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http://www.sao.ru/hq/CG/cold/part3.htm.
http://www.sao.ru/hq/CG/cold/part3.htm.
1. Experimetn COLD: Introduction
Experiment COLD . ... JSEC Astronomy . ... The entire project was called "Experiment Cold". ... The best radiometer (in terms of fluctuation sensitivity) known to us, based on a parametric amplifier with a closed-cycle helium cooling system, was used in the experiment; measures were taken to "cool" the radio telescope itself; and a method of controlling the numerous sources of interference was carefully thought out. ...
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Ссылки http://www.sao.ru/hq/CG/cold/introduc.htm -- 5.0 Кб -- 24.02.2010
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2. Introduction
Next: What is needed Up: PEPSYS general photometry Previous: PEPSYS general photometry . ... If there are no calibration observations of standard and extinction stars, the program-star observations cannot be transformed to a standard system. At the opposite extreme, if there are only observations of standard and extinction stars, there is no time for program-star observations. ... A good distribution of standards in each color index is also needed to determine accurate transformations. ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node261.html -- 3.9 Кб -- 23.02.1996
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3. Galaxy sector, archive 2014
... 2014: . Suppression of cooling by strong magnetic fields in white dwarf stars . ... 69, 439, 2014. Evidence of supercritical accretion in SS433 . ... We discovered a flat portion (white noise) in the power spectrum of SS433 due to an abrupt increase of the disk thickness in the supercritical region. ... Both the hard X-ray radiation and the visual light are seen reflected from the walls of the funnel that forms in the wind of the supercritical disk of SS433. ... Archive . ...
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Ссылки http://www.sao.ru/Doc-en/Science/results/ar_galaxy/res2014.html -- 9.4 Кб -- 10.04.2016
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4. Group for study of galaxies and cosmology, history
... In LABORATORY OF RADIO ASTROPHYSICS OF SPECIAL ASTROPHYSICAL OBSERVATORY OF RAS . ... History . ... Current problems of the group research interests: . study for cosmic microwave background, . study of radio galaxies (identification, evolution, statistical investigation of population), . investigation of the RATAN-600 antenna, . observations in the survey mode with RATAN-600 and their analysis, . creation of the software for data analysis. vo @ sao.ru ( Oleg Verkhodanov ) ...
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Ссылки http://www.sao.ru/hq/lran/vo/group/gr_resea_E.html -- 2.5 Кб -- 02.10.2012
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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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