Following the first two of three workshops intended to promote upgrades that will realize the ALMA 2030 vision, it is planned to complete the workshop trilogy with an ALMA Front-End Development Workshop, entitled “The ALMA 2030 Vision: A next generation of front-end receivers”. This workshop will be held online the week of September 27-30 (inclusive), 2021.

ALMA is very pleased to share the positive news that science observations re-started on 17 March 2021. These were the first Cycle 7 data to be acquired since the Observatory shutdown, due to the Covid-19 pandemic, in March 2020. The first newly-acquired datasets have now been calibrated and imaged, and have successfully passed the ALMA quality assurance stages.

The ALMA Director, on behalf of the Joint ALMA Observatory (JAO) and the partner organizations in East Asia, Europe, and North America, is pleased to announce the ALMA Cycle 8 2021 Call for Proposals (CfP) for scientific observations to be scheduled from October 2021 to September 2022. More details can be found on the ALMA Science Portal.

The annual public release of ESO VLT/VLTI instruments data reduction software packages is scheduled for end of May 2021. Please note that the new pipeline packages will be released for the following operating systems: Fedora 28 – 32, CentOS 7 and macOS 10.14 – 10.15. ESO is working toward full support for macOS 11, but for the time being it is not possible to say when MacPorts binary packages for the pipelines on macOS 11 will be provided. Nevertheless, the use of MacPorts is recommended as opposed to installing from install_esoreflex script. Using MacPorts the pipelines will build and install from source in macOS 11, thus installations will take a bit longer than for those OS versions that are supported with binary packages.

The Offices for Science and the Astronomy Faculty are very pleased to present the 2021 ESO Fellows. Here is an introduction to the Fellows due to start in Germany and Chile later this year.

The 4th Azores School on Observational Cosmology will take place in Angra do Heroísmo (Terceira Island, Portugal) from 6 to 12 September 2021. The school is jointly organized by CAUP/IA, ESO and University of Azores, and the topic for this edition will be 'Fundamental cosmology from the ELT and space'. Should the COVID-19 situation make an in-person school impossible in September, the school will be online.

A new release of the Public ESO Spectroscopic Survey for Transient Objects (PESSTO) is available, including spectra and images from its ePESSTO extension, and the delivery of a new transient catalogue, globally covering 7 years of observations, from April 2012 to April 2019, for a total of 45 GB. This new release brings to 2323 the number of observed supernovae and optical transients, with calibrated 1D spectra for 2314 of them, doubling the number of objects previously published (1168 in the previous version).   

Astronet is a consortium of European funding agencies, established for the purpose of providing advice on long-term planning and development of European Astronomy. Astronet is now developing a new Science Vision & Infrastructure Roadmap with an outlook for the next 20 years. A delivery date to European funding agencies of mid-2021 is anticipated. After some delays due to the global pandemic, the first drafts of the chapters for the document are now available from the Panels asked to draft them, and input by the Eurpean astronomy and space science community as possible is very welcome.   

The INSPIRE project is an ESO Large Programme (ID: 1104.B- 0370, PI: C. Spiniello) which uses X-Shooter (in UVB, VIS, NIR band) to spectroscopically follow up 52 red ultra Compact Massive Galaxies selected from the KiDS VST ESO Public Survey. The goals of INSPIRE (Spiniello et al. 2021a, Spiniello et al. 2021b) is to obtain the first catalogue of spectroscopically confirmed relics in the redshift range 0.1<z<0.5, bridge the gap between the three local confirmed relics and the high-z red nuggets, use the final statistic on confirmed relics to put a stringent constraint on the predictions from simulations on the initial burst of star formation in galaxies.

The VISTA EXtension to Auxiliary Surveys (VEXAS, Spiniello & Agnello, 2019, A&A, 630) project aims at building wide and spatially homogeneous multi-wavelength catalogues (from X- ray to radio) providing reference magnitudes, colors and morphological information for a large number of scientific uses. Currently the VEXAS catalogue is the widest and deepest public optical-to-IR photometric and spectroscopic database in the Southern Hemisphere, comprising more than 90 million objects with reliable photometry measured in at least one of the VISTA infrared bands, two of the WISE bands and three optical bands.