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Aim of this study was to assess the accuracy of ventricular septal defects (VSD) using high pitch computed tomography angiography (CTA) of the chest in children below 1 year of age, compared to the intraoperative findings and echocardiography. Out of 154 patients that underwent Dual-Source CTA of the chest using a high-pitch protocol at low tube voltages (70–80 kV), 55 underwent surgical repair of a VSD (median age 8 days, range 1–348 days). The margins of the VSDs and their relation to the surrounding structures were reproduced by en-face views using multiplanar reformations (MPR). Absolute diameter, normalized area and relative area compared to the aortic valve annulus were used for discrimination between restrictive and non-restrictive defects. Localization was classified into four subtypes. The results were compared to two-dimensional echocardiography and intraoperative findings. Median absolute size of VSDs did not differ significantly between CTA-measurements (10.8 mm, range 2.8–18.1 mm) and intraoperative findings (12.0 mm, 3.0–25.0 mm, p = 0.09). Echocardiographic values were significantly lower (9.6 mm, 3.0–18.5 mm, both p < 0.01). The classification of the location and orientation matched the intraoperative situs in 96.4% of all cases using CT and in 87.3% using echocardiography. Echocardiography missed the relation to valves in 11% of all cases. Pre-interventional sensitivity and specificity for detection of a VSD were 97.2/98.9% compared to echocardiography. Median radiation dose was 0.32 mSv (range 0.12–2.00 mSv) and differed significantly between second and third generation Dual-Source CT (0.43 vs. 0.22 mSv, p = 0.003). Size and subtype of VSDs can be accurately assessed by CTA of the chest in patients with complex congenital heart defects at a very low radiation dose. [ABSTRACT FROM AUTHOR]

Objectives: We evaluated the performance of blood and faecal biomarkers for differentiating between endoscopic inflammation and mucosal healing, and clinically active disease and sustained clinical remission, and determined the predictive value for a flare in patients with ulcerative colitis [UC]. Methods: Clinical Activity Index [CAI], faecal lactoferrin [FLA], calprotectin [CAL], PMN-elastase [PMN-e], C-reactive protein [CRP], white blood cells [WBC], Endoscopic Index [EI], and UC-Disease Activity Index [DAI] were determined repeatedly during 12 months and at acute flares. Results: Of 91 patients [45 female; mean age 48.1 ± 13.4 years] entering in remission, 42 [46%] patients developed a clinical flare. A total of 529 CAI and 179 EI assessments were performed. Median levels for active disease confirmed by EI [n = 35] vs clinical remission with endoscopic inflammation [n = 37] vs mucosal healing [n = 107] for FLA were 44/37/4 μg/g, CAL 25/20/10 μg/g [both p < 0.0001], PMN-e 0.06/0.03/0.02 μg/g, CRP 0.7/0.2/0.2 mg/dl [both p < 0.001], and WBC 7.0/6.5/6.4/nl [p = 0.1]. There was no difference for any of the markers for defining mucosal healing by EI = 0 vs EI = 1 with the exception of PMN-e [p = 0.03], where the difference was very small and with questionable clinical relevance. Using manufacturers' cut-offs, only FLA at baseline was associated with a significant higher relative risk [RR] of flaring [RR 1.69; p = 0.018]. Using optimised cut-offs, CAL, PMN-e, and CRP were also predictive of a flare. Conclusions: Faecal biomarkers FLA, CAL, and PMN-e were able to distinguish between UC patients with mucosal healing from clinical remission and mild disease, showed significant correlations with endoscopy, and were predictive of a flare. [ABSTRACT FROM AUTHOR]

The irreversible conversion of methane into higher hydrocarbons in Titan's stratosphere implies a surface or subsurface methane reservoir. Recent measurements from the cameras aboard the Cassini orbiter fail to see a global reservoir, but the methane and smog in Titan's atmosphere impedes the search for hydrocarbons on the surface. Here we report spectra and high-resolution images obtained by the Huygens Probe Descent Imager/Spectral Radiometer instrument in Titan's atmosphere. Although these images do not show liquid hydrocarbon pools on the surface, they do reveal the traces of once flowing liquid. Surprisingly like Earth, the brighter highland regions show complex systems draining into flat, dark lowlands. Images taken after landing are of a dry riverbed. The infrared reflectance spectrum measured for the surface is unlike any other in the Solar System; there is a red slope in the optical range that is consistent with an organic material such as tholins, and absorption from water ice is seen. However, a blue slope in the near-infrared suggests another, unknown constituent. The number density of haze particles increases by a factor of just a few from an altitude of 150 km to the surface, with no clear space below the tropopause. The methane relative humidity near the surface is 50 per cent.