Publicaciones en colaboración con investigadores/as de Osservatorio Astronomico di Capodimonte (6)

2022

  1. MAGAZ3NE: High Stellar Velocity Dispersions for Ultramassive Quiescent Galaxies at z ≳ 3* * The spectra presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.

    Astrophysical Journal, Vol. 938, Núm. 2

2020

  1. An Extremely Massive Quiescent Galaxy at z = 3.493: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models

    Astrophysical Journal Letters, Vol. 890, Núm. 1

  2. The Massive Ancient Galaxies at z > 3 NEar-infrared (MAGAZ3NE) Survey: Confirmation of Extremely Rapid Star Formation and Quenching Timescales for Massive Galaxies in the Early Universe*

    Astrophysical Journal, Vol. 903, Núm. 1

  3. The Rapid buildup of massive early-type galaxies: Supersolar metallicity, high velocity dispersion, and young age for an early-type galaxy at z = 3.35

    Astrophysical Journal, Vol. 905, Núm. 1

2010

  1. A path to the stars: The evolution of the species

    Advances in Astronomy, Vol. 2010

  2. A path to the stars: The evolution of the species in the hunting to the GRBs

    Proceedings of SPIE - The International Society for Optical Engineering