Press Releases

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eso0005 — Organisation Release
Next VLT Instrument Ready for the Astronomers
8 February 2000: The commissioning of the FORS2 multi-mode astronomical instrument at KUEYEN , the second FOcal Reducer/low dispersion Spectrograph at the ESO Very Large Telescope, was successfully finished today. This important work -- that may be likened with the test driving of a new car model -- took place during two periods, from October 22 to November 21, 1999, and January 22 to February 8, 2000.
eso0004 — Organisation Release
And Then There Were Three...!
28 January 2000: This was a night to remember at the ESO Paranal Observatory! For the first time, three 8.2-metre Very Large Telescopes (VLTs) were observing in parallel, with a combined mirror surface of nearly 160 metres squared. In the evening of January 26, the third 8.2-metre Unit Telescope, MELIPAL ("The Southern Cross" in the Mapuche language), was pointed to the sky for the first time and successfully achieved "First Light". During this night, a number of astronomical exposures were made that served to evaluate provisionally the performance of the new telescope. The ESO staff expressed great satisfaction with MELIPAL and there were broad smiles all over the mountain.
eso0003 — Organisation Release
Final Tests before MELIPAL "First Light"
21 January 2000: Happy expectations are again growing at ESO's Paranal Observatory. For the third time in less than two years, the special moment of "First Light" for an 8.2-metre VLT Unit Telescope is getting close -- now is the turn of MELIPAL.
eso0002 — Organisation Release
"First Light" Approaches for VLT MELIPAL
12 January 2000: After the first two Unit Telescopes of ESO's Very Large Telescope started their operation in 1999, the year 2000 will witness the "first light" of the other two telescopes, starting with MELIPAL.
eso0001 — Organisation Release
ESO PR Highlights in 1999
5 January 2000: Many different activities took place at ESO during the past year. They range from technological and scientific feats to official and astronomical events at the ESO sites in Europe and Chile.
eso9954 — Photo Release
One Hundred Thousand Galaxies at a Glance
21 December 1999: A main scientific application of wide-angle imaging in astronomy is the census and photometric and morphological classification (i.e. by colour and shape) of large quantities of celestial objects in order to identify sources of particular interest that warrant in-depth follow-up observations. This is normally done by means of spectroscopy , a basic observing technique that allows much more comprehensive physical diagnostics than does an image. However, detailed spectral observations requires the great light-collecting power of large telescopes such as the Very Large Telescope (VLT). In the past, many important classes of astronomical objects have been discovered by such survey work. Another central goal of wide-field imaging is the identification and characterisation of structures that extend over large sky areas, e.g., of the Milky Way in which we live, of comparatively nearby galaxies, and even of the Universe as a whole. The structure of astronomical objects reveals much about their history of formation which, because of the inherently very long ("astronomical") timescales, cannot be directly observed.
eso9953 — Science Release
New VLT Observations Address the Age of the Universe
16 December 1999: Recent observations with the FORS1 instrument at the first 8.2-m VLT Unit Telescope (ANTU) by an international group of astronomers [1] have resulted in crucial new information about some small and faint stars within an old star cluster in the Milky Way.
eso9952 — Organisation Release
REOSC Delivers the Best Astronomical Mirror in the World to ESO
14 December 1999: On December 14, 1999, REOSC , the Optical Department of the SAGEM Group , finished the polishing of the fourth 8.2-m main mirror for the Very Large Telescope (VLT) of the European Southern Observatory. The mirror was today delivered to ESO at a ceremony at the REOSC factory in Saint Pierre du Perray, just south of Paris.
eso9951 — Organisation Release
Recent Views from the Paranal Observatory
8 December 1999: A series of photographs from the Paranal Observatory was obtained with large-format cameras in mid-November 1999 by the ESO EPR Team.
eso9950 — Organisation Release
Third VLT 8.2-m Mirror Successfully Coated and Installed at MELIPAL
3 December 1999: In the course of the current installation of ESO's Very Large Telescope (VLT) , a delicate operation has just been successfully achieved at the Paranal Observatory. The coated 8.2-m Zerodur main mirror for the third VLT 8.2-m Unit Telescope, MELIPAL , is now in place!
eso9949 — Organisation Release
VLT Commissioning Data Now Publicly Available
29 November 1999: "First Light" was achieved in May 1998 for VLT ANTU, the first 8.2-m Unit Telescope at the Paranal Observatory. Since then, thousands of detailed images and spectra of a great variety of celestial objects have been recorded with this major new research facility. While some of these were obtained for scientific programmes and were therefore directed towards specific research needs, others were made during the "Commissioning Phases" in 1998/99 for the two major astronomical instruments, FORS1 (FOcal Reducer and Spectrograph) and ISAAC (Infrared Spectrometer And Array Camera). They were carried out in order to test thoroughly the performance of the telescope and its instruments before the new facility was handed over to the astronomers on April 1, 1999. The Commissioning data are accordingly of variable quality and, contrarily to the science data, normally not intensity calibrated. However, while some of these frames are short test exposures that mainly served to ascertain the image quality under various observing conditions, a substantial fraction still contains scientifically valuable data.
