The annual public release of ESO VLT/VLTI instruments data reduction software packages is scheduled for the beginning of June 2020. Please note that the new pipeline packages will be released for the following operating systems: Fedora 28-31, CentOS 7 and macOS 10.11–10.14. For macOS version 10.15 we recommend using MacPorts. We expect pipelines will build and install from source in macOS 10.15, thus installations will take a bit longer than for those OS versions that are supported with binary packages. We are working toward full support for macOS 10.15, but for the time being we cannot say when we will provide MacPorts packages for the pipelines on 10.15.

Given ongoing developments related to the COVID-19 pandemic, ESO is doing its best to guarantee that the proposal submission and review processes remain optimal within the restrictions imposed by this crisis. Since containment measures deployed in some of ESO’s Member States have disrupted scientific activities in those countries, the proposal submission deadline has been postponed from 26 March to 23 April 12:00 CEST. ESO will continue to follow developments closely and may provide additional updates regarding Phase 1 in the next weeks.

The ALMA Director, on behalf of the Joint ALMA Observatory and the partner organisations in East Asia, Europe, and North America, is pleased to announce that the ALMA Cycle 8 Call for Proposals for scientific observations opened on March 17. Users of any nationality or affiliation are invited to submit proposals. Please note that, due to the COVID-19 pandemic, the original deadline of 15:00 UT on 15 April 2020 has now been delayed to no earlier than 15:00 UT on 19 May 2020. As ALMA continues to monitor the conditions worldwide, it will assess the feasibility of this deadline and provide additional updates to the community as needed. The next update to the community will be provided no later than 21 April 2020 on the status of the call and the support for the scientific community.

In response to the rapidly evolving COVID-19 pandemic around the world ESO has been following the measures adopted by governments in Germany and Chile and closely observing the situation in other countries. Our highest priority remains the safety and wellbeing of all staff and visitors at ESO’s sites. To minimise the risk of infection the presence of staff has been significantly reduced at the observatories over the past week leading to a number of restrictions to the ongoing science operation. Over the coming weekend, the staff at the observatories will be further reduced to the minimal teams required to ensure the safety of the facilities and the remaining people on site.

As a consequence science operation will cease at all sites.

Due to the COVID-19 outbreak that has spread to Chile, the ALMA Director has made the decision to suspend science operations with ALMA, effective immediately. This decision has been taken to protect the safety of ALMA staff, many of whom travel long distances by bus and by plane to reach the remote ALMA site in the Atacama Desert in northern Chile.

ALMA is strongly committed to ensure that the proposal review process is as fair and impartial as possible. Analysis of the proposal rankings in previous cycles has identified systematics that may signify the presence of biases in the review process (see Systematics in the ALMA Proposal Review Rankings). In an effort to reduce biases as much as possible, ALMA will use a dual-anonymous proposal review process starting in Cycle 8.

Due to recent developments related to SOXS at the NTT, Large Programme proposals will be accepted in Period 106 for SOFI runs in Period 106 and for EFOSC2 runs in Periods 106 and 107. Users should be aware, however, that these programmes may be terminated ahead of the expected time, depending on the progress with SOXS. This will be reviewed again ahead of the release of the Period 108 Call for Proposals.

ESO Garching, Germany, 12–16 October 2020 

Following the spread of COVID-19 (the coronavirus), this workshop has been postponed from April to October and registration has been re-opened. All participants who registered for the original workshop should register again to confirm their attendance in October. More information about the workshop itself can be found below and via the workshop website.

The VISTA Kilo-degree Infrared Galaxy Public Survey (VIKING, ESO Programme ID: 179.A-2005, PIs: A. Edge and W. Sutherland) is a wide area (covering a final area of 1350 square degrees), intermediate-depth (5-sigma detection limit J~21 on Vega system) near-infrared imaging survey, in the five broadband filters Z, Y, J, H, Ks. The sky coverage has maximum overlap with the Kilo-Degree Survey KiDS in the optical bands. This fourth and final VIKING data release covers all of the highest quality data taken during the survey to its completion and, when combined with the first three releases, includes all fields that met the team’s quality control thresholds in seeing (< 1.3”) and atmospheric transmission (thin cirrus or clearer).

The VISTA Hemisphere Survey (VHS, ESO Programme ID: 79.A-2010, PI R. McMahon) is a wide-area, multi-band, near-infrared survey, which when combined with other VISTA public surveys, will result in the coverage of the whole southern celestial hemisphere (declination < 0; 20 000 square degrees), to a depth 30 times fainter than 2MASS/DENIS in at least two filters (J and Ks), with a minimum exposure time of 60 seconds per filter and a median 5-sigma point source depth of AB = 20.8 and 20.0 in J and Ks filters respectively.