Scene Flow Evaluation 2015


The stereo 2015 / flow 2015 / scene flow 2015 benchmark consists of 200 training scenes and 200 test scenes (4 color images per scene, saved in loss less png format). Compared to the stereo 2012 and flow 2012 benchmarks, it comprises dynamic scenes for which the ground truth has been established in a semi-automatic process. Our evaluation server computes the percentage of bad pixels averaged over all ground truth pixels of all 200 test images. For this benchmark, we consider a pixel to be correctly estimated if the disparity or flow end-point error is <3px or <5% (for scene flow this criterion needs to be fulfilled for both disparity maps and the flow map). We require that all methods use the same parameter set for all test pairs. Our development kit provides details about the data format as well as MATLAB / C++ utility functions for reading and writing disparity maps and flow fields. More details can be found in Object Scene Flow for Autonomous Vehicles (CVPR 2015).

Our evaluation table ranks all methods according to the number of erroneous pixels. All methods providing less than 100 % density have been interpolated using simple background interpolation as explained in the corresponding header file in the development kit. Legend:

  • D1: Percentage of stereo disparity outliers in first frame
  • D2: Percentage of stereo disparity outliers in second frame
  • Fl: Percentage of optical flow outliers
  • SF: Percentage of scene flow outliers (=outliers in either D0, D1 or Fl)
  • bg: Percentage of outliers averaged only over background regions
  • fg: Percentage of outliers averaged only over foreground regions
  • all: Percentage of outliers averaged over all ground truth pixels


Note: On 13.03.2017 we have fixed several small errors in the flow (noc+occ) ground truth of the dynamic foreground objects and manually verified all images for correctness by warping them according to the ground truth. As a consequence, all error numbers have decreased slightly. Please download the devkit and the annotations with the improved ground truth for the training set again if you have downloaded the files prior to 13.03.2017 and consider reporting these new number in all future publications. The last leaderboards before these corrections can be found here (optical flow 2015) and here (scene flow 2015). The leaderboards for the KITTI 2015 stereo benchmarks did not change.

Important Policy Update: As more and more non-published work and re-implementations of existing work is submitted to KITTI, we have established a new policy: from now on, only submissions with significant novelty that are leading to a peer-reviewed paper in a conference or journal are allowed. Minor modifications of existing algorithms or student research projects are not allowed. Such work must be evaluated on a split of the training set. To ensure that our policy is adopted, new users must detail their status, describe their work and specify the targeted venue during registration. Furthermore, we will regularly delete all entries that are 6 months old but are still anonymous or do not have a paper associated with them. For conferences, 6 month is enough to determine if a paper has been accepted and to add the bibliography information. For longer review cycles, you need to resubmit your results.
Additional information used by the methods
  • Multiview: Method uses more than 2 temporally adjacent images
  • Motion stereo: Method uses epipolar geometry for computing optical flow
  • Additional training data: Use of additional data sources for training (see details)

