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/

  • The Coronal Power Spectrum from MHD Mode Conversion above Sunspots
    Sunspots are intense regions of magnetic flux that are rooted deep below the photosphere. It is well established that sunspots host magnetohydrodynamic waves, with numerous observations showing a connection to the internal acoustic (or p-)modes of the Sun. The p-modes are fast waves below the equipartition layer and are thought to undergo a double
    Miriyala, Hemanthi et al.

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    2
    2025
    Citations
    1
  • The conceptual design of the 50-meter Atacama Large Aperture Submillimeter Telescope (AtLAST)
    The (sub)millimeter sky contains a vast wealth of information that is both complementary and inaccessible to other wavelengths. Over half the light we receive is observable at millimeter and submillimeter wavelengths, yet we have mapped only a small portion of the sky at sufficient spatial resolution and sensitivity to detect and resolve distant
    Mroczkowski, Tony et al.

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    2
    2025
    Citations
    26
  • The baryonic mass estimates of the Milky Way halo in the form of high-velocity clouds
    The halo of our Galaxy is populated with a significant number of high-velocity clouds (HVCs) moving with a speed up to 500 km/s. It is suggested that these HVCs might contain a non-negligible fraction of the missing baryons. The main aim of the current paper is to estimate the baryonic mass of the Milky Way halo in the form of HVCs in order to
    Tahir, Noraiz et al.

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    2
    2025
    Citations
    0
  • The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the interstellar medium of z ∼ 5 star-forming galaxies
    Context. Recent observations suggest a significant and rapid buildup of dust in galaxies at high redshift (z > 4); this presents new challenges to our understanding of galaxy formation in the early Universe. Although our understanding of the physics of dust production and destruction in a galaxy's interstellar medium (ISM) is improving
    Sawant, P. et al.

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    2
    2025
    Citations
    1
  • Testing disc reprocessing models for AGN optical variability by comparison of X-ray and optical power spectra of NGC 4395
    It is generally thought that active galactic nucleus (AGN) optical variability is produced, at least in part, by reprocessing of central X-rays by a surrounding accretion disc, resulting in wavelength-dependent lags between bands. Any good model of AGN optical variability should explain not only these lags, but also the overall pattern of
    Beard, M. W. J. et al.

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    2
    2025
    Citations
    2
  • State-dependent signatures of jets and winds in the optical and infrared spectrum of the black hole transient GX 339–4
    GX 339–4 is one of the prototypical black hole X-ray transients, exhibiting recurrent outbursts that allow detailed studies of black hole accretion and ejection phenomena. In this work we present four epochs of optical and near-infrared spectroscopy obtained with X-shooter at the Very Large Telescope. The dataset includes two hard state spectra
    Ambrifi, A. et al.

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    2
    2025
    Citations
    0