نتایج جستجو برای: fwhm

تعداد نتایج: 2910  

Journal: :IEEE Photonics Journal 2022

We demonstrated a tilted fiber Bragg grating (TFBG)-based modulated amplified spontaneous emission (ASE) source, followed by the broadband, continuous-wave (CW) mid-infrared laser generated intracavity difference-frequency generation (DFG). By flattening spectrum of ASE source during its power amplification and injecting another 1018 nm in optical parametric oscillation(OPO) cavity, nonlinear f...

Journal: :Physics in medicine and biology 2017
S E Brunner D R Schaart

Due to detector developments in the last decade, the time-of-flight (TOF) method is now commonly used to improve the quality of positron emission tomography (PET) images. Clinical TOF-PET systems based on L(Y)SO:Ce crystals and silicon photomultipliers (SiPMs) with coincidence resolving times (CRT) between 325 ps and 400 ps FWHM have recently been developed. Before the introduction of L(Y)SO:Ce...

2008
Jack W. Sulentic Rumen Bachev Paola Marziani C. Alenka Negrete Deborah Dultzin

We have been exploring a spectroscopic unification for all known types of broad line emitting AGN. The 4D Eigenvector 1 (4DE1) parameter space shows promise as a unification capable of organizing quasar diversity on a sequence primarily governed by Eddington ratio. This paper considers the role of Civλ1549 measures with special emphasis on the Civλ1549 line shift as a principal 4DE1 diagnostic....

Journal: :Physics in medicine and biology 2007
Sang-June Park W Leslie Rogers Sam Huh Harris Kagan Klaus Honscheid Don Burdette Enrico Chesi Carlos Lacasta Gabriela Llosa Marko Mikuz Andrej Studen Peter Weilhammer Neal H Clinthorne

A very high resolution positron emission tomography (PET) scanner for small animal imaging based on the idea of inserting a ring of high-granularity solid-state detectors into a conventional PET scanner is under investigation. A particularly interesting configuration of this concept, which takes the form of a degenerate Compton camera, is shown capable of providing sub-millimeter resolution wit...

2015
Diego Cecchin Davide Poggiali Lucia Riccardi Paolo Turco Franco Bui Stefano De Marchi

Introduction. It is well known that resolution on a gamma camera varies as a function of distance, scatter and the camera's characteristics (collimator type, crystal thickness, intrinsic resolution etc). Manufacturers frequently provide only a few pre-calculated resolution values (using a line source in air, 10-15 cm from the collimator surface and without scattering). However, these are typica...

2016
Heerajnarain Bulluck Stefania Rosmini Amna Abdel-Gadir Anish N Bhuva Thomas A Treibel Marianna Fontana Shane Weinmann Alex Sirker Anna S Herrey Charlotte Manisty James C Moon Derek J Hausenloy

AIMS The four most promising semiautomated techniques (5-SD, 6-SD, Otsu and the full width half maximum (FWHM)) were compared in paired acute and follow-up cardiovascular magnetic resonance (CMR), taking into account the impact of microvascular obstruction (MVO) and using automated extracellular volume fraction (ECV) maps for reference. Furthermore, their performances on the acute scan were com...

2014
Christopher Nguyen Zhaoyang Fan Yibin Xie James Dawkins Eleni Tseliou Xiaoming Bi Behzad Sharif Rohan Dharmakumar Eduardo Marbán Debiao Li

BACKGROUND Despite the established role of late gadolinium enhancement (LGE) cardiovascular magnetic resonance (CMR) in characterizing chronic myocardial infarction (MI), a significant portion of chronic MI patients are contraindicative for the use of contrast agents. One promising alternative contrast free technique is diffusion weighted CMR (dwCMR), which has been shown ex vivo to be sensitiv...

2004
Violet A. Taylor Rolf A. Jansen Rogier A. Windhorst

We present measurements of sky surface brightness and seeing on Mount Graham, obtained at the Vatican Advanced Technology Telescope (VATT) during 16 observing runs between 1999 April and 2003 December. We show that the sky surface brightness is significantly darker during photometric conditions and can be highly variable over the course of a single observing run, as well as from one run to the ...

1997
Lindsey F. Smith A. Maeder

We consider the relationships between the classification parameters of WN stars in the new 3-dimensional classification of Smith et al. (1996) and the corresponding and related parameters that define stellar atmosphere models. Specifically, we consider: FWHM of HeII 4686 vs. v∞; hydrogen content by direct inspection vs. hydrogen content by modelling and vs. colour (b-v)0; ionisation subclass an...

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