Posters should be prepared in A0 format (i.e. 841 × 1189 mm or 33.11 × 46.81 inches), in portrait layout. An electronic version of each poster will be uploaded to the workshop’s Slack channel. The ...

In general, a finding chart has to be attached to each OB. Exceptions are possible for some instruments, in which case this is specified in the instrument-specific rules, which can be found by ...

ALMA provides unique and spectacular results in a large variety of scientific themes (e.g. results obtained during the long baseline campaign) while completion of the ALMA baseline capabilities is ...

To facilitate the organisation of the conference, ESO requires a set of personal data from each participant. This data will be processed solely for the purpose of organising the workshop and will not ...

To ensure the observing efficiency and flexibility of Service Mode observing, ESO has implemented a number of rules, procedures and limitations on programmes scheduled for Service mode. Typically, ...

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 ...

The field of view in imaging mode consists in 4 quadrants of 7' x 8' each, separated by a cross 2' wide. Note that there is some slight vignetting on 2 corners along the 8' direction. The CCD size in ...

It might happen that one or more arms are not available for allocation due to technical problems for a certain period of time. This information is posted under 'Timeline of instrument status' on the ...

The expected Paranal Instrumentation and Facilities to be offered in Period of the call and changes foreseen for the following two periods are presented at the overview page.

The Science Verification observations are part of a very important check of the entire operational procedures and a verification of the scientific status of the VISTA telescope and camera. Furthermore ...

There is currently no agreed plan for making the frequency range 67GHz to 84GHz available with ALMA. This frequency range is particularly significant for studies of the deuterium chemistry which probe ...

This proposal addresses suggested in the “ALMA 2030 Roadmap” document call for “Larger bandwidths and better receiver sensitivity”. The reasons and justification for a wider IF band and improved noise ...