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/

  • 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
    9
  • 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
  • MAGIC observations and multifrequency properties of the flat spectrum radio quasar 3C 279 in 2011
    Aims: We study the multifrequency emission and spectral properties of the quasar3C 279 aimed at identifying the radiation processes taking place in the source. Methods: We observed 3C 279 in very-high-energy (VHE, E> 100 GeV) γ-rays, with the MAGIC telescopes during 2011, for the first time in stereoscopic mode. We combined these measurements with
    Sitarek, J. et al.

    Advertised on:

    7
    2014
    Citations
    42
  • MAGIC long-term study of the distant TeV blazar PKS 1424+240 in a multiwavelength context
    Aims: We present a study of the very high-energy (VHE; E> 100 GeV) γ-ray emission of the blazar PKS 1424+240 observed with the MAGIC telescopes. The primary aim of this paper is the multiwavelength spectral characterization and modeling of this blazar, which is made particularly interesting by the recent discovery of a lower limit of its redshift
    Miranda, J. M. et al.

    Advertised on:

    7
    2014
    Citations
    58
  • IPHAS and the symbiotic stars. III. New discoveries and their IR spectral energy distributions
    Context. The IPHAS Hα survey provides a rich database to search for emission-line sources in the northern Galactic plane. Aims: We are systematically searching for symbiotic stars in the Milky Way using IPHAS. Our final goal, a complete census of this class of objects in the Galaxy, is a fundamental figure for discussing their overall properties
    Rodríguez-Flores, E. R. et al.

    Advertised on:

    7
    2014
    Citations
    44
  • Infrared properties of blazars: putting the GASP-WEBT sources into context
    The infrared properties of blazars can be studied from the statistical point of view with the help of sky surveys, like that provided by the Wide-field Infrared Survey Explorer and the Two Micron All Sky Survey. However, these sources are known for their strong and unpredictable variability, which can be monitored for a handful of objects only. In
    Raiteri, C. M. et al.

    Advertised on:

    7
    2014
    Citations
    26