Publicaciones

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  • Optical Studies of V:404-CYGNI the X-Ray Transient GS:2023+338 - Part Three - the Secondary Star and Accretion Disc
    We present new results from the analysis of 55 high-resolution spectra of V404 Cyg (the optical counterpart of the X-ray transient GS 2023+338) taken in 1991 July-August which, added to our 1990 July Hα spectra, establish the most complete spectroscopic data base in quiescence of this new black hole candidate. In addition, we present multicolour
    Casares, J. et al.

    Fecha de publicación:

    12
    1993
    Número de citas
    105
  • Optical Study of the Hyper-luminous X-Ray Source 2XMM J011942.7+032421
    We present the identification and characterization of the optical counterpart to 2XMM J011942.7+032421, one of the most luminous and distant ultra-luminous X-ray sources (ULXs). The counterpart is located near a star-forming region in a spiral arm of the galaxy NGC 470 with u, g, and r magnitudes of 21.53, 21.69, and 21.71 mag, respectively. The
    Gutiérrez, C. M. et al.

    Fecha de publicación:

    12
    2014
    Número de citas
    10
  • Optical Study of the X-ray Transient XTE J2123-058
    We present the results of optical photometry of the X-ray transient XTE J2123-058. CCD R-band images, have been obtained since 2 Jul until 29 Sep 1998. Following the behaviour of the XTE/ASM lightcurve, the system decline optically from the begining of August at approximately 0.1 mag/day. Despite the drop in luminosity, we observe a dramatic
    Zurita, C. et al.

    Fecha de publicación:

    12
    1998
    Número de citas
    0
  • Optical Variability of the Blazar OJ 287
    An international collaboration of fourty scientists have been involved in multifrequency observations of the blazar OJ 287, as well as of a few other complementary objects, taken both photometrically and spectroscopically. We present the optical light curve of OJ 287 obtained between the fall of 1993 through the present. Over 1200 photometric
    Sadun, A. et al.

    Fecha de publicación:

    12
    1994
    Número de citas
    0
  • Optimization of Planck-LFI on-board data handling
    To asses stability against 1/f noise, the Low Frequency Instrument (LFI) on-board the Planck mission will acquire data at a rate much higher than the data rate allowed by the science telemetry bandwith of 35.5 Kbps. The data are processed by an on-board pipeline, followed on-ground by a decoding and reconstruction step, to reduce the volume of data
    Maris, M. et al.

    Fecha de publicación:

    12
    2009
    Número de citas
    4
  • Orbital and physical properties of planets and their hosts: new insights on planet formation and evolution
    Aims: We explore the relations between physical and orbital properties of planets and properties of their host stars to identify the main observable signatures of the formation and evolution processes of planetary systems. Methods: We used a large sample of FGK dwarf planet-hosting stars with stellar parameters derived in a homogeneous way from the
    Adibekyan, V. Zh. et al.

    Fecha de publicación:

    12
    2013
    Número de citas
    80