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http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p470.pdf.
http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p470.pdf.
1. http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p470.pdf
Magnetic Stars, 2011, pp. ... It follows, in particular, from Fig. 1a, where points show the central intensity of line in 2008 2009, and asterisks -- the ELODIE Archive (EA) spectra in 2002 2003 smoothed to the resolution of the MSS. ... Figure 2a demonstrates the distribution of temperature in the atmosphere in the phase = 0.07 and Fig. 2b -- in the phase = 0.53 of the rotation period, obtained from the hydrogen line profiles in 2008 2009. ...
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Ссылки http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p470.pdf -- 101.4 Кб -- 11.08.2011
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2. http://www.sao.ru/hq/lizm/conferences/pdf/2003/2003_p247.pdf
Magnetic stars, 2004, 247-249 Study of magnetic fields of different luminosity hot stars Butkovskaya V., Plachinda S. Crimean Astrophysical Observatory, Nauchny, Crimea, 98409, Ukraine Abstract. Circular sp ectrop olarimetric observations of four different luminosity hot stars were obtained in an attempt to detect magnetic fields via longitudinal ° Zeeman effect in the sp ectral line HeI 6678.149 A: Pegasi (Sp B2 IV), Orionis (Sp B2 I I I), Orionis (Sp B3 I I Ie), Persei (Sp B1 Ib). ...
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Ссылки http://www.sao.ru/hq/lizm/conferences/pdf/2003/2003_p247.pdf -- 116.8 Кб -- 21.04.2010
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3. List of Figures
Next: List of Tables Up: No Title Previous: Contents . A dark current CCD exposure with cosmic ray events which are removed with non--linear filters. A) original, (B) 5*5 median filter, (C) 5*1 median filter, and (D) 5*1 recursive filter. Removal of cosmic ray events on a CCD spectral exposure with different techniques: (A) original, (B) median filter, (C) recursive filter and (D) stack comparison. ... Images RINGS and OFFRINGS. ... This image is obtained by the command visual/cube . ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node2.html -- 10.0 Кб -- 23.02.1996
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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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