... In the spectrometry of point sources, the advantage of obtaining long slit spectra over using single aperture spectra is that it provides a simultaneous spectrum of the background on both sides of the point source. ... The STECF IRAF layered package "specres" provides two tasks to extract point source spectra from 2-D images (either longslit, multislit or cross-dispersed) and decompose the full background over the image. ... A Point Source Function spectrum image is required as a 2-D spectrum. ...

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... A new technological vision on the future of the VLBI backend area let envision a fully digital implementation of what was until now performed in the analog domain. ... Very Long Baseline Interferometry (VLBI), radio astronomy, VLBI backend systems, VLBI backend area, domains transition point, radio observatories digital technology, data handling process, signal path, RFI and calibration effects, DSP algorithms, sensitivity of the observatories, global applications. ...

The XV_VTDF is a viewer for TDF format files (extension to TIFF 6.0 format for storage of high-resolution satellite data). More information about TDF format and relevant topics, as well as satellite data in this format you may receive from Space Monitoring Information Support lab (Space Research Institute, Moscow, Russia) . ... XV_VTDF <filename> - load TDF file at startup (default size) . ... The XV_VTDF operates with fixed-size satellite images in TDF format. ... Back to SMIS Home Page . ...

Russian Version ( KOI-8 , Win ) . Institute of Astronomy of the RAS . ... Self-consistent simulation of chemical and dynamical evolution of protostellar clouds . Chemical evolution of galaxies . ... Soon after my birth I was moved (I was not able to move on my own in those times, you know) in Novouljanovsk, small town to the south of Uljanovsk. ... Since that time my life and work is bound to the Institute of Astronomy of the Russian Academy of Sciences. ... Back to the INASAN home page . ...

... title='Кольцо с бриллиантами из белого золота - Камея - Камея' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> . Размер (Ш*В*Г): 102*123*51 Эта великолепная серия многофункциональных винтажных сундуков задумана дизайнерами как реплика в сторону колониальных интерьеров 18-19-х веков. ... Сундуки и коробки . ... Цвет: серебристый . ... Золото комбинированное 585. Цвет: белый . ... Размер INT: 50 . ... Комплект из 2 белых трусиков. ... Цвет: Белый . ...

Institute of Nuclear Physics Russian Akademy of Sciences BAKSAN (KABARDINO-BALKARIYA,tower ELBRUS), RUSSIA BAKSAN ( BKSN ), 6 NM64 NEUTRON MONITOR (REMOVED FROM NLC2) CORRECTED FOR PRESSURE Altitude 1700 M Mean= 4708.4 May 2007 Geographic Coordinates ... (1965)= 5.6 GV; SF= 100 Pressure Coefficient= -0.73 %/mb Corrected to 820 mb Standard Pressure Comment: 1.000 4706 4704 4696 4682 4699 4705 4711 4727 4714 4705 4707 4733 4705 4722 4727 4721 4702 4703 4707 4703 4703 4693 4684 ...

... The mount is also adjustable so you can orient the axis of rotation to make it parallel with the Earth's axis of rotation (see the section on Polar Alignment). ... Locate the opening in the equatorial mount on the DEC axis. ... To mount the telescope tube: 1. ... ADJUSTING THE MOUNT FOR POLAR ALIGNMENT In order for the clock drive to track accurately, the telescope's axis of rotation must be parallel to the Earth's axis of rotation, a process known as polar alignment. ... R.A. & DEC axis ! ...

Winer Observatory P.O. Box 797, Sonoita, Arizona 85637-0797, USA . ... The building is about 106 ft. long by 26 ft. wide and is divided into two parts: a shop area to the north, 54 ft. long by 26 ft. wide with parapet walls containing the control room, and the observatory area 52 ft. long by 26 ft. wide. ... Shop Wall Counterforts . ... The shop roof is suspended between parapet walls, that is, the walls are higher than the roof, to permit the observatory roof to roll unimpeded over the shop roof. ...