scholarly journals Contrast invariant features for human detection in far infrared images

Author(s):  
Daniel Olmeda ◽  
Arturo de la Escalera ◽  
Jose Maria Armingol
Author(s):  
Bassem Besbes ◽  
Sonda Ammar ◽  
Yousri Kessentini ◽  
Alexandrina Rogozan ◽  
Abdelaziz Bensrhair
Keyword(s):  

Author(s):  
Daniel Olmeda ◽  
Arturo de la Escalera ◽  
José Maria Armingol
Keyword(s):  

2013 ◽  
Vol 20 (4) ◽  
pp. 347-360 ◽  
Author(s):  
Daniel Olmeda ◽  
Cristiano Premebida ◽  
Urbano Nunes ◽  
Jose Maria Armingol ◽  
Arturo de la Escalera

1989 ◽  
Vol 98 ◽  
pp. 1572 ◽  
Author(s):  
A. P. Marston

2017 ◽  
Vol 873 ◽  
pp. 347-352
Author(s):  
Yong Hao Xiao ◽  
Hong Zhen

Human detection is a keyproblem in computer vision. Recently, some research has been focusing on the detection ofpedestrianusing infrared images. The infrared images have outstanding merit. It depends only on object's temperature, but not on color or texture. In this paper, the pedestrian crowd detection approach is proposed. The approach is compose of ROI blocks extraction and crowd block recognition. ROI blocks can be extracted with circle gradient operator and weighted geometric filtering. Crowd blocks are recognized by support vector machine, which combines histogram of oriented gradient and circle gradient. The experimental results show thatthe approach works effectively in different scenes.


1989 ◽  
Vol 120 ◽  
pp. 227-230
Author(s):  
C. Eiroa ◽  
M. Casali

ABSTRACT:Near-infrared images of the Serpens molecular cloud core have been carried out at UKIRT (Mauna Kea Observatory) using the infrared array camera, IRCAM. A large-scale diffuse nebulosity extending over the central part of the core is observed. Over 100 K-sources are detected in the 30 arc min2 cloud core. Some of them are PMS objects which were previously unknown. For the first time, a near-infrared counterpart of the far-infrared source Seroens FIRS1 has been detected. The 2.2 µm source appears as a point like object at the apex of an extended knotty, jet-like nebulosity oriented towards the northwest. In addition, a group of 11 stellar objects is seen in the position of the IR/radio source SVS4. These objects are embedded in a very faint nebulosity and form one of the densest clustering of young stars found in dark clouds.


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