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/

  • Deep Extragalactic VIsible Legacy Survey (DEVILS): evolution of the morphology–density relation
    Galaxies with different morphological characteristics likely have different evolutionary histories, such that understanding the mechanisms that drive morphological change can provide valuable insights into the galaxy evolution process. These mechanisms largely correlate with local environment, ultimately leading to the well-known local morphology
    Davies, L. J. M. et al.

    Advertised on:

    9
    2025
    Citations
    0
  • Dark energy survey: Modeling strategy for multiprobe cluster cosmology and validation for the full six-year dataset
    We introduce an updated To&Krause2021 model for joint analyses of cluster abundances and large-scale two-point correlations of weak lensing and galaxy and cluster clustering (termed CL + 3 × 2 pt analysis) and validate that this model meets the systematic accuracy requirements of analyses with the statistical precision of the final Dark Energy
    To, Chun-Hao et al.

    Advertised on:

    9
    2025
    Citations
    5
  • Continuum, CO, and water vapour maps of the Orion Nebula: First millimetre spectral imaging with CONCERTO
    Context. The millimetre spectrum of Galactic regions and galaxies is rich in continuum and molecular lines. This diversity is mostly explored using either broad-band photometry or high-resolution heterodyne spectroscopy. Aims. We aim to map the millimetre continuum emission of Galactic regions with an intermediate spectral resolution between
    Désert, F. -X. et al.

    Advertised on:

    9
    2025
    Citations
    1
  • Compositional Characterization of the Polana-Eulalia Complex with JWST
    Determining the distribution of water throughout the main asteroid belt can inform us about the formation and evolution of the early Solar System. A powerful method for probing water abundance involves the observation and characterization of carbon-rich (C-complex) asteroids in the "3-μm region," which contains the fundamental OH stretching mode
    McClure, Lucas et al.

    Advertised on:

    9
    2025
    Citations
    0
  • Compositional Characterization of Cliff-Type Trans-Neptunian Objects
    Introduction: Trans-Neptunian Objects (TNOs) harbor materials from the early solar nebula (e.g., Gladman et al. 2008; Tegler et al. 2016). Observations from the NIRSpec instrument onboard the James Webb Space Telescope (JWST) included >50 TNOs during Cycle 1 for the large program "Discovering the Compositions of TNOs" (DiSCo-TNOs; #2418; PI: N
    McClure, Lucas et al.

    Advertised on:

    9
    2025
    Citations
    0
  • Composition of asteroid 84 Klio with NIRSpec/JWST
    Primitive C-complex asteroids, primarily located in the main asteroid belt, are commonly associated with carbonaceous chondrites (CCs) due to their low geometric albedo (typically pv<10%) and similar spectral shape [e.g. 1]. The presence of hydrated minerals and organics in CCs attests to the accretion of volatiles by their parent body in the early
    Le Pivert-Jolivet, Tania et al.

    Advertised on:

    9
    2025
    Citations
    0