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/

  • Discovery of Ubiquitous Fast-Propagating Intensity Disturbances by the Chromospheric Lyman Alpha Spectropolarimeter (CLASP)
    High-cadence observations by the slit-jaw (SJ) optics system of the sounding rocket experiment known as the Chromospheric Lyman Alpha Spectropolarimeter (CLASP) reveal ubiquitous intensity disturbances that recurrently propagate in either the chromosphere or the transition region or both at a speed much higher than the speed of sound. The CLASP/SJ
    Kubo, M. et al.

    Advertised on:

    12
    2016
    Citations
    22
  • Discovery of a Metal-poor Field Giant with a Globular Cluster Second-generation Abundance Pattern
    We report on the detection, from observations obtained with the Apache Point Observatory Galactic Evolution Experiment spectroscopic survey, of a metal-poor ([Fe/H] = -1.3 dex) field giant star with an extreme Mg-Al abundance ratio ([Mg/Fe] = -0.31 dex; [Al/Fe] = 1.49 dex). Such low Mg/Al ratios are seen only among the second-generation population
    Fernández-Trincado, J. G. et al.

    Advertised on:

    12
    2016
    Citations
    67
  • Archaeoastronomy in Bronze Age Sites of La Mancha (Spain)
    We present archaeoastronomical results of an interdisciplinary project to study Bronze Age sites of the socalled Cultura de las Motillas in the Spanish region of La Mancha. We find that winter solstice sunrise was of special importance in the funerary  and perhaps religious  practises of these peoples. The impressive megalithic monumental complex
    Esteban, C. et al.

    Advertised on:

    12
    2016
  • Accurate parameters for HD 209458 and its planet from HST spectrophotometry
    We present updated parameters for the star HD 209458 and its transiting giant planet. The stellar angular diameter θ = 0.2254 ± 0.0017 mas is obtained from the average ratio between the absolute flux observed with the Hubble Space Telescope and that of the best-fitting Kurucz model atmosphere. This angular diameter represents an improvement in
    del Burgo, C. et al.

    Advertised on:

    12
    2016
    Citations
    30
  • Abundance ratios and IMF slopes in the dwarf elliptical galaxy NGC 1396 with MUSE
    Deep observations of the dwarf elliptical (dE) galaxy NGC 1396 (MV = -16.60, Mass ˜4 × 108 M⊙), located in the Fornax cluster, have been performed with the Very Large Telescope/Multi Unit Spectroscopic Explorer spectrograph in the wavelength region from 4750 to 9350 Å. In this paper, we present a stellar population analysis studying chemical
    Puzia, T. et al.

    Advertised on:

    12
    2016
    Citations
    38