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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  • Multiwavelength observations of the extraordinary accretion event AT2021lwx
    We present observations from X-ray to mid-infrared wavelengths of the most energetic non-quasar transient ever observed, AT2021lwx. Our data show a single optical brightening by a factor >100 to a luminosity of 7 × 10 45 erg s -1 and a total radiated energy of 1.5 × 10 53 erg, both greater than any known optical transient. The decline is smooth and
    Wiseman, P. et al.

    Fecha de publicación:

    7
    2023
    Número de citas
    8
  • OzDES Reverberation Mapping Programme: Mg II lags and R-L relation
    The correlation between the broad line region radius and continuum luminosity (R-L relation) of active galactic nuclei (AGNs) is critical for single-epoch mass estimates of supermassive black holes (SMBHs). At z ~ 1-2, where AGN activity peaks, the R-L relation is constrained by the reverberation mapping (RM) lags of the Mg II line. We present 25
    Yu, Zhefu et al.

    Fecha de publicación:

    7
    2023
    Número de citas
    26
  • The MAGPI Survey: impact of environment on the total internal mass distribution of galaxies in the last 5 Gyr
    We investigate the impact of environment on the internal mass distribution of galaxies using the Middle Ages Galaxy Properties with Integral field spectroscopy (MAGPI) survey. We use 2D resolved stellar kinematics to construct Jeans dynamical models for galaxies at mean redshift z ~ 0.3, corresponding to a lookback time of 3-4 Gyr. The internal
    Derkenne, Caro et al.

    Fecha de publicación:

    7
    2023
    Número de citas
    9
  • Polarization of the Lyα Lines of H I and He II as a Tool for Exploring the Solar Corona
    The near-Earth space weather is driven by the quick release of magnetic free energy in the solar corona. Probing this extremely hot and rarified region of the extended solar atmosphere requires modeling the polarization of forbidden and permitted coronal lines. To this end, it is important to develop efficient codes to calculate the Stokes profiles
    Supriya, Hebbur Dayananda et al.

    Fecha de publicación:

    10
    2021
    Número de citas
    4
  • The First Detection of an Orphan Burst at the Rise Phase
    We report on the earliest detection of the optical transient MASTER OT J123248.62-012924.5 coincident within the error box with the optical and X-ray transient AT2021lfa/ZTF21aayokph. In our images the brightness of the object rises monotonically with $7σ$ confidence. We interpret this transient as a gamma-ray burst (GRB) characterized by smooth
    Lipunov, V. M. et al.

    Fecha de publicación:

    11
    2022
    Número de citas
    3
  • CASPER: A mission to study the time-dependent evolution of the magnetic solar chromosphere and transition regions
    Our knowledge about the solar chromosphere and transition region (TR) has increased in the last decade thanks to the huge scientific return of space-borne observatories like SDO, IRIS, and Hinode, and suborbital rocket experiments like CLASP1, CLASP2, and Hi-C. However, the magnetic nature of those solar regions remain barely explored. The
    Orozco Suárez, D. et al.

    Fecha de publicación:

    12
    2022
    Número de citas
    1