000002732 001__ 2732
000002732 005__ 20160706140751.0
000002732 037__ $$aASTROimport-889
000002732 100__ $$aTanga, P.
000002732 245__ $$aScientific perspectives from Gaia data of Solar System objects
000002732 260__ $$c2014
000002732 520__ $$aGaia will collect asteroid observations over 5 years, with a limiting magnitude V~20 (>300,000 objects). Observations will include very precise astrometry and photometry, and low resolution spectra. Over the last few years, the Coordination Unit 4 of Gaia's Data Processing and Analysis Consortium has built the data reduction pipeline that will produce the expected products for Solar System science. We will outline the performances and limitations of these processing chains.   The implementation of the pipelines is mainly devoted to a general treatment for deriving the bulk properties of the largest possible sample of minor planets. The DPAC processing is based uniquely on Gaia data, in order to produce a homogeneous outcome independent from other surveys.
000002732 700__ $$aBerthier, J.
000002732 700__ $$aCellino, A.
000002732 700__ $$aDelbo', M.
000002732 700__ $$aDell'Oro, A.
000002732 700__ $$aHestroffer, D.
000002732 700__ $$aMignard, F.
000002732 700__ $$aMuinonen, K.
000002732 700__ $$aPetit, J.-M.
000002732 700__ $$aPauwels, T.
000002732 700__ $$aThuillot, W.
000002732 773__ $$cEPSC2014-486$$pEuropean Planetary Science Congress 2014, EPSC Abstracts$$v9$$y2014
000002732 85642 $$ahttp://esoads.eso.org/abs/2014EPSC....9..486T
000002732 905__ $$apublished in
000002732 980__ $$aNONREF