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/

  • Refereed
    The European Large Area ISO Survey - VI. Discovery of a new hyperluminous infrared galaxy

    We report the discovery of the first hyperluminous infrared galaxy (HyLIG) in the course of the European Large Area ISO Survey (ELAIS). This object has been detected by ISO at 6.7, 15 and 90μm, and is found to be a broad-line, radio-quiet quasar at a redshift [formmu4]z=1.099. From a detailed multicomponent model fit of the spectral energy

    Morel, T. et al.

    Advertised on:

    11
    2001
    Bibcode
    2001MNRAS.327.1187M
    Citations
    17
  • Refereed
    The European Large Area ISO Survey - VIII. 90-μm final analysis and source counts

    We present a re-analysis of the European Large Area Infrared Space Observatory (ISO) Survey (ELAIS) 90-μm observations carried out with ISOPHOT, an instrument on board the ISO of the European Space Agency. With more than 12 deg2, the ELAIS survey is the largest area covered by ISO in a single programme and is about one order of magnitude deeper

    Héraudeau, Ph. et al.

    Advertised on:

    11
    2004
    Bibcode
    2004MNRAS.354..924H
    Citations
    29
  • Refereed
    The EUSO-Balloon pathfinder

    EUSO-Balloon is a pathfinder for JEM-EUSO, the Extreme Universe Space Observatory which is to be hosted on-board the International Space Station. As JEM-EUSO is designed to observe Ultra-High Energy Cosmic Rays (UHECR)-induced Extensive Air Showers (EAS) by detecting their ultraviolet light tracks "from above", EUSO-Balloon is a nadir-pointing UV

    Adams, J. H. et al.

    Advertised on:

    11
    2015
    Bibcode
    2015ExA....40..281A
    Citations
    29
  • Refereed
    The evolution of Galactic planetary nebula progenitors through the comparison of their nebular abundances with AGB yields

    We study the chemical abundances of a wide sample of 142 Galactic planetary nebulae (PNe) with good-quality observations, for which the abundances have been derived more or less homogeneously, thus allowing a reasonable comparison with stellar models. The goal is the determination of mass, chemical composition and formation epoch of their

    García-Hernández, D. A. et al.

    Advertised on:

    11
    2017
    Bibcode
    2017MNRAS.471.4648V
    Citations
    20
  • Refereed
    The evolution of radio loud quasar host galaxies: AO observations at z ˜ 3

    We report on ESO VLT adaptive optics imaging of one radio-loud quasar at z ˜ 3. In spite of the large distance of the object we are able to detect its surrounding extended nebulosity the properties of which are consistent with an underlying massive galaxy of MK ˜ -27 and effective radius Re = 7 kpc. As far as we know this is the clearest detection

    Falomo, R. et al.

    Advertised on:

    11
    2006
    Bibcode
    2006NewAR..50..732F
    Citations
    1
  • Refereed
    The Evolution of the Number Density of Compact Galaxies

    We compare the number density of compact (small size) massive galaxies at low and high redshift using our Padova Millennium Galaxy and Group Catalogue (PM2GC) at z = 0.03-0.11 and the CANDELS results from Barro et al. at z = 1-2. The number density of local compact galaxies with luminosity weighted (LW) ages compatible with being already passive at

    Poggianti, B. M. et al.

    Advertised on:

    11
    2013
    Bibcode
    2013ApJ...777..125P
    Citations
    83