Browsing by Subject "Galaxies formation"

Now showing items 1-4 of 4

    • A Magellan M2FS spectroscopic survey of galaxies at 5.5 < z < 6.8: program overview and a sample of the ... 
      Jiang, Linhua; Shen, Yue; Bian, Fuyan; Zheng, Zhen Ya; Wu, Jin; Oyarzún, Grecco A.; Blanc Mendiberri, Guillermo; Fan, Xiaohui; Ho, Luis C.; Infante, Leopoldo; Wang, Ran; Wu, Xue Bing; Mateo, Mario; Bailey, John I.; Crane, Jeffrey D.; Olszewski, Edward W; Shectman, Stephen; Thompson, Ian; Walker, Matthew G. (IOP Publishing Ltd, 2017)
      We present a spectroscopic survey of high-redshift, luminous galaxies over four square degrees on the sky, aiming to build a large and homogeneous sample of Ly alpha emitters (LAEs) at z approximate to 5.7 and 6.5, and ...
    • Morpho kinematic properties of field S0 bulges in the CALIFA survey 
      Méndez Abreu, J.; Aguerri, J. A. L.; Falcón Barroso, J.; Galbany, Lluis (Oxford University Press, 2018)
      We study a sample of 28 S0 galaxies extracted from the integral field spectroscopic (IFS) survey Calar Alto Legacy Integral Field Area. We combine an accurate two-dimensional (2D) multicomponent photometric decomposition ...
    • The evolution of the star formation rate function in the Eagle simulations: a comparison with UV, IR and H ... 
      Katsianis, A.; Blanc Mendiberri, Guillermo; Lagos, C. P.; Tejos, Nicolás; Bower, R. G.; Alavi, A.; González Corvalán, Valentino; Theuns, T.; Schaller, M.; López Morales, Sebastián (Oxford university press, 2017)
      We investigate the evolution of the galaxy star formation rate function (SFRF) and cosmic star formation rate density (CSFRD) of z similar to 0-8 galaxies in the Evolution and Assembly of GaLaxies and their Environments ...
    • The rest-frame optical (900nm) galaxy luminosity function at z∼4–7: abundance matching points to limited ... 
      Stefanon, Mauro; Bouwens, Rychard J.; Labbé, Ivo; Muzzin, Adam; Marchesini, Danilo; Oesch, Pascal; González Corvalán, Valentino (IOP Publishing Ltd., 2017)
      We present the first determination of the galaxy luminosity function (LF) at z ∼4, 5, 6, and 7, in the rest-frame optical at l ~ rest 900 nm (z′ band). The rest-frame optical light traces the content in low-mass evolved ...