Evaluation ground truth        Evaluation area

Method Setting Code D1-bg D1-fg D1-all D2-bg D2-fg D2-all Fl-bg Fl-fg Fl-all SF-bg SF-fg SF-all Density Runtime Environment
1 SplatFlow3D code 1.40 2.91 1.65 1.88 6.29 2.61 2.27 6.02 2.89 2.84 10.04 4.04 100.00 0.2 s GPU @ 2.5 Ghz (Python)
2 ScaleRAFTRBO code 1.48 3.46 1.81 1.93 7.72 2.89 2.27 5.63 2.83 2.86 10.91 4.20 100.00 0.1 s 1 core @ 2.5 Ghz (C/C++)
3 RBO 1.48 3.46 1.81 1.91 8.62 3.02 2.13 6.15 2.80 2.72 11.68 4.21 100.00 1 s 1 core @ 2.5 Ghz (C/C++)
4 GAOSF 1.48 3.46 1.81 1.92 8.39 2.99 2.08 7.37 2.96 2.65 12.27 4.25 100.00 1 s GPU @ 2.5 Ghz (Python + C/C++)
5 CamLiRAFT code 1.48 3.46 1.81 1.91 8.11 2.94 2.08 7.37 2.96 2.68 12.16 4.26 100.00 1 s GPU @ 2.5 Ghz (Python + C/C++)
H. Liu, T. Lu, Y. Xu, J. Liu and L. Wang: Learning Optical Flow and Scene Flow with Bidirectional Camera-LiDAR Fusion. TPAMI 2023.
6 RAFT-3D++ 1.48 3.46 1.81 1.91 9.05 3.10 2.09 8.55 3.16 2.63 12.87 4.34 100.00 0.5 s 1 core @ 2.5 Ghz (Python)
7 EFLOW 1.40 2.91 1.65 1.90 7.50 2.84 2.27 7.10 3.07 2.87 11.69 4.34 100.00 0.06 s 1 core @ 2.5 Ghz (Python)
8 CamLiFlow code 1.48 3.46 1.81 1.92 8.14 2.95 2.31 7.04 3.10 2.87 12.23 4.43 100.00 1.2 s GPU @ 2.5 Ghz (Python + C/C++)
H. Liu, T. Lu, Y. Xu, J. Liu, W. Li and L. Chen: CamLiFlow: Bidirectional Camera-LiDAR Fusion for Joint Optical Flow and Scene Flow Estimation. CVPR 2022.
9 M-FUSE
This method makes use of multiple (>2) views.
code 1.40 2.91 1.65 2.14 8.10 3.13 2.66 7.47 3.46 3.43 11.84 4.83 100.00 1.3 s GPU
L. Mehl, A. Jahedi, J. Schmalfuss and A. Bruhn: M-FUSE: Multi-frame Fusion for Scene Flow Estimation. Proc. Winter Conference on Applications of Computer Vision (WACV) 2023.
10 RigidMask+ISF code 1.53 3.65 1.89 2.09 8.92 3.23 2.63 7.85 3.50 3.25 13.08 4.89 100.00 3.3 s GPU @ 2.5 Ghz (Python)
G. Yang and D. Ramanan: Learning to Segment Rigid Motions from Two Frames. CVPR 2021.
11 RAFT3DMR 1.48 3.46 1.81 1.92 8.38 3.00 2.52 9.81 3.74 3.05 14.39 4.94 100.00 1 s 1 core @ 2.5 Ghz (C/C++)
12 CamLiRAFT-NR code 1.48 3.46 1.81 2.05 7.86 3.02 2.76 6.78 3.43 3.64 11.66 4.97 100.00 1 s GPU @ 2.5 Ghz (Python + C/C++)
H. Liu, T. Lu, Y. Xu, J. Liu and L. Wang: Learning Optical Flow and Scene Flow with Bidirectional Camera-LiDAR Fusion. arXiv preprint arXiv:2303.12017 2023.
13 SF2SE3 code 1.40 2.91 1.65 2.20 7.66 3.11 3.17 8.79 4.11 3.75 13.15 5.32 100.00 2.7 s GPU @ >3.5 Ghz (Python)
L. Sommer, P. Schröppel and T. Brox: SF2SE3: Clustering Scene Flow into SE (3)-Motions via Proposal and Selection. DAGM German Conference on Pattern Recognition 2022.
14 RAFT-3D 1.48 3.46 1.81 2.51 9.46 3.67 3.39 8.79 4.29 4.27 13.27 5.77 100.00 2 s GPU @ 2.5 Ghz (Python + C/C++)
Z. Teed and J. Deng: RAFT-3D: Scene Flow using Rigid-Motion Embeddings. arXiv preprint arXiv:2012.00726 2020.
15 MonoFusion 1.48 3.46 1.81 2.34 9.18 3.47 3.93 5.97 4.27 4.81 11.61 5.94 100.00 0.7 s GPU @ 2.5 Ghz (Python)
