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http://www.stsci.edu/~marel/abstracts/abs_R15.html.
http://www.stsci.edu/~marel/abstracts/abs_R15.html.
1. Sample Properties
Next: Redshift Distribution Up: Sample Identification Previous: Previously Identified Sources . ... In Figure 3, we plot the redshift distribution of DXRBS FSRQs opposite that of the 1 Jy and S4 samples. In Figure 4, we plot the redshift distribution of DXRBS BL Lacs opposite the Slew and 1 Jy samples. ... The apparent deficit of objects at the very highest luminosities is a result of the smaller area of sky covered by DXRBS compared to, e.g., the Slew and 1 Jy samples. ...
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Ссылки http://www.eso.org/~ppadovan/survey/dxrbs_paper/node11.html -- 5.2 Кб -- 03.12.2003
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2. Herschel Images and Results for the Magellanic Clouds
The dust properties in the Large and Small Magellanic clouds (LMC/SMC) are studied using the HERITAGE Herschel Key Project photometric data in five bands from 100 to 500 m. Three simple models of dust emission were fit to the observations: a single temperature blackbody modified by a power-law emissivity (SMBB), a single temperature blackbody modified by a broken power-law emissivity (BEMBB), and two blackbodies with different temperatures, both modified by the same power-law emissivity (TTMBB). ...
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Ссылки http://www.stsci.edu/~kgordon/magclouds_results/magclouds_results.html -- 11.7 Кб -- 26.03.2015
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3. Project 6 - RFBR - Multilayer epitaxial heterostructures of high-temperature
... Peter B. Mozhaev , Ph.D. Complicated crystal structure and anisotropy of physical properties of the high critical temperature superconductors (HTSC) makes difficult reproducible fabrication of the multilayered epitaxial heterostructures of HTSC with necessary parameters. ... The goal of this project is study of growth and formation of the multilayer epitaxial heterostructures of HTSC of the ReBa 2 Cu 3 O x family (ReBCO, where Re is the rare earth element). ...
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Ссылки http://www.cplire.ru/html/oxide233/proj6.html -- 4.6 Кб -- 01.09.2005
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4. The very metal-poor local dwarf galaxies
The very metal-poor local dwarf galaxies - the analogs of primordial galaxies in young Universe . ... The goal of this project is the study of the properties of the local eXtremely Metal-Deficient (XMD) dwarf galaxies. ... S.A. Pustilnik, J.-M. Martin . ... Pustilnik S.A. "Dark galaxies" and local very metal-poor gas-rich galaxies: possible interrelations, in: Dark Galaxies and Lost Baryons, Edited by J.Davies and M.Disney, Proceedings of IAU Symposium No. 244, held 25-30 June, 2007 in Cardiff, UK. ...
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Ссылки http://www.sao.ru/precise/Laboratory/Current/MPDG_eng.html -- 8.6 Кб -- 18.02.2008
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5. Database of Optical Properties -- Level: subpage
Here we compare the optical properties of porous particles of two kinds: . ... Below we show the behaviour of the efficiency factors Q ext (x), Q sca (x), Q abs (x), the asymmetry parameter g (x) and albedo (x) as well as for x = 3 and 100 the phase function i (theta) and polarization of scattered radiation p (theta) for different values of the parameters m and P . ... factors . ... Qext(x) . Qsca(x) . ... i (theta) . ... albedo (x) . ...
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Ссылки http://www.astro.spbu.ru/DOP/8-GLIB/op/ -- 25.2 Кб -- 19.11.2010
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6. Initial Distributions of Binary Parameters
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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Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node39.html -- 14.1 Кб -- 26.02.1997
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7. The HIPASS Bright Galaxy Catalog
Old subtables of the extended ``HIPASS Bright Galaxy Catalog'' . ... Koribalski, Staveley-Smith, Kilborn, + HIPASS/ZOA teams 2004, AJ 128, 16 . The 1000 Brightest HIPASS Galaxies: HI Properties . ... The 1000 Brightest HIPASS Galaxies: The HI Mass Function . ... The 1000 Brightest HIPASS Galaxies: Newly Cataloged Galaxies . ... To download the gzipped ps-file click here . ... The Brightest Galaxies from HIPASS . Presented is the distribution of the 700 brightest HIPASS galaxies. ...
