IFUs surveys, a panoramic view of galaxy evolution
arXiv:1410.0295 · doi:10.1017/S1743921314009375
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
arXiv comment8 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 (15)
- The Sloan Digital Sky Survey: Technical Summary
- The Seventh Data Release of the Sloan Digital Sky Survey
- The Cosmic Evolution Survey (COSMOS) -- Overview
- The Atlas3D project -- I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria
- The SAURON project. II. Sample and early results
- GEMS: Galaxy Evolution from Morphologies and SEDs
- The 2dF Galaxy Redshift Survey: Spectral Types and Luminosity Functions
- PMAS: The Potsdam Multi Aperture Spectrophotometer. II. The Wide Integral Field Unit PPak
- Reconstructing the Subsurface Three-Dimensional Magnetic Structure of A Solar Active Region Using SDO/HMI Observations
- The DiskMass Survey. I. Overview
- The ALHAMBRA Project: A large area multi medium-band optical and NIR photometric survey
- Measuring Baryon Acoustic Oscillations along the line of sight with photometric redshifs: the PAU survey
- Insights on the stellar mass-metallicity relation from the CALIFA survey
- A new scaling relation for HII regions in spiral galaxies: unveiling the true nature of the mass-metallicity relation
- The VIRUS-P Exploration of Nearby Galaxies (VENGA): Survey Design, Data Processing, and Spectral Analysis Methods