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Properties of the EXPORT sample: Spectral type determination

Published online by Cambridge University Press:  26 May 2016

Bruno Merín ,
Benjamín Montesinos  and
EXPORT TEAM (A. Alberdi, A. Collier Cameron, J.K. Davies, H.J. Deeg, C. Eiroa, R. Ferlet, F. Garzon, C.A. Grady, A. Harris, K. Horne, L.F. Miranda, A. Mora, R. Oudmaijer, J. Palacios, A. Penny, A. Quirrenbach, H. Rauer, J. Schneider, E. Solano, Y. Tsapras, P.R. Wesselius, D. de Winter)
Bruno Merín
Affiliation:
LAEFF-INTA, P.O. Box 50727, 28080 Madrid, Spain
Benjamín Montesinos
Affiliation:
LAEFF-INTA, P.O. Box 50727, 28080 Madrid, Spain IAA-CSIC, P.O. Box 3004, 18080 Granada, Spain

Abstract

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In this paper we present the results of the spectral classification of stars included in the EXPORT (EXoPlanetary Observational Research Team) sample and observed during the 1998–1999 International Time campaigns in the Canary Island observatories. Intermediate resolution spectra obtained with the Isaac Newton Telescope (INT) were used in this work. In addition to the confirmation of some spectral types and changes to previous classifications, we report new results for stars whose spectral type had not been accurately assigned before.

Type
Part I: Discovery and study of extrasolar planets - current
Information
Symposium - International Astronomical Union , Volume 202: Planetary Systems in the Universe – Observation, Formation and Evolution , 2004 , pp. 87 - 89
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

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