eso9948 — Organisation Release
A Powerful Twin Arrives
17 November 1999: The first, major astronomical instrument to be installed at the ESO Very Large Telescope (VLT) was FORS1 ( FO cal R educer and S pectrograph) in September 1998. Immediately after being attached to the Cassegrain focus of the first 8.2-m Unit Telescope, ANTU , it produced a series of spectacular images, cf. ESO PR 14/98. Many important observations have since been made with this outstanding facility. Now FORS2, its powerful twin, has been installed at the second VLT Unit Telescope, KUEYEN. It is the fourth major instrument at the VLT after FORS1 , ISAAC and UVES. The FORS2 Commissioning Team that is busy installing and testing this large and complex instrument reports that "First Light" was successfully achieved already on October 29, 1999, only two days after FORS2 was first mounted at the Cassegrain focus. Since then, various observation modes have been carefully tested, including normal and high-resolution imaging, echelle and multi-object spectroscopy, as well as fast photometry with millisecond time resolution. A number of fine images were obtained during this work, some of which are made available with the present Press Release.
eso9947 — Photo Release
Solitude of an Observatory
26 October 1999: The La Silla Observatory is located in the Chilean Atacama Desert, one of the driest and loneliest areas of the world. The land around this isolated peak was acquired in 1964 and following some years of construction work, the inauguration of ESO's first observatory took place just over 30 years ago, in March 1969. The solitude of this remote desert site is well illustrated by the above panorama, obtained in 1996.
eso9946 — Science Release
Lots of Small Stars Born in Starburst Region
13 October 1999: An international group of astronomers [1] has used the ESO Very Large Telescope (VLT) at Paranal (Chile) to perform unique observations of an interstellar nebula in which stars are currently being born.
eso9945 — Organisation Release
ALMA Moves!
7 October 1999: The clip contains a full-scale computer animation of the Atacama Large Millimeter Array (ALMA) at the future site of this large astronomical facility.
eso9944 — Organisation Release
Successful "First Light" for VLT High-Resolution Spectrograph
5 October 1999: A major new astronomical instrument for the ESO Very Large Telescope at Paranal (Chile), the UVES high-resolution spectrograph, has just made its first observations of astronomical objects. The astronomers are delighted with the quality of the spectra obtained at this moment of "First Light". Although much fine-tuning still has to be done, this early success promises well for new and exciting science projects with this large European research facility.
eso9943 — Organisation Release
Recent VLT Progress
17 September 1999: Work is progressing well at ESO's Very Large Telescope (VLT) project, both at the Paranal Observatory and in Europe. Here is a brief summary with recent news from this major project, illustrated with photos from the construction.
eso9942 — Science Release
Faintest Methane Brown Dwarf Discovered with the NTT and VLT
18 August 1999: A team of European astronomers [1] has found a cold and extremely faint object in interstellar space, high above the galactic plane. It is a Methane Brown Dwarf of which only a few are known. This is by far the most distant one identified to date.
eso9941 — Photo Release
Report about the Solar Eclipse on August 11, 1999
18 August 1999: This webpage provides information about the total eclipse on Wednesday, August 11, 1999, as it was seen by ESO staff, mostly at or near the ESO Headquarters in Garching (Bavaria, Germany). The zone of totality was about 108 km wide and the ESO HQ were located only 8 km south of the line of maximum totality. The duration of the phase of totality was about 2 min 17 sec.
eso9940 — Organisation Release
The VLT Writes Its Name
13 August 1999: A computer-controlled "Active Optics" system was first developed at ESO in the 1980's. It allows the continuous tuning of the optical system of an astronomical telescope, thus ensuring that it always produces the sharpest possible images of astronomical objects. The first major telescope to profit from this revolution in telescope techniques was the ESO New Technology Telescope (NTT) at the La Silla observatory. Since it began operation in 1990, 75 adjustable supports below the 3.58-m primary mirror, coupled with advanced image analysis and control software, have made this prototype telescope one of the best in the world. Each of the four ESO Very Large Telescope (VLT) Unit Telescopes is equipped with the latest, improved active optics system that controls the primary 8.2-m Zerodur mirror as well as the secondary 1.1-m lightweight beryllium mirror at the top of the telescope structure. This system offers complete control of the optical quality, allowing the VLT to take full advantage of the exceptional atmospheric conditions at Paranal. This is amply confirmed by fine quality of the astronomical observations now performed with the first Unit Telescope, ANTU. In the course of the one-year commissioning period (May 1998 - March 1999), ESO's opticians performed extensive tests and further improvements of the active optics system at ANTU. Here are some interesting examples that illustrate the amazing versatility of this front-line technological system.