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/

  • Activity indexes and velocities for 890 stars (Jenkins+, 2011)
    The activities, rotational velocities, radial velocities and kinematic space motions are presented for over 850 dwarf and subgiant FGK type stars. The chromospheric activities were measured using the CaII HK lines and high resolution and high S/N FEROS spectra. The radial velocities were determined by cross-correlation with a number of template
    Jenkins, J. S. et al.

    Advertised on:

    4
    2011
    Citations
    0
  • Abundances of 650 bulge red giants (Gonzalez+, 2011)
    Listed are the [Mg/Fe], [Ca/Fe], [Ti/Fe] and [Si/Fe] abundance ratios for 650 K giants in four fields of the Galactic Bulge. Abundances were measured using standard 1D local thermodynamic equilibrium MARCS models and spectral synthesis using MOOG. The list also includes the metallicities [Fe/H] presented in Zoccali et al. (2008, Cat. J/A+A/486/177)
    Gonzalez, O. A. et al.

    Advertised on:

    4
    2011
    Citations
    0
  • A Sounding Rocket Experiment for Spectropolarimetric Observations with the Lyα Line at 121.6 nm (CLASP)
    A team consisting of Japan, USA, Spain, and Norway is developing a high-throughput Chromospheric Lyman-Alpha SpectroPolarimeter (CLASP), which is proposed to fly with a NASA sounding rocket in 2014. CLASP will explore the magnetism of the upper solar chromosphere and transition region via the Hanle effect of the Lyα line for the first time. This
    Ishikawa, R. et al.

    Advertised on:

    4
    2011
    Citations
    10
  • VLT-VIMOS integral field spectroscopy of luminous and ultraluminous infrared galaxies. III. The atlas of the stellar and ionized gas distribution
    Context. Luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) are much more numerous at higher redshifts than locally, dominating the star-formation rate density at redshifts ~1-2. Therefore, they are important objects in order to understand how galaxies form and evolve through cosmic time. Local samples provide a unique opportunity to
    Rodríguez-Zaurín, J. et al.

    Advertised on:

    3
    2011
    Citations
    51