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Laurent Koechlin

Researcher at Centre national de la recherche scientifique

Publications -  42
Citations -  326

Laurent Koechlin is an academic researcher from Centre national de la recherche scientifique. The author has contributed to research in topics: Speckle pattern & Angular resolution. The author has an hindex of 10, co-authored 39 publications receiving 317 citations. Previous affiliations of Laurent Koechlin include University of Toulouse & Los Angeles Trade–Technical College.

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Journal ArticleDOI

Dispersed fringe tracking with the multi-r(0) apertures of the Grand Interféromètre à 2 Télescopes.

TL;DR: A new fringe tracker based on photon-counting detectors and real-time image processing has been implemented on the Grand Interféromètre à 2 Télescopes at the Observatoire de la Cote d'Azur.
Journal ArticleDOI

Speckle observations with PISCO in Merate – I. Astrometric measurements of visual binaries in 2004

TL;DR: In this paper, relative astrometric measurements of visual binaries taken during the second semester of 2004 with the Pupil Interferometry Speckle camera and Coronagraph (PISCO) at the 1-m Zeiss telescope of the Brera Astronomical Observatory, in Merate, Italy.
Journal ArticleDOI

The 'Pisco' Speckle Camera at Pic Du Midi Observatory

TL;DR: PISCO as discussed by the authors is a speckle camera designed and built at Observatoire Midi-Pyrenees, which can be set in various operating modes: full pupil imaging, masked-pupil imaging, spectroscopy, wavefront sensor and stellar coronagraphy.
Proceedings ArticleDOI

Hypertelescope imaging: from exo-planets to neutron stars

TL;DR: In this paper, a precursor array of flying mirrors driven by solar sails in geostationary orbit is presented, which can in principle resolve the green spots on an Earth seen at several parsecs.
Journal ArticleDOI

Speckle Observations of Double Stars with PISCO at Pic du Midi: Measurements in 1998

TL;DR: In this paper, the PISCO speckle camera at Pic du Midi was used to detect double binary stars with angular separation in the range 1-10, which were mainly selected among grade 3 orbits to improve the accuracy of their orbits and constrain their masses.