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/

  • CoRoT-8b light and RV curves (Borde+, 2010)
    Light curves in the CoRoT white, blue, green, and red channels. The CoRoT bands are not simply related to any standard photometric systems. Because the applied corrections are channel-specific, the flux in the white channel is not the exact sum of the blue, green, and red fluxes. Also provided are the radial velocity measurements by the SOPHIE and
    Borde, P. et al.

    Advertised on:

    8
    2010
    Citations
    0
  • CoRoT Reveals a Magnetic Activity Cycle in a Sun-Like Star
    The 11-year activity cycle of the Sun is a consequence of a dynamo process occurring beneath its surface. We analyzed photometric data obtained by the CoRoT space mission, showing solarlike oscillations in the star HD49933, for signatures of stellar magnetic activity. Asteroseismic measurements of global changes in the oscillation frequencies and
    García, Rafael A. et al.

    Advertised on:

    8
    2010
    Citations
    258
  • Addendum: Optical re-brightening of the black hole transient XTE J1752-223
    We observed the black hole candidate XTE J1752-223 (ATel #2258) with the William Herschel Telescope (WHT) and the ACAM imager/spectrograph at the Observatorio del Roque de los Muchachos, La Palma, Spain. Two R-band exposures of 60 and 200 s and one I-band exposure of 200 s were taken under photometric conditions and 1.0-1.2-arcsec seeing on Aug 8
    Corral-Santana, J. M. et al.

    Advertised on:

    8
    2010
    Citations
    4
  • Abundance analysis of a sample of evolved stars in the outskirts of ω Centauri
    The globular cluster ω Centauri (NGC 5139) is a puzzling stellar system harboring several distinct stellar populations whose origin still represents a unique astrophysical challenge. Current scenarios range from primordial chemical inhomogeneities in the mother cloud to merging of different sub-units and/or subsequent generations of enriched stars
    Villanova, S. et al.

    Advertised on:

    8
    2010
    Citations
    8