... For the past years I have been working on the problem of synthesis of light curves of close binary systems, consisting of a normal star and a compact object (point object with fixed X-ray luminosity). ... Possible existence of a bright spot on the disk's lateral surface is taken into account. ... The last of then will be published in Gordon and Breach Publishers ( Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ... Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ...

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... Within SAS, a tool is available to check the pile-up fraction in the pn data: epatplot . This tool compares the observed pattern distributions (derived from a pn calibrated and concatenated even list) with the calibrated models. ... The lower panel is the key element for the evaluation of the pile-up fraction: it shows the observed distribution of pattern as a function of energy (PI channel in Analog-Digital Units ), using the same color code. ... Pages maintained by SAS librarian . ...

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• Parameters for EMOS 1

Next: Methods for Structuring and Searching Very Large Catalogs . ... We have explored two automated classification methods: supervised classification using Artificial Neural Networks (ANN) and unsupervised classification using Self Organized Maps (SOM). These methods are used to classify IUE low-dispersion spectra of normal stars with spectral types ranging from O3 to G5. This paper describes the application of automated methods to the problem of the classification of stellar spectra. ...

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• ADASS 2002 Conference Proceedings
• Substepping and its Application to HST Imaging

On the concept of a cold-electron bolometer mixer M. Tarasov1,2, and L. Kuzmin1 Chalmers University of Technology, KemivДgen 9, SE-41296 GЖteborg, Sweden Institute of Radio Engineering and Electronics, Mokhovaya 11 bld. ... CEB mixer combines advantages of Hot Electron Bolometer (HEB) mixer such as high signal frequency and low LO power, and advantages of SIS mixer such as low noise, high IF and immunity to small temperature variations. ... Finally for CEBM we can have moderate power gain. ...

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• Atmospheric influence on the different radioengineering systems functioning.
• ICLP 2003, International Conference on Logic Programming, Mumbai (Bombay),...
• Project 8 - RFBR - Dynamical and non-equilibrium electron transport and

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . Armagh Observatory reports that October was colder than average with normal amounts of sunshine and rainfall. Precipitation amounted to 86.9 mm (3.42 inches), which is about the same as the most recent 30-year (1981-2010) average for October. ... The mean monthly temperature was 8.6 degrees Celsius (47.5 degrees Fahrenheit), which is about 1.5 degrees Celsius below the most recent 30-year average for October. ...

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• sfit help file
• Simon Jeffery's Software Store: PHOT library
• Spectrum v1 - Examples

Pulkovo Photographic Plate Database . To find a certain plate, type its number, choose instrument and click button FIND Instrument: Normal Astrograph 26-inch refractor Plate number: . To find plates with a certain sky area: choose instrument, type coordinates (R.A. and Dec.) of the center of this area, type radius of this area, type (optionally) names of required objects, and click button FIND . ...

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• Pulkovo Databases
• page_17
• plut_pub

Magnetic Stars, 2011, pp. ... 2010). ... 463 Figure 2: Difference between individual and average spectra in Fig. 1 with phase (vertically, on the right) Figure 3: Almost in a year repeatability of spectral lines form (2009.07.05 and 2010.05.31) in an identical phase 464 CHOUNTONOV 4000 3000 Magnetic field, Bz(G) 2000 1000 0 -1000 -2000 2008/05/23 2010/05/31 -3000 0.0 0.2 0.4 0.6 0.8 1.0 phase Figure 4: Longitudinal magnetic field variations with phase (the sine curve, Rivinius et al., ...

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• A unique isolated dwarf spheroidal galaxy KKR25
• Galaxy sector, archive 1995

Asteroids, Comets, Meteors (2008) 8010.pdf SPECTRAL SIGNS OF CARBONACEOUS CHONDRITIC MATERIAL ON (21) LUTETIA V.V. Busarev, Sternberg Astronomical Institute (SAI), Moscow University, Universitetskij pr., ... We have discovered considerable variations in the continuum slope and shape of the visible-range reflectance spectra of the asteroid with rotation in November 2004 (4/5, 5/6 and 7/8) and March 2006 (3/4). ... Resulting normalized (at 0.55 m) and smoothed reflectance spectra are shown in Fig. ...

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• http://selena.sai.msu.ru/Bus/Publications/ms40/15_Busarev_etal.pdf

... Wavelength Calibration . ... 30s wavecal plot . 30s flatfield plot . ... HeNeAr 4400 . B rQrtz 4400 . ... HeNeAr 4500 . ... BrQrtz 4200 . BrQrtz 4500 . ... These figures in the above table show the number of counts received from each of the lamps in a 30 second exposure with the 1.5 arcsec slit. ... Users have the option of taking calibration lamp data at the rotator angle of each object, but in many cases, it should be possible to measure the shift using observations of night sky lines. ...

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• TUI:Scripts:Built In Scripts:SPIcam:Sky Flats
• emerg_close
• TUI:Scripts:Scripting Tutorial:User Input

... Automated Spectral Classification Using Neural Networks E. F. Vieira Laboratorio de AstrofТРsica Espacial y FТРsica Fundamental P.O.Box 50727, 28080 Madrid, Spain, Email: efv@lae#.esa.es J. D. Ponz GSED/ESA, Villafranca P.O.Box 50727, 28080 Madrid, Spain, Email: jdp@vilspa.esa.es Abstract. We have explored two automated classification methods: supervised classification using Artificial Neural Networks (ANN) and unн supervised classification using Self Organized Maps (SOM). ...

