First trimester screening of serum soluble fms-like tyrosine kinase-1 and placental growth factor predicting hypertensive disorders of pregnancy

AbstractObjectiveTo assess the accuracy of first trimester soluble fms-like tyrosine kinase-1 (sFlt-1) and placental growth factor (PlGF) in predicting pregnancy hypertension and pre-eclampsia; and compare with the accuracy of routinely collected maternal and clinical risk factors.Study designIn this population-based cohort study, serum sFlt-1 and PlGF levels were measured in first trimester in 2,681 women with singleton pregnancies in New South Wales, Australia.Main outcome measuresPrediction of pregnancy hypertension and pre-eclampsia.ResultsThere were 213 (7.9%) women with pregnancy hypertension, including 68 (2.5%) with pre-eclampsia. The area under the curve (AUC) for both sFlt-1 and PlGF was not different from chance, but combined was 0.55 (P=0.005). Parity and previous diagnosed hypertension had better predictive accuracy than serum biomarkers (AUC=0.64, P<0.001) and the predictive accuracy for all maternal and clinical information was fair (AUC=0.70, P<0.001 for pregnancy hypertension and AUC=0.74, P<0.001 for pre-eclampsia). Adding sFlt-1 and PlGF to maternal risk factors did not improve the ability of the models to predict pregnancy hypertension or pre-eclampsia.ConclusionsMaternal first trimester serum concentrations of sFlt-1 and PlGF do not predict hypertensive disorders in pregnancy any better than routinely collected clinical and maternal risk factor information. Screening for sFlt-1 and PlGF levels in early pregnancy would not identify those pregnancies at-risk

Angiopoietin 1 and 2 serum concentrations in first trimester of pregnancy as biomarkers of adverse pregnancy outcomes

Objective: To assess Ang-1, Ang-2 and the Ang-1/Ang-2 ratio levels in the first trimester of pregnancy, their association with adverse pregnancy outcomes; and their predictive accuracy. Study Design: This cohort study measured serum Ang-1 and Ang-2 levels in 4,785 women with singleton pregnancies attending first trimester screening in New South Wales, Australia. Multivariate logistic regression models were used to assess the association and predictive accuracy of serum biomarkers with subsequent adverse pregnancy outcomes (small for gestational age, preterm birth, preeclampsia, miscarriage >10 weeks and stillbirth). Results: Median (interquartile range) levels for Ang-1, Ang-2 and the Ang-1/Ang-2 ratio for the total population were 19.6 ng/ml (13.6-26.4), 15.5 ng/ml (10.3-22.7) and 1.21 (0.83-1.73), respectively. Maternal age, weight, country of birth and socio-economic status significantly affected Ang-1, Ang-2 and the Ang-1/Ang-2 ratio levels. After adjusting for maternal and clinical risk factors, women with low Ang-2 levels (90th centile) had increased risk of developing most adverse pregnancy outcomes. Compared to the Ang-1/Ang-2 ratio alone, maternal and clinical risk factors had better predictive accuracy for most adverse pregnancy outcomes. The exception was miscarriage [Ang-1/Ang-2 ratio area under ROC curve (AUC) =0.70; maternal risk factors AUC =0.58]. Overall, adding the Ang-1/Ang-2 ratio to maternal risk factors did not improve the ability of the models to predict adverse pregnancy outcomes. Conclusions: Our findings suggest that the Ang-1/Ang-2 ratio in first trimester is associated with most adverse pregnancy outcomes, but do not predict outcomes any better than clinical and maternal risk factor information.Australian National Health and Medical Research Council (NHMRC) Project Grant (#632653)

First trimester screening of serum soluble fms-like tyrosine kinase-1 and placental growth factor predicting hypertensive disorders of pregnancy

