Publicaciones

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  • Ages of LMC star clusters using ASAD2
    We use ASAD2, the new version of ASAD (Analyzer of Spectra for Age Determination), to obtain the age and reddening of 27 Large Magellanic Cloud (LMC) clusters from full fitting of integrated spectra using different statistical methods [χ2 and Kolmogorov-Smirnov (KS) test] and a set of stellar population models including GALAXEV and MILES. We show
    Asa'd, R. S. et al.

    Fecha de publicación:

    4
    2016
    Número de citas
    15
  • Activity from the Be/X-ray binary system V0332+53 during its intermediate-luminosity outburst in 2008
    Aims: We present a study of the Be/X-ray binary system V 0332+53 with the main goal of characterizing its behaviour mainly during the intermediate-luminosity X-ray event in 2008. In addition, we aim to contribute to the understanding of the behaviour of the donor companion by including optical data from our dedicated campaign starting in 2006
    Caballero-García, M. D. et al.

    Fecha de publicación:

    4
    2016
    Número de citas
    17
  • X-ray long-term variations in the low-luminosity AGN NGC 835 and its circumnuclear emission
    Context. Obscured active galactic nuclei (AGNs) are thought to be very common in the Universe. Observations and surveys have shown that the number of sources increases for near galaxies and at the low-luminosity regime (the so-called LLAGNs). Furthermore, many AGNs show changes in their obscuration properties at X-rays that may suggest a
    González-Martín, O. et al.

    Fecha de publicación:

    3
    2016
    Número de citas
    6
  • X-Ray Absorption, Nuclear Infrared Emission, and Dust Covering Factors of AGNs: Testing Unification Schemes
    We present the distributions of the geometrical covering factors of the dusty tori (f2) of active galactic nuclei (AGNs) using an X-ray selected complete sample of 227 AGNs drawn from the Bright Ultra-hard XMM-Newton Survey. The AGNs have z from 0.05 to 1.7, 2–10 keV luminosities between 1042 and 1046 erg s‑1, and Compton-thin X-ray absorption
    Mateos, S. et al.

    Fecha de publicación:

    3
    2016
    Número de citas
    48
  • Visible spectroscopy of the Polana-Eulalia family complex: Spectral homogeneity
    The Polana-Eulalia family complex is located in the inner part of the asteroid belt, bounded by the ν6 and the 3:1 resonances, where we can find another three collisional families of primitive asteroids (Erigone, Clarissa, and Sulamitis), and a low-albedo population of background objects. This region of the belt is believed to be the most likely
    de León, J. et al.

    Fecha de publicación:

    3
    2016
    Número de citas
    38
  • Transverse momentum spectra of inclusive b jets in pPb collisions at √{sNN} = 5.02 TeV
    We present a measurement of b jet transverse momentum (pT) spectra in proton-lead (pPb) collisions using a dataset corresponding to about 35 nb-1 collected with the CMS detector at the LHC. Jets from b quark fragmentation are found by exploiting the long lifetime of hadrons containing a b quark through tagging methods using distributions of the
    Khachatryan, V. et al.

    Fecha de publicación:

    3
    2016
    Número de citas
    31