CALIFA, the Calar Alto Legacy Integral Field Area survey. III. Second public data release
arXiv:1409.8302 · doi:10.1051/0004-6361/201425080
Abstract
This paper describes the Second Public Data Release (DR2) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. The data for 200 objects are made public, including the 100 galaxies of the First Public Data Release (DR1). Data were obtained with the integral-field spectrograph PMAS/PPak mounted on the 3.5 m telescope at the Calar Alto observatory. Two different spectral setups are available for each galaxy, (i) a low-resolution V500 setup covering the wavelength range 3745-7500 Å with a spectral resolution of 6.0 Å (FWHM), and (ii) a medium-resolution V1200 setup covering the wavelength range 3650-4840 Å with a spectral resolution of 2.3 Å (FWHM). The sample covers a redshift range between 0.005 and 0.03, with a wide range of properties in the Color-Magnitude diagram, stellar mass, ionization conditions, and morphological types. All released cubes were reduced with the latest pipeline, including improved spectrophotometric calibration, spatial registration and spatial resolution. The spectrophotometric calibration is better than 6% and the median spatial resolution is 2.5". Altogether the second data release contains over 1.5 million spectra. It is available at http://califa.caha.es/DR2.
33 pages, 20 figures, 7 tables, submitted to A&A. The CALIFA DR2 homepage http://califa.caha.es/DR2 is open for the public
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- Resolved galaxy scaling relations in the EAGLE simulation: star formation, metallicity and stellar mass on kpc scales
- The EDGE-CALIFA survey: exploring the role of the molecular gas on the galaxy star formation quenching
- Untangling galaxy components: full spectral bulge-disc decomposition
- The PyCASSO database: Spatially resolved stellar population properties for CALIFA galaxies
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- EDGE-CALIFA survey: Self-regulation of Star formation at kpc scales
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- The stellar orbit distribution in present-day galaxies inferred from the CALIFA survey
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- The CALIFA survey: A panoramic view on galaxy properties
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