WINGS-SPE II: A catalog of stellar ages and star formation histories, stellar masses and dust extinction values for local clusters galaxies
J. FritzINAF-Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, 35122 Padova, ItalyB. M. PoggiantiINAF-Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, 35122 Padova, ItalyA. CavaDepartamento de Astrofísica, Universidad de La Laguna, 38205 , La Laguna, Tenerife, SpainT. ValentinuzziDipartimento di Astronomia, vicolo Osservatorio 2, 35122 Padova, ItalyA. MorettiINAF-Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, 35122 Padova, ItalyD. BettoniINAF-Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, 35122 Padova, ItalyA. BressanINAF-Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, 35122 Padova, ItalyW. J. CouchCentre for Astrophysics and Supercomputing, Swinburne University of Technology, Melbourne, AustraliaM. D’OnofrioDipartimento di Astronomia, vicolo Osservatorio 2, 35122 Padova, ItalyA. DresslerObservatories of the Carnegie Institution of Washington, Pasadena, CA 91101, USAG. FasanoINAF-Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, 35122 Padova, ItalyP. KjærgaardCopenhagen University Observatory. The Niels Bohr Insitute for Astronomy Physics and Geophysics, Juliane Maries Vej 30, 2100 Copenhagen, DenmarkM. MolesInstituto de Astrofísica de Andalucía (C.S.I.C.) Apartado 3004, 18080 Granada, SpainA. OmizzoloINAF-Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, 35122 Padova, ItalyJ. VarelaINAF-Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, 35122 Padova, Italy
2010en
ABI
Аннотация
Context. The WIde-field Nearby Galaxy clusters Survey (wings) is a project whose primary goal is to study the galaxy populations in clusters in the local universe (z < 0.07) and of the influence of environment on their stellar populations. This survey has provided the astronomical community with a high quality set of photometric and spectroscopic data for 77 and 48 nearby galaxy clusters, respectively.
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