Instrumentation

The tiny signals from exoplanet atmospheres are an enormous challenge to observe – the planet’s atmosphere typically contributes less than 0.01% of the total brightness of the system. Purpose-built instruments, constructed with this challenge in mind, open the door to new investigations. By pushing towards higher contrast measurements, improved sensitivity, and broader wavelength coverage, it will be possible to study many previously inaccessible planets (including smaller and cooler worlds closer in properties to our Earth).

Artist depiction of the METIS instrument set to be used with the Extremely Large Telescope upon completion. METIS, short for Mid-infrared ELT Imager and Spectrograph, will make full use of the giant main mirror of the telescope to study a wide range of science topics, including exoplanet atmosphere characterization and low and high spectral resolution.

ESO/METIS Consortium/L. Calçada

Artist depiction of the METIS instrument set to be used with the Extremely Large Telescope upon completion. METIS, short for Mid-infrared ELT Imager and Spectrograph, will make full use of the giant main mirror of the telescope to study a wide range of science topics, including exoplanet atmosphere characterization and low and high spectral resolution.

ESO/METIS Consortium/L. Calçada

The APEx Department is involved in several instrumentation projects, in collaboration with the MPIA Technical Departments. These include:

VLTI/GRAVITY+: an upgrade to the GRAVITY K-band interferometry instrument, expected to improve the sensitivity for exoplanet observations by a factor of 5-10
ELT/METIS: an ELT first light instrument focused on high contrast imaging and high-resolution spectroscopy in the mid-infrared
ELT/ANDES: an ELT second light instrument capable of high-resolution spectroscopy in the optical and near-infrared