IFUs surveys, a panoramic view of galaxy evolution

Abstract

We present here a brief summary of the currenly on-going IFU surveys of galaxies in the Local Universe, describing their main characteristics, including their sample selections, instrumental setups, wavelength ranges, and area of the galaxies covered. Finally, we make an emphasis on the main characteristics of the CALIFA survey and the more recent results that has been recently published

8 Pages, 2 Figures, S.F.Sanchez et al. 2014, in IAU Symp. 309, "Galaxy in 3D across the Universe", B. L. Ziegler, F. Combes, H. Dannerbauer, M. Verdugo, Eds. (Cambridge: Cambridge Univ. Press), in press

References in corpus (4)

• The Cosmic Evolution Survey (COSMOS) -- Overview
• Reconstructing the Subsurface Three-Dimensional Magnetic Structure of A Solar Active Region Using SDO/HMI Observations
• The ALHAMBRA Project: A large area multi medium-band optical and NIR photometric survey
• Insights on the stellar mass-metallicity relation from the CALIFA survey

Cited by in corpus (1)

• The SAMI Galaxy Survey: energy sources of the turbulent velocity dispersion in spatially-resolved local star-forming galaxies