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• http://www.stecf.org/conferences/adass/linuxbof.html
• http://www.stecf.org/goods/releases/20040430/goods_isaac_tiles.reg

... Green and blue curves - CYGAM telescope (squares - no constraints on the angle a , triangles - a <0.5 0 ); red curve - EGRET telescope. Effective area versus photon incidence angle to relative the longitudinal telescope axis (squares - no constraints on the angle a , triangles - a <0.5 0 , spectral index g= 2). ... Angular resolution for normal to the axis X incidence versus source power law spectrum index (squares- no constraints on the angle a , triangles- a <0,5 0 ). ... CYGAM (PDF, 450 Kb) . ...

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• Space Research Institute (IKI) Seminar
• DOK-2 Results Page

... Intitul anglais du sujet propos : Normal form of differential equations with constraints . ... Domaine scientifique principal de la th se : Math matiques . Domaine scientifique secondaire de la th se : Math matiques et interactions . ... Particular cases of this problem are the problem of singularity of differential equations y'=f(y) as well as the problem of differential equations with constraints: y'=f(x,y) et g(x,y)=0. ...

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• Labo J.-V.Poncelet: A.Glutsuk
• Algebraic Number Theory
• IUM10 conference: A.Sergeev

spaceweb@oulu.fi - last update: 9 May 1998, 2010 UT (RR) . ... They were first discovered by Russell and Elphic (1978) and Haerendel et al. (1978), who studied the magnetic field measurements in boundary normal coordinates near the magnetopause, and found bipolar signatures in the Bn component (outward along the boundary normal): first outward and then inward (normal FTE) or the other way around (reverse FTE). ... 1996). ... Space Res. 18 , (8)151-(8)160, 1996. ... Space Physics Text Book of Oulu ...

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• Pictures/Рисунки
• Solar Energetic Particles
• Discontinuities and shocks [Oulu]

... Space flight . Crew training . ... Space camp . ... acquiring practical habits and skills of performing all the flight operations envisaged for a flight participant; . maintaining and honing professionally required qualities and skills for a successful activity in conditions of effect of adverse factors of a space flight, as well . ... preparing for the activity outside the spacecraft; . ... preparing for professional activity in conditions of effect of the space flight factors; . ...

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... astro-ph . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . ... Quasar Variability in the Framework of Poissonian Models . ... It is shown that in this very general framework the well established anti-correlation between variability amplitude and wavelength can only be understood as an effect of an underlying spectral component which remains stable on long time-scales, and is redder than the variable component. ...

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. Previous slide . Back to first slide . View graphic version .

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• Context
• CHIAKI's Research
• Introduction

... Jan Feb Mar Apr May Jun Jul Aug Sep . Jan 01 [ 1768 kByte] . Jan 02 [ 1706 kByte] . Jan 03 [ 1705 kByte] . Jan 04 [ 1694 kByte] . Jan 05 [ 1657 kByte] . Jan 06 [ 1724 kByte] . Jan 07 [ 1697 kByte] . Jan 08 [ 1666 kByte] . Jan 09 [ 1759 kByte] . Jan 10 [ 1600 kByte] . Jan 11 [ 1606 kByte] . Jan 12 [ 1692 kByte] . ... Jan 14 [ 1748 kByte] . Jan 15 [ 1672 kByte] . Jan 16 [ 1752 kByte] . ... Jan 18 [ 1711 kByte] . Jan 19 [ 1686 kByte] . ...

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• VLA in 1934
• ODE in 1946
• MOS in 1947

Stellarium 0.12.3 . ... Renderer . FileљStructure . ... core . ... StelVertexAttribute.hpp . ... 53 љ inline int attributeDimensions( const AttributeType type) . ... 122 љ qDebug() << "Unknown vertex attribute type: \"" << typeStr . ... 179 љ // Ensure that every kind of vertex attribute is present at most once. 180 љ foreach ( const StelVertexAttribute & attribute, attributes) . ... 186 љ "Vertex type has more than one vertex position attribute" ); . ... 239 љ #define VERTEX_ATTRIBUTES(...)\ . ...

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• Stellarium: BooleanFader Class Reference
• Stellarium: StelTextureCache< TextureBackend > Class Template Reference
• Stellarium: Member List

Do we need various assumptions to get a good FCN? A new multiple layer spectral method Cheng-li HuangMian Zhang Shanghai Astron. ... No FCN ! ... FCN,FCN,FCN.. Multiple layer spectral method (MLSM) + Linear Operator Method (LOM) Finite Element Method (FEM) · · Traditional approach solves one order ellipsoid only. ... Main Idea of FEM Boundary Surface could be described as: Let's consider how to solve the dynamic equation: Traditional Approach: Equivalent Spherical Domain . ...

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• page_17

Method of Calculating Cometary Orbits . ... A method of constructing a numerical theory of comet motion covering large intervals of time is presented. ... Very Long Baseline Interferometry (VLBI), Near Earth Objects (NEOs), calculating cometary orbits, numerical theory of comet motion covering large intervals of time , radial component of non-gravitational acceleration , transverse component of non-gravitational acceleration , normal component of non-gravitational ...

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• Keywords_107