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Annual Report 2011 Max Planck Institute for Astronomy

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10 I. General<br />

Credit: CAHA<br />

I.2 Observatories, Telescopes, and Instruments<br />

The <strong>Max</strong> <strong>Planck</strong> <strong>Institute</strong> <strong>for</strong> <strong>Astronomy</strong> has been a<br />

key driver and partner in the construction and operation<br />

of two large ground-based observatories. During<br />

the 1970s and 1980s the construction of the Calar<br />

Alto Observatory, still the largest observatory on the<br />

European continent, had been the central focus of the<br />

MPIA, and the two largest telescopes with 2.2 m and<br />

3.5 m mirrors are still scheduled <strong>for</strong> competitive observing<br />

programs. Since 2004 the observatory is jointly<br />

operated as Centro Astronomico Hispano Aleman (Caha)<br />

by the <strong>Max</strong> <strong>Planck</strong> Society, represented by the MPIA,<br />

and the Consejo Superior de Investigaciones Científicas<br />

(CSIC), represented by the Instituto de Astrofísica de<br />

Andalucía (IAA), as an organization of Spanish law.<br />

Since 1997, the MPIA has been the coordinating institute<br />

<strong>for</strong> the German participation in the Large Binocular<br />

Telescope (LBT) on Mt. Graham near Tucson, Arizona.<br />

By the end of 2007, the second prime-focus camera was<br />

installed which is now used <strong>for</strong> regular science programs.<br />

The year 2008 has seen the installation and the<br />

beginning of the commissioning of the first of the two<br />

LuCi instruments, jointly built by the Landessternwarte<br />

of the Center <strong>for</strong> <strong>Astronomy</strong> of Heidelberg University<br />

(ZAH), the MPIA, and the MPE. Additional contributions<br />

were also made by the Ruhr University Bochum and<br />

the Fachhochschule Mannheim. Science demonstration<br />

observations with this near-infrared multi-object<br />

spectrometer have commenced in December 2009 and<br />

at the beginning of 2010 the first excellent spectra<br />

and images have been published. Furthermore, the<br />

first adaptive secondary mirror <strong>for</strong> the LBT started its<br />

operation in 2010 and hence the first “sharper than<br />

hubbLe” near infrared LBT-images could be released.<br />

The MPIA also uses its 2.2 m telescope on La Silla,<br />

Chile, operated by the European Southern Observatory<br />

(eso). As of April 1 st 2009 in a new agreement between<br />

the MPG and Eso, the amount of time available at this<br />

telescope <strong>for</strong> MPG researchers has been increased from<br />

25 to 75 percent.<br />

Fig. I.2.1: Areal View of the Calar Alto Observatory (caha).

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