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Public release date: 12-Dec-2012[ | E-mail |
Share ] Contact: Richard Hook
rhook@eso.org
49-893-200-6655
ESO
KMOS successfully installed on ESO's Very Large Telescope
The K-band Multi-Object Spectrograph (KMOS), attached to the Very Large Telescope (VLT) Unit Telescope 1 at ESO's Paranal Observatory in Chile, has successfully achieved first light. During the four-month period from August this 2.5-tonne instrument had been shipped from Europe, reassembled, tested and installed following months of careful planning. This was the culmination of many years of design and construction by teams in the UK and Germany, and at ESO. KMOS is the second of the second generation of instruments to be installed on ESO's VLT (the first was X-shooter: see eso0920 -- http://www.eso.org/public/news/eso0920/).
"KMOS will bring an exciting new capability to the suite of instrumentation at the ESO VLT. Its initial success is a tribute to the dedication of a large team of engineers and scientists. The team looks forward to many future scientific discoveries with KMOS once the instrument commissioning is fully complete," says Ray Sharples (University of Durham, UK), co-principal investigator of KMOS.
To study the early lives of galaxies astronomers need three things: to observe in the infrared [1], to observe many objects at once and, for each one, to map out how their properties vary from place to place [2]. KMOS can do all of these things -- at the same time. Up to now astronomers could either observe many objects at once, or map a single object in detail. A detailed survey might take years for a large sample of objects. But with KMOS, by mapping the properties of many objects simultaneously, such surveys can now be completed in just months.
KMOS has robot arms that can be positioned independently in just the right place to catch the light from 24 distant galaxies, or other objects, simultaneously. Each arm in turn places a 14 by 14 pixel grid on top of the object and each of these 196 points collects light from different parts of the galaxy and splits it into its component colours as a spectrum. These weak signals are then recorded by very sensitive infrared detectors. This extraordinarily complex instrument has more than one thousand optical surfaces that had to be manufactured to high accuracy and carefully aligned [3].
"I remember, eight years ago, when the project started how I was sceptical about the complexity of KMOS. But today we are observing and the instrument is performing wonderfully," says Jeff Pirard, the ESO staff member responsible for the instrument. "Moreover, it has been a real pleasure to work together with the KMOS team. They are very professional and we had a great time working together."
KMOS was designed and built by a consortium of institutes working in partnership with ESO. These are: Centre for Advanced Instrumentation, Department of Physics, Durham University, Durham, UK, Universitats-Sternwarte Munchen, Munich, Germany, the Science and Technology Facilities Council's UK Astronomy Technology Centre, Royal Observatory, Edinburgh, UK, Max-Planck-Institut fur Extraterrestrische Physik, Garching, Germany, Sub-Department of Astrophysics, University of Oxford, Oxford, UK.
"I am excited about the fantastic opportunities KMOS offers to study distant galaxies. The possibility to observe 24 galaxies simultaneously will allow us to build galaxy samples of unprecedented size and quality. The collaboration among all partners and ESO could not have been better and I am very grateful to everybody who contributed to the construction of KMOS," concludes Ralf Bender (Universitats-Sternwarte Munchen and Max-Planck-Institut fur Extraterrestrische Physik, Germany), co-principal investigator.
###
Notes
[1] The expansion of the Universe shifts light to longer wavelengths. This means that much of the light from distant galaxies of interest to astronomers is shifted from visible-light wavelengths to the longer infrared wavelengths. To study galaxy evolution infrared instruments are vital.
[2] This technique, known as integral-field spectroscopy, allows astronomers to simultaneously study the properties of different parts of an object such as a galaxy to see how it is rotating and measure its mass. It also allows the chemical composition and other physical properties to be determined in different parts of the object.
[3] Most of the complex mechanisms in KMOS have to operate at -140 degrees Celsius, which creates major engineering challenges.
More information
The year 2012 marks the 50th anniversary of the founding of the European Southern Observatory (ESO). ESO is the foremost intergovernmental astronomy organisation in Europe and the world's most productive ground-based astronomical observatory by far. It is supported by 15 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the world's largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning the 39-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".
Links
Overview of the VLT instruments: http://www.eso.org/public/images/vlt/
Photos of the VLT: http://www.eso.org/public/images/archive/category/paranal/
KMOS information at the University of Durham: http://www.dur.ac.uk/cfai/projects/kmos/
KMOS information at USM: http://www.usm.uni-muenchen.de/people/wegner/kmos/en/index.php
KMOS science pages at ESO: http://www.eso.org/sci/facilities/develop/instruments/kmos.html
Contacts
Ray Sharples
University of Durham
Durham, UK
Tel: 44-191-334-3719
Email: r.m.sharples@durham.ac.uk
Ralf Bender
Universitts-Sternwarte Mnchen and Max-Planck-Institut fr Extraterrestrische Physik
Munich, Germany
Tel: 49-89-2180-5999
Email: bender@usm.lmu.de
Suzanne Ramsay
ESO
Garching bei Mnchen, Germany
Tel: 49-89-3200-6665
Email: sramsay@eso.org
Richard Hook
ESO, La Silla, Paranal, E-ELT & Survey Telescopes Press Officer
Garching bei Mnchen, Germany
[ | E-mail | Share ] ?
AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert! system.
