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/

  • Self-supervised clustering on image-subtracted data with deep-embedded self-organizing map
    Developing an effective automatic classifier to separate genuine sources from artifacts is essential for transient follow-ups in wide-field optical surveys. The identification of transient detections from the subtraction artifacts after the image differencing process is a key step in such classifiers, known as real-bogus classification problem. We
    Mong, Y. -L. et al.

    Advertised on:

    1
    2023
    Citations
    1
  • Signs of environmental effects on star-forming galaxies in the Spiderweb protocluster at z = 2.16
    We use multi-object near-infrared spectroscopy with VLT/KMOS to investigate the role of the environment in the evolution of the ionized gas properties of narrow-band-selected H α emitters (HAEs) in the Spiderweb protocluster at z = 2.16. Based on rest-frame optical emission lines, H α and [N II]λ6584, we confirm the cluster membership of 39 of our
    Pérez-Martínez, J. M. et al.

    Advertised on:

    1
    2023
    Citations
    14
  • Star formation in IC1396: Kinematics and subcluster structure revealed by Gaia
    Aims: We investigate the star formation history of the IC1396 region by studying its kinematics and completing the population census. Methods: We used multiwavelength data, combining optical spectroscopy to identify and classify new members and near-infrared photometry to trace shocks, jets, and outflows as well as the interactions between the
    Pelayo-Baldárrago, Mara E. et al.

    Advertised on:

    1
    2023
    Citations
    6
  • Star formation in outer rings of S0 galaxies. V. UGC 4599: An S0 with gas probably accreted from a filament
    Aims: Though S0 galaxies are usually thought to be `red and dead', they often demonstrate weak star formation organised in ring structures and located in their outer disks. We try to clarify the nature of this phenomenon and its difference from star formation in spiral galaxies. The nearby moderate-luminosity S0 galaxy UGC 4599 is studied here
    Sil'chenko, O. et al.

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    1
    2023
    Citations
    5
  • STRIDES: automated uniform models for 30 quadruply imaged quasars
    Gravitational time delays provide a powerful one-step measurement of H 0, independent of all other probes. One key ingredient in time-delay cosmography are high-accuracy lens models. Those are currently expensive to obtain, both, in terms of computing and investigator time (10 5-10 6 CPU hours and ~0.5-1 yr, respectively). Major improvements in
    Schmidt, T. et al.

    Advertised on:

    1
    2023
    Citations
    37
  • The Dawes Review 10: The impact of deep learning for the analysis of galaxy surveys
    The amount and complexity of data delivered by modern galaxy surveys has been steadily increasing over the past years. New facilities will soon provide imaging and spectra of hundreds of millions of galaxies. Extracting coherent scientific information from these large and multi-modal data sets remains an open issue for the community and data-driven
    Huertas-Company, M. et al.

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    1
    2023
    Citations
    52