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/

  • SOPHIE velocimetry of Kepler transit candidates. XII. KOI-1257 b: a highly eccentric three-month period transiting exoplanet
    In this paper we report a new transiting warm giant planet: KOI-1257 b. It was first detected in photometry as a planet-candidate by the Kepler space telescope and then validated thanks to a radial velocity follow-up with the SOPHIE spectrograph. It orbits its host star with a period of 86.647661 d ± 3 s and a high eccentricity of 0.772 ± 0.045
    Santerne, A. et al.

    Advertised on:

    11
    2014
    Citations
    66
  • Southern red high proper motion objects (Lodieu+, 2005)
    Table main gives the names, coordinates (J2000), epoch, proper motions, and optical (BjRI) and near-infrared (JHKs) magnitudes for new, red proper motion objects published in this paper. Table obslog1 provides the observing logs for a subset of proper motion objects observed photometrically with FORS1 and ISAAC on the VLT. It includes observing
    Lodieu, N. et al.

    Advertised on:

    11
    2005
    Citations
    0
  • Space experiment TUS on board the Lomonosov satellite as pathfinder of JEM-EUSO
    Space-based detectors for the study of extreme energy cosmic rays (EECR) are being prepared as a promising new method for detecting highest energy cosmic rays. A pioneering space device - the "tracking ultraviolet set-up" (TUS) - is in the last stage of its construction and testing. The TUS detector will collect preliminary data on EECR in the
    Adams, J. H. et al.

    Advertised on:

    11
    2015
    Citations
    9
  • Space Telescope Imaging Spectrograph Ultraviolet Spectroscopy of Early B Supergiants in M31
    We analyze Space Telescope Imaging Spectrograph (STIS) spectra in the 1150-1700 Å wavelength range obtained for six early B supergiants in the neighboring galaxy M31. Because of their likely high (nearly solar) abundance, these stars were originally chosen to be directly comparable to their Galactic counterparts and represent a much needed addition
    Bresolin, Fabio et al.

    Advertised on:

    11
    2002
    Citations
    17
  • Spanish Astronomy
    Astrophysics is a very recent development in Spain, but its spectacular evolution in itself constitutes a singular phenomenon that has aroused the interest of sociologists and historians of science alike....
    Sánchez, F. et al.

    Advertised on:

    11
    2000
    Citations
    0