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Ссылки http://www.atnf.csiro.au/research/multibeam/HIPASS-BGC/tables/ -- 6.4 Кб -- 23.12.2007
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8. Space Scientific and Education project of Lomonosov Moscow State University
The main task of the multimedia lectures "Life of the Earth in the Solar Atmosphere" is to introduce wide range of users to the basic physical characteristics of the Earth, the near-Earth space and the Sun, which mainly forms the properties of the mentioned objects and is responsible for their variations (so-called "space weather"). ... Middle atmosphere of the Earth. ... Radiowaves' passing and spreading in the Earth atmosphere. ... Space radiation passing through the Earth atmosphere. ...
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Ссылки http://cosmos.msu.ru/eng/sunearth.html -- 6.0 Кб -- 05.12.2005
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9. Spectral energy distribution
... 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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Ссылки http://mavr.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
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10. Zen: sncat design
Hide Zen home . ... sncat2sntab.pl - convert old catalog to table sn . ... CREATE TABLE cats ( id integer PRIMARY KEY, name text ); -- a list of properties of galaxy CREATE TABLE properties ( id integer PRIMARY KEY, name text ); CREATE TABLE galaxy ( id integer PRIMARY KEY, name text ); CREATE TABLE galaxy _property ( gid integer REFERENCES galaxy (id), pid integer REFERENCES properties(id), value float, UNIQUE( gid ,pid) ); CREATE t=# select * from galaxy; id | ...
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Ссылки http://www.sai.msu.su/~megera/wiki/sncat_design -- 15.1 Кб -- 10.04.2016
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11. http://www.gao.spb.ru/english/as/j2014/presentations/kudryashova.pdf
... St Petersburg 23, September 2014 1 Motivation · Origin of Martian moons? ... Considered error sources: Phobos a priori ephemerides; Phobos a priori GM value; measurements noise; different strategies; · Methods: real data analysis; simulations. ... St Petersburg 23, September 2014 8 Simulations: sensitivity of the measurements to the a priori GM value Simulations: zero noise+ IMCCE a priori ephemerides +GMPH = 7.16 * 105 m3/sec2. ... St Petersburg 23, September 2014 14 Thank you! ...
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Ссылки http://www.gao.spb.ru/english/as/j2014/presentations/kudryashova.pdf -- 482.3 Кб -- 28.09.2014
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12. Clumpy dust disks
... Abstract: We present Monte Carlo radiative transfer simulations for spiral galaxies modelled as a stellar disk and a two-phase clumpy dust distribution. ... As a general result, clumpy models are less opaque than the corresponding homogeneous models. ... 0.00 0.15 0.50 0.1 0.5 1.0 2.0 5.0 10.0 0.25 X . ... We have also produced several homogeneous models, to compare to the clumpy models. ... Homogeneous and clumpy models with the same tauV have the same dust mass. ...
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Ссылки http://www.arcetri.astro.it/~sbianchi/clumping.html -- 14.5 Кб -- 29.03.2002
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13. http://xmm.vilspa.esa.es/sas/8.0.0/doc/rgsrmfgen/ChangeLog
... Version 1.8 - 2006-02-22 (AI) ----------- + config/rgsrmfgen.par keyword typo fixed. ... Version 1.6 - 2005-09-13 (CG) ----------- + energy/wavelength conversion accuracy fixed - SPR 2549 Version 1.5.3 - 2004-03-15 (CG) ------------- + parameter name update in docu (ebins rows) Version 1.5.2 - 2004-02-06 (CG) ------------- + bogus with executable permission Version 1.5.1 - 2004-02-05 (CG) ------------- + bug introduced in 1.5 (calib.cc - small angle scattering) fixed ...
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Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/rgsrmfgen/ChangeLog -- 11.1 Кб -- 23.05.2008
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14. http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf
THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE BY MEANS OF DIGITAL MODELS. ... The surface brightness of Mercury was measured Danjon (1933, 1949, 1953) and Harris (1961) in phase angle 3o-123o. The analysis of the various data of the integral photometric gives the results of determination of the main photometric constants for Mercury. ... THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE: S.G. Pugacheva The surface brightness of the Mercurian images was established on the geologic map Mercury. ...
