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/

  • MuSICa image slicer prototype at 1.5-m GREGOR solar telescope
    Integral Field Spectroscopy is an innovative technique that is being implemented in the state-of-the-art instruments of the largest night-time telescopes, however, it is still a novelty for solar instrumentation. A new concept of image slicer, called MuSICa (Multi-Slit Image slicer based on collimator-Camera), has been designed for the integral
    Calcines, A. et al.

    Advertised on:

    7
    2014
    Citations
    10
  • Morphology and environment of galaxies with disc breaks in the S4G and NIRS0S
    We study the surface brightness profiles of disc galaxies in the 3.6 μm images from the Spitzer Survey of Stellar Structure in Galaxies (S4G) and Ks-band images from the Near-Infrared S0-Sa galaxy Survey (NIRS0S). We particularly connect properties of single exponential (type I), downbending double exponential (type II), and upbending double
    Laine, J. et al.

    Advertised on:

    7
    2014
    Citations
    63
  • Morphological classification of PM2GC galaxies (Calvi+, 2013)
    The PM2GC (Calvi et al., 2011MNRAS.416..727C, cat. J/MNRAS/416/727) is a data base built on the basis of the Millennium Galaxy Catalogue (MGC), a deep and wide B-imaging survey along an equatorial strip of ~38deg2 obtained with the Isaac Newton Telescope (INT). The design, execution, reduction, object detection and preliminary analysis of this
    Calvi, R. et al.

    Advertised on:

    7
    2014
    Citations
    0
  • Molecular line emission in NGC 1068 imaged with ALMA. I. An AGN-driven outflow in the dense molecular gas
    Aims: We investigate the fueling and the feedback of star formation and nuclear activity in NGC 1068, a nearby (D = 14 Mpc) Seyfert 2 barred galaxy, by analyzing the distribution and kinematics of the molecular gas in the disk. We aim to understand if and how gas accretion can self-regulate. Methods: We have used the Atacama Large Millimeter Array
    García-Burillo, S. et al.

    Advertised on:

    7
    2014
    Citations
    417
  • MEGARA: a new generation optical spectrograph for GTC
    MEGARA (Multi-Espectrógrafo en GTC de Alta Resolución para Astronomía) is an optical Integral-Field Unit (IFU) and Multi-Object Spectrograph (MOS) designed for the GTC 10.4m telescope in La Palma. MEGARA offers two IFU fiber bundles, one covering 12.5x11.3 arcsec2 with a spaxel size of 0.62 arcsec (Large Compact Bundle; LCB) and another one
    Gil de Paz, A. et al.

    Advertised on:

    7
    2014
    Citations
    10
  • Masgomas-4: Physical characterization of a double-core obscured cluster with a massive and very young stellar population
    Context. The discovery of new, obscured massive star clusters has changed our understanding of the Milky Way star-forming activity from a passive to a very active star-forming machine. The search for these obscured clusters is strongly supported by the use of all-sky, near-IR surveys. Aims: The main goal of the MASGOMAS project is to search for and
    Ramírez Alegría, S. et al.

    Advertised on:

    7
    2014
    Citations
    7