... The measured bolometric flux and corrected NPOI angular diameter yield an effective temperature of 8600+/-500 K. Least-squares comparisons of synthetic spectral energy distributions from 1220 Г: to 3.6 cm with the observations provide estimates for the effective temperature and the mass-loss rate of ~=8400+/-100 K and (8+/-3)Г-10-7 Msolar yr-1, respectively. ... ADS Citation Query . citations = 34 . citations vs. year [year,citations] . ...

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• A New Database of Observed Spectral Energy Distributions of Nearby Starburst
• SODRM Statistical Summary 2012
• KPNO IRIM Observations of the Hubble Deep Field

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

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• Results scientific researchs LRS
• Determination of atmospheric parameters and calculation of chemical composition
• Results scientific researchs 20

. Spectral Energy Distribution of the microquasar LS 5039. This is a composite: observations were not taken simultaneously. From Paredes, Bosch-Ramon, Romero, A , 451, 259 (2006).

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• The AstroStat Slog Blog Archive [ArXiv] Bimodal Color Distribution in GCS,
• Comments on: chi-square distribution [Eqn] By: Alex By: vlk By: aneta By: aneta
• The AstroStat Slog Blog Archive chi-square distribution [Eqn]

Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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• Amplitude Distribution
• Initial binary parameters
• Test of the Initial Mass-Ratio Distribution

Next: Pulsations Up: PHYSICAL CHARACTERISTICS Previous: PHYSICAL CHARACTERISTICS . The fundamental properties of RCBs may be deduced from their spectra at maximum light. ... The properties of a stellar atmosphere may be measured from both the large-scale features - the broad-band flux distribution - and the detailed spectrum of absorption lines. ... They show that, in general, hydrogen makes up less than one part per thousand down to less than one part per million of the stellar atmosphere. ...

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• Armagh Observatory
• Galactic distribution and absolute magnitudes
• Refereed Journal Publications 2004

An investigation of the spectral energy distribution (SED) of the compact steep-spectrum (CSS) source and possible radio-loud narrow-line Seyfert 1 galaxy (NLS1), PKS 2004-447, is presented. ... Analysis of a non-contemporaneous, low-resolution optical spectrum suggests that the narrow-line region (NLR) is much more reddened than the X-ray emitting region suggesting that the gas-to-dust ratio in PKS 2004-447 may be very different than in our own Galaxy. ...

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• The galaxy IC 2554
• Distribution of Schedule Files
• FCC 35

Proposal Identi cation No.: T1057 Date Received: 1997-Oct- 1 20:15:45 Technical Page Proposal Type: Regular General Category: Terrestrial Aeronomy Sub-Category: Radar Observation Category: Ionospheric Total Time Requested: 36 Hours Proposal Title: Study of unusual electron distribution functions in the winter day time E-region ABSTRACT: The variations of the density, temperature and energy distribution function of the electrons may give some clues about the energy balance in the Ionosphere. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/ZhoutagT2403tp.pdf
• Radar Meteor Workshop

XMMґNewton CCF Release Note XMMґCCFґRELґ135 EPIC MOS Spectral Response Distribution R. D. Saxton, S. Sembay 10 Dec 2002 1 CCF components Name of CCF VALDATE EVALDATE List of Blocks changed CAL VERSION XSCS flag EMOS1 REDIST 0020.CCF 1999ґ12ґ10 2000ґ07ґ15 CCD REDISTRIBUTION ґn 3.152 NO EMOS1 REDIST 0021.CCF 2000ґ07ґ15 2000ґ11ґ09 CCD REDISTRIBUTION ґn 3.152 NO EMOS1 REDIST 0022.CCF 2000ґ11ґ09 2001 ґ04ґ18 ... Mosґ1, epoch 1 (rev 62) imaging mode response, all patterns. ...

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• http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0169-1-1.ps.gz
• http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0183-1-0.ps.gz
• http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0145-1-1.ps.gz

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• The Galaxy Gallery Page VII: Infrared Imaging
• Evidence for Dark Matter
• Physics 410/510 Observational Cosmology

The radial distribution of metallicity of star-forming galaxies in a galaxy cluster can inform us about the mass assembly and enrichment history of the galaxy cluster. ... Both galaxy clusters are cool-core clusters at redshift z т?? ... The gas-phase metallicity of star- forming galaxies in MACS1115+01 exhibit anti-correlation with projected distance т??0.15 ТБ 0.08 dex/Mpc, whereas the radial metallicity distribution of RXJ1532+30 is statistically flat (т??0.09 ТБ 0.12 dex/Mpc). ...

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• David Nicholls: CV and publications
• The SMS Survey
• COALA - Computational Astrophysics Laboratory

... The goal of this analysis is to determine to what extent the systematic errors affect the measured eclipse depth and time of mid-eclipse. ch1 0.120 0.120 0.300 ch2 0.120 0.120 0.300 0.00213 0 .0 0 0 Tmid Kurtosis Poly Wave MCMC ch1 ch2 9 13 0.06 0.92 1.5 - 0 .2 3 0.00094 0.000 Figure 3: p vs. rank plots showing that with the extra systematic error added the results for the depth in channel 1 (left) and channel 2 (right) become close to Gaussian. ...

