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/

  • The properties of galaxies in voids

    We present a comparison of the properties of galaxies in the most underdense regions of the Universe, where the galaxy number density is less than 10 per cent of the mean density, with galaxies from more typical regions. We have compiled a sample of galaxies in 46 large nearby voids that were identified using the Sloan Digital Sky Survey DR4, which

    Patiri, Santiago G. et al.

    Advertised on:

    11
    2006
    Citations
    105
  • The puzzling interpretation of NIR indices: The case of NaI2.21

    We present a detailed study of the Na I line strength index centred in the K band at 22 100 Å (NaI2.21 hereafter) relying on different samples of early-type galaxies. Consistent with previous studies, we find that the observed line strength indices cannot be fit by state-of-the-art scaled-solar stellar population models, even using our newly

    Aguado, D. S. et al.

    Advertised on:

    11
    2017
    Citations
    13
  • The quiescent spectral energy distribution of V404 Cyg

    We present a multiwavelength study of the black hole X-ray binary V404 Cyg in quiescence, focusing upon the spectral energy distribution (SED). Radio, optical, ultraviolet (UV) and X-ray coverage is simultaneous. We supplement the SED with additional non-simultaneous data in the optical through infrared where necessary. The compiled SED is the most

    Hynes, R. I. et al.

    Advertised on:

    11
    2009
    Citations
    64
  • The quiet Sun magnetic field observed with ZIMPOL on THEMIS. I. The probability density function

    Context: The quiet Sun magnetic field probability density function (PDF) remains poorly known. Modeling this field also introduces a magnetic filling factor that is also poorly known. With these two quantities, PDF and filling factor, the statistical description of the quiet Sun magnetic field is complex and needs to be clarified. Aims: In the

    Bommier, V. et al.

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    11
    2009
    Citations
    25
  • The rapid fading of V1647 Orionis: the sudden end of a FUor-type eruption?

    The young eruptive star V1647 Ori started a rapid fading in October 2005 and now is only 1 mag above the pre-outburst level. Colour changes indicate that the fading is not due to increasing extinction.

    Kospal, Agnes et al.

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    11
    2005
    Citations
    24