Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • Thesis
    DETAILED STELLAR POPULATION ANALYSIS OF EARLY-TYPE GALAXIES WITH REDSHIFT TO CONSTRAIN THEIR EVOLUTION
    Una de las cuestiones básicas de la Astronomía moderna es cómo las galaxias de las diferentes familias han evolucionado desde su formación. Una de estas familias, las galaxias de tipos tempranos (ETGs, del inglés Early-Type Galaxy), formadas por galaxias elípticas y lenticulares y que contienen la mayor parte de la materia luminosa del Universo, ha
    Anna Ferré Mateu

    Advertised on:

    5
    2013
    Bibcode
    TESIS
  • Thesis
    BÚSQUEDA DE LA MATERIA BARIÓNICA EN EL SUPERCÚMULO DE CORONA BOREALIS
    Uno de los parámetros mas relevantes en la descripción del Universo es la densidad bariónica media. Esta ha sido estimada a través de las abundancias de los elementos primordiales y confirmada en estudios recientes del espectro de potencias del Fondo Cósmico de Microondas (FCM). Sin embargo, las observaciones de la materia bariónica en el universo
    Carmen Pilar Padilla Torres

    Advertised on:

    7
    2013
    Bibcode
    TESIS
  • Refereed
    Integral Field Spectroscopy of Planetary Nebulae with MUSE
    The Multi-Unit Spectroscopic Explorer (MUSE) is a large integral field unit mounted on the ESO Very Large Telescope. Its spatial (60 arcsecond field) and wavelength (4800-9300Å) coverage is well suited to detailed imaging spectroscopy of extended planetary nebulae, such as in the Galaxy. An overview of the capabilities of MUSE applied to Planetary
    Walsh, Jeremy R. et al.

    Advertised on:

    4
    2020
    Bibcode
    2020Galax...8...31W
    Citations
    7
  • Refereed
    A prediction about the age of thick discs as a function of the stellar mass of the host galaxy
    One of the suggested thick disc formation mechanisms is that they were born quickly and in situ from a turbulent clumpy disc. Subsequently, thin discs formed slowly within them from leftovers of the turbulent phase and from material accreted through cold flows and minor mergers. In this Letter, I propose an observational test to verify this
    Comerón, S.

    Advertised on:

    1
    2021
    Bibcode
    2021A&A...645L..13C
    Citations
    3
  • Refereed
    Atomic data for the Gaia-ESO Survey
    Context. We describe the atomic and molecular data that were used for the abundance analyses of FGK-type stars carried out within the Gaia-ESO Public Spectroscopic Survey in the years 2012 to 2019. The Gaia-ESO Survey is one among several current and future stellar spectroscopic surveys producing abundances for Milky-Way stars on an industrial
    Heiter, U. et al.

    Advertised on:

    1
    2021
    Bibcode
    2021A&A...645A.106H
    Citations
    109
  • Non-refereed
    Classifying MaNGA galaxies with unsupervised machine learning techniques
    We explore the use of unsupervised machine learning to classify a sample of >9000 nearby galaxies of all types from the SDSS MaNGA survey. Our aim is to find a classification that correlates with physical properties and that arises naturally when combining maps of the average properties of the stellar populations. We use the SimCLR (Simple
    Sarmiento, R. et al.

    Advertised on:

    1
    2021
    Bibcode
    2021AAS...23711307S
    Citations
    0