International audienceWe describe the fringe-packet tracking system used to equalize the optical path lengths at the Infrared Optical Telescope Array interferometer. The measurement of closure phases requires obtaining fringes on three baselines simultaneously. This is accomplished by use of an algorithm based on double Fourier interferometry for obtaining the wavelength-dependent phase of the fringes and a group-delay tracking algorithm for determining the position of the fringe packet. A comparison of data acquired with and without the fringe-packet tracker shows a factor of ~3 reduction of the error in the closure-phase measurement. The fringe-packet tracker has been able so far to track fringes with signal-to-noise ratios as low as 1.8 ...
Context. The fringe sensor unit (FSU) is the central element of the phase referenced imaging and mic...
The major emphasis in the field of interferometry is the determination of optical path difference of...
Context. A turbulent atmosphere causes atmospheric piston variations leading to rapid chan...
We describe the fringe-packet tracking system used to equalize the optical path lengths at the Infra...
We describe the fringe–packet tracking software installed at the infrared optical telescope array (I...
We describe the fringe-packet tracking software installed at the infrared optical telescope array (I...
The fringe tracker system of the ASSI (Active Stabilization in Stellar Interferometry) beam combinin...
This paper reports on the measurement of optical path difference of spectral interference signal by ...
Large stellar telescope is indispensable for astronomy. Aperture synthesis is a well-known technique...
International audienceContext. The GRAVITY instrument was commissioned on the VLTI in 2016 and is no...
Differential measurements with dual feed stellar interferometers using large baselines can deliver e...
Measurement of interferometric parameters values is affected by phase disturbance due especially to ...
To enable optical long baseline interferometry toward faint objects, long integrations are necessary...
PHASECam is the fringe tracker for the Large Binocular Telescope Interferometer (LBTI). It is a near...
Context. The fringe sensor unit (FSU) is the central element of the phase referenced imaging and mic...
The major emphasis in the field of interferometry is the determination of optical path difference of...
Context. A turbulent atmosphere causes atmospheric piston variations leading to rapid chan...
We describe the fringe-packet tracking system used to equalize the optical path lengths at the Infra...
We describe the fringe–packet tracking software installed at the infrared optical telescope array (I...
We describe the fringe-packet tracking software installed at the infrared optical telescope array (I...
The fringe tracker system of the ASSI (Active Stabilization in Stellar Interferometry) beam combinin...
This paper reports on the measurement of optical path difference of spectral interference signal by ...
Large stellar telescope is indispensable for astronomy. Aperture synthesis is a well-known technique...
International audienceContext. The GRAVITY instrument was commissioned on the VLTI in 2016 and is no...
Differential measurements with dual feed stellar interferometers using large baselines can deliver e...
Measurement of interferometric parameters values is affected by phase disturbance due especially to ...
To enable optical long baseline interferometry toward faint objects, long integrations are necessary...
PHASECam is the fringe tracker for the Large Binocular Telescope Interferometer (LBTI). It is a near...
Context. The fringe sensor unit (FSU) is the central element of the phase referenced imaging and mic...
The major emphasis in the field of interferometry is the determination of optical path difference of...
Context. A turbulent atmosphere causes atmospheric piston variations leading to rapid chan...