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: http://www.eso.org/sci/publications/announcements.page3.html
Дата изменения: Unknown
Дата индексирования: Sun Apr 10 01:50:15 2016
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Поисковые слова: arp220
Schloss Ringberg, Tegernsee, Germany, 6 БЂ“ 9 March 2016
The APEX 12 m submillimetre telescope has significantly contributed to a wide variety of astronomical science areas, ranging from the discoveries of new molecules to large and deep imaging of the submillimetre sky. Continuing on the success of the 2012 and 2014 Ringberg meetings devoted to APEX science, APEX2016 aims at presenting new science results and examining opportunities for the near future.
The first stage of commissioning of the new VLTI instrument GRAVITY has been completed with the successful combination of light from the four VLT Auxiliary Telescopes. During the commissioning, the Trapezium star cluster in Orion (M42) was observed and о‘1 Orionis F was discovered to be a binary. See Release eso1601 for more details.
The 97th Observing Programmes Committee (OPC) met on 17БЂ“19 November 2015. A total of 1093 (10-hour equivalent) nights of Visitor Mode and Service Mode observations were allocated on the VLT/VLTI, VISTA, VST, the 3.6-metre and NTT and APEX telescopes. The submission deadline for Phase 2 Service Mode observations is 4 February 2016; see separate announcement.
The Cryogenic high-resolution InfraRed Echelle Spectrograph (CRIRES) is currently undergoing a major upgrade led by ESO in collaboration with a consortium. The upgrade project (CRIRES+), which will significantly expand the scientific capabilities of CRIRES, recently achieved two major milestones: optical Final Design Review (FDR) in June 2015 and Preliminary Design Review (PDR) in September 2015. The current schedule foresees commissioning of CRIRES+ in Q1 2018.
The allocation of ESO telescope time for Period 97 (1 April БЂ“ 30 September 2016) is expected to be emailed in the week beginning 21 December 2015. With the release of the telescope schedule, preparation of Service Mode (SM) observations (Phase 2) starts. The deadline for the submission of the Phase 2 material for Period 97 observations is 4 February 2016.
ESO Headquarters, Garching, Germany, 9БЂ“13 May 2016
The NEON Archive School on proposal preparation and data reduction for X-shooter and KMOS is open for registration. The School is preferentially targeted to PhD students, but advanced MSc's, postdocs and senior researchers may also apply. Introduction to Phase 1 and 2 for both instruments and hands-on experience with data reduction tools will be provided. Details can be found here. The number of participants is limited to 25 and registration closes on 15 February 2016.
Active Galactic Nuclei (AGN) are being discovered in ever-larger numbers over the whole electromagnetic spectrum (radio, infrared, optical/UV, X-ray and нЁ-ray), providing different windows on AGN physics. The main goal of the Workshop is to paint the AGN БЂњbig pictureБЂќ, which comes out of the multi-wavelength surveys, and understand the intrinsic and fundamental properties of AGN and the phys