The ESO Science Newsletter is intended to keep the community informed about current activities of interest at ESO. The newsletter appears roughly every two to three months or whenever important news ...
MATISSE is a four-telescope beam combination instrument operating in the L (between 3.2 and 3.9 μm), M (between 4.5 and 5.0 μm), and N (between 8.0 and 13.0 μm) bands. It operates in a spectroimaging ...
All documents and other files linked from this page and highlighted by a red bullet have an internal access only because we need to know who has the documents so we can send updates as necessary. If ...
E-ELT PUBLICATIONS AND DOCUMENTATION Project documents E-ELT Top Level Requirements Observatory Instruments ELT-CAM (now MICADO) ELT-IFU (now HARMONI) ELT-MIDIR (now METIS) ELT-HIRES (now ANDES) ...
The telescope structure is an alt-az mount (see Figure 1) and it is divided into two main parts: the Azimuth Structure and the Altitude Structure. The main structure, including the hosted units and ...
Technology development and R&D are vital activities at ESO to making our vision and mission possible. We aim to develop and secure key technologies which will keep our facilities at the forefront of ...
The procedures for obtaining flat fields are described in greater detail elsewhere (follow the links under the different spectroscopic modes). The different types of flat fields used for spectroscopy ...
The complete adapter-rotator units comprise two major subsystems:the opto-mechanical part and the control system. The Opto-Mechanicalpart consists of five main sub-components: The Large Structure The ...
The FEROS instrument is a state-of-the-art bench-mounted, high-resolution, environmentally controlled, astronomical Échelle spectrograph. It is opertated at the European Southern Observatory (ESO) in ...
Instrument Science Team: Fernando Comeron (ESO, Chair), Stephane Charlot (IAP), Andrea Cimatti(Bologna), Jean-Paul Kneib (OAMP), Konrad Kuijken (Leiden) Within the next few years photometric redshifts ...
ESO's mission is to provide its astronomical community with worldwide competitive ground-based observing capabilities to probe the Universe from its first billion year to the present time. In order to ...
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