First on-sky interference fringes at 810 nm with the CHARA array using servo controlled hectometric outdoor fibre links

ABSTRACT In the framework of the ALOHA (Astronomical Light Optical Hybrid Analysis) project, we have implemented a fibre-linked interferometer connecting two telescopes of the CHARA (Center for High Angular Resolution Astronomy) array to the recombination beam facility using servo controlled hectometric outdoor fibres (240 m). During two consecutive nights, on-sky fringes at 810 nm were recorded on the star Vega (mag 0), with servo control of the fibre lengths. The optical path difference was set close to zero using internal fringes found before the on-sky observations. The repeatability of the delay line position offset between internal and on-sky fringes was less than 0.2 mm. The efficiency of the servo control systems has been demonstrated, leading to an enhancement of the signal-to-noise ratio from 68.9 with the servo off to 91.6 with the servo on. This result is a cornerstone for the ALOHA project goal of interferometry at 3.5 $\mu$m and a seminal step for the future kilometric infrared fibre-linked interferometer at CHARA.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2024-11-08
DOI
https://doi.org/10.1093/mnras/stae2522
Citations
2
Primary Topic
Astronomy and Astrophysical Research
Type
article
Field-Weighted Citation Impact
1.01

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article

First on-sky interference fringes at 810 nm with the CHARA array using servo controlled hectometric outdoor fibre links

Marc Fabert, Gail H. Schaefer, Julie Magri, C. Farrington et al.
2 citations
Monthly Notices of the Royal Astronomical Society
Astronomy and Astrophysical Research
1.01
article

First on-sky interference fringes at 810 nm with the CHARA array using servo controlled hectometric outdoor fibre links

Marc Fabert, Gail H. Schaefer, Julie Magri, C. Farrington, Lucien Lehmann, Olli Majoinen, Robert W. Ligon, Steve Golden, Narsireddy Anugu, Laurent Delage, Douglas R. Gies, Nicholas J. Scott, Rodolphe Krawczyk, Theo A. ten Brummelaar, Ludovic Grossard, Matt Anderson, François Reynaud, Jean-Michel Le Duigou, Norm Vargas, Craig Woods, Victor Castillo
article en
2 citations

Abstract

ABSTRACT In the framework of the ALOHA (Astronomical Light Optical Hybrid Analysis) project, we have implemented a fibre-linked interferometer connecting two telescopes of the CHARA (Center for High Angular Resolution Astronomy) array to the recombination beam facility using servo controlled hectometric outdoor fibres (240 m). During two consecutive nights, on-sky fringes at 810 nm were recorded on the star Vega (mag 0), with servo control of the fibre lengths. The optical path difference was set close to zero using internal fringes found before the on-sky observations. The repeatability of the delay line position offset between internal and on-sky fringes was less than 0.2 mm. The efficiency of the servo control systems has been demonstrated, leading to an enhancement of the signal-to-noise ratio from 68.9 with the servo off to 91.6 with the servo on. This result is a cornerstone for the ALOHA project goal of interferometry at 3.5 $\mu$m and a seminal step for the future kilometric infrared fibre-linked interferometer at CHARA.

Monthly Notices of the Royal Astronomical SocietyVol. 536(1)
Centre National de la Recherche Scientifique (FR), Leonardo (United States) (US), Georgia State University (US), Centre National d'Études Spatiales (FR), Thales (Germany) (DE), Mount Wilson Observatory (US), Université de Limoges (FR)
National Science Foundation, Georgia State University, Centre National d’Etudes Spatiales, Institut national des sciences de l'Univers, Office of the Vice President for Research and Economic Development, University at Buffalo
Openalex Percentile: Top 19%
Astronomy and Astrophysical Research
1.01
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