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/

  • Chromospheric Flashes in a Solar Pore: Insights from Multiline Spectropolarimetric Diagnostics
    Solar pores are strongly magnetized regions without a photospheric penumbra, with predominantly vertical magnetic fields. We present a multiline investigation of flashes in a pore using high-resolution Swedish Solar Telescope observations in Fe I 6302, Ca II (λ8542 and K), and Hβ, complemented with (extreme-)UV observations from the Interface
    Dubey, Sandeep et al.

    Advertised on:

    3
    2026
    Citations
    0
  • Calibrating Mid-infrared Emission Features as Diagnostics of Star Formation in Infrared-luminous Galaxies via Radiative Transfer Modeling
    Luminous infrared (IR) galaxies are key sites of obscured stellar mass assembly at z > 0.5. Their star formation rates (SFRs) are often estimated using the luminosities of the 6.2 and 11.2 μm polycyclic aromatic hydrocarbon (PAH) features or those of the [Ne II] and [Ne III] fine-structure lines, as they are minimally affected by obscuration. It is
    Robinson, Loren et al.

    Advertised on:

    3
    2026
    Citations
    0
  • Binarity at LOw Metallicity (BLOeM): Projected rotational velocities
    The Binarity at LOw Metallicity (BLOeM) survey is an ESO large programme designed to obtain multi-epoch spectroscopy for 929 massive stars in the Small Magellanic Cloud (SMC). It will provide binary fractions and orbital configurations of binary systems and search for dormant black hole binary candidates (OB+BH). We present projected rotational
    Lennon, D. J. et al.

    Advertised on:

    3
    2026
    Citations
    0
  • Appraising the Necklace: A post-common-envelope carbon dwarf inside an apparently carbon-poor planetary nebula
    Context. The Necklace nebula is a bipolar, post-common-envelope planetary nebula, the central star of which has been shown to have a dwarf carbon star companion. Aims. We aim to understand the origins of the Necklace and its dwarf carbon central star. Methods. We study the carbon abundance of the nebula through far-ultraviolet spectroscopy obtained
    Jones, David et al.

    Advertised on:

    3
    2026
    Citations
    0
  • A Warm Massive Pair of Planets around TOI-1232 Revealed with Transit-timing Variations and Doppler Spectroscopy
    TOI-1232 is a G dwarf star with a mass of 1.0 6 − 0.06 + 0.07 M ⊙ , a radius of 1.07 ± 0.05 R ⊙, and a slightly higher metallicity than solar of Fe/H = 0.18 ± 0.05. The star hosts a transiting warm Jovian-mass planet, TOI-1232 b, with an orbital period of P b = 14.25 6 − 0.001 + 0.001 days, identified with data from multiple sectors of the TESS
    Mihaylov, Deyan P. et al.

    Advertised on:

    3
    2026
    Citations
    0
  • A Morphology Catalog of Galaxies in CEERS: Evolution in the Size and Color Gradients of Galaxies Since Cosmic Dawn
    We present measurements of morphological parameters from fitting 53,885 galaxies detected to a magnitude limit of F356W < 28.5 in the CEERS NIRCam imaging with GALFIT in six broadband filters: F115W, F150W, F200W, F277W, F356W, and F444W. We provide a public catalog of Sérsic indices, effective semimajor axes, axis ratios, integrated magnitudes
    McGrath, Elizabeth J. et al.

    Advertised on:

    3
    2026
    Citations
    0