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Formation Epochs, Star Formation Histories, and Sizes of Massive Early-Type Galaxies in Cluster and Field Environments at z = 1.2: Insights from the Rest-Frame Ultraviolet

  • Authors: Alessandro Rettura, P. Rosati, M. Nonino, R. A. E. Fosbury, R. Gobat, N. Menci, V. Strazzullo, S. Mei, R. Demarco, and H. C. Ford

RETTURA et al. 2010 The Astrophysical Journal 709 512.

  • Provider: AAS Journals

Caption: Figure 2.

Top panel: iK s vs. Vi color–color plot of BC03 CSP models at z = 1.24 superimposed on our GOODS ETG photometry at z = 1.24 ± 0.15 in blue circles. The squares account for SFHs with various τ models. The grids are drawn for seven different τ's and five ages (2, 2.5, 3, 3.5, and 4 Gyr): the colored lines represent iso-metallicity colors of Z . The black arrow indicates an extinction of E( BV) = 0.2 as parameterized with the reddening curve of (Cardelli et al. 1989). Bottom left panel: iK s vs. Bi color–color diagram of the same models and data: B band (λ rest ~ 2000 Å) is mandatory to break the age–SFH degeneracy at z = 1.24.

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