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Citation: Vasudeva K, Andersen K, Zeyzus-Johns B, Hitchens TK, Patel SK, Balducci A, et al. (2014) Imaging Neuroinflammation In Vivo in a Neuropathic Pain Rat Model with Near-Infrared Fluorescence and 19F Magnetic Resonance. PLoS ONE 9(2): e90589. https://doi.org/10.1371/journal.pone.0090589

Php designer 7 free download. Editor: Jian-Xin Gao, Shanghai Jiao Tong University School of Medicine, China

Received: May 16, 2013; Accepted: February 3, 2014; Published: February 28, 2014

Copyright: © 2014 Vasudeva et al. This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.

Funding: Funding for this work was provided by a Hunkele Dreaded Disease Award to JAP, a Samuel and Emma Winters Foundation Award to JAP, a Pennsylvania’s Commonwealth Universal Research Enhancement (CURE) Award to JMJ and a Pittsburgh Tissue Engineering Initiative Interface Seed Grant to JMJ & JAP. The funders had no role in study design, data collection and analysis, decision to publish, or preparation of the manuscript.

Competing interests: Anthony Balducci is employed by Celsense Inc, Pittsburgh, PA. V-Sense DM NIR is produced and marketed by Celsense Inc, Pittsburgh, PA. This relationship with Celsense Inc. does not alter the authors’ adherence to all the PLOS ONE policies on sharing data and materials.

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Detection of polarized gamma-ray emission from the Crab nebula with the Hitomi Soft Gamma-ray Detector

In this study, we present the results from the Hitomi Soft Gamma-ray Detector (SGD) observation of the Crab nebula. The main part of SGD is a Compton camera, which in addition to being a spectrometer, is capable of measuring polarization of gamma-ray photons. The Crab nebula is one of the brightest X-ray/gamma-ray sources on the sky, and the only source from which polarized X-ray photons have been detected. SGD observed the Crab nebula during the initial test observation phase of Hitomi. We performed data analysis of the SGD observation, SGD background estimation, and SGD Monte Carlo simulations, and successfully detectedmore »
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