Andrew Yee[_1_]
January 28th 07, 05:11 PM
ESO Education and Public Relations Dept.
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Text with all links and the photos are available on the ESO Website at URL:
http://www.eso.org/outreach/press-rel/pr-2006/pr-51-06.html
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For Immediate Release: 22 December 2006
ESO Press Photo 51/06
Little Brother Joins the Large Family
First Light for VLT's Auxiliary Telescope No.4
On the night of 15 December 2006, the fourth and last-to-be-installed VLTI
Auxiliary Telescope (AT4) obtained its 'First Light'. The first images
demonstrate that AT4 will be able to deliver the excellent image quality
already delivered by the first three ATs. It will soon join its siblings to
perform routinely interferometric measurements.
The VLT is composed of four 8.2-m Unit Telescope (Antu, Kueyen, Melipal and
Yepun). They have been progressively put into service together with a vast
suite of the most advanced astronomical instruments and are operated every
night in the year.
Contrary to other large astronomical telescopes, the VLT was designed from
the beginning with the use of interferometry as a major goal. The VLT
Interferometer (VLTI) combines starlight captured by two or three 8.2- VLT
Unit Telescopes, dramatically increasing the spatial resolution and showing
fine details of a large variety of celestial objects.
However, most of the time the large telescopes are used for other research
purposes. They are therefore only available for interferometric observations
during a limited number of nights every year. Thus, in order to exploit the
VLTI each night and to achieve the full potential of this unique setup, some
other (smaller), dedicated telescopes were included into the overall VLT
concept.
These telescopes, known as the VLTI Auxiliary Telescopes (ATs), are mounted
on tracks and can be placed at precisely defined "parking" observing
positions on the observatory platform. From these positions, their light
beams are fed into the same common focal point via a complex system of
reflecting mirrors mounted in an underground system of tunnels.
The Auxiliary Telescopes are real technological jewels. They are placed in
ultra-compact enclosures, complete with all necessary electronics, an air
conditioning system and cooling liquid for thermal control, compressed air
for enclosure seals, a hydraulic plant for opening the dome shells, etc.
Each AT is also fitted with a transporter that lifts the telescope and
relocates it from one station to another. It moves around with its own
housing on the top of Paranal, almost like a snail.
The VLTI is arguably the world's most advanced optical device of this type.
It has already demonstrated its powerful capabilities by addressing several
key scientific issues, such as determining the size and the shape of a
variety of stars (ESO PR 22/02, PR 14/03, PR 31/03, and PR 09/06), measuring
distances to stars (ESO PR 25/04), probing the innermost regions of the
proto-planetary discs around young stars (ESO PR 27/04 and PR 35/06) or
making the first detection by infrared interferometry of an extragalactic
object (ESO PR 17/03).
National contacts for the media:
Belgium: Dr. Rodrigo Alvarez, +32-2-474 70 50
Finland: Ms. Riitta Tirronen, +358 9 7748 8369
Denmark: Dr. Michael Linden-Vnle, +45-33-18 19 97
France: Dr. Daniel Kunth, +33-1-44 32 80 85
Germany: Dr. Jakob Staude, +49-6221-528229
Italy: Dr. Leopoldo Benacchio, +39-347-230 26 51
The Netherlands: Ms. Marieke Baan, +31-20-525 74 80
Portugal: Prof. Teresa Lago, +351-22-089 833
Sweden: Dr. Jesper Sollerman, +46-8-55 37 85 54
Switzerland: Dr. Martin Steinacher, +41-31-324 23 82
United Kingdom: Mr. Peter Barratt, +44-1793-44 20 25
----------------------------------------------------------------------------
ESO Press Information is available on Receive email notification
the WWW at about important news from ESO:
http://www.eso.org/outreach/press-rel/. subscribe to the
----------------------------------------------------------------------------
(c) ESO Education & Public Relations Department
Karl-Schwarzschild-Strasse 2, D-85748 Garching, Germany
----------------------------------------------------------------------------
----------------------------------------------------------------------------
Text with all links and the photos are available on the ESO Website at URL:
http://www.eso.org/outreach/press-rel/pr-2006/pr-51-06.html
----------------------------------------------------------------------------
For Immediate Release: 22 December 2006
ESO Press Photo 51/06
Little Brother Joins the Large Family
First Light for VLT's Auxiliary Telescope No.4
On the night of 15 December 2006, the fourth and last-to-be-installed VLTI
Auxiliary Telescope (AT4) obtained its 'First Light'. The first images
demonstrate that AT4 will be able to deliver the excellent image quality
already delivered by the first three ATs. It will soon join its siblings to
perform routinely interferometric measurements.
