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arxiv: 1412.3509 · v1 · pith:ELUSIOG7new · submitted 2014-12-11 · 🌌 astro-ph.GA

The Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO)

R. Carrera (1 , 2) , L. Casamiquela (3) , L. Balaguer-N\'u\~nez (3) , C. Jordi (3) , E. Pancino (4 , 5) , C. Allende-Prieto (1
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S. Blanco-Cuaresma (6 7) C. E. M\'artinez-V\'azquez (1 S. Murabito (1 A. del Pino (1 A. Aparicio (1 C. Gallart (1 A. Recio-Blanco (8) ((1) Instituto de Astrof\'isica de Canarias La Laguna Tenerife Spain (2) Departamento de Astrof\'isica Universidad de La Laguna (3) Dept. d'Astronomia i Meteorologia Institut de Ci\'encies del Cosmos Universitat de Barcelona (IEEC-UB) Barcelona (4) Osservatorio Astronomico di Bologna Bologna Italy (5) ASI Science Data Center Frascati (6) CNRS/Univ. Bordeaux LAB UMR 5804 Floirac France (7) Observatoire de Gen\'eve Universit\'e de Gen\'eve Sauverny Switzerland (8) Laboratoire Lagrange (UMR7293) Universit\'e de Nice Sophia Antipolis CNRS Observatoire de la Cote d'Azur Nice France)
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keywords openabundanceschemicalobservatoriesoccasospanishclusterclusters
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We present the motivation, design and current status of the Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO). Using the high resolution spectroscopic facilities available at Spanish observatories, OCCASO will derive chemical abundances in a sample of 20 to 25 open clusters older than 0.5 Gyr. This sample will be used to study in detail the formation and evolution of the Galactic disc using open clusters as tracers.

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