1. Experimental evaluation of achromatic phase shifters for mid-infrared starlight suppression
- Author
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Gappinger, Robert O., Diaz, Rosemary T., Ksendzov, Alexander, Lawson, Peter R., Lay, Oliver P., Liewer, Kurt M., Loya, Frank M., Martin, Stefan R., Serabyn, Eugene, and Wallace, James K.
- Subjects
Achromatic devices -- Research ,Phase shift (Nuclear physics) -- Equipment and supplies ,Interferometry -- Methods ,Extrasolar planets -- Spectra ,Spectra (Spectroscopy) -- Research ,Bandwidth -- Research ,Bandwidth allocation ,Bandwidth technology ,Astronomy ,Physics - Abstract
Phase shifters are a key component of nulling interferometry, one of the potential routes to enabling the measurement of faint exoplanet spectra. Here, three different achromatic phase shifters are evaluated experimentally in the mid-infrared, where such nulling interferometers may someday operate. The methods evaluated include the use of dispersive glasses, a through-focus field inversion, and field reversals on reflection from antisymmetric flat-mirror periscopes. All three approaches yielded deep, broadband, mid-infrared nulls, but the deepest broadband nulls were obtained with the periscope architecture. In the periscope system, average null depths of 4 x [10.sup.-5] were obtained with a 25% bandwidth, and 2 x [10.sup.-5] with a 20% bandwidth, at a central wavelength of 9.5 [micro]m. The best short term nulls at 20% bandwidth were approximately 9 x [10.sup.-6], in line with error budget predictions and the limits of the current generation of hardware. OCIS codes: 120.3180, 120.4570, 350.1260.
- Published
- 2009