Photometric characterization of the asteroseismic COROT targets R

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Photometric characterization of the asteroseismic COROT targets R. Garrido P. J. Amado V. Costa

Photometric characterization of the asteroseismic COROT targets R. Garrido P. J. Amado V. Costa S. Martín-Ruíz I. Olivares A. Rolland Spanish contribution

Ground based observing preparatory activities Goal: improve our knowledge of the COROT targets Asterosismology

Ground based observing preparatory activities Goal: improve our knowledge of the COROT targets Asterosismology program Strömgren photometry: OSN (IAA) Teff log g [Fe/H] variability ~ 100 nights Exoplanets program DENIS y 2 MASS Large field photometry (Megacam/CFH) High resolution échelle spectroscopy: several T 2 m Teff log g abundancies vsini SB 2 anomalies variability ~ 200 nights Images in the vicinity of the main targets • Schmidt plates • Adaptative optics in T 4 M (CFH et TNG) Some nights Spanish contribution Data base available in GAUDI www. http: //sdc. laeff. esa. es/gaudi/

Stromgren photometry SNO Spanish contribution

Stromgren photometry SNO Spanish contribution

Stromgren photometry SNO Spanish contribution

Stromgren photometry SNO Spanish contribution

Stromgren photometry SNO Spanish contribution

Stromgren photometry SNO Spanish contribution

Physical calibration : Temp. Logg @ Spanish contribution ams. astro. univie. ac. at/templogg/

Physical calibration : Temp. Logg @ Spanish contribution ams. astro. univie. ac. at/templogg/

Spanish contribution

Spanish contribution

Effects on the equilibrium models • Model without rotation • Different models Spanish contribution

Effects on the equilibrium models • Model without rotation • Different models Spanish contribution

Spanish contribution

Spanish contribution

GAUDI • Base de datos GAUDI gaudi COROTSKY Spanish contribution

GAUDI • Base de datos GAUDI gaudi COROTSKY Spanish contribution

Technical Spanish contribution

Technical Spanish contribution

Technical Spanish contribution

Technical Spanish contribution

Present and future work • • • Monitoring secondary targets Extension of the Strömgren

Present and future work • • • Monitoring secondary targets Extension of the Strömgren input catalogue down to V=9. 5 mag Comparison of physical parameters from spectra and photometry Spanish contribution