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/

  • SIMULATIONS OF THE SOLAR CHROMOSPHERE IN THE TWO-FLUID APPROXIMATION
    This work presents the study of wave propagation and the Rayleigh-Taylor instability in the solar atmosphere using a two-fluid model. The solar atmosphere is strongly stratified and permeated by magnetic fields with a complex configuration, thus creating very different regimes throughout its layers. Of the different layers of the solar atmosphere
    Beatrice Popescou Braileau

    Advertised on:

    4
    2020
  • CONSTRUCCIÓN DE MAPAS Y ESTIMACIÓN DE ESPECTROS DE POTENCIAS PARA EL EXPERIMENTO QUIJOTE. APLICACIÓN A LOS DATOS DEL INSTRUMENTO MFI.
    En esta tesis se han abordado varios de los pasos necesarios (análisis del ruido instrumental, construcción de mapas, estimación de espectros de potencias) para el procesado de los datos de un experimento de polarización del Fondo Cósmico de Microondas (FCM), enfocándolos a la explotación cientı́fica del experimento QUIJOTE. En particular se
    Alba Eva Peláez Santos

    Advertised on:

    11
    2019
  • SEARCHING FOR AND CHARACTERISING THE HIGH REDSHIFT STAR-FORMING GALAXY POPULATION IN THE EARLY UNIVERSE
    This thesis focuses on the study of LAEs and LBGs at z=3.4-6.8, a period of time between ~0.8-2 Gyr after the Big Bang, hosting the end of the reionisation epoch. To reach such deep galaxies, we have made use of the SHARDS survey of the GOODS-N field, with 200 h of exposure time with GTC. The 25 consecutive medium-band filters in the optical/NIR
    Pablo Arrabal Haro

    Advertised on:

    12
    2019
  • SPECTROSCOPIC AND PHYSICAL CHARACTERIZATION OF THE GALACTIC O-TYPE STARS TARGETED BY THE IACOB & OWN SURVEYS
    Las estrellas O representan una fase fundamental en el zoológico de las estrellas masivas. Ionizan el material a su alrededor e inundan su entorno con material procesado a través de fuertes vientos estelares y explosiones de supernova. Además de la pérdida de masa, factores como la rotación y la multiplicidad (así como la interacción entre ellos)
    Gonzalo Holgado Alijo

    Advertised on:

    1
    2019
  • SPECTROSCOPIC AND PHOTOMETRIC CHARACTERIZATION OF PRIMITIVE ASTEROID COLLISIONAL FAMILIES
    The study of near-Earth asteroids (NEAs) is very important, due to three main reasons. First, they pose an impact risk for Earth, and damage produced by a possible collision will depend on the speed of the impact, the size of the object, and its composition. Second, given their proximity, they are easy access targets for the visit of space missions
    David Morate González

    Advertised on:

    4
    2018
  • THICK DISCS AND TRUNCATIONS IN SPIRAL GALAXIES
    Our understanding of the evolution of galaxies within their optical radius has made great advances in the last decades. These have been achieved by analysing in detail the internal secular processes, the star formation history, and the Interstellar medium. However, the study of galaxy outskirts, so-called low surface brightness science, is still in
    Cristina Martínez Lombilla

    Advertised on:

    4
    2018