In-lab ALOHA mid-infrared up-conversion interferometer with high fringe contrast @λ = 3.39 μm
We report on the implementation of a mid-infrared (MIR) interferometer prototype for furthermore application in the framework of high-resolution imaging in astronomy. This paper demonstrates the possibility to extend to the L band our experimental study performed on the up-conversion interferometer...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2016-04, Vol.457 (3), p.3115-3118 |
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| container_title | Monthly notices of the Royal Astronomical Society |
| container_volume | 457 |
| creator | Szemendera, L. Darré, P. Baudoin, R. Grossard, L. Delage, L. Herrmann, H. Silberhorn, C. Reynaud, F. |
| description | We report on the implementation of a mid-infrared (MIR) interferometer prototype for furthermore application in the framework of high-resolution imaging in astronomy. This paper demonstrates the possibility to extend to the L band our experimental study performed on the up-conversion interferometer in H band. This in-laboratory preliminary experiment allowed us to get the first fringes with the MIR Astronomical Light Optical Hybrid Analysis (ALOHA) @3.39 μm up-conversion interferometer with a bright quasi monochromatic source (HeNe 3.39 μm). A stable contrast greater than 98 per cent has been reached. This opens the possibility to propose an alternative instrument for the demanding domain of high resolution imaging in the MIR domain. |
| doi_str_mv | 10.1093/mnras/stw196 |
| format | Article |
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| subjects | Engineering Sciences Optics Photonic |
| title | In-lab ALOHA mid-infrared up-conversion interferometer with high fringe contrast @λ = 3.39 μm |
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