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/

  • SDSS-V LVM: Resolving physical conditions in the Trifid Nebula
    Aims. The chemical abundance of the interstellar medium sets the initial conditions for star formation and provides a probe of chemical galaxy evolution models. However, unresolved inhomogeneities in the electron temperature can lead to a systematic underestimation of the abundances. We aim to directly test this effect. Methods. We used the SDSS-V
    Sattler, Natascha et al.

    Advertised on:

    2
    2026
    Citations
    2
  • Revisiting the near-infrared calcium triplet as metallicity indicator
    The near-infrared calcium II triplet (CaT), around 850 nm, is a key metallicity indicator for red giant stars. We present a revised [Fe/H] calibration as a function of CaT line strengths and four luminosity indicators, including the Gaia G band, together with the classical V, I, and $K_s$ bandpasses. For this purpose, we used a sample of 366 red
    Navabi, M. et al.

    Advertised on:

    2
    2026
    Citations
    2
  • Revisiting the Atmosphere of HAT-P-70b with CARMENES High-resolution Transmission Spectroscopy
    Owing to hot and inflated envelopes that facilitate atmospheric studies, ultrahot Jupiters (UHJs) have attracted much attention. Significant progress has been achieved, from enlarging the sample size to broadening the studies to encompass diverse stellar types and ages. Here, we present a transmission spectroscopy study of HAT-P-70b, a UHJ orbiting
    Gan, Tianjun et al.

    Advertised on:

    2
    2026
    Citations
    0
  • Reconstructing CGM Dust in Nearby Galaxies - 2D Extinction Maps from the LBT LIGHTS Survey
    Dust in the circumgalactic medium (CGM) has been detected statistically, using tens of thousands of background galaxies or quasars to measure average attenuation. However, variations in dust properties among galaxies, and the causes of those variations, are lost when stacking. To achieve a sufficient level of precision that enables spatially
    Chuang, Chen-Yu et al.

    Advertised on:

    2
    2026
    Citations
    0
  • PyEMILI: A New Generation Computer-aided Spectral-line Identifier. II. Emission-line Identification and Plasma Diagnostics of a Sample of Gaseous Nebulae
    In order to test the robustness and reliability of the new generation spectral-line identifier PyEMILI, as initially introduced in Paper I, in line identification and establish a reference/benchmark dataset for future spectroscopic studies, we run the code on the line lists of a selected sample of emission-line nebulae, including planetary nebulae
    Tu, Zhijun et al.

    Advertised on:

    2
    2026
    Citations
    0
  • Prompt Searches for Very-high-energy γ-Ray Counterparts to IceCube Astrophysical Neutrino Alerts
    The search for sources of high-energy astrophysical neutrinos can be significantly advanced through a multimessenger approach, which seeks to detect the γ-rays that accompany neutrinos as they are produced at their sources. Multimessenger observations have so far provided the first evidence for a neutrino source, illustrated by the joint detection
    Eisenberger, L. et al.

    Advertised on:

    2
    2026
    Citations
    0