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/

  • Refereed
    The CARMENES search for exoplanets around M dwarfs. Photospheric parameters of target stars from high-resolution spectroscopy. II. Simultaneous multiwavelength range modeling of activity insensitive lines
    We present precise photospheric parameters of 282 M dwarfs determined from fitting the most recent version of PHOENIX models to high-resolution CARMENES spectra in the visible (0.52-0.96 μm) and NIR wavelength range (0.96-1.71 μm). With its aim to search for habitable planets around M dwarfs, several planets of different masses have been detected
    Passegger, V. M. et al.

    Advertised on:

    7
    2019
    Bibcode
    2019A&A...627A.161P
    Citations
    85
  • Refereed
    The CARMENES search for exoplanets around M dwarfs. Detection of a mini-Neptune around LSPM J2116+0234 and refinement of orbital parameters of a super-Earth around GJ 686 (BD+18 3421)
    Although M dwarfs are known for high levels of stellar activity, they are ideal targets for the search of low-mass exoplanets with the radial velocity (RV) method. We report the discovery of a planetary-mass companion around LSPM J2116+0234 (M3.0 V) and confirm the existence of a planet orbiting GJ 686 (BD+18 3421; M1.0 V). The discovery of the
    Lalitha, S. et al.

    Advertised on:

    7
    2019
    Bibcode
    2019A&A...627A.116L
    Citations
    16
  • Refereed
    Stellar content, planetary nebulae, and globular clusters of [KKS2000]04 (NGC 1052-DF2)
    [KKS2000]04 (NGC 1052-DF2) has become a controversial and well-studied galaxy after the claims suggesting a lack of dark matter and the presence of an anomalously bright globular cluster (GC) system around it. A precise determination of its overall star formation history (SFH) and a better characterization of its GC or planetary nebulae (PNe)
    Ruiz-Lara, T. et al.

    Advertised on:

    7
    2019
    Bibcode
    2019MNRAS.486.5670R
    Citations
    19
  • Refereed
    Stellar atmospheric parameters for 754 spectra from the X-shooter Spectral Library
    Context. The X-shooter Spectral Library (XSL) is an empirical stellar library at medium spectral resolution covering the wavelength range from 3000 Å to 24 800 Å. This library aims to provide a benchmark for stellar population studies. Aims: In this work, we present a uniform set of stellar atmospheric parameters, effective temperatures, surface
    Arentsen, Anke et al.

    Advertised on:

    7
    2019
    Bibcode
    2019A&A...627A.138A
    Citations
    63
  • Refereed
    Spitzer Parallax of OGLE-2018-BLG-0596: A Low-mass-ratio Planet around an M Dwarf
    We report the discovery of a Spitzer microlensing planet OGLE-2018-BLG-0596Lb, with preferred planet-host mass ratio q ∼ 2 × 10‑4. The planetary signal, which is characterized by a short (∼1 day) “bump” on the rising side of the lensing light curve, was densely covered by ground-based surveys. We find that the signal can be explained by a bright
    Jung, Youn Kil et al.

    Advertised on:

    7
    2019
    Bibcode
    2019AJ....158...28J
    Citations
    20
  • Thesis
    SOLAR ABUNDANCES FROM THREE-DIMENSIONAL EMPIRICAL MODELS
    El estudio de las abundancias solares se remonta al análisis de Russell de 1929 y, desde entonces, se ha vuelto un tema muy relevante para la astrofísica en general. Esto es debido a que conocer la composición química del Sol es fundamental para construir modelos precisos de la atmósfera y el interior del Sol y de otras estrellas. Además, la
    MELANIA CUBAS ARMAS

    Advertised on:

    7
    2019
    Bibcode
    LINK THESIS