Tipo de publicación: Sin árbitro

  • Publicación
    The Open Cluster Chemical Abundances and Mapping (OCCAM) Survey: Overview and Membership Methods
    The Open Cluster Chemical Analysis and Mapping (OCCAM) survey aims to produce a comprehensive, uniform, infrared-based data set for hundreds of open clusters...
  • Publicación
    The Open Cluster Chemical Abundances from Spanish Observatories Survey (OCCASO)
    We present the motivation, design and current status of the Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO). Using the high...
  • Publicación
    The Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO)
    We present the motivation, design and current status of the Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO). Using the high...
  • Publicación
    The optical AIV of the infrared multi-slit spectrophotometer for GTC, EMIR
    EMIR is a second generation GTC instrument. EMIR's external structure is a huge cylindrical vacuum chamber of 2.2m length and 1.8m in diameter with a weight of...
  • Publicación
    The optical counterpart of the accreting millisecond X-ray pulsar IGR J17498-2921
    We report the optical detection of a faint star consistent with the known position of the 401 Hz transient accreting millisecond X-ray pulsar IGR J17498-2921...
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    The optical counterpart of the east lobe of M87
    Not Available
  • Publicación
    The optical counterpart of the new Fermi LAT flaring source J0109+6134 near the Galactic Plane
    The position of the recently discovered transient gamma-ray source J0109+6134 (ATEL #2414) lies within the footprints of the IPHAS (Drew et al. 2005, MNRAS, 362...
  • Publicación
    The Optical Counterpart to XTE J1817-330.
    We report the counterpart to the X-ray transient and black hole candidate XTE J1817-330 (ATEL #714). Our observations consist of a series of 5s and 10s g'-band...
  • Publicación
    The optical counterparts of Accreting Millisecond X-Ray Pulsars during quiescence
    Using data obtained with the ESO-Very Large Telescope, we have performed a deep optical and NIR photometric study of the fields of three Accreting Millisecond X...