Joint ESO, ALMA, NAOJ, NRAO Workshop:
ESO Vitacura, Santiago, Chile, 16–20 May 2016

Results from ALMA Long Baseline observations and from SPHERE, Gemini Planet Imager (GPI) and other high-contrast adaptive optics (AO) instruments have given a taste of what to expect over the next few years in the fields of protoplanetary and debris discs, and planet formation. For the first time observations of the regions where planets form are achievable. The workshop will discuss the state-of-the-art results, offering a panchromatic view, with a balance between observations and theory. Discussions will be scheduled on how facilities, such as JWST, E-ELT and TMT, and advances in modeling, will advance the field of planetary formation.

The Run Progress Report web pages allow PIs and delegates to follow the progress of their Service Mode observations. Now they also indicate when pipeline-processed reduced data are available for download. These reduced data are automatically generated using certified master calibrations and appear within two months of the data acquisition. Please see the Run Progress Legend for more details on how to take advantage of this new service.

The User Support Department (USD) extends its thanks to all those Principal Investigators and their Phase 2 delegates who filled in this September's on-line User Satisfaction Survey. As of mid-September, 100 responses were received from our targeted campaign. We have contacted, where possible, those respondents who provided detailed comments. A summary report of this latest User Satisfaction Survey is now available.

A detailed report on the outcome of the ALMA Early Science Cycle 3 Proposal Review Process is available. The report details the proposal review process, proposal statistics and regional distributions, the proposal distribution across science categories and receiver bands, as well as the anticipated observing pressure as a function of Local Sidereal Time and configuration. The accepted high priority Cycle 3 projects are listed here.

The Call for Proposals for ESO Period 97 (1 April 2016 – 30 September 2016) closed on 1 October 2015. 1020 proposals were received (the second highest, after Period 84), including 22 for Large Programmes, 48 for Target of Opportunity and 5 for Monitoring Programmes, for a total of 2212 nights. The number of proposals received shows an increase of 6.5% over Period 96.

The ESO research studentship programme provides an outstanding opportunity for Ph.D. students to experience the exciting scientific environment at one of the world's leading observatories for a period of up to two years.

The refurbishment of the VLTI laboratory, in preparation for the arrival of GRAVITY, has been completed and VLTI is ready to re-start science observations. Successful recommissioning occurred during August and September. The GRAVITY instrument was transported from the Paranal Integration Hall to the VLTI laboratory in early October 2015, an important milestone in its Assembly, Integration and Verification (AIV) and Commissioning process.

The fourth ALMA user survey was conducted between the 1 May and 1 June 2015. A total of 536 users (representing 15% of the users who were sent the questionnaire and 44% of the Cycle 3 PIs) responded to the survey. This survey focused on topics related to proposal preparation and submission, including interaction with the ARC / ARC nodes for ALMA proposal preparation and usability of tools such as the ALMA Science Portal or the helpdesk. A summary is available.

The latest ALMA Status Report, available here, includes Cycle 2 Early Science observing progress (including Cycle 1 Transfer projects), project completion and data delivery summary, Extension and Optimization of Capabilities (EOC) activity, and preparations for Cycle 4, since the last Report (November 2014).

New data products resulting from the VST Public Survey ATLAS are now available via the dedicated Phase3 query interface at the Science Archive Facility.