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Galilei-G4 和 Cassini 测量正常眼和屈光手术后眼角膜屈光力和散光的重复性和可比性。

Repeatability and comparability of the Galilei-G4 and Cassini in measuring corneal power and astigmatism in normal and post-refractive surgery eyes.

机构信息

Department of Ophthalmology, Cullen Eye Institute, Baylor College of Medicine, 6565 Fannin, NC205, Houston, TX, 77030, USA.

Department of Ophthalmology, Weill Cornell Ophthalmology, Weill Cornell, New York, NY, USA.

出版信息

Sci Rep. 2021 Aug 9;11(1):16141. doi: 10.1038/s41598-021-94319-w.

DOI:10.1038/s41598-021-94319-w
PMID:34373485
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC8352897/
Abstract

To assess the repeatability and comparability of the Galilei G4 versus the Cassini topographer in post-refractive eyes and in normal eyes, including older patients representative of an initial cataract evaluation. Simulated keratometric (simK), total corneal and posterior corneal power and astigmatism were evaluated in both post-refractive and normal eyes. Repeatability was measured by calculating within-subject standard deviation (Sw), coefficient of variation (CoV), and intraclass correlation coefficient (ICC). Vector analyses and Bland-Altman plots were employed to assess agreement between devices. We studied 32 subjects with a history of refractive surgery and 32 subjects without a history of refractive surgery undergoing cataract surgery. The mean age was 55 ± 18.5 years and the age range was 21.5-91.5 years. In non-refractive and post-refractive eyes, the ICC was > 0.9 (P < 0.001) for all corneal powers and for simK and total corneal astigmatism for both analyzers. The ICC for posterior corneal astigmatism magnitude using the Galilei was 0.62 and 0.67 and for the Cassini 0.55 and 0.38 in normal and post-refractive eyes, respectively. In both post-refractive and normal eyes, the Galilei G4 and Cassini analyzers have high repeatability in simK, total, and posterior corneal power and low repeatability for posterior corneal astigmatism.

摘要

为了评估 Galilei G4 和 Cassini 角膜地形仪在屈光手术后眼和正常眼中的可重复性和可比性,包括代表初始白内障评估的老年患者。在屈光后眼和正常眼中评估了模拟角膜曲率(simK)、总角膜和后角膜力和散光。通过计算组内标准差(Sw)、变异系数(CoV)和组内相关系数(ICC)来测量重复性。采用向量分析和 Bland-Altman 图来评估设备之间的一致性。我们研究了 32 例有屈光手术史的患者和 32 例无屈光手术史的患者,这些患者正在接受白内障手术。平均年龄为 55 ± 18.5 岁,年龄范围为 21.5-91.5 岁。在非屈光和屈光后眼中,两种分析仪的所有角膜力和 simK 以及总角膜散光的 ICC 均>0.9(P<0.001)。使用 Galilei 测量的后角膜散光大小的 ICC 分别为 0.62 和 0.67,而使用 Cassini 的 ICC 分别为 0.55 和 0.38,分别为正常眼和屈光后眼。在屈光后眼和正常眼中,Galilei G4 和 Cassini 分析仪在 simK、总角膜力和后角膜力方面具有较高的重复性,而在后角膜散光方面具有较低的重复性。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2f92/8352897/958eb394e11f/41598_2021_94319_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2f92/8352897/711e65f7b817/41598_2021_94319_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2f92/8352897/03419ced66b3/41598_2021_94319_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2f92/8352897/f68eab6abf7d/41598_2021_94319_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2f92/8352897/958eb394e11f/41598_2021_94319_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2f92/8352897/711e65f7b817/41598_2021_94319_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2f92/8352897/03419ced66b3/41598_2021_94319_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2f92/8352897/f68eab6abf7d/41598_2021_94319_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2f92/8352897/958eb394e11f/41598_2021_94319_Fig4_HTML.jpg

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