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http://www.sao.ru/hq/ssl/IRAS04296/IRAS04296_9.html.
http://www.sao.ru/hq/ssl/IRAS04296/IRAS04296_9.html.
1. The peculiar post-AGB supergiant IRAS04296+3429: optical spectroscopy and its
... The optical spectrum of the infrared source IRAS04296+3429 (optical counterpart - G0Ia star, V=14.2) was obtained with the echelle spectrometer PFES at the prime focus of the 6m telescope. ... 1995, Szczerba et al. 1996), our detailed modelling of its spectral energy distribution suggested that this source also should show the 30 m band. ... Stars: abundances - Stars: atmospheres - Stars: AGB and post-AGB - Stars: individual: IRAS04296+3429 . ... Spectral energy distribution . ...
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Ссылки http://www.sao.ru/hq/ssl/IRAS04296/IRAS04296_9.html -- 7.7 Кб -- 01.10.2012
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2. Maximum limits
... The planning and reduction programs are distributed with array sizes set large enough to let most observers work without difficulty. However, you might need to reduce a very large data set, or to deal with a very large number of passbands (9 is the nominal limit). ... The main problem is holding the matrix of normal equations during the iterations; on the other hand, star catalogs can be made quite large without paying much of a price in terms of performance. ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node304.html -- 6.8 Кб -- 23.02.1996
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3. articles_lebedev_en
... Glagolevsky Yu.V., Kozlova K.I., Lebedev V.S. , Polosukhina N.S., . ... Lebedev V.S. Spot analysis of rigidly rotating Ap-stars . IzvSAO, 8:20(1976). Glagolevsky Yu.V., Kozlova K.I., Kumajgorodskaya R.N., Lebedev V.S. , Polosukhina N.S., Chunakova N.M. The results of spectrophotometric studies of magnetic and peculiar stars: 21 Per, Beta CBr, Gamma Boo and Gamma UMi . ... Lebedev V.S. , Lebedeva I.A. Simulation of photographic measurement process of stellar magnetic fields . ...
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Ссылки http://www.sao.ru/hq/dolly/index_lebedev/articles_lebedev_en.html -- 19.4 Кб -- 28.02.2014
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4. Informational system "Evolution of RG"
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. ...
5. http://www.sao.ru/drabek/CCDP/SITe/502datsh.pdf
... Corresponding gates in each row are connected in parallel at both edges of the array. ... Other gates. ... otherwise indicated, 45 kpixels/sec and standard voltages using a dual slope CDS circuit (8 µs integration time) Minimum Format Pixel Size Imaging Area Dark current (MPP), 20° C equivalent Readout noise Front Back Full Well signal Output gain CTE per pixel Typical 512 x 512 pixels 24 µm x 24 µm 12.3 mm x 12.3 mm 50 pa/cm2 5 electrons 7 electrons 350,000 electrons 1.5 µV/ electron 0 ...
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Ссылки http://www.sao.ru/drabek/CCDP/SITe/502datsh.pdf -- 643.8 Кб -- 11.11.1998
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