Publication type: Non-refereed

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    High-resolution astronomical observations using deconvolution from wavefront sensing
    Deconvolution from wavefront sensing is a new technique of high-resolution imaging through atmospheric turbulence developed at ONERA. The capabilities of the...
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    High-Resolution Atmospheric Emission Spectroscopy at 120 cm-1 and 535 cm-1 with a Rapid-Scan Interferometer and 91 cm Airborne Telescope
    Not Available
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    High-Resolution Calibration of the SDSS/SEGUE Spectroscopic Analysis Pipeline
    We present a discussion of efforts to obtain external validation of the estimated atmospheric parameters (Teff, log g, [Fe/H]) obtained from medium-resolution...
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    High-resolution Ground-based European Solar Physics
    This communication reviews some of the most challenging topics in high-resolution ground-based Solar Physics. The most powerful European facilities are...
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    High-resolution IBIS Observations and Comparison with 3D Simulations
    We present first comparisons between high resolution observations of the quiet photosphere, obtained with the Interferometric BIdimensional Spectrometer (IBIS)...
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    High-resolution IBIS Observations and Comparison with 3D Simulations .
    High resolution observations of a very quiet region of the solar surface have been obtained with IBIS (Interferometric BIdimensional Spectrometer) in the non...
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    High-resolution imaging in the visible on large ground-based telescopes
    Lucky Imaging combined with a low order adaptive optics system has given the highest resolution images ever taken in the visible or near infrared of faint...
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    High-resolution imaging of active galactic nuclei
    A sample of active galaxies and quasars was observed with a photon-counting detector (IPCS) working in time-resolved imaging mode. The observing and data...
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    High-Resolution Imaging of Stars, Dust, and Star Formation in Nuclear Rings in Galaxies
    Nuclear rings in barred spiral galaxies offer an opportunity to study starburst properties, as well as the evolution of star formation in the central regions of...