Telescopes and Instrumentation
As set out in its convention, ESO provides state of the art facilities for Europe's astronomers and promotes and organises cooperation in astronomical research. Today, ESO operates some of the world's largest and most advanced observational facilities at three sites in northern Chile: La Silla, Paranal and Chajnantor. These are the best locations known in the southern hemisphere for astronomical observations. With other activities such as technology development, conferences and educational projects, ESO also plays a decisive role in forming a European Research Area for astronomy and astrophysics.
The Very Large Telescope (VLT) at Cerro Paranal is ESO's premier site for observations in the visible and infrared light. All four Unit Telescopes (UTs) of 8.2 metres diameter operate individually using a large collection of instruments.
The VLT offers also the possibility of combining the light from the four UTs to work as an interferometer. The Very Large Telescope Interferometer (VLTI), with its own suite of instruments, ultimately providing imagery at the milliarcsecond level as well as astrometry at 10 microarcsecond precision. In addition to the 8.2-metre diameter telescopes the VLTI is complemented by four Auxiliary Telescopes (AT) of 1.8-metre diameter to improve its imaging capabilities and enable full nighttime use on a year-round basis.
Two telescopes for imaging surveys are also in operation at Paranal, the VLT Survey Telescope (VST, 2.6-metre diameter) for the visible, and the Visible and Infrared Survey Telescope for Astronomy (VISTA, 4.1-metre) for the infrared.
La Silla Observatory
ESO operates two major telescopes (the ESO 3.6-metre telescope and the New Technology Telescope (NTT)) at the La Silla Observatory. They are equipped with state of the art instruments either built completely by ESO or by external consortia, with substantial contribution by ESO.
APEX, the Atacama Pathfinder Experiment, is a collaboration between Max Planck Institut für Radioastronomie (MPIfR) at 50%, Onsala Space Observatory (OSO) at 23%, and the European Southern Observatory (ESO) at 27% to construct and operate a modified ALMA prototype antenna as a single dish on the 5100-metre high site of Llano Chajnantor. The telescope was supplied by VERTEX Antennentechnik in Duisburg, Germany. APEX has a suite of heterodyne spectrometers and wide-field bolometer cameras operating in most of the atmospheric windows from 0.2 to 1.4 mm. The telescope is operated by ESO.
The Atacama Large Millimeter/submillimeter Array, or ALMA, is an international collaboration to operate a telescope of revolutionary design to study the Universe from a site in the foothills of Chile's Andes Mountains. ALMA is composed of 66 high precision antennas, operating at wavelengths of 0.32 to 3.6 mm. Its main 12-metre array has fifty antennas, each 12 metres in diameter, acting together as a single telescope — an interferometer. An additional compact array of four 12-metre and twelve 7-metre antennas complements this. The ALMA antennas can be arranged in different configurations, where the maximum distance between antennas can vary from 150 metres to 16 kilometres. The ALMA correlator, a specialised computer that combines the information received by the antennas, can perform a remarkable 16 000 million-million (1.6x1016) operations per second.
ALMA was inaugurated in 2013, but early scientific observations with a partial array had already begun in 2011.
ALMA is a partnership of ESO (representing its Member States), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (South Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ.
ESO has been working together with its user community of European astronomers and astrophysicists to define the new giant telescope needed by the middle of the next decade: the European Extremely Large Telescope (E-ELT). The E-ELT will be the largest optical/near-infrared telescope in the world: the world’s biggest eye on the sky. The mirror stretches over almost half the length of a soccer field.
The start of E-ELT construction is planned for late 2014, with start of operations planned for early in the next decade.
The site of the E-ELT will be Cerro Armazones, 20 kilometres from Paranal, site of the VLT.
With a 39-metre primary mirror and its adaptive optics concept, the E-ELT may revolutionise our perception of the Universe, much as Galileo's telescope did, 400 years ago, when he first pointed a telescope to the sky.
For more information please read the E-ELT page.