ESO telescope bibliography (telbib) records were recently enhanced to provide more comprehensive access to data products in the ESO Science Archive. All telbib records are linked to raw data of the Programme IDs used in the research as before. In addition, the library has identified all programmes for which data products exist in the Archive. If data products are available, an additional link is displayed, providing direct access. A script is run regularly to identify new Programme IDs in telbib records for which data products have become available, as well as new data products for existing Programme IDs.  

The User Support Department (USD) extends its thanks to all those Principal Investigators and their Phase 2 delegates who filled in this September's online Paranal Service Mode User Satisfaction Survey. A total of 185 responses were received from our targeted campaign. As in the past, where possible, we have contacted those respondents who provided detailed comments. A summary report based on this latest User Satisfaction Survey is now available.

The Next Generation Transit Survey (NGTS) is a ground-based exoplanet survey designed to detect Neptune and super-Earth sized planets orbiting around bright stars, using the transit method. The NGTS facility consists of 12 fully-robotic 20-cm f/2.8 telescopes located on ESO ground in Paranal. Each telescope has a 2.8 x 2.8 deg² field of view and is equipped with a custom filter with a bandpass of 520-890 nm, which increases sensitivity to late-K and early-M stars.

This data release provides 1D spectra of 103 individual afterglows that were observed with the X-shooter spectrograph within 48 hours of the GRB trigger. The data release includes a few late-time host observations also for completeness. The total collection of spectra represents all GRB afterglows that have been followed up with XSHOOTER before 31 March 2017. This date marks the end of the XS-GRB legacy follow-up programme. Redshifts have been measured for 97% of these sources, covering a redshift range from 0.059 to 7.84, hence this dataset provides a unique resource to study the ISM across cosmic time.

The ESO research studentship programme provides an outstanding opportunity for PhD students to experience the exciting scientific environment at one of the world's leading observatories. ESO's studentship positions are open to students enrolled in a university PhD programme in astronomy or related fields. Students accepted into the programme work on their doctoral project under the formal supervision of their home university, but they come to ESO to work and study under the co-supervision of an ESO staff astronomer for a period of between one and two years.

The deadline for proposal submission for Period 103 (1 April 2019 - 30 September 2019) was 27 September, 2018. 914 valid proposals were submitted, including 20 Large Programmes, of which one is a GTO Large Programme. The number of proposals for Period 103 is very similar to that of Periods 91 (893), 92 (892), 93 (898), 94 (901), 98 (901), 99 (887), 100 (895), 101 (899) and 102 (916) so the plateau observed since peaks in Periods 95 (934), 96 (960) and 97 (1024) remains. On the VLT the most requested ESO instrument was X-shooter with 258 nights, followed by MUSE with 226 nights, and FORS2 with 145 nights. HARPS on the ESO 3.6-metre was the most demanded instrument at La Silla, with a request of 190 nights, though the combined request on the NTT was larger (246 nights).

The response to our call for volunteers for the Distributed Peer Review (DPR) experiment was very enthusiastic, well beyond our original expectations. Out of the 272 scientists that had initially expressed their interest, 172 (63%) submitted a proposal for Period 103 as Principal Investigators (PIs) and will hence serve as reviewers. This corresponds to about 23% of all PIs in Period 103. This is also a reminder that the DPR process will run in parallel to the regular proposal review by the Observing Programmes Committee and will have no effect on the final ranking of the proposals.

ESO wishes to warmly thank its community for the enthusiastic response and collaborative spirit, which will ensure the success of the experiment! An in-depth analysis of the experiment and its results will be presented in due course.

The latest edition of ESO's quarterly journal, The Messenger, is now available online. In issue 173 you will find information about Service Mode and Visitor Mode at Paranal, as well as new plans for proposal submission and selection. This issue also contains several articles presenting science highlights from ESO and ALMA facilities, news from ESO fellows and students, reports from workshops, and a tribute to Leon Lucy.

ESO, Garching, Germany, 6–8 May 2019

4MOST is a state-of-the-art, high-multiplex, optical spectroscopic survey facility currently under construction for ESO’s 4-metre VISTA telescope. During the first five years of operations 4MOST will be used to execute a comprehensive programme of both Galactic and extragalactic Public Surveys, and 30% of the observing time during this period will be available to the community. The process of selecting Community Public Surveys will be initiated by a Call for Letters of Intent for Public Spectroscopic Surveys, to be issued by ESO in mid-2019. In preparation of this Call, ESO and the 4MOST Consortium are jointly organising a workshop to prepare the ESO community for this exciting scientific opportunity, to assist potential PIs in successfully responding to the Call, and to foster scientific collaborations between the community and the 4MOST Consortium.

ESO, Garching, Germany, 17–21 June 2019  

The VLT provides a powerful suite of visible and infrared instruments, including unique capabilities like coherent and incoherent combinations of the four 8-metre Unit Telescopes and a multi-laser guided adaptive optics system.  In combination with ALMA, it represents comprehensive coverage across  the full parameter space encompassing ground-based observations in visible, infrared and sub-mm wavelengths. With the advent of ESO's Extremely Large Telescope (ELT) the VLT will take on a new role. It will still serve a large community and will continue to provide unique data. Its strengths will include a suite of versatile instrumentation on four 8-metre telescopes, the spatial resolution achievable by interferometry and a flexible operational model. The VLT, VLTI and the instrumentation have been maintained at peak performance and new capabilities have been developed.

A discussion of future science served by the VLT should be the basis for its development in the ELT era. The ELT, VLT in its many functions and the ESO 4-metre telescopes will form a powerful astrophysics resource. The new role of the VLT needs to be defined and this workshop will provide a discussion forum aimed at shaping the VLT's future.