The Large Binocular Telescope is
unlike any other telescope in the world, it has two identical 8.4 m mirrors
mounted side-by-side on a common altitude-azimuth mounting for a combined
collecting area of a single 11.8 m telescope. The entire telescope and
enclosure is very compact due to the fast focal ratio (F/1.14) of the primary
mirrors.
The Observatory is located in south-eastern
Arizona near Safford in the Pinaleno Mountains on Emerald Peak at an altitude
of 3200m.
It is mainly used for the
search for extra solar planets, and infrared observations of deep space nebulae
and galaxies.
Over the last 6 months the
telescope has had new state-of the art infrared cameras installed, a process
that was only completed a few weeks ago ready for the 2016 observing season.
The new science instrument is called LINC-NIRVANA. It is a near infrared imaging instrument for
the Large Binocular Telescope designed to offer both multi adaptive optics, and
interferometric beam combination for ultra high spatial resolution. The
instrument is a collaboration between the German and Italian partners.
The Large Binocular Cameras are
two wide-field cameras mounted on the prime focus swing arms of the telescope.
LBC Blue is blue-optimized for observations from approximately 3500 to 6500
angstroms, while LBC Red is red-optimized for observations from approximately
5500 angstroms to 1 micron. The LBCs are used simultaneously in binocular mode.
LUCI 1 and LUCI2 (Shown above) is a pair of
infrared multi-mode instruments. In seeing-limited mode, each has a 4
arc-minute square field of view and will be capable of long-slit and multi-slit
spectroscopy as well as imaging in the near infrared bands from 0.85 to 2.4
microns. Each instrument will ultimately include diffraction-limited optics
(not available yet) covering a 30-arcsecond field of view for use with the
adaptive secondary mirrors.
This is the first light A LUCI2 seeing-limited image of Westerhout 3, in the K band - FWHM: 0.54"
Westerhout 3 (W3) is a giant molecular cloud about 6200 light-years away in the Perseus Arm, one of the Milky Way galaxy’s main spiral arms, that hosts both low and high-mass star formation. W3 Main and W3 (OH) contain the most recent high-mass star formation.
Richard Pearson
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