Prevalence of β thalassaemia trait and Haemoglobin E disorders among students aged between 14-17yrs in Kurunegala district, Sri Lanka.

Introduction: Knowledge on frequency of carrier status of thalassaemia in a country is very important to form a plan of reducing the disease burden. In Sri Lanka, the amount of research done regarding the topic is insufficient considering the amount of thalassaemia carriers who are being detected island wide, which is increasing in numbers annually. Kurunegala is one of the districts in Sri Lanka where thalassaemia is prevalent.

Angiotensin converting enzyme inhibitors and angiotensin receptor blockers have no effect on the outcomes of endovascular revascularization in tibial arterial occlusive disease.

The effects of angiotensin converting enzyme inhibitors and angiotensin receptor blockers (ACEI/ARBs) on angiogenesis, myocardial remodeling and intermittent claudication have been studied. Clinical studies have shown reduced re-intervention after cardiac stenting with the use of ACEI/ARBs. We hypothesized that the use of ACEI/ARBs decreases re-interventions after endovascular revascularization in tibial artery disease (TAD) patients.

Multiple Galactic Sources with Emission Above 56 TeV Detected by HAWC.

We present the first catalog of gamma-ray sources emitting above 56 and 100 TeV with data from the High Altitude Water Cherenkov Observatory, a wide field-of-view observatory capable of detecting gamma rays up to a few hundred TeV. Nine sources are observed above 56 TeV, all of which are likely galactic in origin. Three sources continue emitting past 100 TeV, making this the highest-energy gamma-ray source catalog to date.

Publisher Correction: Very-high-energy particle acceleration powered by the jets of the microquasar SS 433.

In this Letter, owing to a production error, the penultimate version of the PDF was published. The HTML version was always correct. The PDF has been corrected online.

Very-high-energy particle acceleration powered by the jets of the microquasar SS 433.

SS 433 is a binary system containing a supergiant star that is overflowing its Roche lobe with matter accreting onto a compact object (either a black hole or neutron star). Two jets of ionized matter with a bulk velocity of approximately 0.26c (where c is the speed of light in vacuum) extend from the binary, perpendicular to the line of sight, and terminate inside W50, a supernova remnant that is being distorted by the jets.