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

  • The MURALES survey. IV. Searching for nuclear outflows in 3C radio galaxies at z < 0.3 with MUSE observations
    We analyze VLT/MUSE observations of 37 radio galaxies from the Third Cambridge catalogue (3C) with redshift < 0.3 searching for nuclear outflows of ionized gas. These observations are part of the MURALES project (a MUse RAdio Loud Emission line Snapshot survey), whose main goal is to explore the feedback process in the most powerful radio-loud AGN
    Speranza, G. et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    19
  • DRAGO camera
    DRAGO: Un pequeño instrumento, un gran camino
    El pasado 24 de enero tuvo lugar la puesta en órbita de DRAGO ( Demonstrator for Remote Analysis of Ground Observations), el primer instrumento desarrollado por IACTEC-Espacio. Semanas después llegaban sus primeras imágenes infrarrojas de la Tierra, con una calidad a la altura de las expectativas más optimistas. DRAGO es el resultado de cuatro años
    A. Oscoz et al.

    Fecha de publicación:

    6
    2021
  • From science to industry, technology transference with CubeSats
    The Instituto de Astrofísica de Canarias (IAC) has as main objective to promote and carry out all types of research in astrophysics and its related fields. This mission means that the IAC has been involved in instrumental developments for both ground-based and space observations for decades. This accumulated experience led the IAC to launch an
    I. Bustamante et al.

    Fecha de publicación:

    7
    2020
  • Evidence of the multi-thermal nature of spicular downflows. Impact on solar atmospheric heating
    Context. Spectroscopic observations of the emission lines formed in the solar transition region commonly show persistent downflows on the order of 10−15 km s −1. The cause of such downflows, however, is still not fully clear and has remained a matter of debate. Aims: We aim to understand the cause of such downflows by studying the coronal and
    Bose, Souvik et al.

    Fecha de publicación:

    10
    2021
    Número de citas
    14
  • Fornax 3D project: Assessing the diversity of IMF and stellar population maps within the Fornax Cluster
    The stellar initial mass function (IMF) is central to our interpretation of astronomical observables and to our understanding of most baryonic processes within galaxies. The universality of the IMF, suggested by observations in our own Milky Way, has been thoroughly revisited due to the apparent excess of low-mass stars in the central regions of
    Martín-Navarro, I. et al.

    Fecha de publicación:

    10
    2021
    Número de citas
    19
  • HD 22496 b: The first ESPRESSO stand-alone planet discovery
    Context. The ESPRESSO spectrograph is a new powerful tool developed to detect and characterize extrasolar planets. Its design allows an unprecedented radial velocity precision (down to a few tens of cm s −1) and long-term thermomechanical stability. Aims: We present the first stand-alone detection of an extrasolar planet by blind radial velocity
    Lillo-Box, J. et al.

    Fecha de publicación:

    10
    2021
    Número de citas
    8