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The WIYN One Degree Imager Optical Design

机译:WIYN一度成像仪光学设计

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The main advantage of the WIYN One Degree Imager (ODI) over other wide-field imagers will be its exceptional image quality. The fine pixel scale (0.11') provides uncompromised sampling of stellar PSFs under most conditions (seeing >0.3'). The telescope routinely delivers the site seeing (median ~ 0.7') which is often below 0.5' FWHM, and can be as low as 0.25'. The ODI specifications require the optics to maintain native high quality images. A two-element, fused silica, corrector meets the geometric error budget of 0.10' images, but the first element requires a mildly aspheric surface. The other element serves as the dewar window. A pair of cemented prisms (fused silica plus PBL6Y) serve as an ADC, which is essential to meet the image quality requirements for many observing programs. We describe the optical design details and its performance, the tolerances required, and the trade-offs considered for anti-reflection coatings. This paper is an update to a preliminary three-element design.
机译:WIYN一度成像仪(ODI)优于其他广角成像仪的主要优点是其卓越的图像质量。精细的像素比例(0.11')在大多数情况下(参见> 0.3')可提供对恒星PSF的完美采样。望远镜通常会看到的位置(中值〜0.7')通常低于0.5'FWHM,并且可以低至0.25'。 ODI规范要求光学器件保持原始的高质量图像。两元素熔融石英校正器可满足0.10'图像的几何误差预算要求,但第一个元素需要适度的非球面表面。另一个元素用作杜瓦瓶窗口。一对胶合棱镜(熔融石英加PBL6Y)用作ADC,这对于满足许多观察程序的图像质量要求至关重要。我们描述了光学设计的细节及其性能,所需的公差以及抗反射涂层的折衷考虑。本文是对初始三元素设计的更新。

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