Rome, Italy, 9–13 September 2019 

Over the next decade, the commissioning of ESO’s Extremely Large Telescope (ELT), as well as of the GMT and TMT will allow us to see the high-redshift Universe using new "eyes" with unprecedented power. By themselves or in combination with other facilities, these new eyes will have the potential to transform our understanding of the formation and early evolution of galaxies and black holes, first light and cosmic reionisation, as well as the evolution of the intergalactic and circumgalactic media. This conference will bring together an international group of experts to review the current state of the art in the study of the high-redshift universe and discuss how best to use giant telescopes to learn about it.  

ESO, Garching, Germany, 9–13 September 2019 

More than 60 years ago, the Magellanic Clouds provided crucial impetus for the construction of large telescopes in the Southern hemisphere and the foundation of ESO. This workshop will provide a fertile forum for shaping the future of research related to the Magellanic Clouds by showcasing state-of-the-art results based on advanced observational programmes as well as discussions of expectations and projections in anticipation of highly multiplexed wide-field spectroscopic surveys (e.g., 4MOST, MOONS) which will come online in the 2020s. This conference also marks the quincentenary of Ferdinand Magellan's arrival in the southern hemisphere during his circumnavigation of the Earth. Very recently, in 2018, there was also Henrietta Leavitt's 150th birthday and the 110th anniversary of her discovery of the period-luminosity relation among Magellanic Cloud Cepheids.

Gothenburg, Sweden, 7–11 October 2019 

The 8th European Radio Interferometry School (ERIS) at Gothenberg will provide a week of lectures and tutorials on how to achieve scientific results from radio interferometry. Please register via the school website by 3 May. The topics covered by the lectures/tutorials will include the following:

• Calibration and imaging of continuum, spectral line, and polarisation data.
• Observing techniques for low frequencies (e.g., LOFAR), intermediate frequencies (e.g., VLA and e-MERLIN), high frequencies (e.g., ALMA and NOEMA), and VLBI (e.g., EVN).
• Extracting the information from astronomical data and interpreting the results.
• Choosing the most suitable array and observing plan for your project.  

ESO, Garching, Germany, 16–19 September 2019 

At the turn of this decade, a number of moderate-sized telescopes were equipped with digital cameras of around 10 square degrees. The relative cost of detectors and computing had reduced to a level where rapid, real-time processing of the imaging data provided monitoring of large sky areas every few days. This revolutionised the field of time domain astronomical surveys and we have witnessed a vast array of new discoveries.  The global community have mapped the solar system, star forming regions in our galaxy, local group galaxies, and the local and high-redshift Universe leading to the discovery of new types of transients. We have discovered low luminosity stellar explosions in nearby galaxies and the most luminous supernovae beyond a redshift of 3, exotic transients in the nuclei of galaxies including tidal disruption events, stellar mergers, unusual novae and previously unknown species of stellar outbursts. The diversity in the explosive Universe is remarkable.

Cagliari, Italy 14–18 October 2019

Registration has now opened for the next ALMA-wide science conference and the list of invited speakers has been published at the meeting website.
ALMA is the world’s most sensitive facility for millimetre/submillimetre astronomical observations, and will soon be fully operational in all of the originally planned bands. Since its first observations, ALMA has routinely delivered groundbreaking scientific results that span nearly all areas of astrophysics. Science topics at this conference will include all fields of astronomy, from cosmology and galaxies in the distant Universe, nearby galaxies and the Galactic Center, interstellar medium and star formation in our Galaxy, astrochemistry, circumstellar disks, exoplanets, solar system, stellar evolution, and the Sun. As in previous editions of the conference series, we expect to discuss the scientific priorities for the implementation of the ALMA Development Roadmap.

ESAC, Madrid, Spain, 19–22 November 2019 

ESA/ESO SCIOPS WORKSHOP 2019 – Working Together in Support of Science – Cross Facilities Collaboration in the Multi Messenger Era

The upcoming ESA/ESO SCIOPS 2019 Workshop will take place at ESAC and will address the following areas:

• collaboration between large scientific teams in the multi-messenger era;
• how space- and ground-based observatories communicate their transient and observational capabilities, and can prepare and adapt them to provide scientists with access to time and data for multi-messenger programmes;
• cultural and policy changes needed to enable multi-facility time allocation, prioritisation of observations, publication of information on upcoming observations and data sharing;
• tools, services and standards to support coordination between facilities for the selection and publication of targets by survey facilities, coordination and publication of follow-up observations among observatories, as well as for publishing, searching, analysing and visualising data;
• tools and services to support collaboration between teams.
  
  

The ESO Archive Science Portal (ASP) provides the primary entry point for interactive searching and browsing of the ESO Science Archive in terms of processed datasets. Until recently, the ASP supported searching for only one target at a time. Because many users have requested it, the possibility of searching by a user-provided list of targets has now been added. In the first implementation of this feature the list may contain up to 1000 target names or coordinates (J2000 or Galactic). The power of the existing graphical user interface remains fully available in the list search mode, including the option of adding and adjusting any of the seventeen non-positional search parameters. The new software release also features a refurbished download menu to accommodate downloading the results of the list search and it includes several bug fixes.

The annual public release of ESO VLT/VLTI instruments data reduction software packages is scheduled for the end of May 2019. Please note that the new pipeline packages will be released for the following operating systems: Fedora 26–29, CentOS 7, Scientific Linux 7 and macOS 10.11–10.14. In addition to the release of data reduction pipelines in May, some instruments with pipelines under active development have intermediate releases throughout the year. To get announcements of new pipeline releases, please send an e-mail or visit the VLT Instrument Pipelines webpage.

The ESO Phase 2 Proposal Preparation version 3 (P2PP3) software used for the preparation of observations with the Paranal telescopes has now been officially decommissioned. Since Period 102, P2PP3 has been replaced by the p2 web application. Users can familiarise themselves with the application using the p2 demo site, and also test programmatic preparation of observations using the Phase 2 Application Programming Interface (API) (p2API). If you have developed a script or utility that makes use of the p2API, and you would like to share it please read the API contributed software webpage and e-mail the User Support Department.  

The ALMA Cycle 7 Call for Proposals for scientific observations is open for submissions. ALMA Cycle 7 is currently scheduled from October 2019 to September 2020. Users of any nationality or affiliation are invited to to submit proposals before the deadline at 15:00 UT on 17 April 2019. It is anticipated that 4300 hours will be available on the 12-metre array time and 3750 hours on the Atacama Compact Array (ACA) (also known as the Morita Array), including a supplementary call. Proposals must be prepared and submitted using the ALMA Observing Tool (OT), which is available for download from the ALMA Science Portal. Proposals will be assessed by competitive peer review by a single international review committee.