Review of pedestrian detection techniques in automotive far-infrared video

2015 ◽  
Vol 9 (8) ◽  
pp. 824-832 ◽  
Author(s):  
Patrick Hurney ◽  
Fearghal Morgan ◽  
Martin Glavin ◽  
Edward Jones ◽  
Peter Waldron
Sensors ◽  
2015 ◽  
Vol 15 (4) ◽  
pp. 8570-8594 ◽  
Author(s):  
Bassem Besbes ◽  
Alexandrina Rogozan ◽  
Adela-Maria Rus ◽  
Abdelaziz Bensrhair ◽  
Alberto Broggi

2021 ◽  
Vol 2021 ◽  
pp. 1-7
Author(s):  
Zhaoli Wu ◽  
Xin Wang ◽  
Chao Chen

Due to the limitation of energy consumption and power consumption, the embedded platform cannot meet the real-time requirements of the far-infrared image pedestrian detection algorithm. To solve this problem, this paper proposes a new real-time infrared pedestrian detection algorithm (RepVGG-YOLOv4, Rep-YOLO), which uses RepVGG to reconstruct the YOLOv4 backbone network, reduces the amount of model parameters and calculations, and improves the speed of target detection; using space spatial pyramid pooling (SPP) obtains different receptive field information to improve the accuracy of model detection; using the channel pruning compression method reduces redundant parameters, model size, and computational complexity. The experimental results show that compared with the YOLOv4 target detection algorithm, the Rep-YOLO algorithm reduces the model volume by 90%, the floating-point calculation is reduced by 93.4%, the reasoning speed is increased by 4 times, and the model detection accuracy after compression reaches 93.25%.


Author(s):  
Emmanuel Bercier ◽  
Patrick Robert ◽  
David Pochic ◽  
Jean-Luc Tissot ◽  
Agnes Arnaud ◽  
...  

Author(s):  
Massimo Bertozzi ◽  
Alberto Broggi ◽  
Mirko Felisa ◽  
Stefano Ghidoni ◽  
Paolo Grisleri ◽  
...  

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

2019 ◽  
Vol 57 (1) ◽  
pp. 79-112 ◽  
Author(s):  
Susanna L. Widicus Weaver

The recent advancements in far-infrared (far-IR) astronomy brought about by the Herschel, SOFIA, and ALMA observatories have led to technological advancements in millimeterwave and submillimeterwave laboratory spectroscopy that is used to support molecular observations. This review gives an overview of rotational spectroscopy and its relationship with observational astronomy, as well as an overview of laboratory spectroscopic techniques focusing on both historical approaches and new advancements. Additional topics discussed include production and detection techniques for unstable molecular species of astrochemical interest, data analysis approaches that address spectral complexity and line confusion, and the current state of and limitations to spectral line databases. Potential areas for new developments in this field are also reviewed. To advance the field, the following challenges must be addressed: ▪ Data acquisition speed, spectral sensitivity, and analysis approaches for complex mixtures and broadband spectra are the greatest limitations—and hold the greatest promise for advancement—in this field of research. ▪ Full science return from far-IR observatories cannot be realized until laboratory spectroscopy catches up with the data rate for observations. ▪ New techniques building on those used in the microwave and IR regimes are required to fill the terahertz gap.


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