1111.0962 (S. F. Sanchez et al.)

CALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation    [PDF]

S. F. Sanchez, R. C. Kennicutt, A. Gil de Paz, G. van de Ven, J. M. Vılchez, L. Wisotzki, C. J. Walcher, D. Mast, J. A. L. Aguerri, S. Albiol-Perez, A. Alonso-Herrero, J. Alves, J. Bakos, T. Bartakova, J. Bland-Hawthorn, A. Boselli, D. J. Bomans, A. Castillo-Morales, C. Cortijo-Ferrero, A. de Lorenzo-Caceres, A. del Olmo, R. -J. Dettmar, A. Dıaz, S. Ellis, J. Falcon-Barroso, H. Flores, A. Gallazzi, B. Garcıa-Lorenzo, R. Gonzalez Delgado, N. Gruel, T. Haines, C. Hao, B. Husemann, J. Iglesias-Páramo, K. Jahnke, B. Johnson, B. Jungwiert, V. Kalinova, C. Kehrig, D. Kupko, A . R. Lopez-Sanchez, M. Lyubenova, R. A. Marino, E. Marmol-Queralto, I. Marquez, J. Masegosa, S. Meidt, J. Mendez-Abreu, A. Monreal-Ibero, C. Montijo, A. M. Mourao, G. Palacios-Navarro, P. Papaderos, A. Pasquali, R. Peletier, E. Perez, I. Perez, A. Quirrenbach, M. Relaño, F. F. Rosales-Ortega, M. M. Roth, T. Ruiz-Lara, P. Sanchez-Blazquez, C. Sengupta, R. Singh, V. Stanishev, S. C. Trager, A. Vazdekis, K. Viironen, V. Wild, S. Zibetti, B. Ziegler

We present here the Calar Alto Legacy Integral Field Area (CALIFA) survey, which has been designed to provide a first step in this direction.We summarize the survey goals and design, including sample selection and observational strategy.We also showcase the data taken during the first observing runs (June/July 2010) and outline the reduction pipeline, quality control schemes and general characteristics of the reduced data. This survey is obtaining spatially resolved spectroscopic information of a diameter selected sample of $\sim600$ galaxies in the Local Universe (0.005< z <0.03). CALIFA has been designed to allow the building of two-dimensional maps of the following quantities: (a) stellar populations: ages and metallicities; (b) ionized gas: distribution, excitation mechanism and chemical abundances; and (c) kinematic properties: both from stellar and ionized gas components. CALIFA uses the PPAK Integral Field Unit (IFU), with a hexagonal field-of-view of $\sim1.3\sq\arcmin'$, with a 100% covering factor by adopting a three-pointing dithering scheme. The optical wavelength range is covered from 3700 to 7000 {\AA}, using two overlapping setups (V500 and V1200), with different resolutions: R\sim850 and R\sim1650, respectively. CALIFA is a legacy survey, intended for the community. The reduced data will be released, once the quality has been guaranteed. The analyzed data fulfill the expectations of the original observing proposal, on the basis of a set of quality checks and exploratory analysis. We conclude from this first look at the data that CALIFA will be an important resource for archaeological studies of galaxies in the Local Universe.

View original: http://arxiv.org/abs/1111.0962