نتایج جستجو برای: mm wave detector

تعداد نتایج: 462640  

Given the sensitivity of current ground-based Gravitational Wave (GW) detectors, any continuous-wave signal we can realistically expect will be at a level or below the background noise. Hence, any data analysis of detector data will need to rely on statistical techniques to separate the signal from the noise. While with the current sensitivity of our detectors we do not expect to detect any tru...

Journal: :Physics in medicine and biology 2009
Dennis R Schaart Herman T van Dam Stefan Seifert Ruud Vinke Peter Dendooven Herbert Löhner Freek J Beekman

Silicon photomultipliers (SiPMs) are of great interest to positron emission tomography (PET), as they enable new detector geometries, for e.g., depth-of-interaction (DOI) determination, are MR compatible, and offer faster response and higher gain than other solid-state photosensors such as avalanche photodiodes. Here we present a novel detector design with DOI correction, in which a position-se...

Journal: :Physics in medicine and biology 2007
Sang-June Park W Leslie Rogers Neal H Clinthorne

A small animal positron emission tomography (PET) instrument using a high-resolution solid-state detector insert in a conventional PET system was investigated for its potential to achieve sub-millimeter spatial resolution for mouse imaging. Monte Carlo simulations were used to estimate the effect of detector configurations (thickness, length and radius) on sensitivity. From this initial study, ...

2008
K. GODA O. MIYAKAWA E. E. MIKHAILOV N. MAVALVALA

K. GODA1, O. MIYAKAWA2, E. E. MIKHAILOV3, S. SARAF4, R. ADHIKARI2, K. MCKENZIE5, R. WARD2, S. VASS2, A. J. WEINSTEIN2 AND N. MAVALVALA1* LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA The College of William and Mary, Williamsburg, Virginia 23187, USA Rochester Instit...

2015
Sheila Dwyer Daniel Sigg Stefan W. Ballmer Lisa Barsotti Nergis Mavalvala Matthew Evans

Citation Dwyer, Sheila, et al. "Gravitational wave detector with cosmological reach. Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Twenty years ago, construction...

2008
François Portet

Automatic detection of atrial activity (P waves) in an electrocardiogram (ECG) is a crucial task to diagnose the presence of arrhythmias. The P wave is difficult to detect and most of the approaches in the literature have been evaluated on normal sinus rhythms and rarely considered arrhythmia contexts other than atrial flutter and fibrillation. A novel knowledge-based P wave detector algorithm ...

2016
Jason Y. Cheng Holly Ning Barbara C. Arora Ying Zhuge Robert W. Miller

The dose measurements of the small field sizes, such as conical collimators used in stereotactic radiosurgery (SRS), are a significant challenge due to many factors including source occlusion, detector size limitation, and lack of lateral electronic equilibrium. One useful tool in dealing with the small field effect is Monte Carlo (MC) simulation. In this study, we report a comparison of Monte ...

Journal: :Investigative radiology 2013
Fabian Morsbach Lotus Desbiolles André Plass Sebastian Leschka Bernhard Schmidt Volkmar Falk Hatem Alkadhi Paul Stolzmann

OBJECTIVES The objective of this study was to assess the value of an integrated circuit (IC) detector, potentially improving spatial resolution by means of reduced cross talk between detector channels, in coronary computed tomographic (CT) angiography regarding image quality and stenosis quantification compared with conventional detector technology. MATERIALS AND METHODS In the ex vivo part o...

2002
Ronald W. Hellings

The nonlinear aspect of gravitational wave generation that produces power at harmonics of the orbital frequency, above the fundamental quadrupole frequency, is examined to see what information about the source is contained in these higher harmonics. We use an order (4/2) post-Newtonian expansion of the gravitational wave waveform of a binary system to model the signal seen in a spaceborne gravi...

2005
S. Bickman D. DeMille

Two large-area, low noise, high speed fluorescence detectors have been built. One detector consists of a photodiode with an area of 28 mm x 28 mm and a low noise transimpedance amplifier. This detector has a input light-equivalent spectral noise density of less than 3 pW/ √ Hz, can recover from a large scattered light pulse within 10 μs, and has a bandwidth of at least 900 kHz. The second detec...

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