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ESO - Science Announcements
 
 

Science Announcements

ESO Period 95 Proposal Statistics

Published: 17 Oct 2014

The proposal submission for ESO Period 95 (1 April тАУ 30 September 2015) closed on 01 October 2014. 931 proposals were received, including 17 Large Programme and 50 Target of Opportunity (ToO) proposals, for a total of 2428 nights.

Agreement Signed to Build MOONS

Published: 15 Oct 2014

The Multi-Object Optical and Near-infrared Spectrograph (MOONS) is a red and near-infrared (0.64 тАУ 1.8 ѕ®m), medium (R=4000) and high (R=20000) resolution, multi-object spectrograph with 1024 fibres, planned for installation at the  VLT Nasmyth focus in 2018. The agreement to build MOONS was recently signed between ESO and the MOONS Consortium, composed of institutes from the ESO Member States and led by the UK STFC. See the public announcement for details.

Release of New Imaging Data for VISTA Magellanic Clouds Survey

Published: 13 Oct 2014

New data products from the VISTA Survey of the Magellanic system Public Survey (VMC) are now available via the dedicated Phase 3 query interface. The current release is based on the observations of five new VMC survey tiles (three in the LMC and two in the SMC), as well as on improved reduction of two tiles released earlier.

Baryons at Low Densities: the Stellar Halos around Galaxies

Published: 10 Oct 2014

ESO Workshop, ESO Headquarters, Garching, Germany, 23тАУ27 February 2015

Stellar halos are ubiquitous in luminous galaxies, but their low surface brightness hampers detailed study in distant galaxies. With the advent of large cameras and surveys, several late- and early-type galaxies have revealed similar low luminosity extended structures. These halos have complex morphologies with multiple stellar components, kinematics and substructures indicating the merger history. The halo morphologies resemble the density maps from cosmological simulations of galaxy formation in a hierarchical Universe.

Ultra-deep Ks-band Imaging Data of the UDS and GOODS-South Fields Released

Published: 07 Oct 2014

The HAWK-I Ultra Deep Survey and GOODS Survey (HUGS) is an near-infrared imaging survey executed with HAWK-I (PI: A. Fontana); an overview can be found here. HUGS covers two CANDELS extragalactic fields: a sub-area of the UKIDSS Ultra-Deep Survey (UDS) and GOODS-South. HUGS delivers the deepest, highest quality images ever collected in the K-band: to Ks=27.3 (1№Г) in UDS and to Ks=27.8 in GOODS-South. Deep Y-band images in the UDS field have also been acquired.

IMPRS Studentships

Published: 07 Oct 2014

If you wish to conduct a PhD in astronomy-astrophysics within one of the largest centres of astrophysical research in the world, which covers every subject from planets, stars, and galaxies to cosmology, you should seriously consider applying to the IMPRS studentship programme in Munich.