Protostars and Planets VI, Heidelberg, July 15-20, 2013
Poster 2K020
CARMENES AT PPVI. 2. CARMENCITA HERBS AND SPICES TO HELP YOU PREPARE A GENUINE TARGET SAMPLE
Caballero, J. A. (Centro de Astrobiología, Spain)
Cortés-Contreras, M. (Universidad Complutense de Madrid, Spain)
Alonso-Floriano, F. J. (Universidad Complutense de Madrid, Spain)
López-Santiago, J. (Universidad Complutense de Madrid, Spain)
Klutsch, A. (Universidad Complutense de Madrid, Spain)
Montes, D. (Universidad Complutense de Madrid, Spain)
Morales, J. C. (Institut de Cičncies de l\'Espai, Spain)
Abellán de Paco, F. J. (Universidad Complutense de Madrid, Spain)
Amado, P. J. (Instituto de Astrofísica de Andalucía, Spain)
Béjar, V. J. S. (Instituto de Astrofísica de Canarias, Spain)
Jeffers, S. (Institut für Astrophysik Göttingen, Germany)
Mundt, R. (Max-Planck-Institut für Astronomie, Germany)
Quirrenbach, A. (Landessternwarte Königstuhl, Germany)
Reiners, A. (Institut für Astrophysik Göttingen, Germany)
Ribas, I. (Institut de Cičncies de l\'Espai, Spain)
Zechmeister, M. (nstitut für Astrophysik Göttingen, Germany)
Abstract:
ARMENCITA, the CARMENES Cool star Information and daTa Archive, is the M-dwarf database from where we will choose our best target sample. As part of our guaranteed time observations, about 300 late-type M dwarfs will be monitored by CARMENES from Calar Alto during over 600 nights. CARMENCITA currently catalogues over 2000 carefully-selected M dwarfs northern of delta > −23 deg. For each star, we tabulate dozens of parameters (accurate astrometry, spectral typing, photometry in 20 bands from the ultraviolet to the mid-infrared, rotational and radial velocities, X-ray count rates and hardness ratios, close and wide multiplicity data and many more) compiled from the literature or measured by us with new data. The private on-line catalogue, including preparatory science observations (i.e., high-resolution imaging, low- and high-resolution spectroscopy), will be eventually public as a CARMENES legacy.
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