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• http://www.mrao.cam.ac.uk/wp-content/uploads/2014/05/DHomeier.pdf
• http://www.mrao.cam.ac.uk/~krause/KA-nam-2006-poster.pdf

... Visible Distribution of Galaxies. ... Features of Elliptical, Lens-Shaped, Spiral and Irregular Galaxies. Galaxies with Bar. ... Distribution of Surface Brightness of Surface and Spiral Galaxies. ... Color Characteristics of Galaxies. ... Methods of Galaxies' Mass Determination. ... Hidden Mass of Spiral Galaxies. ... Features of Dark Matter Distribution in E and SO Galaxies. ... The Whole Number of Galaxies and Their Density by the Results of Observation on the 'Hubble' Space Telescope. ...

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• Theoretical Astrophysics
• Olexiy V. Agapitov presentations & posters
• INFRARED FOURIER-SPECTROMETER SICH-F

International workshop "Europa lander: science goals and experiments" Space Research Institute (IKI), Moscow, Russia 9-13 February 2009 Near-Surface Atmosphere of Europa V.I. Shematovich Institute of Astronomy RAS, 48 Pyatnitskaya str., ... Near-surface atmosphere of Europa: O2 kinetic energy distributions ґ Model C Surface source of O2: surface sputtering by high-energy magnetospheric ions (blue line). ... Near-surface atmosphere of Europa: ionization chemistry in the H2O+H2+O2-dominant atmosphere ...

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• Nonequilibrium distributions
• PhSRM
• The summary plot of time distribution of the multisatellites magnetic

... Ciel Espace, le magazine qui vous guide toujours plus loin . ... des pages consacr?йes ?а la publication de vos photos Mais c'est aussi une vraie communaut?й avec laquelle partager votre passion et nourrir votre curiosit?й. Accueil Mati?иre noire : une observation d?йfie les astronomes . ... A la une . ... En effet, selon les mod?иles th?йoriques, les concentrations de mati?иre noire sont les lieux o?? naissent les galaxies. ... Une mati?иre noire au comportement ordinaire ? ... Etat du ciel . ...

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... 2014: . Suppression of cooling by strong magnetic fields in white dwarf stars . ... 69, 439, 2014. Evidence of supercritical accretion in SS433 . ... We discovered a flat portion (white noise) in the power spectrum of SS433 due to an abrupt increase of the disk thickness in the supercritical region. ... Both the hard X-ray radiation and the visual light are seen reflected from the walls of the funnel that forms in the wind of the supercritical disk of SS433. ... Archive . ...

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• Metagalaxy sector, archive 2006
• Physics of Magnetic Stars 2007
• Solar system scientific results 2003

Next: Power of test Up: Basic principles of Previous: Test statistics . In principle, it is possible to compute a value of the statistic for a single frequency and to test its consistency with a random signal ( ). ... The factor N means that there is an increased probability of accepting a given value of the statistic as consistent with a random signal. ... In the command individual descriptions, we often refer to probability distributions of specific statistics. ...

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• THE 4.85 GHZ NORTHERN SKY CATALOG
• "Structure" publications in 1996 year
• Sky and redshift distribution

... We have developed an integrated system that performs astronomical observations in Near Infrared bands operating two-dimensional instruments at the Italian National Infrared Facility's ARNICA and LONGSP . ... The user interface is organized as widget-based X11 client. ... 1993; Di Giacomo et al. 1993). ... Moreover, if the interprocess communication interface includes support for networking, the software immediately becomes network distributed software. ... DESQview/X User Guide 1993, Quarterdeck . ...

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• Modelling Spectro-photometric Characteristics of Eclipsing Binaries
• A Distributed System for ``Phase II'' Proposal Preparation
• Synthetic Images of the Solar Corona from Octree Representation of 3-D Electron

Variations of total ozone content and lower ozone stratosphere temperature in Antarctic Region during winter-spring period A.V. Grytsai National Taras Shevchenko University of Kyiv Astronomy and Space Physics Department assen@univ.kiev.ua Data, used in the work work Total ozone: Total Ozone Mapping Spectrometer (TOMS) measurements during 1979 - 2005 and Ozone Monitoring Instrument (OMI) ones for 2006, for http://toms.gsfc.nasa.gov/ftpdata.html. ... A long-term TOC decrease is significant. ...

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• Research - Page 2
• Observations - Page 2
• Доклады 'Atmosphere researches. Challenge for Ukraine'

... The main field of my investigations is stellar spectrophotometry. As a result of scientific activity of our group spectrophotometric catalog was created including energy distribution data on 900 stars in the range 3200-7600AA and 250 stars in the range 6000-10800AA (Voloshina et al., Spectrophotometry of Bright Stars, ed. I.N.Glushneva, 1982, Moscow, Nauka, in Russian). ...

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. Language [RU/EN] Search: . Home . UP . Research . Projects . Services . Info . News . Events . Personal . Archive . Ionosphere and radiowave propagation: structure . The main page . Information . Publications: . 2011 - 2015 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2000 - 2004 . 1995 - 1999 . Participation in International symposiums and conferences: . 2013 - 2015 . 2011 - 2012 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2002 - 2004 . N.V. Pushkov . 09/04/2016 23:52 MSK . webmaster@izmiran.ru .

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• Publications for 1995-1999
• Distribution of the analyzed SEPs with different >100 MeV proton fluxes (J100)