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
    Far-infrared constraints on the contamination by dust-obscured galaxies of high-z dropout searches
    The spectral energy distributions (SED) of dusty galaxies at intermediate redshift may look similar to very high-redshift galaxies in the optical/near infrared (NIR) domain. This can lead to the contamination of high-redshift galaxy searches based on broad-band optical/NIR photometry by lower redshift dusty galaxies because both kind of galaxies
    Boone, F. et al.

    Advertised on:

    10
    2011
    Bibcode
    2011A&A...534A.124B
    Citations
    14
  • Non-refereed
    Faint emission lines in planetary nebulae with a [WC] nucleus
    We present first results from the analysis of a sample of 14 planetary nebulae with [WC] nucleus with detected faint carbon and oxygen recombination lines (RLs). The results are based on deep echelle spectra obtained with MIKE on the 6.5 m Magellan-Clay telescope in Chile.
    García-Rojas, J. et al.

    Advertised on:

    10
    2011
    Bibcode
    2011RMxAC..40..169G
    Citations
    0
  • Non-refereed
    Evolution of the NIR Morphologies of Disk Galaxies since z˜1: A `Glance' into GOODS-South with HST-WFC3
    Hereby we present an exploratory study of the surface brightness radial profiles (μ-r profiles hereafter) of massive (M˜>109.5 M&sun;) disk galaxies in the redshift range 0 ˜ z ˜ 1. We use recently acquired images from HST-WFC3 in the H160 band, and archive data from SDSS-DR7, to trace the rest-frame z' band at all redshifts. The comparison of
    Azzollini, R. et al.

    Advertised on:

    10
    2011
    Bibcode
    2011ASPC..446..297A
    Citations
    0
  • Refereed
    Evolution of Super Star Cluster Winds with Strong Cooling
    We study the evolution of super star cluster winds driven by stellar winds and supernova explosions. Time-dependent rates at which mass and energy are deposited into the cluster volume, as well as the time-dependent chemical composition of the re-inserted gas, are obtained from the population synthesis code Starburst99. These results are used as
    Wünsch, Richard et al.

    Advertised on:

    10
    2011
    Bibcode
    2011ApJ...740...75W
    Citations
    46