... The nodes defined by the specified region and lattice spacing will be set equal to one of three possible values depending on whether the node is outside, on the polygon perimeter, or inside the polygon. ... The xy-files simply represent data point locations and the mask is set to the inside or outside value depending on whether a node is within a maximum distance from the nearest data point. ... Default is grid registration]. ... S Set nodes depending on their distance from the nearest data point. ...

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• E-P transitions for different orbits
• Effect of sources evolution on
• Concluding Remarks and Future Prospects

... The distinction of our approach is in that we unite the Actor Prolog concurrent ob ject-oriented logic language [ 1,2,3] with the Structural Analysis and Design Technique (SADT) diagrams to obtain new issues in the following areas: 1. ... Graphic user interface management. ... The individual blocks of visual user interface based on the SADT diagrams are implemented by using parallel processes of Actor Prolog. ... We applied the visual programming method for logic programming of Internet agents [4]. ...

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• Actor Prolog User Guide. SADT.
• Open Systems Handbook: A Guide to Building Open Systems
• Getting Started in Actor Prolog. Oil Production.

... Microlocal Analysis is a theory of Pseudo-Differential Operators and Fourier Integral Operators (PDOs and FIOs). ... Microlocal analysis comes in few flavors. ... We will consider semi-classical PDOs and FIOs: one can always get from there to standard PDOs and FIOs but semi-classical theory has more applications. Less formal description of (semi-classical) microlocal analysis is ``a semi-classical limit of quantum mechanics'' or ``high-frequency limit of electrodynamics'' (etc). ...

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• IUM10 conference: M.Blank
• Workshop on geometric analysis and spectral theory. Abstracts

... I also found it great fun as a single player game as I tested it out: I just made it my goal to kill everybody and considered that to be a 'win'. ... In deathmatch, you and your buddies will no doubt try to make it to the tiny center island to get the BFG9000, but this is a bit difficult when everyone is trying to do it! ... EXAMPLE COMMAND LINE: C:\DOOM>ipxsetup -deathmatch -episode 2 -file DETHWALK.WAD -nodes 4 -skill 4 Try "-nomonsters -skill 1" for a clean pistolfight with no BFG. ...

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• http://crydee.sai.msu.ru/ftproot/pub/rec/games/idgames/levels/doom/p-r/riker11.txt
• http://crydee.sai.msu.ru/ftproot/pub/rec/games/idgames/levels/doom/d-f/ds2v1.txt
• http://crydee.sai.msu.ru/ftproot/pub/rec/games/idgames/levels/doom2/s-u/surreal2.txt

... Under certain conditions, like those in the nucleus of a QSO, all atoms can be made to emit light at particular wavelengths. ... If that source is approaching the observer, the wave is squashed up onto itself making the wavelength shorter. ... This is redshift. ... You can see how the section of the QSO spectrum which we observe changes with redshift. ... We then see how far we had to slide the observed spectrum along the scale to make it match and that is the objects redshift. ... The 2QZ team . ...

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... This is possible at modest cost due to the low moments of inertia of the telescope and enclosure. ... This same performance will be achieved in higher winds when the telescope enclosure is facing away from the wind, or by using wind screens. ... The telescope system (MILT) will be remotely operable with an on-site operator's assistance by an astronomer located at one of the ARC member institutions. ... Mean Wind Speed . ... Offsets > 10 deg: 1 arc sec rms max . ... 5 sec max, tracking to tracking . ...

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• Primary mirror support
• Fiber Positioning System Performance
• TCC UDP Packets

Ground Support of RadioAstron . Control and Tracking Stations . RadioAstron satellite control (command transmission, telemetry, orbit measurements) will be conducted from Evpatoria and Bear Lake control stations. ... Coarse orbit measurements will be carried out from control stations. Each measurement takes ten minutes. ... Orbit measurements at tracking stations give only radial component of spacecraft velocity but the measurements are going continuously during observing sessions. ...

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• Abstract

The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...

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• Description of SED models
• Description of system SEDs
• FADPS - Flexible Astronomical Data Processing System

RTT150 . ... This search system is designed for generating the necessary information on series of pointings (observations of each source consist of sets of exposures with different filters and sometimes with different exposure times) for observed sources. Search results appear at the separate page as a table with the following data: . DATE - real (not evening!) observations date (in YYYY-MM-DD format); . ... Bin - minimal CCD binning mode (may vary during the observations); . ...

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• RTT150 Technical Description

... An Orion of a Different Color . ... It is a familiar object though, the grand stellar nursery known as the Orion Nebula . But the striking picture combines images taken through three separate filters, each designed to record different emission lines - light from Sulfur, Oxygen, and Hydrogen atoms glowing in the tenuous nebular gas. At such low densities , Sulfur and Hydrogen atoms emit red colors while Oxygen glows green. ... Publications with keywords: Orion Nebula . ... The Heart Of Orion . ...

