The Call for Proposals for observations at ESO telescopes in Period 104 (1 October 2019 – 31 March 2020) has been released. Please consult the Period 104 document for the main news items and policies related to applying for time on ESO telescopes. All technical information about the offered instruments and facilities is contained on ESO webpages that are linked from the Call. The proposal submission deadline is 12:00 CET 28 March 2019.
ESO announces the forthcoming deployment of its new tool for the preparation and submission of observing proposals. This represents the first part of a broader overhaul of the ESO Phase 1 system (p1) that, in the near future, will also entail a significant modernisation of the Observing Programmes Committee refereeing process and related tools. ESO will start to offer the new p1 system during Period 103 for the submission of DDT proposals. A demo version where users can experiment with the new system will soon be available. Further announcements will be made via the usual ESO communication channels.
Science workshops are an essential component of ESO's programmes and represent a unique opportunity to promote and foster ideas and collaborations within the scientific community. Every year, through the Directorate for Science, ESO provides support and funding to organise two workshops in Santiago and four in Garching, as well as co-funding some external workshops (see ESO Workshops calendar).
A new Call has been issued inviting community astronomers to team up with ESO staff and fellows in Chile and/or in Germany to submit proposals for ESO workshops to be held in 2020. Note that ESO has implemented a Code of Conduct for Workshops and Conferences, which applies to all meetings held at ESO premises. ESO-funded workshops that are held outside ESO premises are required to adopt their own codes of conduct.
In April 1999, the first of the twin workhorses of the VLT, FORS1, started regular science operations. In September 1999 its twin, FORS2 arrived at Paranal and entered regular service in April 2000. Over the years, the two FORS instruments have provided unique data, leading to many astronomical discoveries. Both instruments have been amongst the most prolific Paranal instruments. In March there will be a one-day event celebrating the scientific discoveries made with these successful instruments. Registration is open and further details are available at the meeting website.
The theme for the First CTA Symposium is “Science opportunities with CTA”. Through a combination of invited and contributed talks, as well as poster sessions, the meeting aims to gather the larger multi-wavelength and multi-messenger communities and set up new channels of communications and synergies among them and their results (see the preliminary programme). Registration is now open and there is also a call for contributed talks.
Registration is now open for the ESO ALMA Development workshop. This workshop aims to bring together a wide range of groups working on the continued development of ALMA in order to optimally coordinate these activities in light of the three-yearly ESO call for development studies, which is expected to be issued before the workshop. A particular emphasis will be given on presenting the ALMA 2030 development roadmap. Further details, including an outline of the programme can be found on the workshop webpage. The registration deadline is 2 May 2019.
The Atacama Large Millimeter/Submillimeter Array (ALMA) is the world’s most sensitive facility for millimeter/submillimeter 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. Following conferences in Puerto Varas (Chile, 2012), Tokyo (Japan, 2014), and Indian Wells (USA, 2016), the ALMA partnership is organising the next ALMA Science Conference in Cagliari this October. Registration will open in the second week of March.
VVVX is an ESO Public Survey that was approved as part of the second cycle of Public Surveys with VISTA. This project extends the VISTA Variables in the Via Lactea (VVV) survey parameter space both in area coverage and time. Primarily, VVVX includes portions of the southern galactic plane that were not covered by VVV. Furthermore, it will provide additional epochs to the VVV area in order to improve proper motion precision and keep monitoring the long term variable stars.
The Kilo-Degree Survey KiDS is one of the ESO Public Surveys carried out with OmegaCAM at the VST. Once complete, it will have observed 1350 square degrees in four filters (u, g, r, i). Designed to be a weak-lensing shear tomography survey, it will also map the large-scale matter distribution in the universe and constrain the equation of state of dark energy. Its secondary science cases include galaxy evolution to Milky Way structure and from the detection of white dwarfs to high-redshift quasars. This data release covers 1107 square-degrees and more than doubles the sky area covered by the previous three releases combined.
All qualifying GIRAFFE Medusa data have now been processed into stacked 1D spectra, whenever the observing block that created the raw products contains more than one SCIENCE exposure. Backwards processing of stacks for the historical part is also completed such that more than 360 000 1D spectra products are available as processed in-house products from the Archive Science portal. Single-exposure 1D spectra are also produced and can be found as associated ancillary files or as science products, if originating observing block contains a single exposure only.
The La Silla Observatory was officially inaugurated on 25 March 1969. This conference celebrates the 50th anniversary of the inauguration of La Silla. Its historical significance will be reviewed and possible future scenarios discussed. In addition the research areas where La Silla telescopes have made important contributions will be reviewed.
