Science Announcements

2018 VLTI Summer School

Published: 10 Jun 2018

Lisbon, Portugal, July 9-14, 2018

By combining the light from four telescopes, ESO's Very Large Telescope Interferometer (VLTI) delivers angular resolution at milli-arcsecond scales, and astrometry at tens of micro-arcseconds. The available instrumentation covers the H to N bands, with low to moderately high spectral resolution. As long-baseline optical interferometric observing techniques are not widespread in the community, VLTI schools are periodically organised. The next school will take place from 9–14 July in Lisbon and will provide practical hands-on training on observational programme preparation, data reduction and analysis. Full lodging and subsistence costs will be provided to all attendees. The registration deadline is 1 July 2018, and may close earlier if all available places are filled.

Workshop: Network for Young Researchers in Instrumentation for Astrophysics (NYRIA)

Published: 09 Jun 2018

Leiden Observatory, The Netherlands, 8-12 October, 2018

The Network for Young Researchers in Instrumentation for Astrophysics (NYRIA) is organising its fourth annual workshop at Leiden Observatory. This international group of early career researchers was created after a summer school which took place in 2014 in Santiago, Chile. Many of the participants have convened every year since, organising a meeting or workshop at different institutes in Europe whilst expanding this network.
The meeting aims to create a space to present the work of the attendants, to hold open discussions and to encourage collaborations between participants and institutes. The workshop will include a series of talks by all participants and guest speakers, tours of the Leiden University and facilities in Dwingeloo, and a hack-a-thon, in which all participants will work together on a current instrumentation problem.

ESO Workshop: The Galactic Bulge at the crossroads

Published: 09 Jun 2018

Pucón, Chile, December 10-14, 2018

The bulge is a primary component of the Milky Way, comprising ∼25% of its mass. All major Galactic stellar populations intersect there, reaching their highest densities. Exploring the bulge is fundamental to understanding Galactic formation, structure and evolution. With the advent of multiplexed spectrographs on 8-metre class telescopes, and the availability of wide-field near-infrared photometry, our knowledge of the structural, chemical and kinematical properties of the Galactic bulge has improved dramatically in the last few years. At the same time, the interpretation of the data is not straightforward, and many fundamental questions remain. In this context, a host of exciting new results are expected in 2018. This conference aims to gather the international astronomical community to discuss these developments, and to begin to establish a consensus on their interpretation.

ALMA Cycle 6 Proposal Submission Statistics

Published: 08 Jun 2018

The deadline for proposal submission for Cycle 6 was 19 April 2018. 1838 proposals were submitted, including 18 Large Programmes. This is a further increase on the 1661 proposals received for Cycle 5. The oversubscription rate remains high (over 6 on the 12-metre array for the European applicants). Detailed proposal submission statistics are available in a dedicated report. The report provides a summary of items such as the number of submitted proposals and time requested, subscription rates, and comparisons with the number of hours requested in previous Cycles.

KMOS@5 Workshop: Star Formation and Galaxy Formation in 3D

Published: 01 Jun 2018

ESO Headquarters, Garching, Germany, 3–6 December, 2018

The KMOS@5 workshop will bring together scientists working on all areas of star and galaxy formation using near-infrared IFU spectroscopy. KMOS's five-year milestone offers a perfect opportunity to assess the impact of this instrument on its core science cases and to develop new strategies and programmes, also in preparation for future IFU instruments.

MUSE Narrow Field Mode Science Verification

Published: 30 Apr 2018

GALACSI is part of the Adaptive Optics Facility (AOF), and is thus associated with the Deformable Secondary Mirror (DSM) and the 4 Laser Guide Star Facility (4LGSF). It defines an AO system developed to increase the performance of the MUSE instrument in narrow-field mode. Commissioning is proceeding and Science Verification is planned for August 2018, for which applications are invited.

2018 ESO Studentships

Published: 25 Apr 2018

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 for a period of up to two years.

ESO Period 102 Proposal Submission Statistics

Published: 24 Apr 2018

The deadline for proposal submission for Period 102 (1 October 2018 - 1 April 2019) was 28 March, 2018. 916 valid proposals were submitted, including 23 Large Programmes, of which four are GTO Large Programmes. The number of proposals for P102 is very similar to that of Periods 91 (893), 92 (892), 93 (898), 94 (901), 98 (901), 99 (887), 100 (895) and 101 (899). This confirms the levelling off observed after the peak of Periods 95 (934), 96 (960) and 97 (1024).

Workshop: A Revolution in Stellar Physics with Gaia and Large Surveys

Published: 21 Apr 2018

Warsaw University Library, Warsaw, Poland, 3–7 September 2018

The era of Gaia-enabled revolutions in almost all areas of astrophysics has started. In particular, and crucially, Gaia's exquisite astrometry and photometry combined with data from other large stellar surveys (ground- and space-based) will allow major progress in our understanding of stellar physics. The workshop will focus on the advances in our understanding of stellar physical processes made possible by combining the astrometry and photometry of Gaia with data from other large photometric, spectroscopic, and asteroseismic stellar surveys. Asteroseismology, in particular, has been essential to probe the interiors of stars. These combined data will permit detailed studies of stellar physics to a level that is unprecedented in the history of stellar astrophysics. More details are available on the workshop page or by email. The registration and abstract submission deadline has recently been extended to 5 May 2018.

Upgrade to ESO Telescope Bibliography Interface

Published: 20 Apr 2018

The ESO Telescope Bibliography, telbib, connects ESO data papers with observations in the Science Archive and provides a variety of publication statistics. Search results can be visualised in various ways, resulting in "on-the-fly" graphs. In addition, telbib also provides a set of predefined charts. Following requests from telbib users, the underlying data tables of all charts are now also available for download via the web. This new download option gives users more flexibility to process data according to their needs. Note that all telbib charts are interactive and the data exported into CSV or XLS tables will correspond to the selection made by the user.

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