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/

  • J-PLUS: Toward a homogeneous photometric calibration using Gaia BP/RP low-resolution spectra

    Aims: We present the photometric calibration of the 12 optical passbands for the Javalambre Photometric Local Universe Survey (J-PLUS) third data release (DR3) comprising 1642 pointings of two square degrees each. Methods: We selected nearly 1.5 million main sequence stars with a signal-to-noise ratio larger than ten in the 12 J-PLUS passbands and

    López-Sanjuan, C. et al.

    Advertised on:

    3
    2024
    Citations
    0
  • Revealing the characteristics of the dark GRB 150309A: Dust extinguished or high-z?

    Context. Dark gamma-ray bursts (GRBs) constitute a significant fraction of the GRB population. In this paper, we present a multi-wavelength analysis (both prompt emission and afterglow) of an intense (3.98 × 10−5 erg cm−2 using Fermi-Gamma-Ray Burst Monitor) two-episodic GRB 150309A observed early on until ∼114 days post burst. Despite the strong

    Castro-Tirado, A. J. et al.

    Advertised on:

    3
    2024
    Citations
    0
  • The EDGE-CALIFA Survey: An Extragalactic Database for Galaxy Evolution Studies

    The EDGE-CALIFA survey provides spatially resolved optical integral-field unit and CO spectroscopy for 125 galaxies selected from the Calar Alto Legacy Integral Field Area Survey (CALIFA) Data Release 3 sample. The Extragalactic Database for Galaxy Evolution (EDGE) presents the spatially resolved products of the survey as pixel tables that reduce

    Wong, Tony et al.

    Advertised on:

    3
    2024
    Citations
    0
  • The elusive atmosphere of WASP-12 b. High-resolution transmission spectroscopy with CARMENES

    To date, the hot Jupiter WASP-12 b has been the only planet with confirmed orbital decay. The late F-type host star has been hypothesized to be surrounded by a large structure of circumstellar material evaporated from the planet. We obtained two high-resolution spectral transit time series with CARMENES and extensively searched for absorption

    Czesla, S. et al.

    Advertised on:

    3
    2024
    Citations
    0
  • Fundamental physics with ESPRESSO: a new determination of the D/H ratio towards PKS1937-101

    Primordial abundances of light elements are sensitive to the physics of the early Universe and can directly constrain cosmological quantities, such as the baryon-to-photon ratio $\eta _{10}$, the baryon density, and the number of neutrino families. Deuterium is especially suited for these studies: its primordial abundance is sensitive and

    Guarneri, Francesco et al.

    Advertised on:

    4
    2024
    Citations
    0
  • CHEOPS observations of KELT-20 b/MASCARA-2 b: An aligned orbit and signs of variability from a reflective day side

    Context. Occultations are windows of opportunity to indirectly peek into the dayside atmosphere of exoplanets. High-precision transit events provide information on the spin-orbit alignment of exoplanets around fast-rotating hosts. Aims: We aim to precisely measure the planetary radius and geometric albedo of the ultra-hot Jupiter (UHJ) KELT-20 b

    Singh, V. et al.

    Advertised on:

    3
    2024
    Citations
    0