... VLBI Schedule . ... DAS #1 IFP#1-LO 8200 - 8216 MHz USB RCP . ... DAS #1 IFP#1-HI 8216 - 8232 MHz USB RCP . ... DAS #1 IFP#2-LO 8200 - 8216 MHz USB LCP . ... DAS #1 IFP#2-HI 8216 - 8232 MHz USB LCP . ... DAS #2 IFP#1-LO 8456 - 8472 MHz USB RCP . ... DAS #2 IFP#1-HI 8472 - 8488 MHz USB RCP . ... DAS #2 IFP#2-LO 8456 - 8472 MHz USB LCP . ... DAS #2 IFP#2-HI 8472 - 8488 MHz USB LCP . ... IFP#1-LO 8200 - 8216 MHz USB RCP . ... IFP#1-HI 8216 - 8232 MHz USB RCP . ... IFP#2-LO 8456 - 8472 MHz USB RCP . ...

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. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

. INSTITUTO ISAAC NEWTON . Casilla 8-9, Correo 9, Santiago, Chile . e-Mail: inewton@terra.cl . Contact address in St.Petersburg: resh@astro.spbu.ru . Money Order since Feb 2001

Main Sections LabIR main page . Instrument page . ... Special Sections Software Page . ... LabIR staff . Companion Pages Skysoft Home . Tirgo Page . ... LabIR Hotlist . ... Arcetri Infrared Instrumentation Group . Largo E.Fermi 5 I-50125 Firenze . Phone (Italy) 055 2752 289 . Fax (Italy) 055 2752 292 . ... Firenze, August 1997 ...

About us . ... Telescopes . ... Apart from the 6-meter telescope BTA two small telescopes are operative at SAO: the 1-m and 0.6-m telescopes, both manufactured by Carl Zeiss, Jena, are located near the BTA. ... These telescopes are used for adjusting the equipment and techniques of observations used at the BTA. ... The observational time allocation and also a brief description of the equipment of the 1-m telescope, which is used either permanently or mainly on this telescope, are presented below. ...

... Southern . ... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Discovery and characterisation of Pre Main Sequence stars in southern star forming regions . ... Observing with ESO Telescopes . ... ESO-MIDAS . ... Using a robust method to identify Pre-Main Sequence (PMS) stars through their photometric excess in the Hн± band, we have recently studied the star formation history in several star burst clusters in the Galaxy, Small and Large Magellanic Clouds. ...

This diagram illustrates a frame-like layout with 'position: fixed'. The illustration shows a four-panel frameset. The top panel ("header") covers the entire width of the frameset and takes up 15% of the vertical space. ... To the right of the sidebar and below the header is the "main" area, whose dimensions are computed based on remaining available space. Finally, at the bottom, the "footer" area is 100px high and covers the entire width of the frameset. ...

... They are concerned with Attitude Control System of the spacecraft, satellite visibility from tracking stations, limits on the satellite autonomous operations during the orbit, and needs for auxiliary operations with the spacecraft. ... Among the operational constraints the most important one is the number of programmed slews per orbit, which determines the maximum number of radio sources to be observed during one orbit. ... System temperature (K) . ... Progress of the RadioAstron Project in Pictures...

Main Page Data Structures File List Data Fields Globals . Info on an observing target. ... target_id . char . ... double . ... decep0 . float . equinox . ... dec_err . ... char _target::target[17] . double _target::raep0 . double _target::decep0 . float _target::equinox . double _target::ra_err . double _target::dec_err . double _target::sysvel . char _target::veltyp[9] . ... The documentation for this struct was generated from the following file: . ...