output
20022024
most citedAutomatic Liver and Lesion Segmentation in CT Using Cascaded Fully Convolutional Neural Networks and 3D Conditional Random Fields

643 citations

Showing 2016Show all

7 papers · 1 filter

cs.LO20169 cited

A Light-Weight Approach for Verifying Multi-Threaded Programs with CPAchecker

Dirk Beyer, Karlheinz Friedberger

Verifying multi-threaded programs is becoming more and more important, because of the strong trend to increase the number of processing units per CPU socket. We introduce a new con…

astro-ph.SR2016107 cited

Magnetic massive stars as progenitors of "heavy" stellar-mass black holes

V. Petit, Z. Keszthelyi, R. MacInnis +7

The groundbreaking detection of gravitational waves produced by the inspiralling and coalescence of the black hole (BH) binary GW150914 confirms the existence of "heavy" stellar-ma…

astro-ph.SR201654 cited

Modeling the early evolution of massive OB stars with an experimental wind routine

Zsolt Keszthelyi, Joachim Puls, Gregg Wade

Stellar evolution models of massive stars are very sensitive to the adopted mass-loss scheme. The magnitude and evolution of mass-loss rates significantly affect the main sequence…

cs.CV2016643 cited

Automatic Liver and Lesion Segmentation in CT Using Cascaded Fully Convolutional Neural Networks and 3D Conditional Random Fields

Patrick Ferdinand Christ, Mohamed Ezzeldin A. Elshaer, Florian Ettlinger +10

Automatic segmentation of the liver and its lesion is an important step towards deriving quantitative biomarkers for accurate clinical diagnosis and computer-aided decision support…

math.LO2016

From Nonstandard Analysis to various flavours of Computability Theory

Sam Sanders

As suggested by the title, it has recently become clear that theorems of Nonstandard Analysis (NSA) give rise to theorems in computability theory (no longer involving NSA). Now, th…

astro-ph.SR2016148 cited

The IACOB project: III. New observational clues to understand macroturbulent broadening in massive O- and B-type stars

S. Simón-Díaz, M. Godart, N. Castro +5

We aim to provide new empirical clues about macroturbulent spectral line broadening in O- and B-type stars to evaluate its physical origin. We use high-resolution spectra of ~430 s…