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 distribution and origin of metals in simulated Milky Way-like galaxies
    Chemical properties of stellar populations are a key observable that can be used to shed light on the assembly history of galaxies across cosmic time. In this study, we investigate the distribution and origin of chemical elements in different stellar components of simulated Milky Way-like galaxies in relation to their mass assembly history, stellar
    Iza, F. G. et al.

    Advertised on:

    9
    2025
    Citations
    0
  • SpecDis: Value Added Distance Catalog for 4 Million Stars from DESI Year-1 Data
    We present the SPECDIS value-added stellar distance catalog accompanying DESI Data Release 1. SPECDIS trains a feed-forward neural network (NN) with Gaia parallaxes and gets the distance estimates. To build up an unbiased training sample, we do not apply selections on parallax error or signal-to-noise (S/N) of the stellar spectra, and instead, we
    Li, Songting et al.

    Advertised on:

    9
    2025
    Citations
    4
  • Solvent-Free Solid State Dechlorination of C 60 Cl 6 and C 60 Cl 12 with Cesium Iodide
    Cataldo, Silvia et al.

    Advertised on:

    9
    2025
    Citations
    0
  • Probing Thin Winds in Massive OB Stars of the SMC with JWST/NIRSPEC Brα Spectroscopy
    Mass loss is a key physical process in the evolution of massive stars, the impact of which propagates into galactic evolution, population synthesis models, the interpretation of high-redshift galaxies, and explosive events such as supernovae. However, there are currently substantial uncertainties in the low-metallicity, low-luminosity thin wind
    Garcia, Miriam et al.

    Advertised on:

    9
    2025
    Citations
    0
  • Polarized, variable radio emission from the scallop-shell binary system DG CVn
    DG CVn is an eruptive variable star and represents the closest member of the known sample of complex periodic variables, or scallop-shell stars. Over the years, this M dwarf binary system has shown significant flaring activity at a wide range of frequencies. Here, we present a detailed analysis of ∼14 hours of radio observations of this stellar
    Kaur, Simranpreet et al.

    Advertised on:

    9
    2025
    Citations
    0
  • PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. II. Physical Properties from Decision-tree-based Spectral Energy Distribution Fitting of NUV-U-B-V-I Photometry with Categorical Priors Set by Hα Emission, Cluster Mor
    This paper is the second in a series presenting the catalogs and properties of the largest sample to date of ∼100,000 star clusters and compact associations, in 38 spiral galaxies observed by the PHANGS-HST Treasury survey. Here, we present spectral energy distribution (SED) fitting techniques used to compute the age, mass, and reddening for each
    Thilker, David A. et al.

    Advertised on:

    9
    2025
    Citations
    0