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http://www.sao.ru/cats/cgi-bin/vsop.cgi.

1. Radio spectra of 3CR sources with CATS identificatios
The spectra of the 299 3CR-sources are based on ~40000 flux points, selected from the catalogs in CATS database. In order to plot 'on-line' radio spectrum of a source from the 3CR catalog . you need use the below 'Search'-window for the fitting parameters . Input from the first position in the window: . ... For example, type in the window: . 405.0 1 -e 10 40000 "Enter" . ... 405.0 "Enter" . ... Output (replacing) gif-files: 3CRnnn.n.gif The list of the 3CRnnn.n radio sources. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/cgi-bin/3c.cgi -- 4.5 Кб -- 01.10.2012
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2. Radio sources identfification
... LABORATORY OF RADIO ASTRONOMICAL OBSERVATIONS . Radio sources identification is one of the most important tasks of the current radio astrophysics. ... Optical idetification. ... Optical identifications of subsample of steep spectra radio sources from RC catalog using 6m SAO telescope of SAO RAS: optical observations. ... Astronomy Reports. ... Identification of radio sources with data of various radio catalogs allows one to construct continual spectrum of the object and its radio structure. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/lran/vo/rs_idE.html -- 8.9 Кб -- 01.10.2012
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3. Study of radio spectra and variability of GPS sources
... The results of long-term monitoring of Gigahertz-Peaked Spectrum sources were found the statistically significant differences (0.05 significance level) in the high-frequency spectral index distribution between subgroups of galaxies and quasars. ... This can mean that the electron energy distribution for GPS galaxies is steeper than for GPS quasars. ... The first area corresponds to GPS-quasars that have statistically larger value of redfhift, second area corresponds to GPS-galaxies. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2011/Mingaliev/ -- 4.9 Кб -- 02.10.2012
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4. 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 ...
[ Текст ]  Ссылки http://www.sao.ru/drabek/CCDP/SITe/502datsh.pdf -- 643.8 Кб -- 11.11.1998
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