Mira Ceti-type stars (miras) were carried out in three spectral ranges: optical, infrared, and radio. ...

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• Rudnitskij Georgij M. Home Page
• Monstr's link
• Hot links of Comet WWW site