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 ...
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 ...
Institute codes can be found using the following pull-down menus. First look up the country corresponding to the affiliation of your Co-I(s) and then find the codes corresponding to your Co-I(s) ...
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 ...
The Wide Field Imager (WFI) is a focal reducer-type camera which is permanently mounted at the Cassegrain focus of the 2.2-m MPG/ESO telescope at La Silla. With field of view of 34'x33', Nyquist ...
alpha(2000) = 08h 43m 13.46s , delta(2000) = +03d 23' 55.1'' ...
The HAWAII 1024 x 1024 readout is structured in four independent quadrants having four outputs. Six CMOS-level clocks, two 5V power supplies (one analog and one digital), on e fixed dc bias and one ...
The M2 Unit is an opto mechanical system constituted by a convex hyperbolic Beryllium mirror ("M2 mirror"), by the electromechanism used tosupport the mirror and to control its position, and by the ...
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 ...
Several teams provide support in regard to ESO's telescopes and instruments, e.g. support for observing proposal preparation and submission, observation scheduling, data flow operation, information ...
This page contains information about the seeing on La Silla Observatory (ESO, Chile) as reported by the night assistants working in the 4 biggest telescopes (ESO NTT , ESO 3.60m , ESO/MPI 2.20m , ...
The 3.58-m New Technology Telescope (NTT) was the first in the world to have a computer-controled mirror ans ESO 3.6-m telescope.
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