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Ссылки http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf -- 205.0 Кб -- 25.02.2009
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15. Project: PAHs
... Spectra obtained with the 6-m telescope of SAO RAS are used along with archival data from Spitzer and several ground-based telescopes to infer a strength of PAH emission, age, properties of the UV radiation field, and metallicity of studied HII complexes. Physical properties (age, radiation field parameters, metallicity) are related to the F 8 /F 24 ratio used as a proxy for the PAH abundance in order to reveal factors that may influence the PAH evolution in HII complexes. ... Projects | ...
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Ссылки http://www.inasan.rssi.ru/~khramtsova/project_PAH2.html -- 6.2 Кб -- 23.02.2015
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16. Statistics 310 2007-2008
... Alanna Connors (Eureka Sci), Pavlos Protopapas (IIC/CfA) . 18 Sep 2007 . ... Abstract: . ... Group . ... Spinning Stellar Black Holes . ... Our group has been pioneering the use of X-ray continuum fitting to measure black hole spins, and has published results on four black hole X-ray binary systems. ... 05 Feb 2008 . ... Lee, H. / Connors, A. / Protopapas, P. / McDowell, J., / Izem, R. / Blondin, S. / Lee, H. / Zezas, A., & Lee, H. / Liu, J.C. / van Dyk, D. / Rice, J. Fall/Winter 2007-2008 . ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_0708/ -- 10.1 Кб -- 01.10.2012
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17. Introduction to Plasma Physics
Plasma models and main parameters. ... Magnetic diffusion. ... Double- adiabatic invariants for a plasma in strong magnetic field. One- fluid MHD. ... Frozen-in properties of magnetic field in plasma. ... Force- free magnetic field configurations. ... Dispersion of plasma waves in linear theory. ... Waves in non- magnetic plasma. ... Electromagnetic waves in plasma. ... Dispersion relation for waves in cold magnetized plasma. ... High- frequency electromagnetic waves in cold magnetized plasma. ...
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Ссылки http://space.univ.kiev.ua/courses/intr_plasm.html -- 3.5 Кб -- 23.02.2005
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18. Elena_projects
... Projects . Current projects . Semiconductor materials, nanopowder technologies, microstructure, texture, recrystallization, physical properties of compacted CdTe, CdZnTe (with N.N. Kolesnikov, D.N. Borisenko, A.V. Timonina, B.A. Gnesin) . ... Recent projects . ... grant of Russian Foundation for Basic Researches) . ... grant of Russian Foundation for Basic Researches) (project by M.A. Lebedkin) . ... grant of Russian Foundation for Basic Researches) (project by B.A. Gnesin) . ...
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Ссылки http://www.issp.ac.ru/lpcbc/Elena_projects.html -- 5.1 Кб -- 25.01.2011
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19. http://www.mso.anu.edu.au/seminars/abstracts/20150612-1400.html
The Hubble constant is one of the most important parameters in the cosmological model, setting both the size and age of the Universe. ... The Mega-SH0ES project aims exactly this bye measuring the Hubble constant with percent-level uncertainty. I will give an overview of the Mega-SH0ES project and the techniques it is using, including the Parallel Astrometric Spatial Scanning (PASS) on WFC3, Infrared Cepheids, and 17 New Type Ia Supernova host galaxies. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150612-1400.html -- 4.3 Кб -- 10.04.2016
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20. Using Massively Parallel Processing of a NLTE Spectrum Synthetic Code and an
... The nebular spectra of SNeIa can be used to determine the mass, density, and distribution of the SN ejecta, and the distance and reddening to the SN. Synthetic spectra can very rapidly be computed in NLTE and compared to the observed ones. Given the relatively large number of parameters, it is convenient to explore the parameter space in an automated form. The nebular spectrum synthesis code can be run in parallel on a workstation cluster. ...
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Ссылки http://www.adass.org/adass/proceedings/adass96/smaregliar.html -- 13.8 Кб -- 23.06.1998
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