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/

  • Magnetic activities on two single-lined RS Canum Venaticorum binaries IM Pegasi and σ Geminorum
    We present the study on continuous high-resolution spectroscopic observations of two long-period single-lined RS Canum Venaticorum (RS CVn) binary stars IM Pegasi (IM Peg) and σ Geminorum (σ Gem), obtained with the Hertzsprung SONG telescope during the 2015-2016 season. Chromospheric activity indicators H α, $\rm{Na\,\,{\small I}}$ D 1, D 2 doublet
    Cao, Dongtao et al.

    Advertised on:

    8
    2022
    Citations
    3
  • Optimizing spectral stacking for 21-cm observations of galaxies: accuracy assessment and symmetrized stacking
    We present an assessment of the accuracy of common operations performed in 21-cm spectral line stacking experiments. To this end, we generate mock interferometric data surveying the 21-cm emission at frequency 1310 < ν < 1420 MHz (0.005 < z < 0.084) and covering an area ~6 deg 2 of the sky, mimicking the observational characteristics of real
    Sinigaglia, Francesco et al.

    Advertised on:

    8
    2022
    Citations
    2
  • TESS discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136
    We present the discovery of TOI-2136 b, a sub-Neptune planet transiting a nearby M4.5V-type star every 7.85 d, identified through photometric measurements from the Transiting Exoplanet Survey Satellite (TESS) mission. The host star is located 33 pc away with a radius of R * = 0.34 ± 0.02 R ⊙, a mass of $0.34\pm 0.02 \, \mathrm{M}_{\odot }$, and an
    Gan, Tianjun et al.

    Advertised on:

    8
    2022
    Citations
    14
  • The Fornax3D project: intrinsic correlations between orbital properties and the stellar initial mass function
    Variations of the stellar initial mass function (IMF) in external galaxies have been inferred from a variety of independent probes. Yet the physical conditions causing these variations remain largely unknown. In this work, we explore new spatially resolved measurements of the IMF for three edge-on lenticular galaxies in the Fornax cluster. We
    Poci, A. et al.

    Advertised on:

    8
    2022
    Citations
    6
  • The star formation rates of QSOs
    We examine the far-infrared (FIR) properties of a sample of 5391 optically selected QSOs in the 0.5 < z < 2.65 redshift range down to log [νL ν, 2500(erg s -1)] > 44.7, using SPIRE data from Herschel-ATLAS. We split the sample in a grid of 74 luminosity-redshift bins and compute the average optical-IR spectral energy distribution (SED) in each bin
    Symeonidis, M. et al.

    Advertised on:

    8
    2022
    Citations
    6
  • A low-eccentricity migration pathway for a 13-h-period Earth analogue in a four-planet system
    It is commonly accepted that exoplanets with orbital periods shorter than one day, also known as ultra-short-period (USP) planets, formed further out within their natal protoplanetary disks before migrating to their current-day orbits via dynamical interactions. One of the most accepted theories suggests a violent scenario involving high
    Serrano, Luisa Maria et al.

    Advertised on:

    4
    2022
    Citations
    12