Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • Ready for EURONEAR NEA surveys using the NEARBY moving source detection platform
    In 2015 we started a PhD thesis aiming to write a moving objects processing system (MOPS) aimed to detect near Earth asteroids (NEAs) in astronomical surveys planned within the EURONEAR project. Based on this MOPS experience, in 2017 we proposed the NEARBY project to the Romanian Space Agency, which awarded funding to the Technical University of
    Vaduvescu, O. et al.

    Fecha de publicación:

    10
    2021
    Número de citas
    2
  • Radio spectral properties of star-forming galaxies in the MIGHTEE-COSMOS field and their impact on the far-infrared-radio correlation
    We study the radio spectral properties of 2094 star-forming galaxies (SFGs) by combining our early science data from the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) survey with VLA, GMRT radio data, and rich ancillary data in the COSMOS field. These SFGs are selected at VLA 3 GHz, and their flux densities from MeerKAT 1.3
    An, Fangxia et al.

    Fecha de publicación:

    10
    2021
    Número de citas
    35
  • Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model
    Context. Recent results for asteroid rotation periods from the TESS mission showed how strongly previous studies have underestimated the number of slow rotators, revealing the importance of studying those targets. For most slowly rotating asteroids (those with P > 12 h), no spin and shape model is available because of observation selection effects
    Marciniak, A. et al.

    Fecha de publicación:

    10
    2021
    Número de citas
    13
  • Polarization of the Lyα Lines of H I and He II as a Tool for Exploring the Solar Corona
    The near-Earth space weather is driven by the quick release of magnetic free energy in the solar corona. Probing this extremely hot and rarified region of the extended solar atmosphere requires modeling the polarization of forbidden and permitted coronal lines. To this end, it is important to develop efficient codes to calculate the Stokes profiles
    Supriya, Hebbur Dayananda et al.

    Fecha de publicación:

    10
    2021
    Número de citas
    8
  • Polarization of the Lyα Lines of H I and He II as a Tool for Exploring the Solar Corona
    The near-Earth space weather is driven by the quick release of magnetic free energy in the solar corona. Probing this extremely hot and rarified region of the extended solar atmosphere requires modeling the polarization of forbidden and permitted coronal lines. To this end, it is important to develop efficient codes to calculate the Stokes profiles
    Hebbur Dayananda, Supriya et al.

    Fecha de publicación:

    10
    2021
    Número de citas
    0
  • Physical properties of the cubewano 19521 Chaos from a multi-chord stellar occultation
    Trans-Neptunian Objects (TNOs) have had an increasing interest since the discovery of (15760) Albion in 1992. These objects are considered remnants of the Solar System formation, and can thus provide clues about its origin and evolution. One of the best techniques to study TNOs from ground-based telescopes are stellar occultations which, if
    Vara-Lubiano, Mónica et al.

    Fecha de publicación:

    10
    2021
    Número de citas
    0