Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...

... Structure of Data . ... Catalog . ... The SAI OCL Catalog site provides several VO-enabled modes of operation: . VO-enabled catalog data analysis from a browser . ... Endpoint URL is http://ocl.sai.msu.ru/catalog/conesearch/ . ... VO-enabled catalog analysis from a browser . Presently, this recipe works with Firefox (Windows, MacOS, Linux), Internet Explorer (Windows) and Opera (Windows) browsers with Java plugin 1.6 installed. ... Main TOPCAT window with SAI OCL catalog loaded will appear. ...

Optional Cultural Program. Though there several cultural activities in the Basic Workshop Program we are glad to offer you a series of guided cultural excursions designed to offer participants a flexible choice of what they see in the Moscow area. Since many of our participants have been to Moscow before, we offer excursions both to the major tourist sites such as Red Square and Kremlin and also more "off-the beaten-track" tours for those who may have already seen the more popular sites. ...

Download Izmccd (~2.7 MB). ... a) a choice of the best mode of measurements of stars and objects ("Properties/Measurement"), . b) a choice of reference stars. ... 1) necessity of presence on an image of a plenty of stars (we recommend to apply this mode, if on the frame of reference stars is more 100) . ... Sx and Sy depend from residuals at all reference stars (reference stars are marked by blue color). ... These residuals are the image of the star a minus function of a profile for each pixel. ...

... Телескопы . ... Настраивает полярную ось согласно статье Полярная настройка монтировки телескопа с помощью искателя полюса , для визуальных наблюдений достаточно просто увидеть Полярную звезду в искатель. ... Нажимаем ENTER . ... Нам нужно настроить телескоп минимум по трем звездам. ... После установки звезды в перекрестия искателя нажимаем ENTER и нам предлагают подвести звезду в центр поля зрения телескопа. ... Калибровке по трем опорным звездам достаточна для наблюдений и мы нажимаем кнопку UNDO ...

... Next Routine] [List of Routines] NAME: ADD_HEADER PURPOSE: addition information from FITS-headers MPFS-frames DESCRIPTION: The function computes the total exposure, mean value zenit distance and modified FITS header CALLING SEQUENCE: Result =ADD_HEADER( headers ) CATEGORY: reduction MPFS-data INPUTS: Headers = String array FITS-headers from the MPFS data OUTPUTS: Header = String array containing the header from the FITS file. ... OPTIONAL INPUT KEYWORD PARAMETERS: BEFORE = Keyword string name. ...

<OBJECT RUNAT=Server SCOPE=Session ID=MyInfo PROGID="MSWC.MyInfo"> </OBJECT>

... ОБ ОТДЕЛЕ . ... Лукаш В.Н., Михеева Е.В. 'Физическая космология' М: Физматлит, 2010. ... Doroshkevich A., Verkhodanov O. 'CMB component separation in the pixel domain', Phys. Rev. D, vol. 83, id 043002, 2011 г. 4. ... Demianski M., Doroshkevich A.G., Pilipenko S.V., Gottloeber S. 'Simulated evolution of the dark matter large scale structure', MNRAS, 414, 1813-1826, 2011 г. 8. ... Комберг Б.В., Ермаш А.А., 'Морфология и эволюционный статус активных галактик типа NLSyI', Препринт ФИАН ?31, 2011 г. 14....

... 000, 1­13 (2010) Printed 21 September 2011 A (MN L TEX style file v2.2) A universal ultraviolet-optical colour­colour­magnitude relation of galaxies I1gor V. Chilingarian1,2, and Ivan Yu. ... Received 2011 Sep 15; in original form 2011 Feb 6 ABSTRACT The bimodal galaxy distribution in the optical colour­magnitude diagram (CMD) comprises a narrow "red sequence" populated mostly by early-type galaxies and a broad "blue cloud" dominated by star-forming systems. ...

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...