Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • Thesis
    A 3D VIEW OF AGN TRIGGERING
    Active galaxies are these showing strong emission coming from their nuclei. In the case of normal galaxies the nuclear emission has a stellar origin, but in active galactic nuclei (AGN) the emission is produced by accretion of matter into a super-massive black hole (SMBH). Although only a small percentage of galaxies in the nearby Universe
    Ignacio del Moral Castro

    Advertised on:

    2
    2022
    Bibcode
    THESIS
  • Thesis
    A 3D VIEW OF AGN TRIGGERING
    Active galaxies are these showing strong emission coming from their nuclei. In the case of normal galaxies the nuclear emission has a stellar origin, but in active galactic nuclei (AGN) the emission is produced by accretion of matter into a super-massive black hole (SMBH). Although only a small percentage of galaxies in the nearby Universe
    Ignacio del Moral Castro

    Advertised on:

    2
    2022
    Bibcode
    https://www.educacion.gob.es/teseo/mostrarSeleccion.do
  • Refereed
    A 20 Second Cadence View of Solar-type Stars and Their Planets with TESS: Asteroseismology of Solar Analogs and a Recharacterization of π Men c
    We present an analysis of the first 20 second cadence light curves obtained by the TESS space telescope during its extended mission. We find improved precision of 20 second data compared to 2 minute data for bright stars when binned to the same cadence (≍10%-25% better for T ≲ 8 mag, reaching equal precision at T ≍ 13 mag), consistent with pre
    Huber, Daniel et al.

    Advertised on:

    2
    2022
    Bibcode
    2022AJ....163...79H
    Citations
    47
  • Refereed
    TOI-2257 b: A highly eccentric long-period sub-Neptune transiting a nearby M dwarf
    Context. Thanks to the relative ease of finding and characterizing small planets around M-dwarf stars, these objects have become cornerstones in the field of exoplanet studies. The current paucity of planets in long-period orbits around M dwarfs makes such objects particularly compelling as they provide clues about the formation and evolution of
    Schanche, N. et al.

    Advertised on:

    1
    2022
    Bibcode
    2022A&A...657A..45S
    Citations
    21
  • Refereed
    The strange case of Na I in the atmosphere of HD 209458 b. Reconciling low- and high-resolution spectroscopic observations
    Aims: We aim to investigate the origin of the discrepant results reported in the literature about the presence of Na I in the atmosphere of HD 209458 b, based on low- and high-resolution transmission spectroscopy. Methods: We generated synthetic planetary atmosphere models and we compared them with the transmission light curves and spectra observed
    Morello, G. et al.

    Advertised on:

    1
    2022
    Bibcode
    2022A&A...657A..97M
    Citations
    5
  • Refereed
    The polarization angle in the wings of Ca I 4227: A new observable for diagnosing unresolved photospheric magnetic fields
    Context. When observed in quiet regions close to the solar limb, many strong resonance lines show conspicuous linear polarization signals, produced by scattering processes (i.e., scattering polarization), with extended wing lobes. Recent studies indicate that, contrary to what was previously believed, the wing lobes are sensitive to the presence of
    Capozzi, Emilia et al.

    Advertised on:

    1
    2022
    Bibcode
    2022A&A...657A..44C
    Citations
    1