Learning size adaptive local maxima selection for robust nuclei detection in histopathology images

Author(s):  
N. Brieu ◽  
G. Schmidt
Author(s):  
Lekha S Nair ◽  
Ramkishor Prabhu R ◽  
Gowry Sugathan ◽  
Kiran V Gireesh ◽  
Akshay S Nair

2016 ◽  
Vol 35 (1) ◽  
pp. 119-130 ◽  
Author(s):  
Jun Xu ◽  
Lei Xiang ◽  
Qingshan Liu ◽  
Hannah Gilmore ◽  
Jianzhong Wu ◽  
...  

2019 ◽  
Vol 5 (1) ◽  
pp. 21 ◽  
Author(s):  
Haonan Zhou ◽  
Raju Machupalli ◽  
Mrinal Mandal

Accurate and efficient detection of cell nuclei is an important step towards the development of a pathology-based Computer Aided Diagnosis. Generally, high-resolution histopathology images are very large, in the order of billion pixels, therefore nuclei detection is a highly compute intensive task, and software implementation requires a significant amount of processing time. To assist the doctors in real time, special hardware accelerators, which can reduce the processing time, are required. In this paper, we propose a Field Programmable Gate Array (FPGA) implementation of automated nuclei detection algorithm using generalized Laplacian of Gaussian filters. The experimental results show that the implemented architecture has the potential to provide a significant improvement in processing time without losing detection accuracy.


2021 ◽  
pp. 499-508
Author(s):  
Zhi Wang ◽  
Xiaoya Zhu ◽  
Lei Su ◽  
Gang Meng ◽  
Junsheng Zhang ◽  
...  

Author(s):  
Engin Bozaba ◽  
Gizem Solmaz ◽  
Cisem Yazici ◽  
Gulsah Ozsoy ◽  
Fatma Tokat ◽  
...  

2000 ◽  
Vol 179 ◽  
pp. 201-204
Author(s):  
Vojtech Rušin ◽  
Milan Minarovjech ◽  
Milan Rybanský

AbstractLong-term cyclic variations in the distribution of prominences and intensities of green (530.3 nm) and red (637.4 nm) coronal emission lines over solar cycles 18–23 are presented. Polar prominence branches will reach the poles at different epochs in cycle 23: the north branch at the beginning in 2002 and the south branch a year later (2003), respectively. The local maxima of intensities in the green line show both poleward- and equatorward-migrating branches. The poleward branches will reach the poles around cycle maxima like prominences, while the equatorward branches show a duration of 18 years and will end in cycle minima (2007). The red corona shows mostly equatorward branches. The possibility that these branches begin to develop at high latitudes in the preceding cycles cannot be excluded.


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