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/

  • Stellar atmospheric parameters of CARMENES GTO M-dwarfs with spectral synthesis and SteParSyn
    We aim to review the spectral synthesis technique to derive the stellar atmospheric parameters (T eff, log g, and [Fe/H]) of 348 M dwarfs in light of the optical and near-infrared spectra obtained with CARMENES, the high-resolution, double-channel spectrograph installed at the 3.5 m telescope at the Calar Alto observatory (Spain). The analysis
    Marfil, Emilio et al.

    Advertised on:

    3
    2021
    Citations
    0
  • Stellar atmospheric parameters of CARMENES GTO M dwarfs with spectral synthesis and SteParSyn
    We aim to review the spectral synthesis technique to derive the stellar atmospheric parameters (T eff, log g, and [Fe/H]) of 348 M dwarfs in light of the optical and near-infrared spectra obtained with CARMENES, the high-resolution, double-channel spectrograph installed at the 3.5 m telescope at the Calar Alto observatory (Spain). The analysis
    Marfil, Emilio et al.

    Advertised on:

    3
    2021
    Citations
    1
  • Spectral characterization of the craters of Ryugu as observed by the NIRS3 instrument on-board Hayabusa2
    C-type rubble pile asteroid (162173) Ryugu was observed and characterized up close for a year and a half by the instruments on-board the Japanese Aerospace eXploration Agency (JAXA) Hayabusa2 spacecraft. The asteroid exhibits relatively homogeneous spectral characteristics at near-infrared wavelengths (~1.8-3.2 μm), including a very low reflectance
    Riu, Lucie et al.

    Advertised on:

    3
    2021
    Citations
    6
  • Searching for the Alpha-Abundance Bimodality in the M31 Disk
    The recent era of large, ground-based abundance surveys has unraveled the chemical structures of our Milky Way galaxy. The most striking abundance feature is the alpha-abundance bimodality. The low-alpha stars are younger (1-8 Gyr) while the high-alpha stars are older (8-12 Gyr) and have a thicker distribution. There are a number of different
    Nidever, David et al.

    Advertised on:

    3
    2021
    Citations
    0
  • Searching for biomarkers in the potentially habitable atmospheric zones of Y dwarfs
    We report on an ongoing search for biomarkers in the potentially habitable atmospheres of a sample of a dozen Y dwarfs with Teff estimated at around or below 400 K. This work is being carried out using public data from large area optical surveys such as DES and PANStarrs. We focus on a search for g-band emission as an analogue to terrestrial
    Martin, E. et al.

    Advertised on:

    3
    2021
    Citations
    0
  • ROOSTER: a machine-learning analysis tool for Kepler stellar rotation periods
    In order to understand stellar evolution, it is crucial to efficiently determine stellar surface rotation periods. Indeed, while they are of great importance in stellar models, angular momentum transport processes inside stars are still poorly understood today. Surface rotation, which is linked to the age of the star, is one of the constraints
    Breton, S. N. et al.

    Advertised on:

    3
    2021
    Citations
    31