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Found 6 result(s)
RAVE (RAdial Velocity Experiment) is a multi-fiber spectroscopic astronomical survey of stars in the Milky Way using the 1.2-m UK Schmidt Telescope of the Anglo-Australian Observatory (AAO). The RAVE collaboration consists of researchers from over 20 institutions around the world and is coordinated by the Leibniz-Institut für Astrophysik Potsdam. As a southern hemisphere survey covering 20,000 square degrees of the sky, RAVE's primary aim is to derive the radial velocity of stars from the observed spectra. Additional information is also derived such as effective temperature, surface gravity, metallicity, photometric parallax and elemental abundance data for the stars. The survey represents a giant leap forward in our understanding of our own Milky Way galaxy; with RAVE's vast stellar kinematic database the structure, formation and evolution of our Galaxy can be studied.
The Institutional Repository of the University of Burgos is based on the digital collections that include the documents generated by the members of the university community in their academic activities. These are accessible via the Internet, in accordance with the University's Open Access Institutional Policy.
Polish Platform of Medical Research (PPM) is a digital platform presenting the scientific achievements and research potential of 8 Polish medical universities from Bialystok, Gdansk, Katowice, Lublin, Szczecin, Warsaw, Wroclaw, the Nofer Institute of Occupational Medicine in Lodz and the Jagiellonian University Medical College in Cracow that form a partnership for the PPM Project. It incorporates the features of a Current Research Information System and a consortium repository and uses OMEGA-PSIR software. It provides open access to full texts of publications, doctoral theses, research data and other documents. PPM is a central platform that aggregates data from the local platforms of the PPM Project Partners. PPM is accessible for any Internet user.
B2FIND is a discovery service based on metadata steadily harvested from research data collections from EUDAT data centres and other repositories. The service offers faceted browsing and it allows in particular to discover data that is stored through the B2SAFE and B2SHARE services. The B2FIND service includes metadata that is harvested from many different community repositories.
Launched in December 2013, Gaia is destined to create the most accurate map yet of the Milky Way. By making accurate measurements of the positions and motions of stars in the Milky Way, it will answer questions about the origin and evolution of our home galaxy. The first data release (2016) contains three-dimensional positions and two-dimensional motions of a subset of two million stars. The second data release (2018) increases that number to over 1.6 Billion. Gaia’s measurements are as precise as planned, paving the way to a better understanding of our galaxy and its neighborhood. The AIP hosts the Gaia data as one of the external data centers along with the main Gaia archive maintained by ESAC and provides access to the Gaia data releases as part of Gaia Data Processing and Analysis Consortium (DPAC).