A 4-hour-old infant with profound cyanosis on an alprostadil infusion was urgently transferred to Rady Children’s Hospital with suspected CHD. Upon arrival, urgent echocardiography was performed but could not confirm the presence of discrete pulmonary veins or pulmonary venous drainage. Given the difficulty in delineating the anatomy, a cardiac CT scan was performed and demonstrated a nearly atretic common pulmonary vein with multiple small collaterals that drained to systemic veins. Due to the high risk of mortality associated with operative repair, the decision was made to proceed with compassionate withdrawal of care. The described anatomy of common pulmonary vein atresia remains rare, and to our knowledge, fewer than 40 cases have been reported in the literature. Albeit rare, common pulmonary vein atresia should be considered in the differential diagnosis of a severely cyanotic neonate.

Exercise has many health benefits for individuals with Type 1 Diabetes (T1D), however it carries the risk of hypoglycaemia. Research has indicated that intermittent high intensity exercise reduces this risk compared to steady state exercise, potentially via a greater anaerobic component inducing increased lactate and catecholamine response.Six physically active males aged 23 ± 5 years, BMI 24.9 ± 1.8 kg•m-2, Vo2 max 47.9 ± 10.1 ml•kg-1•min-1 diagnosed with Type 1 Diabetes for 9 ± 3 years and a HbA1c concentration of 8.6 ± 0.3% participated in a randomised counterbalanced trial. Participants exercised for 60 min on a cycle ergometer on two occasions separated by 7 days, which consisted of a moderate continuous steady state exercise session at 40% o2 max (CONT), or the same exercise intensity interspersed with 7 s high intensity sprints at 100% Vo2 max every 2 min (INT). Blood glucose concentration was assessed via capillary blood sampling every 10 min during exercise and at regular intervals in the 60 min post exercise (Accu-Chek Aviva, Roche, UK). Additional metabolic measures such as blood lactate concentration and carbohydrate oxidation rates were assessed during exercise. Participants ingested small quantities of a carbohydrate drink, if required, to avoid hypoglycaemia during exercise. Magnitude based inferences were used to compare the two exercise trials and Effect Sizes (ES) calculated using Cohen's d and results presented as mean ± SD.Average blood glucose concentration was lower on the INT trial compared to CONT during both the exercise phase (8.9 ± 1.7 mmol•l-1 vs 7.1 ± 1.1 mmol•l-1; ES 0.55) and the 60 min post-exercise recovery phase (8.1 ± 1.9 mmol•l-1 vs 7.0 ± 1.8 mmol•l-1; ES 0.56). Carbohydrate oxidation was greater on the INT trial compared to CONT (1.9 ± 1.4 g•min-1 vs 1.5 ± 0.6 g•min-1; ES 0.35). Capillary blood lactate concentration was markedly elevated on INT when compared to CONT (5.0 ± 1.4 mmol•l-1 vs 2.4 ± 1.1 mmol•l-1; ES 2.48). Carbohydrate ingestion during exercise was 13 ± 11 g and differed little between trials (ES 0.18).Despite greater anaerobic metabolic response, the addition of intermittent high intensity sprints to 60 min steady-state cycle exercise resulted in greater declines in blood glucose concentration during the exercise and post-exercise period, potentially by inhibition of the counter regulatory hormone response expected on the INT trial. These results would indicate that additional exogenous carbohydrate ingestion may be required for individuals with T1D when intermittent sprints are added to prolonged continuous exercise.

The use of alternative probability density functions to specify risk in farm programming models is explored and compared to a traditional specification using historical data. A method is described that compares risk efficient crop mixes using stochastic dominance techniques to examine impacts of different risk specifications on farm plans. Results indicate that a traditional method using historical farm data is as efficient for risk averse producers as two other methods of incorporating risk in farm programming models when evaluated using second degree stochastic dominance. Stochastic dominance with respect to a function further discriminates among the distributions, indicating that a density function based on the historic forecasting accuracy of the futures market results in a more risk-efficient crop mix for highly risk averse producers. Results also illustrate the need to validate alternative risk specifications perceived as improvements to traditional methods.

