The Herschel★ PEP/HerMES luminosity function – I. Probing the evolution of PACS selected Galaxies to z ≃ 4
C. GruppioniINAF – Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127 Bologna, ItalyF. PozziDipartimento di Astronomia, Università di Bologna, via Ranzani 1, I-40127 Bologna, ItalyL. BisigelloDipartimento di Astronomia, Università di Padova, vicolo dell'Osservatorio 3, I-35122 Padova, ItalyI. DelvecchioDipartimento di Astronomia, Università di Bologna, via Ranzani 1, I-40127 Bologna, ItalyS. BertaMax-Planck-Institut für Extraterrestrische Physik (MPE), Postfach 1312, D-85741 Garching, GermanyL. PozzettiINAF – Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127 Bologna, ItalyG. ZamoraniINAF – Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127 Bologna, ItalyP. AndreaniA. CimattiDipartimento di Astronomia, Università di Bologna, via Ranzani 1, I-40127 Bologna, ItalyO. IlbertLaboratoire d'Astrophysique de Marseille, CNRS-Universitè de Provence, rue Frèdèric Joliot-Curie 38, F-13388 Marseille Cedex 13, FranceE. Le Floc’hCEA-Saclay, Service d'Astrophysique, F-91191 Gif-sur-Yvette, FranceD. LutzMax-Planck-Institut für Extraterrestrische Physik (MPE), Postfach 1312, D-85741 Garching, GermanyB. MagnelliMax-Planck-Institut für Extraterrestrische Physik (MPE), Postfach 1312, D-85741 Garching, GermanyL. MarchettiDepartment of Physical Sciences, The Open University, Milton Keynes MK7 6AA, UKPierluigi MonacoR. NordonMax-Planck-Institut für Extraterrestrische Physik (MPE), Postfach 1312, D-85741 Garching, GermanyS. OliverAstronomy Centre, Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, UKP. PopessoMax-Planck-Institut für Extraterrestrische Physik (MPE), Postfach 1312, D-85741 Garching, GermanyL. RigucciniCEA-Saclay, Service d'Astrophysique, F-91191 Gif-sur-Yvette, FranceI. G. RoseboomAstronomy Centre, Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, UKD. J. RosarioMax-Planck-Institut für Extraterrestrische Physik (MPE), Postfach 1312, D-85741 Garching, GermanyM. SargentCEA-Saclay, Service d'Astrophysique, F-91191 Gif-sur-Yvette, FranceM. VaccariAstrophysics Group, Department of Physics, University of Western Cape, Bellville 7535, Cape Town, South AfricaB. AltieriESA Herschel Science Center, Villafranca del Castillo, E-28692 Madrid, SpainH. AusselCEA-Saclay, Service d'Astrophysique, F-91191 Gif-sur-Yvette, FranceÁ. BongiovanniInstituto de Astrofísica de Canarias, E-38205 La Laguna, SpainJ. CepaInstituto de Astrofísica de Canarias, E-38205 La Laguna, SpainE. DaddiCEA-Saclay, Service d'Astrophysique, F-91191 Gif-sur-Yvette, FranceH. Domínguez-SánchezINAF – Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127 Bologna, ItalyD. ElbazCEA-Saclay, Service d'Astrophysique, F-91191 Gif-sur-Yvette, FranceN. Förster SchreiberMax-Planck-Institut für Extraterrestrische Physik (MPE), Postfach 1312, D-85741 Garching, GermanyR. GenzelMax-Planck-Institut für Extraterrestrische Physik (MPE), Postfach 1312, D-85741 Garching, GermanyÁlvaro IribarremESO, Karl-Schwarzschild-Strasse 2, D-85748 Garching, GermanyM. MagliocchettiINAF–IFSI, Via Fosso del Cavaliere 100, I-00133 Roma, ItalyR. MaiolinoCavendish Laboratory, University of Cambridge, 19 J. J. Thomson Ave., Cambridge CB3 0HE, UKA. PoglitschMax-Planck-Institut für Extraterrestrische Physik (MPE), Postfach 1312, D-85741 Garching, GermanyA. M. Pérez GarcíaESA Herschel Science Center, Villafranca del Castillo, E-28692 Madrid, SpainM. Sánchez‐PortalESA Herschel Science Center, Villafranca del Castillo, E-28692 Madrid, SpainE. SturmMax-Planck-Institut für Extraterrestrische Physik (MPE), Postfach 1312, D-85741 Garching, GermanyL. J. TacconiMax-Planck-Institut für Extraterrestrische Physik (MPE), Postfach 1312, D-85741 Garching, GermanyI. ValtchanovESA Herschel Science Center, Villafranca del Castillo, E-28692 Madrid, SpainA. AmblardNASA, Ames Research Center, Moett Field, CA 94035, USAV. ArumugamInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UKM. BétherminCEA-Saclay, Service d'Astrophysique, F-91191 Gif-sur-Yvette, FranceJ. BöckJet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USAA. BoselliLaboratoire d'Astrophysique de Marseille, CNRS-Universitè de Provence, rue Frèdèric Joliot-Curie 38, F-13388 Marseille Cedex 13, FranceV. BuatLaboratoire d'Astrophysique de Marseille, CNRS-Universitè de Provence, rue Frèdèric Joliot-Curie 38, F-13388 Marseille Cedex 13, FranceD. BurgarellaLaboratoire d'Astrophysique de Marseille, CNRS-Universitè de Provence, rue Frèdèric Joliot-Curie 38, F-13388 Marseille Cedex 13, FranceN. Castro-RodríguezInstituto de Astrofísica de Canarias, E-38205 La Laguna, SpainA. CavaDepartamento de Astrofísica, Facultad de CC. Físicas, Universidad Complutense de Madrid, E-28040 Madrid, SpainA. ChallinorCEA-Saclay, Service d'Astrophysique, F-91191 Gif-sur-Yvette, FranceD. L. ClementsAstrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, UKA. ConleyCenter for Astrophysics and Space Astronomy 389-UCB, University of Colorado, Boulder, CO 80309, USAAsantha CoorayDepartment of Physics and