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eso9823-en-au — Organisation Release
eso9822-en-au — Organisation Release
eso9821-en-au — Organisation Release
eso9820-en-au — Organisation Release
eso9819-en-au — Organisation Release
21 May 1998: One of the most crucial operations before the VLT UT1 First Light was successfully concluded late last evening at Paranal. For the first time ever, an astronomical mirror with a total surface of more than 50 m 2 has been coated with a thin (less than 0.0001 mm) and highly reflective layer of extremely pure aluminium. The very good result of this critical operation guarantees that the VLT UT1 will now be able to capture efficiently the faintest light from celestial objects.
eso9818-en-au — Organisation Release
19 May 1998: With the VLT UT1 First Light just one week away, the ultimate activities that lead up to this important event have started at the Paranal Observatory. Following successful optical alignment tests, cf. ESO Press Release 05/98 , the 8.2-m primary mirror has been removed from the first Unit Telescope (UT1). It is now in the Mirror Maintenance Building (MMB) and is being prepared for coating with a thin, highly reflective aluminium layer.
eso9817-en-au — Organisation Release
eso9816-en-au — Organisation Release
eso9815-en-au — Organisation Release
30 April 1998: This is another video clip with recent footage from the Paranal Observatory, illustrating the continuing progress of the VLT project. It was obtained in mid-April 1998 by the ESO EPR Video Team and forms part of the video tape ( UT1-FLE-VNR1 ) with selected video material for broadcast use, issued in connection with the VLT First Light Event.
eso9814-en-au — Organisation Release
eso9813-en-au — Organisation Release
eso9812-en-au — Organisation Release
eso9811-en-au — Organisation Release
11 March 1998: The European Southern Observatory is building the world's largest optical telescope, the Very Large Telescope (VLT) , at the ESO Paranal Observatory in Chile. The VLT consists of four 8.2-m unit telescopes and several smaller, moveable Auxiliary Telescopes. When coupled as the giant VLT Interferometer (VLTI) , they will together provide the sharpest images ever obtained by any optical telescope. It will in principle be able to see an astronaut on the surface of the Moon, 400,000 km away.
eso9810-en-au — Organisation Release
Another Job Well Done at Paranal — M1 Mirror Cell and Dummy 8.2-m Mirror Attached to First Telescope
10 March 1998: The VLT assembly work at the ESO Paranal Observatory continues in great strides. During the past week, the mirror cell for the 8.2-m main mirror (the M1 cell ) was successfully attached to the bottom of the telescope tube of Unit Telescope 1 (UT1). The present `picture story' illustrates the various phases of this delicate operation.
eso9809-en-au — Organisation Release
5 March 1998: We continue the publication of video clips which illustrate the rapid progress of the VLT project. The present footage of the ISAAC (Infrared Spectrometer and Array Camera) instrument for the ESO Very Large Telescope was obtained last week by the ESO EPR Video Team at the ESO Headquarters in Garching.
eso9808-en-au — Organisation Release
3 March 1998: We continue the publication of video clips which illustrate the rapid progress of the VLT project. The present footage of the FORS (FOcal Reducer/low dispersion Spectrograph) instrument for the ESO Very Large Telescope was obtained by the ESO EPR Video Team during a recent mission to DLR (Deutsche Forschungsanstalt für Luft- und Raumfahrt e.V.) in Oberpfaffenhofen near Munich (Germany).
eso9807-en-au — Organisation Release
17 February 1998: Now that the big mechanical pieces of the first 8.2-metre unit telescope (UT1) of ESO's Very Large Telescope (VLT) have been assembled, the work areas have shifted towards the many other components that are needed to make the first giant optical telescope in the southern hemisphere operational. Although most of these items may be of less impressive dimensions, they are equally indispensable to make a telescope of this size and weight point towards a given direction and follow the motion of the celestial objects to be observed with superior accuracy.
eso9806-en-au — Photo Release
30 January 1998: While famous Comet Hale-Bopp continues its long voyage towards the outer reaches of the solar system, observations proceed with telescopes in the southern hemisphere. These research programmes aim at a better understanding of the further development of this very active comet as it moves away from the Sun and slowly cools. Among the key questions are for instance: "When will it cease to display a dust tail?" and "Will the nucleus undergo outbursts during which much fresh material will be dispensed into space, as this has occasionally happened by other comets (e.g. Halley)?"
eso9805-en-au — Organisation Release
29 January 1998: SOFI, ESO's new infrared imager/spectrometer, saw first light at the NTT telescope on December 6, 1997, as planned and less than two years after the start of its detailed design. The acronym stands for 'Son OF ISAAC', the larger Infrared Spectrometer And Array Camera being built by ESO for the VLT.
eso9804-en-au — Organisation Release
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