In this page, you will find all the manuals needed to prepare and analyze your observations with MIDI. Please be sure todownload that corresponding to the period in ...

GRAVITY is not a monolithic instrument. It is a collection of sub-systems that aims to precisely control the wavefront of the incoming light and its path through the VLTI system before the actual ...

On Tuesday and Wednesday you will be given the opportunity to deliver a flash presentation of your poster during the poster session. Each presentation will have a duration of two minutes. Please, save ...

MUSE is an Integral Field Spectrograph. It splits the field of view into 24 image segments or channels which are further sliced into 48 slices or mini slits, giving a total of 1152 mini slits. Each ...

The VISIR performance estimates listed on this page are based on observations of mid-infrared calibration standard stars. Sensitivities have not changed much with the relocation of VISIR from UT3 ...

All the information about the instrument itself, its modes and their characteristics. Since Period 114, to be used for Phase I and Phase II preparation. (no changed wrt to P113) Also valid in ...

ESO is committed to creating a work environment that is safe, professional and of mutual trust where diversity and inclusion are valued, and where everyone is entitled to be treated with courtesy and ...

AMBER is a spectro-interferometric instrument for the VLTI working in the near-infrared. It is offered in the H-band and K-band. The instrument combines and disperses three beams arriving from three ...

The submission of the Phase 2 package for approved Director's Discretionary Time (DDT) Proposals must follow the same procedure as regular programmes, described in the Instructions for Phase 2 ...

NIRPS, the Near Infra-Red Planet Searcher at the ESO La Silla 3.6m telescope is dedicated to the discovery and characterization of extrasolar planets. Like HARPS is a fibre-fed, high-resolution, cross ...

The Phase Referenced Imaging and Micro-arcsecond Astrometry (PRIMA)project is currently being developed by the European Southern Observatory (ESO) and being installed on the Very Large Telescope ...

The ESO Users Committee (UC) is made of representatives of the ESO users in each member state and includes also a representative from Australia and the host country Chile. It advises the ESO Director ...