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• Астронет > An Orion of a Different Color
• Journal "Peremennye Zvezdy"
• XWare > APOD

... SiD workshop, Fermilab, April 9-11 2007 April 9, 2007 Nick Sinev, SiD design Workshop, Fermilab 1 Topics 1. ... What and how was simulated What and was One column clusters effects Accepted background density Hit reconstruction efficiency Hit efficiency How to improve efficiency Conclusions April 9, 2007 Nick Sinev, SiD design Workshop, Fermilab 2 What is this April 9, 2007 Nick Sinev, SiD design Workshop, Fermilab 3 Marty's idea Shift charge in neighboring columns in opposite directions. ...

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• University of Oregon Center for High Energy Physics - ATLAS
• Energy From the Oceans
• Astronomy 123 Spring 1996

On Systematic Differences in Individual Solutions and IERS Products Zinovy Malkin Institute of Applied Astronomy RAS, St. Petersburg, Russia 1 Present status Proper determination, modelling, and accounting for systematic differences between contributed series is of the great importance in compilation of the IERS products. ... Possible sources of systematic differences are: Ї Different reference systems (e.g. TRF, CRF, geopotential, time scale). ... 87 IERS Technical Note No. ...

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• General description of the database
• Description of database

... Description . Catalog . ... In the Catalog, we publish equatorial (ЮБ 2000 , ЮД 2000 ) and galactic (l,b) coordinates of cluster centers derived as the position of overdensity in 2MASS catalog (Koposov et al. ... Distances, color-excesses and ages are the mean-square values calculated using all available evaluations from different color-magnitude diagrams. ... There are individual pages for every cluster where all available plots and parameters are published. ... 2002). ...

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Who hosts Family ASTRO events? ... How much astronomy do I need to know to lead a Family ASTRO event? How much astronomy do I need to know to attend a Family ASTRO event? ... One key requirement is that leaders attend a one-day Family ASTRO training session before doing their own events. top . ... As a Family ASTRO event leader, you are responsible for securing a venue in which to hold the event, recruiting families to attend, and providing extra materials needed for the activities. top . ...

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• ASP: Using Multicultural Dimensions to Teach Astronomy
• ASP: A Flag for Mars
• ASP: Sharing the Universe

The design of IAO-Diploma has academic (conservative) style. ... The first row consists of three cells. ... Second cell - logo of EAAS - Galaxy, negative image. ... The second row consists of one cell, two lines. ... Second line - words 'International Astronomy Olympiad'. ... There should be a text in English with the name of the awarded student, his or her team, explanation of awarding including the degree of Diploma and the Number of the International Astronomy Olympiad like: Adam Kohl . ...

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• X-Ray Structural Analysis
• Laboratory of spectroscopy of defect structures ISSP RAS
• CdSe Safety Data Sheet

hstpolsim -- Produce simulated polarization input data frames for HST instruments . ... inint = "" [name] . ... Name of the HST instrument for which simulated polarization images are to be produced. ... Name of the instrument specific polarizing filter for simulated images (ignored for SPECIAL instrument). filtname = "" [name] . Name of the instrument specific colour filter for simulated images. ... The header parameter FILTER provides the filter name and POLANG the polarizer angle. ...

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• CONICA: The high resolution near-infrared camera for the ESO VLT
• HSTPOLIMA (V1.00) --- April99 --- HSTPOLIMA (V1.00)
• POLIMODEL (V1.00) --- April99 --- POLIMODEL (V1.00)

... SSAU History . SSAU roadmap . ... Equipment testing began on January 4. ... The magnetometer Shtil-M No. 2 is equipped with six sensors that measure the magnetic field in different compartments of the device, fix electrical discharges and the impact of the space environment on the equipment functionality. ... The magnetometer Shtil-M No. 2 is the third unit of the series, which was created in SSAU Institute of Space Device Engineering led by Professor Nicholay Syomkin. ... e-mail: ssau@ssau.ru . ...

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• Samara University scientists designed new materials for the accumulator of the

To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...

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• MAO NASU :: Topic: The "Flame" description (1/1)
• Traffic Analysis for UARNET -- ursa
• Traffic Analysis for ursa (UARNET)

... 18-Jan-2010 17:22 . ... Apache/2.2.3 (CentOS) Server at www.wdcb.ru Port 80 ...

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• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/f min
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fo Es
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/M3000

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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• VISTA - Visible and Infrared Survey Telescope for Astronomy