Presentation + Paper
28 August 2024 CHARA/Silmaril instrument software and data reduction pipeline: characterization of the instrument in the lab and on-sky
Author Affiliations +
Abstract
The newly installed Silmaril beam combiner at the CHARA array is designed to observe previously inaccessible faint targets, including Active Galactic Nuclei and T-Tauri Young Stellar Objects. Silmaril leverages cuttingedge optical design, low readout noise, and a high-speed C-RED1 camera to realize its sensitivity objectives. In this presentation, we offer a comprehensive overview of the instrument’s software, which manages critical functions, including camera data acquisition, fringe tracking, automatic instrument alignment, and observing interfaces, all aimed at optimizing on-sky data collection. Additionally, we offer an outline of the data reduction pipeline, responsible for converting raw instrument data products into the final OIFITS used by the standard interferometry modeling software. Finally, a thorough analysis of the camera and instrument characterization results will be presented, evaluating instrument performance in terms of sensitivity. The purpose of this paper is to provide a solid reference for studies based on Silmaril data.
Conference Presentation
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Narsireddy Anugu, Theo A. ten brummelaar, Cyprien Lanthermann, Peter G. Tuthill, Edgar R. Ligon III, Gail H. Schaefer, Douglas R. Gies, Grace Piroscia, Adam Taras, Gerard T. van Belle, Makoto Kishimoto, and Marc-Antoine Martinod "CHARA/Silmaril instrument software and data reduction pipeline: characterization of the instrument in the lab and on-sky", Proc. SPIE 13095, Optical and Infrared Interferometry and Imaging IX, 130951B (28 August 2024); https://doi.org/10.1117/12.3019305
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KEYWORDS
Cameras

Telescopes

Sensors

Stars

Data acquisition

Signal to noise ratio

K band

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