The VLT is composed of four 8.2-m Unit Telescope (Antu, Kueyen, Melipal and
Yepun). They have been progressively put into service together with a vast
suite of the most advanced astronomical instruments and are operated every
night in the year.
Contrary to other large astronomical telescopes, the VLT was designed from
the beginning with the use of interferometry as a major goal. The VLT
Interferometer (VLTI) combines starlight captured by two or three 8.2- VLT
Unit Telescopes, dramatically increasing the spatial resolution and showing
fine details of a large variety of celestial objects.
However, most of the time the large telescopes are used for other research
purposes. They are therefore only available for interferometric observations
during a limited number of nights every year. Thus, in order to exploit the
VLTI each night and to achieve the full potential of this unique setup, some
other (smaller), dedicated telescopes were included into the overall VLT
concept.
These telescopes, known as the VLTI Auxiliary Telescopes (ATs), are mounted
on tracks and can be placed at precisely defined "parking" observing
positions on the observatory platform. From these positions, their light
beams are fed into the same common focal point via a complex system of
reflecting mirrors mounted in an underground system of tunnels.
The Auxiliary Telescopes are real technological jewels. They are placed in
ultra-compact enclosures, complete with all necessary electronics, an air
conditioning system and cooling liquid for thermal control, compressed air
for enclosure seals, a hydraulic plant for opening the dome shells, etc.
Each AT is also fitted with a transporter that lifts the telescope and
relocates it from one station to another. It moves around with its own
housing on the top of Paranal, almost like a snail.
The VLTI is arguably the world's most advanced optical device of this type.
It has already demonstrated its powerful capabilities by addressing several
key scientific issues, such as determining the size and the shape of a
variety of stars (ESO PR 22/02, PR 14/03, PR 31/03, and PR 09/06), measuring
distances to stars (ESO PR 25/04), probing the innermost regions of the
proto-planetary discs around young stars (ESO PR 27/04 and PR 35/06) or
making the first detection by infrared interferometry of an extragalactic
object (ESO PR 17/03).
National contacts for the media:
Belgium: Dr. Rodrigo Alvarez, +32-2-474 70 50
Finland: Ms. Riitta Tirronen, +358 9 7748 8369
Denmark: Dr. Michael Linden-Vnle, +45-33-18 19 97
France: Dr. Daniel Kunth, +33-1-44 32 80 85
Germany: Dr. Jakob Staude, +49-6221-528229
Italy: Dr. Leopoldo Benacchio, +39-347-230 26 51
The Netherlands: Ms. Marieke Baan, +31-20-525 74 80
Portugal: Prof. Teresa Lago, +351-22-089 833
Sweden: Dr. Jesper Sollerman, +46-8-55 37 85 54
Switzerland: Dr. Martin Steinacher, +41-31-324 23 82
United Kingdom: Mr. Peter Barratt, +44-1793-44 20 25
----------------------------------------------------------------------------
ESO Press Information is available on Receive email notification
the WWW at about important news from ESO:
http://www.eso.org/outreach/press-rel/. subscribe to the
----------------------------------------------------------------------------
(c) ESO Education & Public Relations Department
Karl-Schwarzschild-Strasse 2, D-85748 Garching, Germany
----------------------------------------------------------------------------