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Título:
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CALIFA: a diameter-selected sample for an integral field spectroscopy galaxy survey
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Autores:
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Walcher, C. J. ;
Wisotzki, L. ;
Bekeraite, S. ;
Husemann, B. ;
Iglesias Páramo, J. ;
Backsmann, N. ;
Barrera Ballesteros, J. ;
Catalán Torrecilla, Cristina ;
Cortijo, C. ;
Olmo, A. del ;
García Lorenzo, B. ;
Falcón Barroso, J. ;
Jilkova, L. ;
Kalinova, V. ;
Mast, D. ;
Marino, Raffaella Anna ;
Méndez Abreu, J. ;
Pasquali, A. ;
Sánchez, S. F. ;
Trager, S. ;
Zibetti, S. ;
Aguerri, J. A. L. ;
Alves, J. ;
Bland-Hawthorn, J. ;
Boselli, A. ;
Castillo Morales, África ;
Cid Fernandes, R. ;
Flores, H. ;
Galbany, L. ;
Gallazzi, A. ;
García Benito, R. ;
Gil de Paz, Armando ;
González Delgado, R. M. ;
Jahnke, K. ;
Jungwiert, B. ;
Kehrig, C. ;
Lyubenova, M. ;
Márquez Pérez, I. ;
Masegosa, J. ;
Monreal Ibero, A. ;
Pérez, E. ;
Quirrenbach, A. ;
Rosales Ortega, F. F. ;
Roth, M. M. ;
Sánchez Blázquez, P. ;
Spekkens, K. ;
Tundo, E. ;
van de Ven, G. ;
Verheijen, M. A. W. ;
Vílchez, J. V ;
Ziegler, B.
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Tipo de documento:
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texto impreso
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Editorial:
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EDP Sciencies, 2014-09
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Dimensiones:
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application/pdf
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Nota general:
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info:eu-repo/semantics/openAccess
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Idiomas:
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Palabras clave:
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Estado = Publicado
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Materia = Ciencias: Física: Astrofísica
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Materia = Ciencias: Física: Astronomía
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Materia = Ciencias: Física: Física atmosférica
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Tipo = Artículo
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Resumen:
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We describe and discuss the selection procedure and statistical properties of the galaxy sample used by the Calar Alto Legacy Integral Field Area (CALIFA) survey, a public legacy survey of 600 galaxies using integral field spectroscopy. The CALIFA "mother sample" was selected from the Sloan Digital Sky Survey (SDSS) DR7 photometric catalogue to include all galaxies with an r-band isophotal major axis between 45 '' and 79 : 2 '' and with a redshift 0 : 005 M-r > -23 : 1 and over a stellar mass range between 10(9.7) and 10(11.4) M-circle dot. In particular, within these ranges, the diameter selection does not lead to any significant bias against - or in favour of - intrinsically large or small galaxies. Only below luminosities of M-r = -19 (or stellar masses
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En línea:
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https://eprints.ucm.es/id/eprint/28159/1/catalantorrecilla02preprint.pdf
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