Post-processing the VLTI fringe-tracking data: First measurements of stars

At the Very Large Telescope Interferometer, the purpose of the fringe-tracker FINITO is to stabilize the optical path differences between the beams, allowing longer integration times on the scientific instruments AMBER and MIDI. Our goal is to demonstrate the potential of FINITO for providing H-band...

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Bibliographic Details
Published in:arXiv.org 2008-12
Main Authors: Jean-Baptiste Le Bouquin, Abuter, Roberto, Haguenauer, Pierre, Bauvir, Bertrand, Popovic, Daniel, Pozna, Ester
Format: Article
Language:English
Subjects:
Beams (radiation)
Laboratory equipment
Post-processing
Recording
Tracking
Transfer functions
Very Large Telescope
Online Access:Get full text
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Summary:At the Very Large Telescope Interferometer, the purpose of the fringe-tracker FINITO is to stabilize the optical path differences between the beams, allowing longer integration times on the scientific instruments AMBER and MIDI. Our goal is to demonstrate the potential of FINITO for providing H-band interferometric visibilities, simultaneously and in addition to its normal fringe-tracking role. We use data obtained during the commissioning of the Reflective Memory Network Recorder at the Paranal observatory. This device has permitted the first recording of all relevant real-time data needed for a proper data-reduction. We show that post-processing the FINITO data allows valuable scientific visibilities to be measured. Over the several hours of our engineering experiment, the intrinsic transfer function is stable at the level of 2%. Such stability would lead to robust measurements of science stars even without the observation of a calibration star within a short period of time. We briefly discuss the current limitations and the potential improvements.
ISSN:2331-8422
DOI:10.48550/arxiv.0812.2328