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  1. No Access

    Chapter and Conference Paper

    VEGA: A Visible Spectrograph and Polarimeter for the VLTI

    The ESO/VLTI has now clearly a position of world leader in the domain of ground-based optical interferometry. With four 8.2 m telescopes and two (four) 1.8 m telescopes, the Paranal Observatory is without any ...

    D. Mourard, P. Antonelli, A. Blazit… in The Power of Optical/IR Interferometry: Re… (2008)

  2. No Access

    Chapter and Conference Paper

    Searching for VLTI Calibrators with the JMMC’s Search Calibrators Tool

    A new version of ASPRO “Virtual observatory” companion tool looking for possible calibrators in the vicinity of a science object has been released. This user dedicated software creates an evolutive catalog of ...

    D. Bonneau, X. Delfosse, S. Cetre… in The Power of Optical/IR Interferometry: Re… (2008)

  3. No Access

    Chapter and Conference Paper

    LMC Cepheids with the VLTI

    We investigate the feasibility of applying the Interferometric Baade Wesselink method on LMC cepheids with the VLTI

    D. Mourard, N. Nardetto, S. Lagarde… in The Power of Optical/IR Interferometry: Re… (2008)

  4. No Access

    Chapter and Conference Paper

    First AMBER/VLTI Observations of Hot Massive Stars

    AMBER is the first near infrared focal instrument of the VLTI. It combines three telescopes and produces spectrally resolved interferometric measures. This paper discusses some preliminary results of the first...

    R. G. Petrov, F. Millour, O. Chesneau… in The Power of Optical/IR Interferometry: Re… (2008)