Direct imaging and spectroscopy can advance our understanding of planet formation and migration through the detection and characterization of extrasolar planets on wide orbits. Accurate photometry and astrometry of detected companions are of crucial importance to derive the planet physical properties.We present an extension of the Locally optimized combination of images (LOCI) method to measure the highest-fidelity photometry as well as accurate astrometry of detected companions. This algorithm is also generalized to Integral-Field Spectrograph (IFS) data processing, giving advantages of a simultaneous angular and spectral differential imaging reduction, retrieving high-fidelity spectra from PSF-subtracted cubes. \ua9 2012 SPIE.Peer reviewe...
The direct exoplanet imaging field will strongly benefit from the higher angular resolution achieved...
Context. The improvement of large size detectors permitted the development of integral field spectro...
Context. The new planet finder for the Very Large Telescope (VLT), the Spectro-Polarimetric High-con...
High-contrast imaging instruments are now being equipped with integral field spectrographs (IFS) to ...
International audienceContext. Angular differential imaging (ADI) and spectral differential imaging ...
Context. Angular differential imaging (ADI) and spectral differential imaging (SDI) are well-establi...
International audienceSPHERE is an instrument aimed to the search for low mass companions around you...
Context. Angular differential imaging (ADI) and spectral differential imaging (SDI) are well-establi...
Context. Combining high-contrast imaging with medium- or high-resolution integral field spectroscopy...
Context. Direct imaging of exoplanets is a challenging task that requires state-of-the-art instrumen...
Observations of extrasolar planets using integral field spectroscopy (IFS), if coupled with an extre...
Among the group of extrasolar planets, transiting planets provide a great opportunity to obtain dire...
The direct imaging of planets around nearby stars is exceedingly difficult. Only about 14 exoplanets...
The direct exoplanet imaging field will strongly benefit from the higher angular resolution achieved...
Context. The improvement of large size detectors permitted the development of integral field spectro...
Context. The new planet finder for the Very Large Telescope (VLT), the Spectro-Polarimetric High-con...
High-contrast imaging instruments are now being equipped with integral field spectrographs (IFS) to ...
International audienceContext. Angular differential imaging (ADI) and spectral differential imaging ...
Context. Angular differential imaging (ADI) and spectral differential imaging (SDI) are well-establi...
International audienceSPHERE is an instrument aimed to the search for low mass companions around you...
Context. Angular differential imaging (ADI) and spectral differential imaging (SDI) are well-establi...
Context. Combining high-contrast imaging with medium- or high-resolution integral field spectroscopy...
Context. Direct imaging of exoplanets is a challenging task that requires state-of-the-art instrumen...
Observations of extrasolar planets using integral field spectroscopy (IFS), if coupled with an extre...
Among the group of extrasolar planets, transiting planets provide a great opportunity to obtain dire...
The direct imaging of planets around nearby stars is exceedingly difficult. Only about 14 exoplanets...
The direct exoplanet imaging field will strongly benefit from the higher angular resolution achieved...
Context. The improvement of large size detectors permitted the development of integral field spectro...
Context. The new planet finder for the Very Large Telescope (VLT), the Spectro-Polarimetric High-con...