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胃排空闪烁显像检测排空延迟的最佳成像时机。

Optimal timing of imaging in gastric emptying scintigraphy for the detection of delayed emptying.

机构信息

Department of Radiology, University of Miami School of Medicine, 1611 NW 12th Avenue, JMH C-248, Miami, Florida 33136, United States.

出版信息

Hell J Nucl Med. 2021 Sep-Dec;24(3):234-238. doi: 10.1967/s002449912416.

Abstract

OBJECTIVE

The purpose of this study was to evaluate a standard 4-h imaging protocol for gastric emptying scintigraphy (GES) in detecting delayed gastric emptying (GE).

SUBJECTS AND METHODS

Gamma camera imaging was performed in the anterior and posterior views at 0, 0.5, 1, 1.5, 2, 2.5 and 4-h as per established Miami method (MIA) and National Standard Protocol (NSP), in accordance with the consensus guidelines of the ANMS/SNM [SNMMI] Societies. Patients (N=1002) received a standardized solid meal radiolabeled with 1mCi of technetium-99 (Tc) sulfur colloid. Quantitative analysis was performed using geometric mean calculation of decay-corrected counts at each imaging time point, expressed as percent emptying or retention.

RESULTS

In our patient cohort, 21% had delayed GE at 4h, whereas 79% had normal emptying with less than 10% retention at 4h. There was a 25% increase in delayed GE studies at 4h versus 2h. From those patients who had delayed GE at 2h, 30% normalized at 4h, while 10% of patients with normal GE at 2h became delayed at 4h thus indicating that more studies changed from abnormal to normal than from normal to abnormal at 4h. Greater than 90% GE was found in 9% of patients at 2 h and 25% of patients at 2.5h and this persisted at 4h. The study at 2h as compared with 4h, had 56% sensitivity, 95% specificity, 70% PPV and 91% NPV.

CONCLUSION

The 4-h imaging was very important in detecting cases that were delayed at 2h but normalized at 4h, and also cases with normal GE at 2h that became abnormal at 4h. These findings support the ANMS/SNM [SNMMI] recommendations. Gastric emptying value ≥90% at 2.5h can be used as threshold in predicting normal GE and the study could be terminated without additional imaging.

摘要

目的

本研究旨在评估一种标准的 4 小时胃排空闪烁显像(GES)成像方案,以检测胃排空延迟(GE)。

材料和方法

根据 ANMS/SNM [SNMMI] 协会的共识指南,按照迈阿密方法(MIA)和国家标准方案(NSP),使用伽马相机在前视图和后视图中进行 0、0.5、1、1.5、2、2.5 和 4 小时的成像。患者(N=1002)接受 1mCi 锝-99(Tc)硫胶体标记的标准化固体餐。使用每个成像时间点经过衰变校正的计数的几何平均值进行定量分析,以排空或保留的百分比表示。

结果

在我们的患者队列中,21%的患者在 4 小时时出现 GE 延迟,而 79%的患者在 4 小时时排空正常,少于 10%的患者出现保留。与 2 小时相比,4 小时时延迟 GE 研究增加了 25%。在那些在 2 小时时出现 GE 延迟的患者中,30%在 4 小时时恢复正常,而在 2 小时时排空正常的 10%的患者在 4 小时时出现延迟,这表明在 4 小时时更多的研究从异常变为正常,而不是从正常变为异常。在 2 小时时,9%的患者排空超过 90%,而在 2.5 小时时,25%的患者排空超过 90%,这一比例在 4 小时时仍然保持。与 4 小时相比,2 小时的研究具有 56%的敏感性、95%的特异性、70%的阳性预测值和 91%的阴性预测值。

结论

4 小时的成像在检测在 2 小时时延迟但在 4 小时时恢复正常的病例以及在 2 小时时排空正常但在 4 小时时变得异常的病例方面非常重要。这些发现支持 ANMS/SNM [SNMMI] 的建议。在 2.5 小时时排空值≥90%可作为预测正常排空的阈值,并且可以终止研究而无需进行额外的成像。

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