The principal finding of this study was a high correlation between the Osteosys Primus and the GE Lunar Prodigy. Whole body fat mass and BMCs were significantly higher in Osteosys Primus. However, lean mass of the arms and legs and whole body BMDs were lower in Osteosys Primus. This is in agreement with the findings of the other cross-calibration studies and the BMD and BMC differences are consistent with the well-known differences in calibration between the manufacturers for measurements of hip and spine BMDs [5, 6, 13, 15].
So far, cross-calibration between DXA equipment for whole body BMDs and body composition measurements has been reported in only a few studies in the last decade [5, 6, 13, 15]. Cross-calibration of body composition and entire body BMC and BMD between Hologic QDR2000 (Hologic Inc. Bedford MA, USA) and GE Healthcare Lunar Prodigy (GE Healthcare, Madison WI, USA) found similar lean body masses throughout the body [13]. However, fat mass and percent fat were significantly higher on the Hologic QDR2000. The difference in calibration between the instruments might be related to the variation between the instruments, even those from the same manufacturer. The DPXL gave lower fat mass values than the iDXA and Prodigy in adults, with a corresponding greater increase in mean lean body mass (LBM) values [16]. These findings correspond to our results. In this study, Osteosys Primus gave higher fat mass values than Lunar Prodigy in adults with corresponding lower mean LBM values. The reasons for the negative correlation of BMI and fat mass (FM) using the k value were explained by Pearson et al. The k value is the ratio of low-energy to high-energy attenuation coefficients in soft tissue, and as the ratio of fat increases in tissue, the attenuation of the beam's high-energy component is lower than the low-energy component. Also, the difference in LBM has been negatively correlated with differences in FMs. That is, as the difference in LBM got bigger, the difference in FM fell [13, 15].
In an in vivo cross-calibration study, the BMD from Primus was consistently lower than that from Prodigy. So far, there has been no comparative cross-calibration study using humans [17]. Park et al. assessed the accuracy and precision of 36 DXA devices from three manufacturers (10 Hologic, 16 Lunar, and 10 Osteosys) using the European Spine Phantom (ESP), in which the three vertebrae represent low (L1), medium (L2), and high (L3) densities, with actual BMD values of 0.496 g/cm2, 0.990 g/cm2, and 1.499 g/cm2, respectively. The average BMDs of L1, L2, and L3 in Osteosys Dexxum-T devices and the Lunar Prodigy device were 0.605 g/cm2 vs. 0.433 g/cm2 in L1, 1.072 g/cm2 vs. 0.928 g/cm2 in L2, and 1.574 g/cm2 vs 1.424 g/cm2, respectively. The BMDs in Osteosys Dexxum-T devices were consistently lower than those from the Lunar Prodigy device[17]. Although this was a comparative study using EPS between different instruments, the findings corresponded with a previous study. According to cross-calibration studies, translational formulas for the Prodigy and Primus devices could be established and are described in supplementary Table 1,2.
In this study, we compared the scan parameters between both devices. Using a higher voltage than GE Lunar, Osteosys Primus is designed to enable more precise measurements. Due to the small pixel size, more measurement time is required compared to GE Lunar equipment, but it has a higher resolution. Compared to the GE Lunar instrument, the exposure dose was not significantly different, despite the long measurement time.
This study had two limitations. First, it was the first study of comparing Osteosys Primus and the GE Lunar Prodigy were included in the study. To generalize the results of this study to other races, further studies including Caucasians are needed [18]. Second, only a single total body phantom was used for calibration. In future studies, whole body phantom should be developed and used for accurate correction.
In summary, there were a very high correlation of BMDs and muscle mass between the Osteosys Primus and the GE lunar prodigy. In addition, body compositions measured by Osteosys Primus were consistently lower than those of the GE Lunar prodigy by 2.4% to 7.7 percent. There was a high agreement between all DXA systems in estimating BMCs and body compositions (R2 = 0.85–0.99).
Nevertheless, cross-calibration equations should be used to examine data across systems to avoid erroneous conclusions.