POPS (Planar Optical Phase Sensor) is a second-generation fringe tracker for the Very Large Telescope Inter-ferometer (VLTI), intended to simultaneously measure the cophasing and coherencing errors of up to six Unit Telescopes (UT) or Auxiliary Telescopes (AT) in real time. The most promising concepts are probably based on the utilization of Integrated Optics (IO) components, and were the scope of a Phase A study led by Observatoire de Grenoble (LAOG). Herein is described a tentative design built around a multi-axial IO chip whose fringes are dispersed downstream on a detector array, and a Chromatic Phase Diversity algorithm presented in another paper of this conference1. We depict the foreseen opto-mechanical, detection and software implem...
Phase Diversity (PD) is a wavefront-sensing technology that offers certain advantages in an Adaptive...
International audienceContext: Recently, an increasing number of scientific publications making use ...
The future PRIMA facility at the Very Large Telescope Interferometer (VLTI) in astrometric mode offe...
POPS (Planar Optical Phase Sensor) is a second-generation fringe tracker for the Very Large Telescop...
In a few years, the second generation instruments of the Very Large Telescope Interferometer (VLTI) ...
International audienceContext. With the arrival of the next generation of ground-based imaging inter...
The NOVA Fringe Tracker (NFT) is a proposed solution tóthe call by ESO for a second generation fring...
The Polarization-Based Collimated Beam Combiner efficiently produces pairwise interference between b...
The Phase Referenced Imaging and Micro Arcsecond Astrometry (PRIMA) facility for the Very Large Tele...
Context. The fringe sensor unit (FSU) is the central element of the phase referenced imaging and mic...
International audienceThe next generation of optical interferometers will provide high-resolution im...
It has been recently demonstrated that integrated optics could enhance accuracy, stability, and ease...
International audienceHierarchical Fringe Tracking (HFT) is a fringe tracking concept optimizing the...
We discuss the basis of a new concept of fringes tracking (FT) called the HFT for Hierarchical Fring...
The PRIMA (Phase-Referenced Imaging and Microarcsecond Astrometry) instrument at ESO/VLTI is schedul...
Phase Diversity (PD) is a wavefront-sensing technology that offers certain advantages in an Adaptive...
International audienceContext: Recently, an increasing number of scientific publications making use ...
The future PRIMA facility at the Very Large Telescope Interferometer (VLTI) in astrometric mode offe...
POPS (Planar Optical Phase Sensor) is a second-generation fringe tracker for the Very Large Telescop...
In a few years, the second generation instruments of the Very Large Telescope Interferometer (VLTI) ...
International audienceContext. With the arrival of the next generation of ground-based imaging inter...
The NOVA Fringe Tracker (NFT) is a proposed solution tóthe call by ESO for a second generation fring...
The Polarization-Based Collimated Beam Combiner efficiently produces pairwise interference between b...
The Phase Referenced Imaging and Micro Arcsecond Astrometry (PRIMA) facility for the Very Large Tele...
Context. The fringe sensor unit (FSU) is the central element of the phase referenced imaging and mic...
International audienceThe next generation of optical interferometers will provide high-resolution im...
It has been recently demonstrated that integrated optics could enhance accuracy, stability, and ease...
International audienceHierarchical Fringe Tracking (HFT) is a fringe tracking concept optimizing the...
We discuss the basis of a new concept of fringes tracking (FT) called the HFT for Hierarchical Fring...
The PRIMA (Phase-Referenced Imaging and Microarcsecond Astrometry) instrument at ESO/VLTI is schedul...
Phase Diversity (PD) is a wavefront-sensing technology that offers certain advantages in an Adaptive...
International audienceContext: Recently, an increasing number of scientific publications making use ...
The future PRIMA facility at the Very Large Telescope Interferometer (VLTI) in astrometric mode offe...