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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  • A feasibility study on the photometric detection of quiescent black hole X-ray binaries
    We investigate the feasibility of detecting quiescent black hole X-ray binaries using optical photometric techniques. To test this, we employ a combination of r-band and H α filters currently available at the Roque de los Muchachos Observatory. Photometric observations of four dynamical black holes (GRO J0422+320, A 0620-00, XTE J1118+480, and XTE
    Casares, J. et al.

    Fecha de publicación:

    12
    2018
    Número de citas
    12
  • When nature tries to trick us. An eclipsing eccentric close binary superposed on the central star of the planetary nebula M 3-2
    Bipolar planetary nebulae (PNe) are thought to result from binary star interactions and, indeed, tens of binary central stars of PNe have been found, in particular using photometric time-series that allow for the detection of post-common envelope systems. Using photometry at the NTT in La Silla we have studied the bright object close to the centre
    Boffin, H. M. J. et al.

    Fecha de publicación:

    11
    2018
    Número de citas
    14
  • Unveiling the environment and faint features of the isolated galaxy CIG 96 with deep optical and HI observations
    Context. Asymmetries in atomic hydrogen (HI) in galaxies are often caused by the interaction with close companions, making isolated galaxies an ideal framework to study secular evolution. The AMIGA project has demonstrated that isolated galaxies show the lowest level of asymmetry in their HI integrated profiles compared to even field galaxies, yet
    Ramírez-Moreta, P. et al.

    Fecha de publicación:

    11
    2018
    Número de citas
    11
  • UNDERSTANDING THE OUTSKIRTS OF DISC GALAXIES
    Las regiones externas de las galaxias contienen múltiples pistas sobre los procesos de formación que dieron lugar a los distintos tipos morfológicos observados en la actualidad y su evolución. Sin embargo, el análisis del Universo a bajo brillo superficial esta limitado por la profundidad de las imágenes actuales y la presencia de diversos tipos de
    Alejandro Serrano Borlaff

    Fecha de publicación:

    11
    2018
  • The WIRCam Ultra Deep Survey (WUDS). I. Survey overview and UV luminosity functions at z ˜ 5 and z ˜ 6
    The aim of this paper is to introduce the WIRCam Ultra Deep Survey (WUDS), a near-IR photometric survey carried out at the CFH Telescope in the field of the CFHTLS-D3 field (Groth Strip). WUDS includes four near-IR bands (Y, J, H and Ks) over a field of view of ˜400 arcmin2. The typical depth of WUDS data reaches between ˜26.8 in Y and J, and ˜26
    Pelló, R. et al.

    Fecha de publicación:

    11
    2018
    Número de citas
    7
  • The Transiting Exoplanet Community Early Release Science Program for JWST
    The James Webb Space Telescope (JWST) presents the opportunity to transform our understanding of planets and the origins of life by revealing the atmospheric compositions, structures, and dynamics of transiting exoplanets in unprecedented detail. However, the high-precision, timeseries observations required for such investigations have unique
    Bean, Jacob L. et al.

    Fecha de publicación:

    11
    2018
    Número de citas
    121