The deadline for proposal submission for Period 110 (1 October 2022 - 31 March 2023) was 25 March, 2022. 871 valid proposals were submitted, including 33 Large Programmes. On the VLT the most requested ESO instrument was MUSE with a request of 449 nights, followed by X-Shooter with 258 nights. HARPS on the ESO 3.6-metre telescope was the most demanded instrument at La Silla (and fourth most demanded instrument overall), with 184 nights.

Following an incremental ramp-up plan, La Silla Paranal Observatory has been supporting science operations for all telescopes and systems over the past months. As of March 29, the Observatory moves one more step ahead, to the ‘Full Operations’ mode. This step lifts several of the limitations that have been present since the beginning of the Covid-19 pandemic, while still maintaining a basic set of sanitary restrictions on site. For science users the most important change is that as of June 2022 the observatory will again welcome visiting astronomers on site.

The latest edition of ESO's quarterly journal, The Messenger, is now available online. In this Issue 186 readers will find an article about the ongoing search for quiescent black holes, which has detected stripped stars instead. The issue continues with an overview of the ALMACAL project, describing this survey based on ALMA calibrator observations. Further, readers will be able to learn more about the processes that drive the evolution of isolated magnetic white dwarfs.

The next Science Operations workshop, SciOps 2022, is dedicated to Artificial Intelligence (AI) for science and operations in Astronomy and will take place in hybrid format on 16-20 May 2022 at the ESO Headquarters in Garching bei München and online. Building on the success of the previous series of similar events, this ESO/ESA workshop aims to facilitate the exchange of current developments and applications of AI-enabled technologies in science operations for space- and ground-based astronomical facilities.

On January 31 2022 the ESO Director General signed the agreement for the design and construction of the Cassegrain U-Band Efficient Spectrograph (CUBES), a very efficient, intermediate resolution spectrograph, that covers the UV region close to the atmospheric cutoff. The agreement was signed with Istituto Nazionale di Astrofisica (INAF), representing the consortium including INAF (Italy), the Science and Technology Facilities Council - UK Astronomy Technology Centre and Durham University (United Kingdom), Landessternwarte Heideberg (Germany), Nicolaus Copernicus Astronomy Center (Poland) and Instituto de Astronomia, Geofísica e Ciências Atmosféricas-Universidade de São Paulo and Laboratório Nacional de Astrofísica (Brazil).

The Users Committee (UC) represents ESO's astronomical community at large and acts as an advisory body to the ESO Director General on matters related to the performance, scientific access, operation and user interfaces to the La Silla Paranal Observatory and ALMA. The annual meeting of the UC is scheduled on 28 and 29 April 2022. During the UC meeting updates from ESO and feedback from the user community are exchanged and openly discussed. Each year one topic is explored in more detail and this year the Special Topic session is dedicated to future of Visitor Mode and remote participation in observations. The UC welcomes input, opinions and suggestions from the community either through direct contact with the UC members or through the Poll designed by the UC.

VISIONS (programme id 198.C-2009, PI J. Alves) is a Near-Infrared ESO second cycle VISTA Public Survey which covers all major nearby star-forming regions accessible from the southern hemisphere. This imaging survey is designed to deliver deep high-sensitivity observations of areas with large amounts of extinction. It includes also control fields which sample the predominant stellar populations in largely extinction-free regions and multiple epochs imaging data over large areas surrounding the targeted star-forming regions to enable the computation of proper motions for sources inaccessible to Gaia.

ANDES is the new name for the high-resolution spectrograph, formerly known as HIRES, for the Extremely Large Telescope (ELT). Another instrument dubbed HIRES is successfully operating on the Keck telescope, so it was decided to rename the ELT spectrograph. Through an open process, the consortium — in consultation with the ESO follow-up team — has decided on "ArmazoNes high Dispersion Echelle Spectrograph", or ANDES. The official start of both ANDES and MOSAIC as two more ELT instrument projects was approved by the ESO Council in December last year.

The Solar System Science with the ELTs conference will focus on ESO’s ELT unique capabilities to address the open questions in the diverse subfields of Solar System science. Special emphasis will be put on how the ELT, alongside with the GMT and TMT, will fit in the rich landscape of ground- and space-based telescopes, in particular with the current and future ESA missions.

The Call for Proposals for observations at ESO telescopes in Period 110 (1 October 2022 - 31 March 2023) has been released. Please consult the Period 110 document for the main news items and policies related to applying for time on ESO telescopes. All technical information about the offered instruments and facilities is contained on ESO webpages that are linked from the Call. The proposal submission deadline is 12:00 CET 25 March 2022.