Publicaciones en colaboración con investigadores/as de York University (Canadá) (25)

2024

  1. Bulge+disc decomposition of HFF and CANDELS galaxies: UVJ diagrams and stellar mass-size relations of galaxy components at 0.2 ≤ z ≤ 1.5

    Monthly Notices of the Royal Astronomical Society, Vol. 532, Núm. 4, pp. 3747-3777

  2. Most of the photons that reionized the Universe came from dwarf galaxies

    Nature, Vol. 626, Núm. 8001, pp. 975-978

  3. The JWST UNCOVER Treasury Survey: Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization

    Astrophysical Journal, Vol. 974, Núm. 1

  4. The JWST-SUSPENSE Ultradeep Spectroscopic Program: Survey Overview and Star Formation Histories of Quiescent Galaxies at 1 < z < 3

    Astrophysical Journal, Vol. 973, Núm. 2

  5. The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning 0.2 ≲ z ≲ 15

    Astrophysical Journal, Supplement Series, Vol. 270, Núm. 1

2022

  1. Extending the evolution of the stellar mass–size relation at z ≤ 2 to low stellar mass galaxies from HFF and CANDELS

    Monthly Notices of the Royal Astronomical Society, Vol. 506, Núm. 1, pp. 928-956

  2. Finite-resolution Deconvolution of Multiwavelength Imaging of 20,000 Galaxies in the COSMOS Field: The Evolution of Clumpy Galaxies over Cosmic Time

    Astrophysical Journal, Vol. 924, Núm. 1

  3. 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

  4. The Number Densities and Stellar Populations of Massive Galaxies at 3 < z < 6: A Diverse, Rapidly Forming Population in the Early Universe

    Astrophysical Journal, Vol. 924, Núm. 1

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 GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0 < z < 1.4 and the complex nature of satellite quenching

    Astronomy and Astrophysics, Vol. 638

  3. 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

  4. 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

2019

  1. HST F160W imaging of very massive galaxies at 1.5 < z < 3.0: Diversity of structures and the effect of close pairs on number density estimates

    Astrophysical Journal, Vol. 871, Núm. 2

  2. Stellar and Dust Properties of a Complete Sample of Massive Dusty Galaxies at 1 ≤ z ≤ 4 from MAGPHYS Modeling of UltraVISTA DR3 and Herschel Photometry

    Astrophysical Journal, Vol. 882, Núm. 1

  3. The Brightest z ⪆ 8 Galaxies over the COSMOS UltraVISTA Field

    Astrophysical Journal, Vol. 883, Núm. 1

  4. The Rest-frame H-band Luminosity Function of Red-sequence Galaxies in Clusters at 1.0 < z < 1.3

    Astrophysical Journal, Vol. 880, Núm. 2

2018

  1. Complete IRAC Mapping of the CFHTLS-DEEP, MUSYC, and NMBS-II Fields

    Publications of the Astronomical Society of the Pacific, Vol. 130, Núm. 994

  2. HFF-DeepSpace Photometric Catalogs of the 12 Hubble Frontier Fields, Clusters, and Parallels: Photometry, Photometric Redshifts, and Stellar Masses

    Astrophysical Journal, Supplement Series, Vol. 235, Núm. 1

  3. Precise weak lensing constraints from deep high-resolution K s images: VLT/HAWK-I analysis of the super-massive galaxy cluster RCS2 J 232727.7-020437 at z = 0.70

    Astronomy and Astrophysics, Vol. 610