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
    Is the activity level of HD 80606 influenced by its eccentric planet?
    Aims: Several studies suggest that the activity level of a planet-host star can be influenced by the presence of a close-by orbiting planet. Moreover, the interaction mechanisms that have been proposed, magnetic interaction and tidal interaction, exhibit a very different dependence on the orbital separation between the star and the planet. A
    Figueira, P. et al.

    Advertised on:

    8
    2016
    Bibcode
    2016A&A...592A.143F
    Citations
    16
  • Refereed
    High spatial resolution optical imaging of the multiple T Tauri system Lk Hα 262/Lk Hα 263
    We report high spatial resolution i' band imaging of the multiple T Tauri system LkHα 262/LkHα 263 obtained during the first commissioning period of the Adaptive Optics Lucky Imager (AOLI) at the 4.2-m William Herschel Telescope, using its Lucky Imaging mode. AOLI images have provided photometry for each of the two components LkHα 263 A and B (0.41
    Velasco, S. et al.

    Advertised on:

    8
    2016
    Bibcode
    2016MNRAS.460.3519V
    Citations
    16
  • Non-refereed
    HARPS3 for a roboticized Isaac Newton Telescope
    We present a description of a new instrument development, HARPS3, planned to be installed on an upgraded and roboticized Isaac Newton Telescope by end-2018. HARPS3 will be a high resolution (R≃115,000) echelle spectrograph with a wavelength range from 380-690 nm. It is being built as part of the Terra Hunting Experiment - a future 10- year radial
    Thompson, S. J. et al.

    Advertised on:

    8
    2016
    Bibcode
    2016SPIE.9908E..6FT
    Citations
    40
  • Non-refereed
    FRIDÁs mechanisms control system structure and tests
    FRIDA will be a near infrared imager and integral field spectrograph covering the wavelength range from 0.9 to 2.5 microns. FRIDA will work in two observing modes: direct imaging and integral field spectroscopy. This paper presents the main structure of the FRIDA mechanisms control system. In order to comply with a high level of re-configurability
    Flores-Meza, R. et al.

    Advertised on:

    8
    2016
    Bibcode
    2016SPIE.9913E..4KF
    Citations
    0
  • Non-refereed
    FRIDA: diffraction-limited imaging and integral-field spectroscopy for the GTC
    FRIDA is a diffraction-limited imager and integral-field spectrometer that is being built for the adaptive-optics focus of the Gran Telescopio Canarias. In imaging mode FRIDA will provide scales of 0.010, 0.020 and 0.040 arcsec/pixel and in IFS mode spectral resolutions of 1500, 4000 and 30,000. FRIDA is starting systems integration and is
    Watson, A. M. et al.

    Advertised on:

    8
    2016
    Bibcode
    2016SPIE.9908E..0PW
    Citations
    5
  • Refereed
    Follow-up observations of extremely metal-poor stars identified from SDSS
    Context. The most metal-poor stars in the Milky Way witnessed the early phases of formation of the Galaxy, and have chemical compositions that are close to the pristine mixture from Big Bang nucleosynthesis, polluted by one or few supernovae. Aims: Only two dozen stars with ([Fe/H] -4) are known, and they show a wide range of abundance patterns
    Aguado, D. S. et al.

    Advertised on:

    8
    2016
    Bibcode
    2016A&A...593A..10A
    Citations
    28