A transiting giant planet in orbit around a 0.2-solar-mass host star.

Planet formation models indicate that the formation of giant planets is substantially harder around low-mass stars due to the scaling of protoplanetary disc masses with stellar mass. The discovery of giant planets orbiting such low-mass stars thus imposes strong constraints on giant planet formation processes. Here we report the discovery of a transiting giant planet orbiting a 0.

Development and validation of a liquid chromatography-tandem mass spectrometry (LC-MS/MS) assay for the quantification of oximes in KIKO mouse plasma.

Chemical warfare nerve agents (CWNAs) are potent and irreversible inhibitors of acetylcholinesterase (AChE). Oxime reactivators are an important part of the standard treatment for CWNA exposure as they can reactivate inhibited AChE. Evaluating the oxime candidates of interest in biological samples requires analytical detection methods and oxime reactivators as a class of compounds have historically been notoriously difficult to isolate, detect and analyze in an analytical laboratory, and there are currently no sensitive or robust analytical detection methods in the literature.

Topping-Off a Long Thoracic Stabilization With Semi-Rigid Constructs May Have Favorable Biomechanical Effects to Prevent Proximal Junctional Kyphosis: A Biomechanical Comparison.

Study DesignIn-vitro cadaveric biomechanical study.ObjectivesLong posterior spinal fusion is a standard treatment for adult spinal deformity. However, these rigid constructs are known to alter motion and stress to the adjacent non-instrumented vertebrae, increasing the risk of proximal junctional kyphosis (PJK).