This study examined the value of a novel 1-step labeled integrin α v β 3 -targeting 18 F-AlF-NOTA-PRGD2 (denoted as 18 F-RGD) scan in assessing sensitivity to concurrent chemoradiotherapy (CCRT) in patients with newly diagnosed glioblastoma multiforme (GBM). Methods: Twenty-five patients with newly diagnosed GBM were enrolled in this study 3-5 wk after surgical resection. All participants were investigated with 18 F-RGD PET/CT on baseline (T1) and at the third week (T2) after the start of CCRT. Tumor volume, maximal and mean standardized uptake value of the tumor (SUV max , SUV mean ), and tumor-to-nontumor ratios of the tumor volume were obtained. The MRI treatment response was assessed at the 11th week (T3). The change in the lesion volume from T1 to T3 on MRI was used as an endpoint to evaluate the predictive ability of 18 F-RGD PET/CT. Results: With 18 F-RGD PET/CT imaging, we successfully visualized the residual lesions of GBM. Twenty-five and 23 18 F-RGD PET/CT scans at baseline and the third week, respectively, were available for analysis. We found that 18 F-RGD PET/CT parameters, both pretreatment SUV max on baseline (P , 0.05) and intratreatment SUV max at the third week (SUV maxT2 ) (P , 0.05) and tumor-to-nontumor ratios at the third week (P , 0.05), were predictive of treatment sensitivity to CCRT. Additionally, the change of volume from T1 to T2 on MRI was also predictive (P , 0.05). According to receiver-operating-characteristic curve analysis, the most significant parameter was SUV maxT2 (area under the curve, 0.846). The threshold of SUV maxT2 was 1.35, and its sensitivity, specificity, and accuracy were 84.6%, 90.0% and 87.0%, respectively. Conclusion: 18 F-RGD PET/CT allows for the noninvasive visualization of GBM lesions and the prediction of sensitivity to CCRT as early as 3 wk after treatment initiation.

The Chinese Small Telescope ARray (CSTAR) is the first telescope facility built at Dome A, Antarctica. During the 2008 observing season, the installation provided long-baseline and high-cadence photometric observations in the i-band for 18,145 targets within 20 deg 2 CSTAR field around the South Celestial Pole for the purpose of monitoring the astronomical observing quality of Dome A and detecting various types of photometric variability. Using sensitive and robust detection methods, we discover 274 potential variables from this data set, 83 of which are new discoveries. We characterize most of them, providing the periods, amplitudes and classes of variability. The catalog of all these variables is presented along with the discussion of their statistical properties.

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