Publicaciones en las que colabora con PABLO GUILLERMO PÉREZ GONZÁLEZ (55)

2020

  1. Integral field spectroscopy and multi-wavelength imaging of the nearby spiral galaxy ngc 5668: A case for megara

    Proceedings of the 10th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics VII, SEA 2012

2013

  1. EXPLORING THE STAR FORMING REGIONS IN VIGOROUS STAR FORMING GALAXIES AT Z=0.84

    FOURTH SCIENCE MEETING WITH THE GTC

  2. Evolutionary paths among different red galaxy types at 0.3 < z < 1.5 and the late buildup of massive E-S0s through major mergers

    Monthly Notices of the Royal Astronomical Society, Vol. 428, Núm. 2, pp. 999-1019

  3. Exploring the star forming regions in vigorous star forming galaxies at Z = 0.84

    Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias

  4. INTEGRAL FIELD SPECTROSCOPY AND MULTI-WAVELENGTH IMAGING OF NEARBY SPIRAL GALAXIES: NGC 5668 AS A PILOT CASE FOR MEGARA

    FOURTH SCIENCE MEETING WITH THE GTC

  5. Integral field spectroscopy and multi-wavelength imaging of nearby spiral galaxies: NGC 5668 as a pilot case for MEGARA

    Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias

  6. MEGARA: The future ifu and MOS of the 10.4 M GTC

    Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias

  7. SPECTROPHOTOMETRIC STUDY IN THE NEAR-IR OF A SAMPLE OF MIPS SELECTED GALAXIES AT Z similar to 2

    FOURTH SCIENCE MEETING WITH THE GTC

  8. Shards: An optical spectro-photometric survey of distant galaxies

    Astrophysical Journal, Vol. 762, Núm. 1

  9. Spectrophotometric study in the near-ir of a sample of mips selected galaxies ATZ∼2

    Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias

  10. THE EVOLUTIONARY PATHS AMONG GALAXY TYPES ON THE RED SEQUENCE AT 0.3 < Z < 1.5

    FOURTH SCIENCE MEETING WITH THE GTC

  11. The evolutionary paths among galaxy types on the Red Sequence at 0.3 < Z < 1.5

    Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias

2010

  1. Deconstructing the K-Band Number Counts

    HIGHLIGHTS OF SPANISH ASTROPHYSICS V