The online interface to the Atacama Pathfinder Experiment (APEX) LABOCA and SABOCA calibration data has been significantly updated. The query pages for zenith opacities and calibration factors are affected. The calibration dataset has been fully re-reduced for both bolometer cameras, leading to improvements and using more precise algorithms to better estimate the sky opacity values. Extensive help pages have been added, including descriptions on how to use these data in BoA.

ESO Headquarters, Garching, Germany, 14–18 July 2014

Galaxies and active galactic nuclei (AGN) are not randomly distributed in the Universe. The distribution of AGN, measured by clustering, enables new insights into the physical conditions that govern the accretion onto supermassive black holes and high precision AGN clustering can provide constraints on cosmological parameters. AGN clustering measurements have gained significant interest in the last decade and upcoming large surveys will generate AGN samples with several million objects. These surveys offer the unique opportunity to study AGN and galaxy co-evolution, AGN physics, and cosmology with AGN clustering measurements.

The December 2013 issue of The Messenger contains a section with summaries of ten of the eleven ESO public surveys, together with an introductory overview on the progress of the public surveys. The whole issue, or individual articles, can be downloaded.

The VISTA Kilo-degree Infrared Galaxy Survey (VIKING), one of the 6 VISTA public surveys, is a wide area (eventually ~1500 square degrees), intermediate-depth (5-sigma detection limit J~21 [Vega]) near-infrared imaging survey, in the 5 broadband filters Z, Y, J, H, Ks. The first VIKING data release, which is based on observations until mid-February 2011, covers 226 square degrees in all 5 filters and consists of 14.7 million sources (including low-reliability single-band detections).

The collection of pipeline-processed high-resolution spectral data obtained with UVES has been significantly extended, now also including the observations that make use of the image slicers. In addition to the previously announced UVES data release, over 10 000 individual spectra, acquired 2003 - 2013, are now available from the Science Archive Facility.

Version 2.5 of the ESO data reduction environment Reflex has been released. Reflex provides an easy interface to run and supervise VLT data reduction pipelines. Reflex can be installed with a self-explanatory installation script and the workflows are pre-configured to run right out of the box on demo or user data. All Reflex workflows come with a detailed step-by-step tutorials, and a detailed discussion of the design principles has been presented by Freudling et al, 2013, AA 559, 96.

The 81st Scientific Technical Committee (STC) meeting was held on 22–23 October 2013. The STC meets twice a year, is composed of representatives from the ESO member states and is the primary interface between the scientific community and the telescope and instrumentation projects. The STC also has sub-committees for the La Silla Paranal Observatory (LSP), ALMA and APEX (European Science Advisory Committee, ESAC) and for E-ELT (ESC). The ESC was constituted by ESO Council in June and met for the first time this October.

The proposal submission deadline for ALMA Early Science Cycle 2 proposals closed on the 5 December 2013. A total of 1382 proposals were received, requesting 7314 hours of 12-metre array time and 3325 hours of Morita Array (ALMA Compact Array, ACA) time. ToO observations were requested in 24 proposals. A total of 1049 individual PIs and 3408 proposers (PIs and CoIs) were involved in the submitted proposals.

ESO-Garching Operations will provide only minimal support during the Christmas–New Year holiday period, mostly limited to core operational tasks. Full support (user) services will resume on 2 January 2014.

Proposers for ESO Period 93 (1 April–30 September 2014) have just been notified of their allocation of observing time on Paranal and La Silla instrumentation. The Phase 2 observation preparation now starts for Service Mode users. The P93 deadline for Phase 2 submission will be on Thursday, 6 February 2014. In order to prepare their Phase 2, we recommend users to download the latest release of P2PP 3.4.0.