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New near-infrared cameras/spectrographs will allow astronomers to watch stars being born

Date:
April 23, 2010
Source:
Max-Planck-Gesellschaft
Summary:
A new instrument, dubbed LUCIFER 1, provides a powerful tool to gain spectacular insights into the universe. It will allow astronomers to observe the faintest and most distant objects in the universe.

The faint irregular dwarf galaxy NGC 1569 is 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.
Credit: Anna Pasquali

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.

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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.

LUCIFER and its twin are mounted at the focus points of the LBT's two giant 8.4-metre (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."

"Already the very first LUCIFER observations of star forming regions are giving us an indication of the enormous potential of the new instrument," said Thomas Henning, the chair of the German LBT-Partners.

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 Jόtte (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 Principal Investigator of LUCIFER said: "From the very beginning, there was uniform excitement about the promise of this instrument for cutting-edge 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 Institute for Astronomy in Heidelberg, Zentrum fur Astronomie der Universitδt Heidelberg, Astrophysikalisches Institut in Potsdam, Max Planck Institute for Extraterrestrial Physics in Garching (Munich), and Max Planck Institute fϋr Radio Astronomy in Bonn), The Ohio State University and Research Corporation (Ohio State University, University of Notre Dame, University of Minnesota, and University of Virginia).


Story Source:

The above story is based on materials provided by Max-Planck-Gesellschaft. Note: Materials may be edited for content and length.


Cite This Page:

Max-Planck-Gesellschaft. "New near-infrared cameras/spectrographs will allow astronomers to watch stars being born." ScienceDaily. ScienceDaily, 23 April 2010. <www.sciencedaily.com/releases/2010/04/100422112639.htm>.
Max-Planck-Gesellschaft. (2010, April 23). New near-infrared cameras/spectrographs will allow astronomers to watch stars being born. ScienceDaily. Retrieved January 30, 2015 from www.sciencedaily.com/releases/2010/04/100422112639.htm
Max-Planck-Gesellschaft. "New near-infrared cameras/spectrographs will allow astronomers to watch stars being born." ScienceDaily. www.sciencedaily.com/releases/2010/04/100422112639.htm (accessed January 30, 2015).

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