PIONIER is a H-band 4-beam combiner instrument at the VLT interferometer. It is originally a visitor instrument that by agreement with IPAG is offered to the ESO community from P96 onwards as a ...
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 ...
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) ...
We list on this page the topics offered by ESO Faculty astronomers to the students interested in the ESO Studentship programme. The deadline to apply for the ESO Studentship is April 20th and October ...
Ephemeris files compatible with observations at the VLT can easily be generated using our online form. For reference, we detail here the format specifications for such files, and we provide links to ...
Please find a list of arc lines in the following table. There is noguaranty for the accuracy of the wavelengths. The optimum choice of lines will depend on the spectral resolution of the grisms and ...
Revealing hidden stars and galaxies: new MOONS instrument at the Very Large Telescope makes first observations ...
Experience spring at ESO's Paranal Observatory: slots now open for free public tours from October through December ...
The 2.2m telescope at La Silla has been in operation since early 1984 and is on indefinite loan to ESO from the Max Planck Gesellschaft. The telescope time is shared between the MPI and ESO Observers.
VISTA (Visible and Infrared Survey Telescope for Astronomy) is a 4-m class specialized wide field survey telescope for the southern hemisphere, equipped with a near infrared camera VIRCAM (VISTA ...
The staff at the ESO ARC provide support to the European users and to the science operations of the ALMA observatory. User support is provided together with the staff in the nodes within the European ...
HARPS is the ESO facility for the measurement of radial velocities with the highest accuracy currently available. It is fibre-fed by the Cassegrain focus of the 3.6m telescope in La Silla. The ...