ALOHA/CHARA at 1.55 μm: sensitivity improvement and on-sky ability to detect astronomical sources in H band

Author:

Darré P.1,Grossard L.1,Delage L.1,Reynaud F.1,Scott N. J.2,Sturmann J.2,Ten Brummelaar T. A.2

Affiliation:

1. XLIM Institut de Recherche (France)

2. CHARA (United States)

Publisher

SPIE

Reference16 articles.

1. Boyd, R.W., [Nonlinear Optics], Academic Press, (2008)

2. Quasi-phase-matched second harmonic generation: tuning and tolerances;Fejer,1992

3. Reynaud, F., Darré, P, Szemendera, L,. Grossard, L., Gomes, J.-T., Delage, L., “ALOHA project: how nonlinear optics can boost interferometry to propose a new generation of instrument for high-resolution imaging,” these proceeding 9907-44.

4. Phase closure retrieval in an infrared-to-visible upconversion interferometer for high resolution astronomical imaging

5. Contrast and phase closure acquisitions in photon counting regime using a frequency upconversion interferometer for high angular resolution imaging

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