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dc.contributor.author
Sánchez, S. F.  
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Garciá Benito, R.  
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Zibetti, S.  
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Walcher, C. J.  
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Husemann, B.  
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Mast, Damian  
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López Fernández, R.  
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López Sánchez, A. R.  
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Lyubenova, M.  
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Marino, R.  
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Márquez, I.  
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Mendez Abreu, J.  
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Mollá, M.  
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Monreal Ibero, A.  
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Ortega Minakata, R.  
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Torres Papaqui, J. P.  
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Pérez, E.  
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Rosales Ortega, F. F.  
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Roth, M. M.  
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Sánchez Blázquez, P.  
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Schilling, U.  
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Spekkens, K.  
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Vale Asari, N.  
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Van Den Bosch, R. C. E.  
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Van De Ven, G.  
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Vilchez, J. M.  
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Wild, V.  
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Wisotzki, L.  
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Ylldlrlm, A.  
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Ziegler, B.  
dc.date.available
2018-11-01T16:00:43Z  
dc.date.issued
2016-06  
dc.identifier.citation
Sánchez, S. F.; Garciá Benito, R.; Zibetti, S.; Walcher, C. J.; Husemann, B.; et al.; CALIFA, the Calar Alto Legacy Integral Field Area survey: IV. Third public data release; EDP Sciences; Astronomy and Astrophysics; 594; 6-2016  
dc.identifier.issn
0004-6361  
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http://hdl.handle.net/11336/63439  
dc.description.abstract
This paper describes the third public data release (DR3) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. Science-grade quality data for 667 galaxies are made public, including the 200 galaxies of the second public data release (DR2). Data were obtained with the integral-field spectrograph PMAS/PPak mounted on the 3.5 m telescope at the Calar Alto Observatory. Three different spectral setups are available: i) a low-resolution V500 setup covering the wavelength range 3745-7500 Å (4240-7140 Å unvignetted) with a spectral resolution of 6.0 Å (FWHM) for 646 galaxies, ii) a medium-resolution V1200 setup covering the wavelength range 3650-4840 Å (3650-4620 Å unvignetted) with a spectral resolution of 2.3 Å (FWHM) for 484 galaxies, and iii) the combination of the cubes from both setups (called COMBO) with a spectral resolution of 6.0 Å and a wavelength range between 3700-7500 Å (3700-7140 Å unvignetted) for 446 galaxies. The Main Sample, selected and observed according to the CALIFA survey strategy covers a redshift range between 0.005 and 0.03, spans the color-magnitude diagram and probes a wide range of stellar masses, ionization conditions, and morphological types. The Extension Sample covers several types of galaxies that are rare in the overall galaxy population and are therefore not numerous or absent in the CALIFA Main Sample. All the cubes in the data release were processed using the latest pipeline, which includes improved versions of the calibration frames and an even further improved image reconstruction quality. In total, the third data release contains 1576 datacubes, including ~1.5 million independent spectra.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
EDP Sciences  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Galaxies: Evolution  
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Galaxies: General  
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Surveys  
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Techniques: Spectroscopic  
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Astronomía  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
CALIFA, the Calar Alto Legacy Integral Field Area survey: IV. Third public data release  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2018-08-15T14:00:28Z  
dc.journal.volume
594  
dc.journal.pais
Francia  
dc.description.fil
Fil: Sánchez, S. F.. Universidad Nacional Autónoma de México; México  
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Fil: Garciá Benito, R.. Instituto de Astrofísica de Andalucía; España  
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Fil: Zibetti, S.. Osservatorio Astrofisico di Arcetri; Italia  
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Fil: Walcher, C. J.. Leibniz-Institut für Astrophysik Potsdam; Alemania  
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Fil: Husemann, B.. European Southern Observatory; Alemania  
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Fil: Mast, Damian. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina  
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Fil: López Fernández, R.. Instituto de Astrofísica de Andalucía; España  
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Fil: López Sánchez, A. R.. Sydney Institute for Astronomy; Australia  
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Fil: Lyubenova, M.. University of Groningen. Kapteyn Astronomical Institute; Países Bajos  
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Fil: Marino, R.. Institut für Astronomie; Suiza  
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Fil: Márquez, I.. Instituto de Astrofísica de Andalucía; España  
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Fil: Mendez Abreu, J.. University of St. Andrews. School of Physics and Astronomy; Reino Unido  
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Fil: Mollá, M.. Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; España  
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Fil: Monreal Ibero, A.. Université Paris Diderot. Observatoire de Paris; Francia  
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Fil: Ortega Minakata, R.. Universidade Federal do Rio de Janeiro. Observatorio do Valongo; Brasil  
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Fil: Torres Papaqui, J. P.. Universidad de Guanajuato. Departamento de Astronomía; México  
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Fil: Pérez, E.. Instituto de Astrofísica de Andalucía; España  
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Fil: Rosales Ortega, F. F.. Instituto Nacional de Astrofísica, Óptica y Electrónica; México  
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Fil: Roth, M. M.. Leibniz-Institut für Astrophysik Potsdam; Alemania  
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Fil: Sánchez Blázquez, P.. Universidad Autónoma de Madrid. Facultad de Ciencias. Departamento de Física Teórica; España  
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Fil: Schilling, U.. Ruhr-Universität Bochum. Astronomisches Institut; Alemania  
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Fil: Spekkens, K.. Royal Military College of Canada. Department of Physics; Canadá  
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Fil: Vale Asari, N.. Universidade Federal de Santa Catarina. Departamento de Física; Brasil  
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Fil: Van Den Bosch, R. C. E.. Max-Planck-Institut für Astronomie; Alemania  
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Fil: Van De Ven, G.. Max-Planck-Institut für Astronomie; Alemania  
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Fil: Vilchez, J. M.. Instituto de Astrofísica de Andalucía; España  
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Fil: Wild, V.. University of St. Andrews. School of Physics and Astronomy; Reino Unido  
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Fil: Wisotzki, L.. Leibniz-Institut für Astrophysik Potsdam; Alemania  
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Fil: Ylldlrlm, A.. Max-Planck-Institut für Astronomie; Alemania  
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Fil: Ziegler, B.. Department of Astrophysics. University of Vienna; Austria  
dc.journal.title
Astronomy and Astrophysics  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1051/0004-6361/201628661  
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info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2016/10/aa28661-16/aa28661-16.html