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/

  • Optical and near-infrared polarization of the black hole X-ray binary A0620−00 in quiescence
    We present simultaneous high-precision optical polarimetric and near-infrared (NIR) to ultraviolet (UV) photometric observations of the low-mass black hole X-ray binary A0620−00 in a quiescent state. Subtracting interstellar polarization, estimated from a sample of field stars, we derived the intrinsic polarization of A0620−00. We show that the
    Kravtsov, Vadim et al.

    Advertised on:

    11
    2025
    Citations
    1
  • On the Origin of Neutron-capture Elements in r-I and r-II Stars: A Differential-abundance Analysis
    We present a strictly line-by-line differential analysis of a moderately r-process-enhanced star (r-I: HD 107752) with respect to a strongly r-process-enhanced star (r-II: CS 31082-0001) to investigate the possible common origin of their heavy-element nucleosynthesis with high-precision abundances. This study employs European Southern Observatory
    Saraf, Pallavi et al.

    Advertised on:

    11
    2025
  • On the computational feasibility of Bayesian end-to-end analysis of LiteBIRD simulations within Cosmoglobe
    We assess the computational feasibility of end-to-end Bayesian analysis of the JAXA-led LiteBIRD experiment by analysing simulated time ordered data (TOD) for a subset of detectors through the Cosmoglobe and Commander3 framework. The data volume for the simulated TOD is 1.55 TB, or 470 GB after Huffman compression. From this we estimate a total
    Aurvik, R. et al.

    Advertised on:

    11
    2025
    Citations
    0
  • Observation of undepleted phosphine in the atmosphere of a low-temperature brown dwarf
    The atmospheres of low-temperature brown dwarfs and gas giant planets are expected to contain the phosphine molecule, PH 3. However, previous observations have shown much lower abundances of this molecule than predicted with atmospheric chemistry models. We report JWST spectroscopic observations of phosphine in the atmosphere of the brown dwarf
    Burgasser, Adam J. et al.

    Advertised on:

    11
    2025
    Citations
    0
  • Nitrogen-bearing Species on Trans-Neptunian Objects Revealed by JWST/DiSCo-TNOs
    C≡N-bearing species are valuable tracers of nitrogen chemistry in the solar system. Ranging from volatile compounds like HCN and CH 3CN in cometary comae to refractory CN-bearing organics in some micrometeorites and interplanetary dust particles, these species originate in, or are derived from, molecular precursors in the interstellar medium (ISM)
    Cryan, S. et al.

    Advertised on:

    11
    2025
    Citations
    0
  • Neural translation for Stokes inversion and synthesis
    Context. The physical conditions in stellar atmospheres, such as temperature, velocity, and magnetic fields, can be obtained by interpreting solar spectro-polarimetric observations. Traditional inversion codes, while successful, are computationally demanding, however, especially for lines whose formation is complex and dictated by nonlocal
    Asensio Ramos, A. et al.

    Advertised on:

    11
    2025
    Citations
    0