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  linkMPE   linkNews   pointerPR20100421
MPE Press Release 2010-04-21

Making the invisible visible

New workhorse for the world's largest optical telescope



Sternentstehungsregion
Star forming region in the Milky Way
Sternentstehungsregion
Sternentstehungsregion
The irregular dwarf galaxy NGC 1569 in optical (top) and infrared light (bottom)
Sternentstehungsregion
The multi-object spectrum shows signatures of various elements in distant galaxies

(Tucson, Ariz.) --- The Large Binocular Telescope (LBT) partners in Germany, the U.S.A. and Italy are pleased to announce that the first of two new innovative near-infrared cameras/spectrographs for the LBT is now available to astronomers for scientific observations at the telescope on Mt. Graham in south-eastern Arizona. After more than a decade of design, manufacturing and testing, the new instrument, dubbed LUCIFER 1, provides a powerful tool to gain spectacular insights into the universe, from the Milky Way up to extremely distant galaxies. LUCIFER 1 has been built by a consortium of German institutes and will be followed by an identical twin instrument that will be delivered to the telescope in early 2011.

LUCIFER's innovative design allows astronomers to observe in unprecedented detail, for example, star forming regions which are commonly hidden by dust clouds. The instrument provides unrivaled flexibility, with features such as a unique robotic arm that can replace spectroscopic masks within the instrument's extreme sub-zero environment.

Pushing the limits
LUCIFER and its twin are mounted at the focus points of the LBT's two giant 8.4-meter (27.6 foot) diameter telescope mirrors. Each instrument is cooled to a chilly -213 degrees Celsius in order to observe in the near-infrared (NIR) wavelength range. Near-infrared observations are essential for understanding the formation of stars and planets in our galaxy as well as revealing the secrets of the most distant and very young galaxies.

LUCIFER is a remarkable new multi-purpose instrument with great flexibility combining a large field of view with a high resolution. It provides three exchangeable cameras for imaging and spectroscopy in different resolutions according to observational requirements. Besides its outstanding imaging capability which presently makes use of 18 high-quality filters, LUCIFER allows the simultaneous spectroscopy of about two dozen objects in the infrared through laser-cut slit-masks. For highest flexibility the masks can be changed even at the cryogenic temperatures, through the innovative development of a unique robotic mask grabber which places the individual masks with absolute precision into the focal plane.

"Together with the large light gathering power of the LBT, astronomers are now able to collect the spectral fingerprints of the faintest and most distant objects in the universe." says Richard Green, the Director of the LBT. "After completion of the LBT adaptive secondary mirror system to correct for atmospheric perturbation, LUCIFER will show its full capability by delivering images with a quality that are otherwise only obtained from space-based observatories."

Where stars are born
"Already the very first LUCIFER observations of star forming regions are giving us a hunch for the enormous potential of the new instrument," said Thomas Henning, the chair of the German LBT-Partners.

Image one (by Arjan Bik) is a snapshot of a stellar nursery in our home galaxy, the Milky Way: a high-mass star forming region inside the giant molecular cloud S255, about 8,000 light-years away from Earth (1 light-year is roughly 10 trillion kilometres). Such clouds are typically opaque to visible light. However, infrared light can penetrate the dust, so that the LUCIFER image reveals the cluster of newly born stars and its complex environment in all their splendour.

Image two (by Anna Pasquali) shows the faint irregular dwarf galaxy NGC 1569, located 6.2 million light-years from Earth. This galaxy contains several large stellar clusters with episodic star formation at a rate of more than 100 times faster than we observe in our own galaxy. In visible light, the core of the galaxy shows only three large stellar clusters, each containing more than one million stars. With LUCIFER it became possible to peer through the cosmic dust and to reveal many more compact star forming regions.

Image three (by Jaron Kurk) is a cut-out of a multi-object spectrum obtained with LUCIFER showing the tell-tale signs of gas heated by young stars at unimaginable distances of billions of light-years. Such a spectrum is the decomposition of light into its different wavelengths (colours). At certain wavelengths, emission lines can be found depending on the chemical composition and physical conditions of an object. They are fingerprints for the investigation of what goes on in stars and galaxies. For distant galaxies, the most interesting lines are found in the near-infrared, where observations were less efficient until now. With LUCIFER and the LBT, large samples of galaxies can now be studied using its multi-object capability.

An outstanding success for German institutes
The instruments have been built by a consortium of five German institutes led by the Center for Astronomy of Heidelberg University (Landessternwarte Heidelberg, LSW) together with the Max Planck Institute for Astronomy in Heidelberg (MPIA), the Max Planck Institute for Extraterrestrial Physics in Garching (MPE), the Astronomical Institute of the Ruhr-University in Bochum (AIRUB) as well as the University of Applied Sciences in Mannheim (Hochschule Mannheim).

Walter Seifert (LSW), Nancy Ageorges (MPE) and Marcus Jütte (AIRUB), responsible for the successful commissioning, spent more than half a year in several runs at the LBT site to make the telescope/instrument combination work efficiently. Holger Mandel, the PI of LUCIFER said: "From the very beginning, there was a uniform excitement about the promise of this instrument for world-beating science. Now, the amazing results speak for themselves."

The Large Binocular Telescope (LBT) is a collaboration among the Italian astronomical community (National Institute of Astrophysics - INAF), The University of Arizona, Arizona State University, Northern Arizona University, the LBT Beteiligungsgesellschaft in Germany (Max-Planck-Institut für Astronomie in Heidelberg, Zentrum fur Astronomie der Universität Heidelberg, Astrophysikalisches Institut in Potsdam, Max-Planck-Institut für Extraterrestrische Physik in Munich, and Max-Planck-Institut für Radioastronomie in Bonn), The Ohio State University and Research Corporation (Ohio State University, University of Notre Dame, University of Minnesota, and University of Virginia).

Editor's Note:
For more images, detailed image captions and additional technical background information, see here:
http://www.mpia.de/Public/menu_q2e.php?Aktuelles/PR/2010/PR2010.html

Further information about the MPE contribution to LUCIFER can be found here:
http://www.mpe.mpg.de/ir/lucifer/index.php?lang=en

 

Contacts

 

Hannelore Hämmerle interner Verweis Dr. Hannelore Hämmerle
Press officer
Max-Planck-Institut für extraterrestrische Physik, Garching
Tel.: +49 89 30000-3980
E-Mail:   hannelore.haemmerle

Reiner Hofmann interner Verweis Dr. Reiner Hofmann
Max-Planck-Institut für extraterrestrische Physik
Tel.: +49 89 30000-3289
E-Mail:   reh
Reiner Hofmann interner Verweis Dr. Jaron Kurk
Max-Planck-Institut für extraterrestrische Physik
Tel.: +49 89 30000-3587
E-Mail:   kurk
Nancy Ageorges interner Verweis Dr. Nancy Ageorges
Max-Planck-Institut für extraterrestrische Physik
Tel.: +49 89 30000-3289
E-Mail:   ageorges

 


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