The Joint ALMA Observatory (JAO) will start Cycle 10 observations in October 2023. A Call for Proposals (CfP) with detailed information on Cycle 10 is anticipated to be issued in April 2023 and the deadline for proposal submission is anticipated to be on 10 May 2023.  The purpose of this pre-announcement is to highlight aspects of the CfP to assist with early planning.

The European Interferometry Initiative (EII) is announcing that registrations are now open for the 11th VLTI School, funded by the Opticon/Radionet Pilot programme, with support from ESO.

The number of participants is limited to a maximum of 50. There is no registration fee. Limited funding will be available for accommodation and travel.

Applications for funding before March 1, 2023, will receive full consideration pending on merit and available budget.

The Fornax3D survey is an integral field spectroscopic survey of the Fornax cluster of galaxies. This new data release contains mosaiced IFS MUSE cubes with their white lamp images for the 31 galaxies brighter than m_B=15 within the virial radius of the cluster. The total data volume is 121.5 Gb. The survey was conducted under the ESO programme 296.B-5054(A), PI M. Sarzi and E. Iodice, with MUSE at the ESO VLT in wide-field mode. This instrument configuration ensures a spatial sampling of 0.2×0.2 arcsec², a wavelength coverage from 4650 to 9300 Å with a spectral sampling of 1.25 Å/pixel, and a nominal spectral resolution of FWHM = 2.5 Å at 7000 Å. The main science goals of the survey are to understand the assembly history of the Fornax cluster and of the early-type galaxies, study the formation of substructures in galaxies and the properties of globular cluster and planetary nebulae population. For more information on the background and goals, please consult the latest paper by Sarzi, Iodice et al. in The Messenger.

The ESO Telescope Bibliography (telbib) is a database of refereed papers that uses data from ESO’s observing facilities. Telbib is used to compute the Basic ESO Publication Statistics (PubStats), now available on a dedicated webpage. 

Publication statistics are available for ESO in general, and for the VLT, VLTI, and Survey telescopes, La Silla facilities, APEX, and ALMA. The use of archival data in ESO data papers is dealt with in a dedicated section. Furthermore, a comparison with the output from other major observatories is provided. 

The latest edition of ESO’s science and technology journal, The Messenger, is now available online. Issue 189 features a summary of the science results of the ALMA large programme ATOMIUM, describing how ALMA has been used to trace the origins of molecules in dust forming oxygen-rich M-type stars. Summary of the science results and upcoming data release of the Fornax3D project, which is a magnitude-limited study of galaxies in the Fornax Cluster with VLT/MUSE, can also be found. 

With the aim of taking full advantage of the complementarity of optical-NIR and sub-millimetre observing facilities, ESO and ALMA have entered into a Joint Proposal agreement, to enable those science cases that require observations with both ALMA and VLT(I) telescopes to have their goals fulfilled.

In this framework, ESO is glad to announce that Joint VLT-ALMA Proposals will be offered as of Period 112 and ALMA Cycle 10, with the formal ESO call to be published at the end of February 2023. By agreement with the ALMA Observatory, ESO may award a maximum of 50 hours of ALMA observing time on each of its arrays to Joint Proposals per year. Similarly, ALMA will be able to allocate up to 50 hours per cycle on the VLT(I) in the yearly ALMA Call for Proposals.

ALMA has resumed performing PI science observations following the cyber-attack. The end-to-end data acquisition and processing workflow and software were successfully re-tested prior to the restart. ALMA is currently taking observations in configuration C-3. User services are also now back online, including access to ALMA user profiles, SnooPI, and the Cycle 9 DDT submission server. As previously announced, ALMA’s most compact configurations (C-1 and C-2) will not be visited again in Cycle 9.

Some Scheduling Blocks (SBs) requiring configuration C-2 were already observed in the days prior to the cyber-attack. Projects with SBs in nominal configurations C-1 and C-2 that can still be observed in configuration C-3 will remain in the observing queue. As per usual ALMA policy, incomplete Cycle 9 Grade A projects will carry over into Cycle 10.

Regarding Cycle 10, due to the disruption caused by the cyber-attack, the Cycle 10 pre-announcement will now be issued in the week of 16^th January.

For any comments or concerns, please contact your local ALMA Regional Centre (ARC) via the ALMA Helpdesk at https://help.almascience.org/.

This collection provides wide-field spectral line imaging data cubes (5 cubes, total volume: 11.50Gb) of the Orion A and B giant molecular clouds in the 12CO (J=3-2) line at a frequency of 345.795990 GHz from observations collected under ESO programme 094.C-0935(A), PI: T. Stanke, and the Swedish programme 094.F-9343. The data were obtained using the SuperCAM 64-pixel heterodyne array camera at the APEX telescope in December 2014. The cubes cover a total area of ~2.7 deg² in the Orion A and B giant molecular clouds. The frequency axis includes the full spectral extent of the CO line detected in the area, including high-velocity line wings from protostellar molecular outflows. The data reveal a wealth of cloud structures and allow for an unbiased search for protostellar molecular outflows over a large portion of a star-forming cloud. A full presentation of the survey overview and data was published in Stanke et al. (2022, A&A 658, A178).

SPHERE (Spectro-Polarimetric High-contrast Exoplanet REsearch) is an extreme adaptive optics system and coronagraphic facility feeding three science instruments: IRDIS, IFS, and ZIMPOL. The primary science goal of SPHERE is imaging, low-resolution spectroscopic, and polarimetric characterisation of extra-solar planetary systems. IRDIS, the infrared dual-band imager and spectrograph, provides classical imaging (CI), dual-band imaging (DBI), dual-polarisation imaging (DPI), and long-slit spectroscopy (LSS) between 0.95 – 2.3 µm.

The first data release covers 602 IRDIS imaging observations acquired between April 2019 and March 2020, i.e., ESO periods P103 and P104. The data were processed by the SPHERE Data Centre, a support service provided by the French community, which is jointly operated by OSUG/IPAG (Grenoble), PYTHEAS/LAM/CESAM (Marseille), OCA/Lagrange (Nice, France), Observatoire de Paris/LESIA (Paris), and Observatoire de Lyon.

After the great success of the programme in the last four editions, we are happy to announce that the call for applications for the 5^th ESO Summer Research Programme is now open. The fully-funded programme is open to all university students not yet enrolled in a PhD course.

Seven projects spanning a variety of topics are offered this year and successful applicants will be invited to work at the ESO Headquarters in Garching for six weeks between July 3 and August 11, 2023. 

Applicants should apply online using the dedicated form before the deadline of 31 January 2023, 23:59 CET.