AbstractObjectiveTo assess the accuracy of first trimester soluble fms-like tyrosine kinase-1 (sFlt-1) and placental growth factor (PlGF) in predicting pregnancy hypertension and pre-eclampsia; and compare with the accuracy of routinely collected maternal and clinical risk factors.Study designIn this population-based cohort study, serum sFlt-1 and PlGF levels were measured in first trimester in 2,681 women with singleton pregnancies in New South Wales, Australia.Main outcome measuresPrediction of pregnancy hypertension and pre-eclampsia.ResultsThere were 213 (7.9%) women with pregnancy hypertension, including 68 (2.5%) with pre-eclampsia. The area under the curve (AUC) for both sFlt-1 and PlGF was not different from chance, but combined was 0.55 (P=0.005). Parity and previous diagnosed hypertension had better predictive accuracy than serum biomarkers (AUC=0.64, P<0.001) and the predictive accuracy for all maternal and clinical information was fair (AUC=0.70, P<0.001 for pregnancy hypertension and AUC=0.74, P<0.001 for pre-eclampsia). Adding sFlt-1 and PlGF to maternal risk factors did not improve the ability of the models to predict pregnancy hypertension or pre-eclampsia.ConclusionsMaternal first trimester serum concentrations of sFlt-1 and PlGF do not predict hypertensive disorders in pregnancy any better than routinely collected clinical and maternal risk factor information. Screening for sFlt-1 and PlGF levels in early pregnancy would not identify those pregnancies at-risk

Electron Bio-Imaging Centre (eBIC): the UK national research facility for biological electron microscopy

The recent resolution revolution in cryo-EM has led to a massive increase in demand for both time on high-end cryo-electron microscopes and access to cryo-electron microscopy expertise. In anticipation of this demand, eBIC was set up at Diamond Light Source in collaboration with Birkbeck College London and the University of Oxford, and funded by the Wellcome Trust, the UK Medical Research Council (MRC) and the Biotechnology and Biological Sciences Research Council (BBSRC) to provide access to high-end equipment through peer review. eBIC is currently in its start-up phase and began by offering time on a single FEI Titan Krios microscope equipped with the latest generation of direct electron detectors from two manufacturers. Here, the current status and modes of access for potential users of eBIC are outlined. In the first year of operation, 222 d of microscope time were delivered to external research groups, with 95 visits in total, of which 53 were from unique groups. The data collected have generated multiple high- to intermediate-resolution structures (2.8–8 Å), ten of which have been published. A second Krios microscope is now in operation, with two more due to come online in 2017. In the next phase of growth of eBIC, in addition to more microscope time, new data-collection strategies and sample-preparation techniques will be made available to external user groups. Finally, all raw data are archived, and a metadata catalogue and automated pipelines for data analysis are being developed

Best practices for managing large CryoEM facilities

Microscopic imaging and technolog

All-sky search for long-duration gravitational wave transients with initial LIGO

We present the results of a search for long-duration gravitational wave transients in two sets of data collected by the LIGO Hanford and LIGO Livingston detectors between November 5, 2005 and September 30, 2007, and July 7, 2009 and October 20, 2010, with a total observational time of 283.0 days and 132.9 days, respectively. The search targets gravitational wave transients of duration 10-500 s in a frequency band of 40-1000 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. All candidate triggers were consistent with the expected background; as a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. For signals from black hole accretion disk instabilities, we set upper limits on the source rate density between 3.4×10-5 and 9.4×10-4 Mpc-3 yr-1 at 90% confidence. These are the first results from an all-sky search for unmodeled long-duration transient gravitational waves. © 2016 American Physical Society

All-sky search for long-duration gravitational wave transients with initial LIGO

We present the results of a search for long-duration gravitational wave transients in two sets of data collected by the LIGO Hanford and LIGO Livingston detectors between November 5, 2005 and September 30, 2007, and July 7, 2009 and October 20, 2010, with a total observational time of 283.0 days and 132.9 days, respectively. The search targets gravitational wave transients of duration 10-500 s in a frequency band of 40-1000 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. All candidate triggers were consistent with the expected background; as a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. For signals from black hole accretion disk instabilities, we set upper limits on the source rate density between 3.4×10-5 and 9.4×10-4 Mpc-3 yr-1 at 90% confidence. These are the first results from an all-sky search for unmodeled long-duration transient gravitational waves. © 2016 American Physical Society