Instrumentation and Telescopes

Ground-based Telescopes and Instrumentation


 


Development and construction of state-of-the-art astronomical instrumentation for large optical telescopes constitutes one of the major activities of the MPIA. These instruments are operated at the telescopes of several ground-based observatories. The MPIA focuses on near-infrared instrumentation projects which are frequently carried out in international consortia.

This page provides an overview of the ground-based instrumentation projects at all development stages comprising instruments that are planned, under development, or in operations as well as decommissioned instruments built by (or with contributions from) the MPIA.

Calar Alto

3.5m telescope
ALFA Adaptive Optics with a Layer for Astronomy Decommissioned
LAICA Large Area Imager for Calar Alto Operational
MOSCA Multi Object Spectrogragh for Calar Alto Operational
OMEGA 2000 Near Infrared Wide-Field Prime Focus Camera (2K detector) Operational
OMEGA CASS New Infrared Prime Focus Multimode Imager / Spectrometer Operational, currently available only in imaging mode
OMEGA PRIME Near Infrared Wide-Field Prime Focus Camera Decommissioned
PYRAMIR Pyramid Infrared Wavefront Sensor Decomissioned
TWIN Double spectrograph for the 3.5m telescope Operational
 
2.2m telescope
AstraLux Lucky Imaging for high spatial resolution Operational
CAFOS Calar Alto Faint Object Spectrograph Operational
COUDÉ COUDÉ with MAGIC Decommissioned
MAGIC MPI for Astronomy general-purpose near-IR Camera Operational
PANIC Panoramic near-infrared camera Under development,
installation in fall 2011
 
1.23m telescope
CCD-Imager Charge Coupled Device Imager for the 1.23m telescope Currently not offered
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ESO/La Silla

WFI Wide field imager on the ESO/MPG 2.2m telescope Operational
AstraLux Sur Lucky Imaging Camera at the 3.5m NTT Operational,
visitor instrument
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ESO/Paranal

ESPRI / PRIMA Exoplanet Search with PRIma, the Differential Delay Line project for PRIMA (Phase-Referenced Imaging and Micro-arcsecond Astrometry) Differential delay lines installed in Sept. 2008, integration and tests of other subsystems in 2009, commissioning in 2010, to become operational in 2011
GRAVITY GRAVITY is an adaptive optics assisted near-infrared instrument for precision narrow-angle astrometry and interferometric phase referenced imaging of faint objects.
It will coherently combine all four beams from the VLT unit telescopes
Under development,
installation 2012
MATISSE Multi AperTure mid-Infrared SpectroScopic Experiment, a mid-infrared imaging spectro-interferometer for the VLTI Under development,
installation 2014
MIDI Mid-infrared Interferometric Instrument for VLTI Operational
NACO NAOS-CONICA adaptive optics system Operational
PARSEC PARSEC – the laser for the VLT Operational
SPHERE Spectroscopic and polarimetric
high-contrast exoplanet research, the VLT planet finder instrument
Under development,
installation 2011
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LBT

LBT-SW LBT Software Development MPIA contributed to this
project until mid-2009
LINC-NIRVANA LBT Interferometric Camera and Near-Infrared / Visible Adaptive Interferometer for Astronomy, an imaging beam combiner for the LBT Under development,
installation 2013
LUCIFER LBT NIR spectroscopic Utility with Camera and Integral-Field Unit for Extragalactic Research, two NIR spectrographs for the LBT LUCIFER1 operational since Dec. 2009.
Installation of LUCIFER2
in spring 2011
ARGOS Advanced Rayleigh guided Ground layer adaptive Optics System, the laser guide star system for the LBT Under development,
installation 2012
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WISE Observatory

LAIWO The Large Area Imager for the Wise Observatory Operational
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UKIRT

MAX Mid infrared Array eXpandible Decommissioned
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E-ELT

METIS Mid infrared E-ELT Imager and Spectrograph
METIS will provide AO supported diffraction limited direct imaging, low resolution longslit spectroscopy, high resolution IFU spectroscopy in the thermal infrared at 3 – 5.5 µm and 8 - 14 µm
Phase A study completed in Dec 2009
MICADO Multi-AO Imaging Camera for Deep Observations. Adaptive optics imaging camera that will provide diffraction limited imaging over a 1' × 1' field of view Phase A study completed in Dec 2009
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Responsible: Martin Kürster
Last updated: March, 31st, 2010