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Open AccessJournal ArticleDOI

CALIFA, the Calar Alto Legacy Integral Field Area survey - III. Second public data release

Sebastián F. Sánchez, +65 more
- 01 Jan 2013 - 
- Vol. 576, pp 1-25
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TLDR
The second public data release (DR2) of the Calar Alto Legacy Integral Field Area (CALIFA) survey as discussed by the authors contains over 1.5 million spectra.
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 A with a spectral resolution of 6.0 A (FWHM); and (ii) a medium-resolution V1200 setup covering the wavelength range 3650-4840 A with a spectral resolution of 2.3 A (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 the cubes in the data release were reduced with the latest pipeline, which includes improved spectrophotometric calibration, spatial registration, and spatial resolution. The spectrophotometric calibration is better than 6% and the median spatial resolution is 2´´ 4. In total, the second data release contains over 1.5 million spectra.

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Journal ArticleDOI

SDSS-IV MaNGA: pyPipe3D Analysis Release for 10,000 Galaxies

TL;DR: In this article , the pyPipe3D pipeline was used to extract spatially resolved spectroscopic properties of both the stellar population and the ionized gas emission lines from the final MaNGA data set included in the Sloan Digital Sky Survey data release 17.
Journal ArticleDOI

Stellar Populations of Nine Passive Spiral Galaxies from the CALIFA Survey: Are They Progenitors of S0s?

TL;DR: In this paper, the stellar population properties of passive spiral galaxies in the CALIFA survey were investigated, and the authors inferred that the diversity in the stellar populations of S 0s may result from different evolutionary pathways of S0 formation, and passive spirals may be one of the possible channels.
Journal ArticleDOI

Star formation quenching stages of active and non-active galaxies

TL;DR: In this paper, the authors proposed a classification based on the maps of the ionised hydrogen distribution, traced by kpc-resolved, equivalent width of H$\alpha$ maps, and the nuclear activity of the galaxies using information from the BPT diagnostic diagrams.
References
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