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首页> 外文期刊>Monthly Notices of the Royal Astronomical Society >Towards a mid-infrared L band up-conversion interferometer: first on-sky sensitivity test on a single arm
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Towards a mid-infrared L band up-conversion interferometer: first on-sky sensitivity test on a single arm

机译:迈向中红外L波段上转换干涉仪:单臂首次空中灵敏度测试

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We report on the first on-sky sensitivity test on a single arm of the Astronomical Light Optical Hybrid Analysis (ALOHA) instrument, an uncooled up-conversion interferometer in the L band (3.5 mu m). Despite a low coupling efficiency (in the range of 1 per cent) between the 1-m class telescope and our instrument, we detect a magnitude L-mag = 2.8 star with a signal-to-noise ratio SNR = 2.7 over a 30 min integration time and with a spectral resolution lambda/Delta lambda = 100. As the ALOHA project aims to shift light from the L band to the near-infrared, the use of very low loss silica optical fibres is an important step towards fibre-linked very long-baseline interferometry in the mid-infrared.
机译:我们报告了天文光光学混合分析(ALOHA)仪器单臂上的首次空中灵敏度测试,该仪器是L波段(3.5微米)的未冷却上转换干涉仪。尽管1-m类望远镜与我们的仪器之间的耦合效率很低(在1%范围内),但我们在30分钟内检测到L-mag = 2.8星的大小,信噪比SNR = 2.7积分时间,且光谱分辨率为lambda / Delta lambda =100。由于ALOHA项目旨在将光从L波段转移到近红外波段,因此使用极低损耗的石英光纤是迈向与光纤相连的非常重要的一步中红外的长基线干涉测量法。

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