Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

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  • Optical imaging for the Spitzer Survey of Stellar Structure in Galaxies. Data release and notes on interacting galaxies
    Context. The Spitzer Survey for Stellar Structure in Galaxies (S4G) and its more recently approved extension will lead to a set of 3.6 and 4.5 μm images for 2829 galaxies, which can be used to study many different aspects of the structure and evolution of local galaxies. Aims: We have collected and re-reduced optical images of 1768 of the survey
    Knapen, J. H. et al.

    Fecha de publicación:

    9
    2014
    Número de citas
    29
  • Optical Imaging of 57 spiral galaxies (Knapen+ 2004)
    All B, R, I and Hα images described in the paper are presented electronically, along with the Ks images from Paper I (Knapen et al., 2003MNRAS.344..527K). The images are in FITS format, with basic parameters like pixel scale and calibration described in the FITS headers. All images have been reduced to the equivalent of 1 second exposure time. The
    Knapen, J. H. et al.

    Fecha de publicación:

    9
    2004
    Número de citas
    0
  • Optical performances of the FM JEM-X masks
    The JEM-X Signal Multiplexing Systems are large HURA codes "written" in a pure tungsten plate 0.5 mm thick. 24.247 hexagonal pixels (25% open) are spread over a total area of 535 mm diameter. The tungsten plate is embedded in a mechanical structure formed by a Ti ring, a pretensioning system (Cu-Be) and an exoskeleton structure that provides the
    Reglero, V. et al.

    Fecha de publicación:

    9
    2001
    Número de citas
    2
  • Optical re-brightening of the black hole binary XTE J1859+226
    Observations of the black hole binary XTE J1859+226 revealed an unexpected optical re-brightening. Images were taken with the Nordic Optical Telescope (NOT) using ALFOSC on Jul 13-14, the William Herschel Telescope (WHT) with ACAM on Aug 8 and the Isaac Newton Telescope (INT) with WFC on Aug 19 at the Observatorio del Roque de los Muchachos, La
    Corral-Santana, J. M. et al.

    Fecha de publicación:

    9
    2010
    Número de citas
    2
  • Optical Spectroscopy of Candidate X-ray Binaries in the Starburst IC 10
    The dwarf irregular galaxy IC10 in Cassiopeia, is the youngest available starburst galaxy and home to many X-ray sources. Using the Gemini multi-object spectrograph (GMOS), in the wavelength range containing H-alpha, we obtained spectra of twenty five stars that are positionally coincident with X-ray sources, at the 95% significance level. The
    Balchunas, Andrew J. et al.

    Fecha de publicación:

    9
    2011
    Número de citas
    0
  • Optical spectroscopy of the low-mass X-ray binary GX9+9
    Phase-resolved medium-resolution VLT spectroscopy of the low-mass X-ray binary GX9+9 has revealed narrow CIII emission lines that move in phase relative to our new estimate of the ephemeris, and show a velocity amplitude of 230 +/- 35 km s-1. We identify the origin of these lines as coming from the surface of the donor star, thereby providing the
    Cornelisse, R. et al.

    Fecha de publicación:

    9
    2007
    Número de citas
    15