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CALIFA: a diameter-selected sample for an integral field spectroscopy galaxy survey

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dc.contributor.authorWalcher, C. J.
dc.contributor.authorWisotzki, L.
dc.contributor.authorBekeraite, S.
dc.contributor.authorHusemann, B.
dc.contributor.authorIglesias Páramo, J.
dc.contributor.authorBacksmann, N.
dc.contributor.authorBarrera Ballesteros, J.
dc.contributor.authorCatalán Torrecilla, Cristina
dc.contributor.authorCortijo, C.
dc.contributor.authorOlmo, A. del
dc.contributor.authorGarcía Lorenzo, B.
dc.contributor.authorFalcón Barroso, J.
dc.contributor.authorJilkova, L.
dc.contributor.authorKalinova, V.
dc.contributor.authorMast, D.
dc.contributor.authorMarino, Raffaella Anna
dc.contributor.authorMéndez Abreu, J.
dc.contributor.authorPasquali, A.
dc.contributor.authorSánchez, S. F.
dc.contributor.authorTrager, S.
dc.contributor.authorZibetti, S.
dc.contributor.authorAguerri, J. A. L.
dc.contributor.authorAlves, J.
dc.contributor.authorBland-Hawthorn, J.
dc.contributor.authorBoselli, A.
dc.contributor.authorCastillo Morales, María África
dc.contributor.authorCid Fernandes, R.
dc.contributor.authorFlores, H.
dc.contributor.authorGalbany, L.
dc.contributor.authorGallazzi, A.
dc.contributor.authorGarcía Benito, R.
dc.contributor.authorGil De Paz, Armando
dc.contributor.authorGonzález Delgado, R. M.
dc.contributor.authorJahnke, K.
dc.contributor.authorJungwiert, B.
dc.contributor.authorKehrig, C.
dc.contributor.authorLyubenova, M.
dc.contributor.authorMárquez Pérez, I.
dc.contributor.authorMasegosa, J.
dc.contributor.authorMonreal Ibero, A.
dc.contributor.authorPérez, E.
dc.contributor.authorQuirrenbach, A.
dc.contributor.authorRosales Ortega, F. F.
dc.contributor.authorRoth, M. M.
dc.contributor.authorSánchez Blázquez, Patricia
dc.contributor.authorSpekkens, K.
dc.contributor.authorTundo, E.
dc.contributor.authorvan de Ven, G.
dc.contributor.authorVerheijen, M. A. W.
dc.contributor.authorVílchez, J. V
dc.contributor.authorZiegler, B.
dc.date.accessioned2023-06-19T13:27:30Z
dc.date.available2023-06-19T13:27:30Z
dc.date.issued2014-09
dc.description© ESO 2014. This study makes uses of the data provided by the Calar Alto Legacy Integral Field Area (CALIFA) survey (http://califs.caha.es). CALIFA is the first legacy survey being performed at Calar Alto. The CALIFA collaboration would like to thank the IAA-CSIC and MPIA-MPG as major partners of the observatory, and CAHA itself, for the unique access to telescope time and support in manpower and infrastructures. The CALIFA collaboration thanks also the CAHA staff for the dedication to this project. We thank Mike Blanton for helpful discussions on the SDSS survey footprint and for providing the NYU low-z catalogue to the community. CJW acknowledges useful discussion with Nick Scott, Davor Krajnovic and Remco van den Bosch as well as support through the Marie Curie Career Integration Grant 303912. We thank the anonymous referee for a careful reading of the paper and several suggestions that improved its presentation. IM acknowledges the financial support from the Spanish grant AYA2010-15169 and from the Junta de Andalucía through TIC-114 and the Excellence Project P08-TIC-03531. R.G.D., E.P. and R.G.B. acknowledge support from the Spanish Ministerio de Economía y Competitividad, through projects AYA2010-15081. RAM is funded by the Spanish programme of International Campus of Excellence Moncloa (CEI). J.I.P. acknowledges financial support from the Spanish MINECO under grant AYA2010-21887-C04-01 and from Junta de Andalucía Excellence Project PEX2011-FQM7058. Support for L.G. is provided by the Ministry of Economy, Development, and Tourism's Millennium Science Initiative through grant IC12009, awarded to The Millennium Institute of Astrophysics, MAS. L.G. acknowledges support by CONICYT through FONDECYT grant 3140566. AM.-I. acknowledges support from Agence Nationale de la Recherche through the STILISM project (ANR-12-BS05-0016-02). AM.-I. and S.B. acknowledge support from BMBF through the Erasmus-F project (grant number 05 A12BA1). JMA acknowledges support from the European Research Council Starting Grant (SEDmorph; P.I. V. Wild). A.G. acknowledges funding from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement No. 267251. K.S. acknowledges financial support from the Natural Sciences and Engineering Research Council of Canada (NSERC). B.J. acknowledges support by the projects RVO67985815 and M100031201 of the Academy of Sciences of the Czech Republic. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. We acknowledge the usage of the HyperLeda database (http://leda.univ-lyon1.fr). Funding for the Sloan Digital Sky Survey (SDSS) has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Aeronautics and Space Administration, the National Science Foundation, the US Department of Energy, the Japanese Monbukagakusho, and the Max Planck Society. The SDSS Web site is http://www.sdss.org/. The SDSS is managed by the Astrophysical Research Consortium (ARC) for the Participating Institutions.The Participating Institutions are The University of Chicago, Fermilab, the Institute for Advanced Study, the Japan Participation Group, The Johns Hopkins University, Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, University of Pittsburgh, Princeton University, the United States Naval Observatory, and the University of Washington.