Astronomy, University of California, Irvine, CA 92697, USAC. D. DowellCalifornia Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125, USAE. DwekObservational Cosmology Lab, Code 665, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USAS. EalesSchool of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff CF24 3AA, UKA. FranceschiniDipartimento di Astronomia, Università di Padova, vicolo dell'Osservatorio 3, I-35122 Padova, ItalyJ. GlennDepartment of Astrophysical and Planetary Sciences, CASA 389-UCB, University of Colorado, Boulder, CO 80309, USAMatt GriffinSchool of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff CF24 3AA, UKE. HatziminaoglouE. IbarUK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UKK. G. IsaakESA Research and Scientific Support Department, ESTEC/SRE-SA, Keplerlaan 1, 2201 AZ Noordwijk, the NetherlandsR. J. IvisonUK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UKG. LagacheInstitut d'Astrophysique Spatiale, batiment 121, Universitè Paris-Sud 11 and CNRS (UMR 8617), F-91405 Orsay, FranceL. LevensonCalifornia Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125, USAN. LuInfrared Processing and Analysis Center, MS 100-22, California Institute of Technology, JPL, Pasadena, CA 91125, USAS. C. MaddenCEA-Saclay, Service d'Astrophysique, F-91191 Gif-sur-Yvette, FranceB. MaffeiSchool of Physics and Astronomy, The University of Manchester, Alan Turing Building, Oxford Road, Manchester M13 9PL, UKG. MainettiDipartimento di Astronomia, Università di Padova, vicolo dell'Osservatorio 3, I-35122 Padova, ItalyH. T. NguyenJet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USAB. O’HalloranAstrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, UKM. J. PageMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UKP. PanuzzoCEA-Saclay, Service d'Astrophysique, F-91191 Gif-sur-Yvette, FranceΑνδρέας ΠαπαγεωργίουSchool of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff CF24 3AA, UKC. P. PearsonRAL Space, Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire OX11 0QX, UKI. Pérez-FournonDepartamento de Astrofísica, Universidad de La Laguna (ULL), E-38205 La Laguna, Tenerife, SpainM. PohlenSchool of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff CF24 3AA, UKD. RigopoulouDepartment of Astrophysics, Denys Wilkinson Building, University of Oxford, Keble Road, Oxford OX1 3RH, UKM. Rowan-RobinsonAstrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, UKB. SchulzInfrared Processing and Analysis Center, MS 100-22, California Institute of Technology, JPL, Pasadena, CA 91125, USAD. ScottDepartment of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, CanadaN. SeymourCSIRO Astronomy and Space Science, PO Box 76, Epping, NSW 1710, AustraliaD. L. ShupeInfrared Processing and Analysis Center, MS 100-22, California Institute of Technology, JPL, Pasadena, CA 91125, USAA. J. SmithAstronomy Centre, Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, UKJ. A. StevensCentre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, Hertfordshire AL10 9AB, UKM. SymeonidisMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UKM. TrichasHarvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USAK. E. TugwellMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UKL. VigrouxInstitut d'Astrophysique de Paris, UMR 7095, CNRS, UPMC Univ. Paris 06, 98bis boulevard Arago, F-75014 Paris, FranceL. WangAstronomy Centre, Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, UKGeraldine A. WrightUK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UKC. K. XuInfrared Processing and Analysis Center, MS 100-22, California Institute of Technology, JPL, Pasadena, CA 91125, USAM. ZemcovJet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USAS. BardelliINAF – Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127 Bologna, ItalyC. M. CarolloT. ContiniInstitut de Recherche en Astrophysique et Plantologie, CNRS, Universit de Toulouse, 14 avenue E. Belin, F-31400 Toulouse, FranceO. Le FèvreLaboratoire d'Astrophysique de Marseille, CNRS-Universitè de Provence, rue Frèdèric Joliot-Curie 38, F-13388 Marseille Cedex 13, FranceS. J. LillyV. Mainieri
2013en
ABI
Аннотация
Understanding the origin and growth of the galaxies we ob- \nserve today is one of the main problems of current cosmol- \nogy. The luminosity function (LF) provides one of the fun- \ndamental tools to probe the distribution of galaxies over \ncosmological time, since it allows us to assess the statisti- \ncal nature of galaxy formation and evolution. When com- \nputed at di erent redshifts, the LF constitutes the most di- \nrect method for exploring the evolution of a galaxy popula- \ntion, describing the relative number of sources of di erent \nluminosities counted in representative volumes of the Uni- \nverse. The LF computed for di erent samples of galaxies \ncan provide a crucial comparison between the distribution \nof di erent galaxy types, i.e. galaxies at di erent redshifts, \nin di erent enviroments or selected at di erent wavelengths.
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