Mass-metallicity relation explored with CALIFA
- S. F. Sánchez
- F. F. Rosales-Ortega
- B. Jungwiert
- J. Iglesias-Páramo
- J. M. Vílchez
- R. A. Marino
- C. J. Walcher
- B. Husemann
- D. Mast
- A. Monreal-Ibero
- R. Cid Fernandes
- E. Pérez
- R. González Delgado
- R. García-Benito
- L. Galbany
- G. van de Ven
- K. Jahnke
- H. Flores
- J. Bland-Hawthorn
- A. R. López-Sánchez
- V. Stanishev
- D. Miralles-Caballero
- A. I. Díaz
- P. Sánchez-Blazquez
- M. Mollá
- A. Gallazzi
- P. Papaderos
- J. M. Gomes
- N. Gruel
- I. Pérez
- T. Ruiz-Lara
- E. Florido
- A. de Lorenzo-Cáceres
- J. Mendez-Abreu
- C. Kehrig
- M. M. Roth
- B. Ziegler
- J. Alves
- L. Wisotzki
- D. Kupko
- A. Quirrenbach
- D. Bomans
DOIAbstract
We studied the global and local ℳ-Z relation based on the first data available from the CALIFA survey (150 galaxies). This survey provides integral field spectroscopy of the complete optical extent of each galaxy (up to 2−3 effective radii), with a resolution high enough to separate individualH i
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