Results 261 to 270 of about 2,662,849 (293)

Enhancing early prediction of pathological complete response in breast cancer using attention-based convolutional neural networks in digital pathology. [PDF]

Digit Health
Comes MC, Lupo A, Bozzi A, Fanizzi A, Cirillo A, Nunzio G, Pastena MI, Rizzo A, Guven DC, Vitale E, Zito FA, Bove S, Massafra R.   +12 more
europepmc   +1 more source

Automatic Quality Control System and Adenoma Detection Rates During Routine Colonoscopy: A Randomized Clinical Trial.

JAMA Netw Open
Liu J, Zhou R, Liu C, Liu H, Cui Z, Guo Z, Zhao W, Zhong X, Zhang X, Li J, Wang S, Xing L, Zhao Y, Ma R, Ni J, Li Z, Li Y, Zuo X.   +17 more
europepmc   +1 more source

Determining the Impact of a Physiotherapist-Led Primary Care Model for Low Back Pain: Protocol and Analysis Plan for a Cluster Randomized Controlled Trial and Embedded Process Evaluation.

JMIR Res Protoc
Miller J, Donnelly C, McClintock C, Varette K, Camargo Y, Marsh J, Taljaard M, Mamun MSA, Bacchus G, Barber D, Cooper L, French S, Hill J, Green M, MacDermid J, Norman K, Richardson J, Tranmer J, Wideman T.   +18 more
europepmc   +1 more source

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Suppressed heat conductivity in the intracluster medium: implications for the magneto-thermal instability

Monthly notices of the Royal Astronomical Society, 2020
In the outskirts of the intracluster medium (ICM) in galaxy clusters, the temperature decreases with radius. Due to the weakly collisional nature of the plasma, these regions are susceptible to the magneto-thermal instability (MTI), which can sustain ...
Thomas Berlok, E. Quataert, M. Pessah, C. Pfrommer   +3 more
semanticscholar   +1 more source

Metals in the intracluster medium

AIP Conference Proceedings, 2012
We derived radial abundance profiles of O, Mg, Si, S and Fe in the intracluster medium (ICM) of several clusters and groups of galaxies up to about 0.3 r180 with Suzaku and those of Fe in 28 nearby brightest clusters of galaxies up to 0.3-0.5 r180 with XMM. Within 0.05 r180, Fe abundance scatters from 0.5 to 1 solar.
Kyoko Matsushita, Kosuke Sato, Eri Sakuma, Takayuki Tamura   +3 more
openaire   +1 more source

Turbulence in the Intracluster Medium

2014
We review our knowledge about turbulence in the intracluster medium, a very hot, dilute plasma that permeates clusters of galaxies. A thorough understanding of turbulence in the intracluster medium is crucial for the use of clusters to determine cosmological parameters.
Brüggen, M., Vazza, F.
openaire   +1 more source

Imaging the Hot Intracluster Medium

1992
Clusters of galaxies contain large amounts of hot, diffuse x—ray emitting gas. Observations of this gas can be used to measure the gas mass, the cluster virial mass, and the cluster morphology. From these measurements. a lower limit to the baryonic mass in clusters, the formation efficiency of galaxies in different environments, and the presence and ...
C. Jones, W. Forman
openaire   +1 more source

The Intracluster Medium

1992
Clusters of galaxies are full of hot, diffuse plasma, with typical temperatures and electron densities of T ~ 7x107 K and n e ~ 10-3 cm-3, This intraclustermedium (ICM) produces copious X-ray emission, and typical cluster X-ray luminositiesare L x ~ 1043 - 1045 ergs s-1.
openaire   +1 more source

Chemical enrichment of the Intracluster Medium

Astronomische Nachrichten, 2005
X-ray observations (e.g. Fukazawa et al. 1998) show that the Intracluster Medium (ICM) contains metals with abundances ~ 0.2 - 0.3 Z ⊙. Since heavy elements are produced mainly in stars of cluster galaxies, they must have been transported into the intracluster space.
Baumgartner, Verena, Breitschwerdt, Dieter   +1 more
openaire   +1 more source

Construction of Medium-Sized Rings by Gold Catalysis

Chemical Reviews, 2021
Ronald L Reyes, Tomohiro Iwai, Masaya Sawamura   +2 more
exaly