Paper
26 July 2016 ALOHA/CHARA at 1.55 μm: sensitivity improvement and on-sky ability to detect astronomical sources in H band
P. Darré, L. Grossard, L. Delage, F. Reynaud, N. J. Scott, J. Sturmann, T. A. Ten Brummelaar
Author Affiliations +
Abstract
The interferometric concept named ALOHA (Astronomical Light Optical Hybrid Analysis) offers an alternative for high resolution imaging in the mid-infrared domain by shifting the astronomical light to shorter wavelength where optical guided components from telecommunications are available and efficient. A prototype with two arms converting a signal from 1.55 μm to 630 nm is used to validate the concept in laboratory and on-sky. Thanks to collaboration with the CHARA team, photometric tests were achieved with a single arm of the interferometer and have allowed to predict instrument performance in its interferometric configuration in order to obtain first fringes in H band.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
P. Darré, L. Grossard, L. Delage, F. Reynaud, N. J. Scott, J. Sturmann, and T. A. Ten Brummelaar "ALOHA/CHARA at 1.55 μm: sensitivity improvement and on-sky ability to detect astronomical sources in H band", Proc. SPIE 9907, Optical and Infrared Interferometry and Imaging V, 990724 (26 July 2016); https://doi.org/10.1117/12.2232315
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KEYWORDS
Astronomy

Signal to noise ratio

Interferometry

Interferometers

Infrared radiation

Prototyping

Modulators

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