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/

  • Proper motions of field L and T dwarfs (Jameson+, 2008)
    In order to measure proper motions for known L and T dwarfs we observed 142 L and T dwarfs from the DwarfArchive (detailed in Table 1, see http://spider.ipac.caltech.edu/staff/davy/ARCHIVE/ for discovery references) with declinations between -30{deg} and 60{deg} and J-band magnitudes of less than 16.5. The images were taken using WFCAM on UKIRT
    Jameson, R. F. et al.

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    3
    2009
    Citations
    0
  • POLAR investigation of the Sun—POLARIS
    The POLAR Investigation of the Sun (POLARIS) mission uses a combination of a gravity assist and solar sail propulsion to place a spacecraft in a 0.48 AU circular orbit around the Sun with an inclination of 75° with respect to solar equator. This challenging orbit is made possible by the challenging development of solar sail propulsion. This first
    Appourchaux, T. et al.

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    3
    2009
    Citations
    22
  • Photolytic Decomposition of Hydrogenated C70: C70H38 and C70D38
    The hydrogenated C70 fullerenes C70H38 and C70D38 have been photolyzed at 245nm under Ar or He flow. The photolysis rate constant have been measured: k = 1.54x10-3s-1 for C70H38, and the photolysis of C70D38 occurs at a rate of 1.17x10-3s-1. A remarkable isotope effect in the photolysis of the two molecules has been determined kH/kD = 1.32. The
    Manchado, A. et al.

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    3
    2009
    Citations
    0
  • Periodic Very High Energy γ-Ray Emission from LS I +61°303 Observed with the MAGIC Telescope
    The MAGIC collaboration has recently reported the discovery of γ-ray emission from the binary system LS I +61°303 in the TeV energy region. Here we present new observational results on this source in the energy range between 300 GeV and 3 TeV. In total, 112 hr of data were taken between 2006 September and December covering four orbital cycles of
    Albert, J. et al.

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    3
    2009
    Citations
    121