Despite the potential of declared serving size to encourage appropriate portion size consumption, most countries including Australia have not developed clear reference guidelines for serving size. The present study evaluated variability in manufacturer-declared serving size of discretionary food and beverage products in Australia, and how declared serving size compared with the 2013 Australian Dietary Guideline (ADG) standard serve (600 kJ). Serving sizes were obtained from the Nutrition Information Panel for 4466 packaged, discretionary products in 2013 at four large supermarkets in Sydney, Australia, and categorised into fifteen categories in line with the 2013 ADG. For unique products that were sold in multiple package sizes, the percentage difference between the minimum and the maximum serving size across different package sizes was calculated. A high variation in serving size was found within the majority of food and beverage categories – for example, among 347 non-alcoholic beverages (e.g. soft drinks), the median for serving size was 250 (interquartile range (IQR) 250, 355) ml (range 100–750 ml). Declared serving size for unique products that are available in multiple package sizes also showed high variation, particularly for chocolate-based confectionery, with median percentage difference between minimum and maximum serving size of 183 (IQR 150) %. Categories with a high proportion of products that exceeded the 600 kJ ADG standard serve included cakes and muffins, pastries and desserts (≥74 % for each). High variability in declared serving size may confound interpretation and understanding of consumers interested in standardising and controlling their portion selection. Future research is needed to assess if and how standardising declared serving size might affect consumer behaviour.

While more and more long-period giant planets are discovered by direct imaging, the distribution of planets at these separations (≳5 AU) has remained largely uncertain, especially compared to planets in the inner regions of solar systems probed by RV and transit techniques. The low frequency, the detection challenges, and heterogeneous samples make determining the mass and orbit distributions of directly imaged planets at the end of a survey difficult. By utilizing Monte Carlo methods that incorporate the age, distance, and spectral type of each target, we can use all stars in the survey, not just those with detected planets, to learn about the underlying population. We have produced upper limits and direct measurements of the frequency of these planets with the most recent generation of direct imaging surveys. The Gemini NICI Planet-Finding Campaign observed 220 young, nearby stars at a median H-band contrast of 14.5 magnitudes at 1”, representing the largest, deepest search for exoplanets by the completion of the survey. The Gemini Planet Imager Exoplanet Survey is in the process of surveying 600 stars, pushing these contrasts to a few tenths of an arcsecond from the star. With the advent of large surveys (many hundreds of stars) using advanced planet-imagers we gain the ability to move beyond measuring the frequency of wide-separation giant planets and to simultaneously determine the distribution as a function of planet mass, semi-major axis, and stellar mass, and so directly test models of planet formation and evolution.

In February 2013, the LEECH (LBTI Exozodi Exoplanet Common Hunt) survey began its 100-night campaign from the Large Binocular Telescope atop Mount Graham in Arizona. LEECH neatly complements other high-contrast planet imaging efforts by observing stars in L' band (3.8 microns) as opposed to the shorter wavelength near-infrared bands (1–2.3 microns). This part of the spectrum offers deeper mass sensitivity for intermediate age (several hundred Myr-old) systems, since their Jovian-mass planets radiate predominantly in the mid-infrared. In this proceedings, we present the science goals for LEECH and a preliminary contrast curve from some early data.

We have carried out high contrast imaging of 70 young, nearby B and A stars to search for brown dwarf and planetary companions as part of the Gemini NICI Planet-Finding Campaign. Our survey represents the largest, deepest survey for planets around high-mass stars (≈1.5–2.5 M⊙) conducted to date and includes the planet hosts β Pic and Fomalhaut. Despite detecting two new brown dwarfs, our observations did not detect new planets around our target stars, and we present upper limits on the fraction of high-mass stars that can host giant planets that are consistent with our null result.