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/

  • Non-refereed
    Color-Magnitude Diagrams, Probabilistic Synthesis Models and the Upper Mass Limit of the Initial Mass Function
    We present the underlying relations between color-magnitude diagrams (CMDs) and synthesis models through the use of stellar luminosity distribution functions. CMD studies make direct use of the stellar luminosity distribution function while, in general, synthesis models only use its mean value, even though high-order moments can also be obtained
    Cerviño, M. et al.

    Advertised on:

    6
    2011
    Bibcode
    2011ASPC..440..133C
    Citations
    4
  • Refereed
    Clear detection of dusty torus signatures in a weak-line radio galaxy: the case of PKS 0043-42
    We report the clearest detection to date of dusty torus signatures in a weak-line radio galaxy (WLRG). The deep Spitzer InfraRed Spectrograph (IRS) rest-frame mid-infrared (MIR) spectrum of the WLRG PKS 0043-42 (z= 0.116) shows a clear spectral turnover at λ≳ 20 μs suggestive of warm dust, as well as a 9.7-μm silicate absorption feature. In
    Ramos-Almeida, C. et al.

    Advertised on:

    6
    2011
    Bibcode
    2011MNRAS.413.2358R
    Citations
    13
  • Refereed
    Blue not brown: UKIRT Infrared Deep Sky Survey T dwarfs with suppressed K-band flux
    We have used blue near-infrared colours to select a group of 12 spectroscopically confirmed United Kingdom InfraRed Telescope (UKIRT) Infrared Deep Sky Survey (UKIDSS) T dwarfs later than T4. From amongst these, we identify the first two kinematic halo T-dwarf candidates. Blue near-infrared colours have been attributed to collisionally induced
    Murray, D. N. et al.

    Advertised on:

    6
    2011
    Bibcode
    2011MNRAS.414..575M
    Citations
    50
  • Refereed
    Beryllium abundances in stars with planets. Extending the sample
    Context. Chemical abundances of light elements such as beryllium in planet-host stars allow us to study the planet formation scenarios and/or investigate possible surface pollution processes. Aims: We present here an extension of previous beryllium abundance studies. The complete sample consists of 70 stars that host planets and 30 stars without
    Gálvez-Ortiz, M. C. et al.

    Advertised on:

    6
    2011
    Bibcode
    2011A&A...530A..66G
    Citations
    12