Public release date: 12-Dec-2012[ | E-mail |
Share ] Contact: Richard Hook
rhook@eso.org
49-893-200-6655
ESO
KMOS successfully installed on ESO's Very Large Telescope
The K-band Multi-Object Spectrograph (KMOS), attached to the Very Large Telescope (VLT) Unit Telescope 1 at ESO's Paranal Observatory in Chile, has successfully achieved first light. During the four-month period from August this 2.5-tonne instrument had been shipped from Europe, reassembled, tested and installed following months of careful planning. This was the culmination of many years of design and construction by teams in the UK and Germany, and at ESO. KMOS is the second of the second generation of instruments to be installed on ESO's VLT (the first was X-shooter: see eso0920 -- http://www.eso.org/public/news/eso0920/).
"KMOS will bring an exciting new capability to the suite of instrumentation at the ESO VLT. Its initial success is a tribute to the dedication of a large team of engineers and scientists. The team looks forward to many future scientific discoveries with KMOS once the instrument commissioning is fully complete," says Ray Sharples (University of Durham, UK), co-principal investigator of KMOS.
To study the early lives of galaxies astronomers need three things: to observe in the infrared [1], to observe many objects at once and, for each one, to map out how their properties vary from place to place [2]. KMOS can do all of these things -- at the same time. Up to now astronomers could either observe many objects at once, or map a single object in detail. A detailed survey might take years for a large sample of objects. But with KMOS, by mapping the properties of many objects simultaneously, such surveys can now be completed in just months.
KMOS has robot arms that can be positioned independently in just the right place to catch the light from 24 distant galaxies, or other objects, simultaneously. Each arm in turn places a 14 by 14 pixel grid on top of the object and each of these 196 points collects light from different parts of the galaxy and splits it into its component colours as a spectrum. These weak signals are then recorded by very sensitive infrared detectors. This extraordinarily complex instrument has more than one thousand optical surfaces that had to be manufactured to high accuracy and carefully aligned [3].
"I remember, eight years ago, when the project started how I was sceptical about the complexity of KMOS. But today we are observing and the instrument is performing wonderfully," says Jeff Pirard, the ESO staff member responsible for the instrument. "Moreover, it has been a real pleasure to work together with the KMOS team. They are very professional and we had a great time working together."
KMOS was designed and built by a consortium of institutes working in partnership with ESO. These are: Centre for Advanced Instrumentation, Department of Physics, Durham University, Durham, UK, Universitats-Sternwarte Munchen, Munich, Germany, the Science and Technology Facilities Council's UK Astronomy Technology Centre, Royal Observatory, Edinburgh, UK, Max-Planck-Institut fur Extraterrestrische Physik, Garching, Germany, Sub-Department of Astrophysics, University of Oxford, Oxford, UK.
"I am excited about the fantastic opportunities KMOS offers to study distant galaxies. The possibility to observe 24 galaxies simultaneously will allow us to build galaxy samples of unprecedented size and quality. The collaboration among all partners and ESO could not have been better and I am very grateful to everybody who contributed to the construction of KMOS," concludes Ralf Bender (Universitats-Sternwarte Munchen and Max-Planck-Institut fur Extraterrestrische Physik, Germany), co-principal investigator.
###
Notes
[1] The expansion of the Universe shifts light to longer wavelengths. This means that much of the light from distant galaxies of interest to astronomers is shifted from visible-light wavelengths to the longer infrared wavelengths. To study galaxy evolution infrared instruments are vital.
[2] This technique, known as integral-field spectroscopy, allows astronomers to simultaneously study the properties of different parts of an object such as a galaxy to see how it is rotating and measure its mass. It also allows the chemical composition and other physical properties to be determined in different parts of the object.
[3] Most of the complex mechanisms in KMOS have to operate at -140 degrees Celsius, which creates major engineering challenges.
More information
The year 2012 marks the 50th anniversary of the founding of the European Southern Observatory (ESO). ESO is the foremost intergovernmental astronomy organisation in Europe and the world's most productive ground-based astronomical observatory by far. It is supported by 15 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the world's largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning the 39-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".
Links
Overview of the VLT instruments: http://www.eso.org/public/images/vlt/
Photos of the VLT: http://www.eso.org/public/images/archive/category/paranal/
KMOS information at the University of Durham: http://www.dur.ac.uk/cfai/projects/kmos/
KMOS information at USM: http://www.usm.uni-muenchen.de/people/wegner/kmos/en/index.php
KMOS science pages at ESO: http://www.eso.org/sci/facilities/develop/instruments/kmos.html
Contacts
Ray Sharples
University of Durham
Durham, UK
Tel: 44-191-334-3719
Email: r.m.sharples@durham.ac.uk
Ralf Bender
Universitts-Sternwarte Mnchen and Max-Planck-Institut fr Extraterrestrische Physik
Munich, Germany
Tel: 49-89-2180-5999
Email: bender@usm.lmu.de
Suzanne Ramsay
ESO
Garching bei Mnchen, Germany
Tel: 49-89-3200-6665
Email: sramsay@eso.org
Richard Hook
ESO, La Silla, Paranal, E-ELT & Survey Telescopes Press Officer
Garching bei Mnchen, Germany
[ | E-mail | Share ] ?
AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert! system.
Source: http://www.eurekalert.org/pub_releases/2012-12/e-2gt121012.php
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