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/

  • Erratum
    Erratum: "The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III" (2011, ApJS, 193, 29)
    Not Available
    Aihara, Hiroaki et al.

    Advertised on:

    8
    2011
    Bibcode
    2011ApJS..195...26A
    Citations
    59
  • Erratum
    Erratum: "Scattering Polarization of the Ca II IR Triplet for Probing the Quiet Solar Chromosphere" (2010, ApJ, 722, 1416)
    Not Available
    Manso Sainz, R. et al.

    Advertised on:

    8
    2011
    Bibcode
    2011ApJ...737..106M
    Citations
    0
  • Refereed
    Do galaxies form a spectroscopic sequence?
    We identify a spectroscopic sequence of galaxies, analogous to the Hubble sequence of morphological types, based on the Automatic Spectroscopic K-means-based (ASK) classification. Considering galaxy spectra as multidimensional vectors, the majority of the spectral classes are distributed along a well-defined curve going from the earliest to the
    Ascasibar, Y. et al.

    Advertised on:

    8
    2011
    Bibcode
    2011MNRAS.415.2417A
    Citations
    22
  • Refereed
    Dissecting the size evolution of elliptical galaxies since z˜ 1: puffing-up versus minor-merging scenarios
    At a fixed stellar mass, the size of low-redshift early-type galaxies is found to be a factor of 2 larger than that of their counterparts at z˜ 1, a result with important implications for galaxy formation models. In this paper, we have explored the buildup of the local mass-size relation of elliptical galaxies using two visually classified samples
    Trujillo, I. et al.

    Advertised on:

    8
    2011
    Bibcode
    2011MNRAS.415.3903T
    Citations
    171
  • Non-refereed
    Diagnostics for spectropolarimetry and magnetography
    An assessment on the capabilities of modern spectropolarimeters and magnetographs is in order since most of our astrophysical results rely upon the accuracy of the instrumentation and on the sensitivity of the observables to variations of the sought physical parameters. A contribution to such an assessment will be presented in this talk where
    del Toro Iniesta, Jose Carlos et al.

    Advertised on:

    8
    2011
    Bibcode
    2011IAUS..273...37D
    Citations
    5