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Learning for Disparity Estimation through Feature Constancy

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Stereo matching algorithms usually consist of four steps, including matching cost calculation, matching cost aggregation, disparity calculation, and disparity refinement. Existing CNN-based methods only adopt CNN to solve parts of the four steps, or use different networks to deal with different steps, making them difficult to obtain the overall optimal solution. In this paper, we propose a network architecture to incorporate all steps of stereo matching. The network consists of three parts. The first part calculates the multi-scale shared features. The second part performs matching cost calculation, matching cost aggregation and disparity calculation to estimate the initial disparity using shared features. The initial disparity and the shared features are used to calculate the feature constancy that measures correctness of the correspondence between two input images. The initial disparity and the feature constancy are then fed to a sub-network to refine the initial disparity. The proposed method has been evaluated on the Scene Flow and KITTI datasets. It achieves the state-of-the-art performance on the KITTI 2012 and KITTI 2015 benchmarks while maintaining a very fast running time.

Zhengfa Liang, Yiliu Feng, Yulan Guo, Hengzhu Liu, Wei Chen, Linbo Qiao, Li Zhou, Jianfeng Zhang• 2017

Related benchmarks

TaskDatasetResultRank
Stereo MatchingKITTI 2015 (test)
D1 Error (Overall)2.36
144
Disparity EstimationKITTI 2015 (test)
D1 Error (bg, all)2.14
77
Stereo MatchingKITTI 2012 (test)
Outlier Rate (3px, Noc)1.71
76
Stereo MatchingScene Flow (test)
EPE1.4
70
Stereo MatchingKITTI 2015 (non-occluded)
D1 Error (Background)2.1
25
Disparity EstimationScene Flow (test)
EPE1.4
24
Stereo MatchingMiddlebury non-occluded
Bad Pixel Rate (2.0)24.8
20
Stereo MatchingETH3D (non-occluded)
Bad 1.0 Error4.23
19
Stereo MatchingMiddlebury v3
Average Error6.56
17
Stereo MatchingMiddlebury 2014
Bad Pixel Rate (Thresh 2.0, All)29.5
12
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