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1. SCINTILLATION PARAMETERS FOR 49 PULSARS
Scintillation parameters for 49 pulsars . S. Johnston (RCfTA, University of Sydney, Australia), . ... We report on multi-epoch, multi-frequency observations of 64 pulsars with high spectral and time resolution. Scintillation parameters were obtained for 49 pulsars, including 13 millisecond pulsars. ... There is a significant correlation between the scintillation speeds and the product of the pulsar's period and period derivative for the `normal' pulsars. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Simon.Johnston/papers/viss3.html -- 2.7 Кб -- 02.10.2012
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2. The main observational parameters
... Column 1 gives the object name from the Case or Markarian catalogs. ... For Markarian galaxies the errors of coordinates usually lie inside 2'' (Lipovetsky [ 1983 ]). Column 4 gives the eye-estimated apparent blue magnitudes according to the same sources. ... Other names of a galaxy we give in column 7. ... In column 3 we cite the original emission-line code of the galaxy for the strength of [O III ] doublet according to the Case catalog (s - strong, m - medium, w - weak). ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Laboratory/Publications/1997/CasePR/node7.html -- 10.4 Кб -- 10.01.1998
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3. HST Image Restoration with Variable Resolution
... Bayesian and maximum entropy algorithms that use a constant balancing parameter present large residuals in the low or the high S/N regions depending on the value chosen for the parameter. ... This variation of the balancing parameter implies a variable resolution in the restoration, allowing high resolution with low bias in high S/N regions and a lower resolution with lower artifacts in poor S/N regions. We have applied the algorithm to the FOC and WF/PC cameras of the HST. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/nunezj.dir/nunezj.html -- 3.6 Кб -- 18.04.1994
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4. TwoFitlines: An Spectrum and Line Analysis Tool
Next: A New IRAF Catalog Access Tool for Astrometry . Up: Iraf Packages . ... Twofitlines is a tool developed within IRAF, optimized to be used with data containing multiple spectra along the spatial axis of the detector. A given spectral feature can be decomposed in one or several Gaussian components. ... A given spectral feature can be modeled using one or more components (currently only Gaussian profiles are available), . ... Close spectral features could be modeled simultaneously. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/P2-36/ -- 12.0 Кб -- 12.10.2000
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5. Database "Stellar Spectra"
... Panchuk V.E. Database "Stellar Spectra" consists of following main units: . ... obtained with various modifications of high resolution echelle-spectrometers at the 6-m telescope. ... Using the spectra obtained at BTA in combination with high resolution echelle-spectrometers LYNX and PFES , Chentsov E.L., Klochkova V.G. and Panchuk V.E. prepare now the next spectral atlas. ... The CATALOGUE of spectral photoplates obtained at the Main Stellar Spectrograph of the 6m telescope. ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/ssl/db.html -- 6.9 Кб -- 01.10.2012
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/ssl/db.html -- 6.9 Кб -- 01.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/ssl/db.html -- 6.9 Кб -- 01.10.2012
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6. Parameters
... Meta Index / Home Page This section documents the parameters recognized by this task (if any). ... boxhalfsize . yes . ... This should match the value of -boxsize supplied to eboxdetect . ... The cal calculates the truncation point so that the included part of the PSF contains approximately the fraction of total flux specified by the present parameter. ... If psfestyle =`dss', the task looks for the mean energy value in the data subspace of the image set supplied to the present parameter. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/econvolverprep/node4.html -- 10.0 Кб -- 02.07.2008
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7. http://star.arm.ac.uk/~csj/papers/abstracts/sdbb.abstract
Physical parameters for subdwarf B stars with composite spectra R. Aznar Cuadrado, C.S. Jeffery, Armagh Observatory, College Hill, Armagh BT61 9DG New intermediate-resolution spectra have been obtained for a number of subdwarf B stars having both single and composite spectra. Physical parameters have been determined for the sdB stars and, in composite-spectrum systems, their cool companions. ... The surface gravity of the cool star is measured using the infrared calcium triplet. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/papers/abstracts/sdbb.abstract -- 2.0 Кб -- 01.07.2002
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8. AZ Key parameters, 1997
. Intervals of available data are coded by blue color. To read availability charts user should know the descriptor ("name") of the KP subset of interest. Table annotations include also number of version for each subset. Plot resolution is exactly one pixel per hour. Data are considered as available if at least one data point is present during that hour.
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/ibelova/az_cat7.htm -- 3.0 Кб -- 12.05.1999
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9. AGES Database Search
... All the parameters provided in this database have been obtained using the the MIRIAD ( Sault et al. 1995 ) task MBSPECT . MBSPECT makes a spectrum of the velocity (or frequency) axis of a cube. The spectrum is beam-weighted, over the width specified, for the other image axes. ... Robust parameters are calculated by using an algorithm which minimises the mean absolute deviation of the flux-weighted velocities. mask= This specifies the x-axis ranges to be excluded from any continuum fit. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~ages/public/glossary.shtml -- 10.0 Кб -- 10.04.2016
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10. http://www.mrao.cam.ac.uk/~anthony/latex/Richards.ps
Maxima Paul L. Richards et al. U.C. Berkeley, USA The MAXIMA team has recently released measurements of the cosmic microwave background temperature anisotropy from the rst ight (MAXIMA-1). These results include a 10 square degree map of  122 square degrees of the surface of last scattering with 10 arcmin resolution, a power spectrum over the range 36 < l < 785, and a bayesian analysis of the constraints on cosmological parameters obtained from this power spectrum. ...
[ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~anthony/latex/Richards.ps -- 21.3 Кб -- 24.06.2000
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11. http://www.gao.spb.ru/english/as/j2014/presentations/filippova.pdf
... G., Filippova A.S. Presented by: Filippova A.S Achievements · Refined model based on the celestial-mechanics methods is presented that is a generalized version of the previously developed basic model · Subtle effects are qualitatively explained based on the amplitude-frequency analysis and the computer numerical modelling of the oscillatory pole motion, where the key feature is the Chandler wobble 2 Basic Model of the Polar Oscillations ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/as/j2014/presentations/filippova.pdf -- 1324.2 Кб -- 28.09.2014
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12. http://www.iki.rssi.ru/eng/2013niokr.pdf
... Contacts: Evgeny A. Loupian, Dr. Sci., e-mail: evgeny@smis.iki.rssi.ru Sergey A. Bartalev, Dr. Sci., e-mail: bartalev@smis.iki.rssi.ru Web interface for burnt area mapping using Landsat data Stellar Tracker In 2013 IKI RAN together with the NPK "Electrooptics" completed the phase of the five-year research on studying the ways to build a stellar inertial navigation system (SINS) for aviation applications. ... Fig. 1 shows the SINS layout created on the basis of the astronomical camera. ... Fig.1. ...
[ Текст ]  Ссылки http://www.iki.rssi.ru/eng/2013niokr.pdf -- 651.3 Кб -- 12.02.2014
[ Текст ]  Ссылки http://www.cosmos.ru/eng/2013niokr.pdf -- 651.3 Кб -- 12.02.2014
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13. Derived parameters
. Next: Absolute magnitudes Up: Command line procedures Previous: Limb darkening Contents . Subsections . Absolute magnitudes . Distances . Diameters . Orbital inclinations, semi-major axes, and secondary masses . Christian Hummel 2015-04-28
[ Сохраненная копия ]  Ссылки http://www.eso.org/~chummel/oyster/manual/node119.html -- 3.4 Кб -- 28.04.2015
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14. MILLIMETRON
... The project assumes creation of an international space observatory - the interferometer "Earth - Space - Space" in order to perform of astronomical investigations in millimeter, submillimeter and infrared regions with extremely high sensitivity (to a few nanoJanskies units of flux density in continuum spectrum) and extremely high angular resolution (to a parts of microsecond of arc or, possibly, nanosecond). ... radio-interferometric channels of the system "Space - Space", region 0.2 - 3 mm; . ...
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/submillimetron/mm/default.htm -- 10.5 Кб -- 05.04.1999
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15. Linear polarization: wavelength dependence
... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/DOP/8-GLIB/ASTNOTES/node7.html -- 18.9 Кб -- 19.11.2010
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16. Keywords_54
The IAA RAS fundamental ephemerides of planets and the Moon (EPM): their model, parameters, accuracy . ... In the seventies of the last century, Ephemerides of Planets and the Moon (EPM) of IAA RAS was originated and have been developed since that time. The current state of the last updated version of EPM s ephemerides (EPM2010) integrated in the PPN metric over the 1800тИЪ2200 time interval is presented. ... ephemerides, major planet, the Moon numerical integration. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/EDITION/transaction/transaction_ann26/54.htm -- 4.3 Кб -- 09.04.2016
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17. http://selena.sai.msu.ru/Shev/Publications/ms38/ms085.pdf
Microsymposium 38, MS085, 2003 (A4 format) REMOTE DETERMINATION OF LUNAR SOIL MATURITY. ... Shevchenko et al. [6, 7], and Pinet et al. [8] developed the method to determine the maturity of lunar soil by using spectropolarimetric ratio Pmax(B)/Pmax(R) for blue (B) and red (R) spectral regions. On the basis of known laboratory results and telescopic data, it was found that ratio Pmax(419nm)/Pmax(641nm) could be used as a remote sensing parameter of lunar soil maturity. ...
[ Текст ]  Ссылки http://selena.sai.msu.ru/Shev/Publications/ms38/ms085.pdf -- 280.5 Кб -- 06.10.2008
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18. http://www.ssau.ru/files/science/conferences/itnt2015/itnt_2015_70.pdf
TOOLS OF TEST GENERATION FOR SATELLITES CONTROL PROGRAMS Andrey Tyugashev, Ekaterina Myasnikova, Elena Sopchenko S.P. Korolyov Samara State Aerospace University (National Reseach University) The paper presents a research in the field of test automation for testing spacecraft control programs. ... Programmers or designers of spacecraft systems write tests manually. ... Tests are carried out by issuing the control actions on the spacecraft and condition monitoring systems parameters of the spacecraft. ...
[ Текст ]  Ссылки http://www.ssau.ru/files/science/conferences/itnt2015/itnt_2015_70.pdf -- 161.6 Кб -- 04.08.2015
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19. East Siberian Center for the Earth's Ionosphere Research. Ionospheric parameter
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Here we present the ionospheric parameters variations for quiet conditions. ...
[ Сохраненная копия ]  Ссылки http://rp.iszf.irk.ru/esceir/isr/vozmnren.htm -- 3.4 Кб -- 04.06.2001
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20. Notation
... The operators will be explained as they are used. The general notion to keep in mind is that any combination of these operators results in a 2- D affine coordinate transformation in the TF plane, which may be represented using the homogeneous coordinates often used in computer graphicsfoley. ... S _t_c,f_c = g_t_c,f_c,(_t) | ... We denote a time shift to the position , with an operator that has a multiplicative law of composition : (Table 1). ... Note that these two operators do not commute. ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/~vab/Wavelet.rsc/Chirplet.dir/node7.html -- 9.2 Кб -- 15.04.1998
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