About: RAVE (survey)

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RAVE (RAdial Velocity Experiment) is a multi-fiber spectroscopic astronomical survey of stars in the Milky Way using the 1.2-metre UK Schmidt Telescope of the Australian Astronomical Observatory (AAO). The RAVE collaboration consists of researchers from over 20 institutions around the world and is coordinated by the Leibniz Institute for Astrophysics Potsdam (AIP).

Attributes	Values
rdf:type	yago:WikicatAstronomicalCataloguesOfStars yago:WikicatAstronomicalSurveys yago:Abstraction100002137 yago:Act100030358 yago:Activity100407535 yago:Catalog106487897 yago:Communication100033020 yago:Database106637824 yago:Event100029378 yago:Examination100635850 yago:Information106634376 yago:Investigation100633864 yago:List106481320 yago:Message106598915 yago:PsychologicalFeature100023100 yago:Work100575741 yago:YagoPermanentlyLocatedEntity organisation yago:Survey100644503
rdfs:label	RAdial Velocity Experiment (de) RAVE (survey) (en)
rdfs:comment	Das Radial Velocity Experiment (RAVE) ist eine spektroskopische Durchmusterung des Südhimmels. Dazu wird ein Multi-Objekt-Spektrograf am 1,2-Meter-UK-Schmidt-Teleskop des Anglo-Australian Observatory (Australien) benutzt. RAVE ist ein Gemeinschaftsprojekt von Wissenschaftlern aus über 20 Institutionen weltweit unter Federführung des Leibniz-Instituts für Astrophysik Potsdam (AIP). Das Projekt startete im Jahr 2003 und bis zum Ende der Datenerhebungsphase am 5. April 2013 wurden 574.630 Spektren von 483.330 Sternen aufgezeichnet. (de) RAVE (RAdial Velocity Experiment) is a multi-fiber spectroscopic astronomical survey of stars in the Milky Way using the 1.2-metre UK Schmidt Telescope of the Australian Astronomical Observatory (AAO). The RAVE collaboration consists of researchers from over 20 institutions around the world and is coordinated by the Leibniz Institute for Astrophysics Potsdam (AIP). (en)
dcterms:subject	Observational astronomy Siding Spring Observatory Astronomical surveys
Wikipage page ID	28832678 (xsd:integer)
Wikipage revision ID	1098763563 (xsd:integer)
Link from a Wikipage to another Wikipage	Robot Metallicity Charge-coupled device Proper motion Cosmology Mass Sagittarius Dwarf Elliptical Galaxy Effective temperature Full moon Galaxies PhysOrg Macquarie University Siding Spring Observatory Parallax Phase space Photometry (astronomy) 6dF Galaxy Survey UK Schmidt Telescope Data reduction Galactic Center Null result Observational astronomy ESA Escape velocity Siding Spring Observatory Diffraction grating Leibniz Institute for Astrophysics Potsdam Stellar halo Spectral resolution Astronomical surveys Astrometry Astronomical survey Dwarf galaxies Stellar streams VizieR Australian Astronomical Observatory Photometric parallax method Southern hemisphere Dark halo Milky Way Radial velocity Sloan Digital Sky Survey Spectroscopic Fiber optics Surface gravity Elemental abundance Transverse velocity Gaia mission Galaxy formation University of Padova
Link from a Wikipage to an external page	http://www.rave-survey.aip.de/rave/ http://adsabs.harvard.edu/abs/2013AJ....146..134K http://www.aao.gov.au/ukst/ http://www.physorg.com/news10751.html
sameAs	RAVE (survey) RAVE (survey) RAVE (survey) RAVE (survey) RAVE (survey)
dbp:wikiPageUsesTemplate	dbt:Citation_needed dbt:Cite_journal dbt:Cite_web dbt:Convert dbt:Portal_bar dbt:Reflist dbt:Use_Australian_English dbt:Use_dmy_dates dbt:Infobox_astronomical_survey
has abstract	Das Radial Velocity Experiment (RAVE) ist eine spektroskopische Durchmusterung des Südhimmels. Dazu wird ein Multi-Objekt-Spektrograf am 1,2-Meter-UK-Schmidt-Teleskop des Anglo-Australian Observatory (Australien) benutzt. RAVE ist ein Gemeinschaftsprojekt von Wissenschaftlern aus über 20 Institutionen weltweit unter Federführung des Leibniz-Instituts für Astrophysik Potsdam (AIP). Das Hauptziel von RAVE ist die Messung der Radialgeschwindigkeiten einer repräsentativen Anzahl von Sternen der fast der gesamten südlichen Hemisphäre unter Ausnutzung des Dopplereffekts. Aus den aufgenommenen Spektren werden außerdem noch weitere Eigenschaften der Sterne gewonnen, namentlich die effektive Temperatur, Oberflächengravitation und Metallizität. Ferner wurden auch photometrische Parallaxen (Entfernungsmessungen) und Häufigkeiten von einzelnen chemischen Elementen bestimmt. Das Projekt startete im Jahr 2003 und bis zum Ende der Datenerhebungsphase am 5. April 2013 wurden 574.630 Spektren von 483.330 Sternen aufgezeichnet. (de) RAVE (RAdial Velocity Experiment) is a multi-fiber spectroscopic astronomical survey of stars in the Milky Way using the 1.2-metre UK Schmidt Telescope of the Australian Astronomical Observatory (AAO). The RAVE collaboration consists of researchers from over 20 institutions around the world and is coordinated by the Leibniz Institute for Astrophysics Potsdam (AIP). 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. On April 5, 2013 RAVE concluded its phase of data taking. In an almost ten year observing campaign, a total of 574,630 spectra have been obtained on 483,330 individual stars by a small team of AAO observers, with other observers making occasional visits from RAVE participating institutions. (en)
gold:hypernym	Survey
prov:wasDerivedFrom	wikipedia-en:RAVE_(survey)?oldid=1098763563&ns=0

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