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 ...

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 ...

Garching lies about 13 km north-east of Munich and 17 km south-west of Munich international airport (Franz Josef Strauss). Please follow these instructions to travel to Garching. To consult the time ...

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 ...

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 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 ...

The ESO Paranal Observatory is located in one of the darkest sky regions available for observational astronomy. This page includes information reagrding the Natural Sky Brightness of the site under ...

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 ...

This list contains the suitable spectrophotometric calibrators whichshould be used to calibrate the correlated flux of the targets observedwith MIDI. The entries are shared elements between the MIDI ...