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/

  • Refereed
    Gaia Early Data Release 3. Summary of the contents and survey properties (Corrigendum)
    Gaia Collaboration et al.

    Advertised on:

    6
    2021
    Bibcode
    2021A&A...650C...3G
    Citations
    97
  • Refereed
    Optical spectroscopy of blazars for the Cherenkov Telescope Array
    Context. Blazars are the most numerous class of high-energy (HE; E ∼ 50 MeV−100 GeV) and very high-energy (VHE; E ∼ 100 GeV−10 TeV) gamma-ray emitters. Currently, a measured spectroscopic redshift is available for only about 50% of gamma-ray BL Lacertae objects (BL Lacs), mainly due to the difficulty in measuring reliable redshifts from their
    Goldoni, P. et al.

    Advertised on:

    6
    2021
    Bibcode
    2021A&A...650A.106G
    Citations
    20
  • Refereed
    The Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation. I. Programme overview
    The Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of structure formation (CHEX-MATE) is a three-mega-second Multi-Year Heritage Programme to obtain X-ray observations of a minimally-biased, signal-to-noise-limited sample of 118 galaxy clusters detected by Planck through the Sunyaev-Zeldovich effect. The
    CHEX-MATE Collaboration et al.

    Advertised on:

    6
    2021
    Bibcode
    2021A&A...650A.104C
    Citations
    59
  • Refereed
    KMT-2019-BLG-0371 and the Limits of Bayesian Analysis
    We show that the perturbation at the peak of the light curve of microlensing event KMT-2019-BLG-0371 is explained by a model with a mass ratio between the host star and planet of q ∼ 0.08. Due to the short event duration (t E ∼ 6.5 days), the secondary object in this system could potentially be a massive giant planet. A Bayesian analysis shows that
    Kim, Yun Hak et al.

    Advertised on:

    7
    2021
    Bibcode
    2021AJ....162...17K
    Citations
    13