dc.description.abstractWe 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 < z < 0 : 03. The mother sample contains 939 objects, 600 of which will be observed in the course of the CALIFA survey. The selection of targets for observations is based solely on visibility and thus keeps the statistical properties of the mother sample. By comparison with a large set of SDSS galaxies, we find that the CALIFA sample is representative of galaxies over a luminosity range of -19 > 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 < 10(9.7) M-circle dot) is there a prevalence of galaxies with larger isophotal sizes, especially of nearly edge-on late-type galaxies, but such galaxies form < 10% of the full sample. We estimate volume-corrected distribution functions in luminosities and sizes and show that these are statistically fully compatible with estimates from the full SDSS when accounting for large-scale structure. For full characterization of the sample, we also present a number of value-added quantities determined for the galaxies in the CALIFA sample. These include consistent multi-band photometry based on growth curve analyses; stellar masses; distances and quantities derived from these; morphological classifications; and an overview of available multi-wavelength photometric measurements. We also explore different ways of characterizing the environments of CALIFA galaxies, finding that the sample covers environmental conditions from the field to genuine clusters. We finally consider the expected incidence of active galactic nuclei among CALIFA galaxies given the existing pre-CALIFA data, finding that the final observed CALIFA sample will contain approximately 30 Sey2 galaxies.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMarie Curie Career Integration Grant
dc.description.sponsorshipJunta de Andalucía
dc.description.sponsorshipMinisterio de Economia y Competitividad (MINECO)
dc.description.sponsorshipSpanish programme of International Campus of Excellence Moncloa (CEI)
dc.description.sponsorshipUnión Europea. FP7
dc.description.sponsorshipMinistry of Economy, Development, and Tourism's Millennium Science Initiative
dc.description.sponsorshipCONICYT through FONDECYT
dc.description.sponsorshipAgence Nationale de la Recherche through the STILISM project
dc.description.sponsorshipBMBF through the Erasmus-F project
dc.description.sponsorshipEuropean Research Council
dc.description.sponsorshipEuropean Union
dc.description.sponsorshipNatural Sciences and Engineering Research Council of Canada (NSERC)
dc.description.sponsorshipAcademy of Sciences of the Czech Republic
dc.description.sponsorshipNational Aeronautics and Space Administration
dc.description.sponsorshipAlfred P. Sloan Foundation
dc.description.sponsorshipNational Science Foundation
dc.description.sponsorshipUS Department of Energy
dc.description.sponsorshipJapanese Monbukagakusho
dc.description.sponsorshipMax Planck Society
dc.description.sponsorshipAstrophysical Research Consortium (ARC)
dc.description.sponsorshipUniversity of Chicago
dc.description.sponsorshipFermilab
dc.description.sponsorshipInstitute for Advanced Study
dc.description.sponsorshipJapan Participation Group
dc.description.sponsorshipJohns Hopkins University
dc.description.sponsorshipLos Alamos National Laboratory
dc.description.sponsorshipMax-Planck-Institute for Astronomy (MPIA)
dc.description.sponsorshipMax-Planck-Institute for Astrophysics (MPA)
dc.description.sponsorshipNew Mexico State University
dc.description.sponsorshipUniversity of Pittsburgh
dc.description.sponsorshipPrinceton University
dc.description.sponsorshipUnited States Naval Observatory
dc.description.sponsorshipUniversity of Washington
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/28159
dc.identifier.doi10.1051/0004-6361/201424198
dc.identifier.issn0004-6361
dc.identifier.officialurlhttp://arxiv.org/pdf/1407.2939.pdf
dc.identifier.relatedurlhttp://www.aanda.org
dc.identifier.urihttps://hdl.handle.net/20.500.14352/33757
dc.journal.titleAstronomy & Astrophysics
dc.language.isoeng
dc.publisherEDP Sciencies
dc.relation.projectIDSFEHG (303912)
dc.relation.projectIDAstroFIt (267251)
dc.relation.projectIDAYA2010-15169
dc.relation.projectIDAYA2010-15081
dc.relation.projectIDAYA2010-21887-C04-01
dc.relation.projectIDTIC-114
dc.relation.projectIDP08-TIC-03531
dc.relation.projectIDPEX2011-FQM7058
dc.relation.projectIDIC12009
dc.relation.projectID3140566
dc.relation.projectIDANR-12-BS05-0016-02
dc.relation.projectID05 A12BA1
dc.relation.projectIDRVO67985815
dc.relation.projectIDM100031201
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordDigital Sky Survey
dc.subject.keywordPotsdam Multiaperture Spectrophotometer
dc.subject.keywordActive Galactic Nuclei
dc.subject.keywordX-Sigma Relation
dc.subject.keywordRedshift Survey
dc.subject.keywordLuminosity Function
dc.subject.keywordTarget Selection
dc.subject.keywordNearby Galaxies
dc.subject.keywordDisk Galaxies
dc.subject.keywordVirgo Cluster.
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.subject.ucmFísica atmosférica
dc.subject.unesco2501 Ciencias de la Atmósfera
dc.titleCALIFA: a diameter-selected sample for an integral field spectroscopy galaxy survey
dc.typejournal article
dc.volume.number569
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