Publicaciones en las que colabora con IGNACIO NEGUERUELA DIEZ (67)

2024

  1. The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

    Monthly Notices of the Royal Astronomical Society, Vol. 530, Núm. 3, pp. 2688-2730

2021

  1. A massive open cluster hiding in full sight

    Monthly Notices of the Royal Astronomical Society, Vol. 505, Núm. 2, pp. 1618-1628

2018

  1. An atlas of cool supergiants from the Magellanic Clouds and typical interlopers: A guide for the classification of luminous red stars

    Astronomy and Astrophysics, Vol. 618

  2. Berkeley 51, a young open cluster with four yellow supergiants

    Monthly Notices of the Royal Astronomical Society, Vol. 477, Núm. 3, pp. 2976-2990

  3. Clusters with K-type (super)giants

    Proceedings of the 13th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics X, SEA 2018

  4. How do massive stars form? Finding targets for MIRADAS

    Proceedings of the 13th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics X, SEA 2018

  5. NGC 3105: A young open cluster with low metallicity

    Astronomy and Astrophysics, Vol. 616

2017

  1. Confirmation of six Be X-ray binaries in the Small Magellanic Cloud

    Monthly Notices of the Royal Astronomical Society, Vol. 467, Núm. 2, pp. 1526-1530

  2. NGC 6067: A young and massive open cluster with high metallicity

    Monthly Notices of the Royal Astronomical Society, Vol. 469, Núm. 2, pp. 1330-1353

  3. Open clusters as laboratories for the AGB/SN mass transition

    Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society

  4. The little-studied cluster Berkeley 90 - III. Cluster parameters

    Monthly Notices of the Royal Astronomical Society, Vol. 465, Núm. 1, pp. 784-797

  5. The young open cluster NGC 7067 using Strömgren photometry

    Monthly Notices of the Royal Astronomical Society, Vol. 466, Núm. 3, pp. 3636-3647

2016

  1. Exploring the Obscured Milky Way with Multi-Object Spectroscopy

    MULTI-OBJECT SPECTROSCOPY IN THE NEXT DECADE: BIG QUESTIONS, LARGE SURVEYS, AND WIDE FIELDS