16 ScaleRAFT code 1.48 3.46 1.81 2.31 7.42 3.16 4.45 4.76 4.50 5.31 10.18 6.12 100.00 0.1 s 1 core @ 2.5 Ghz (C/C++)
17 UberATG-DRISF 2.16 4.49 2.55 2.90 9.73 4.04 3.59 10.40 4.73 4.39 15.94 6.31 100.00 0.75 s CPU+GPU @ 2.5 Ghz (Python)
W. Ma, S. Wang, R. Hu, Y. Xiong and R. Urtasun: Deep Rigid Instance Scene Flow. CVPR 2019.
18 Scale-flow-ADF58 1.48 3.46 1.81 2.44 7.95 3.36 4.36 7.00 4.80 5.28 11.71 6.35 100.00 0.1 s 1 core @ 2.5 Ghz (C/C++)
19 Scale-flow code 1.48 3.46 1.81 2.55 8.24 3.50 5.24 5.71 5.32 6.06 11.32 6.94 100.00 0.8 s GPU @ 2.5 Ghz (Python)
H. Ling, Q. Sun, Z. Ren, Y. Liu, H. Wang and Z. Wang: Scale-flow: Estimating 3D Motion from Video. Proceedings of the 30th ACM International Conference on Multimedia 2022.
20 ACOSF 2.79 7.56 3.58 3.82 12.74 5.31 4.56 12.00 5.79 5.61 19.38 7.90 100.00 5 min 1 core @ 3.0 Ghz (Matlab + C/C++)
C. Li, H. Ma and Q. Liao: Two-Stage Adaptive Object Scene Flow Using Hybrid CNN-CRF Model. International Conference on Pattern Recognition (ICPR) 2020.
21 ISF 4.12 6.17 4.46 4.88 11.34 5.95 5.40 10.29 6.22 6.58 15.63 8.08 100.00 10 min 1 core @ 3 Ghz (C/C++)
A. Behl, O. Jafari, S. Mustikovela, H. Alhaija, C. Rother and A. Geiger: Bounding Boxes, Segmentations and Object Coordinates: How Important is Recognition for 3D Scene Flow Estimation in Autonomous Driving Scenarios?. International Conference on Computer Vision (ICCV) 2017.
22 Stereo expansion code 1.48 3.46 1.81 3.39 8.54 4.25 5.83 8.66 6.30 7.06 13.44 8.12 100.00 2 s GPU @ 2.5 Ghz (Python)
G. Yang and D. Ramanan: Upgrading Optical Flow to 3D Scene Flow through Optical Expansion. CVPR 2020.
23 Binary TTC 1.48 3.46 1.81 3.84 9.39 4.76 5.84 8.67 6.31 7.45 13.74 8.50 100.00 2 s GPU @ 1.0 Ghz (Python)
A. Badki, O. Gallo, J. Kautz and P. Sen: Binary TTC: A Temporal Geofence for Autonomous Navigation. The IEEE Conference on Computer Vision and Pattern Recognition (CVPR) 2021.
24 PRSM
This method makes use of multiple (>2) views.
code 3.02 10.52 4.27 5.13 15.11 6.79 5.33 13.40 6.68 6.61 20.79 8.97 99.99 300 s 1 core @ 2.5 Ghz (C/C++)
C. Vogel, K. Schindler and S. Roth: 3D Scene Flow Estimation with a Piecewise Rigid Scene Model. ijcv 2015.
25 DTF_SENSE
This method makes use of multiple (>2) views.
2.08 3.13 2.25 4.82 9.02 5.52 7.31 9.48 7.67 8.21 14.08 9.18 100.00 0.76 s 1 core @ 2.5 Ghz (C/C++)
R. Schuster, C. Unger and D. Stricker: A Deep Temporal Fusion Framework for Scene Flow Using a Learnable Motion Model and Occlusions. IEEE Winter Conference on Applications of Computer Vision (WACV) 2021.
26 OSF+TC
This method makes use of multiple (>2) views.
4.11 9.64 5.03 5.18 15.12 6.84 5.76 13.31 7.02 7.08 20.03 9.23 100.00 50 min 1 core @ 2.5 Ghz (C/C++)
M. Neoral and J. Šochman: Object Scene Flow with Temporal Consistency. 22nd Computer Vision Winter Workshop (CVWW) 2017.
27 SENSE code 2.07 3.01 2.22 4.90 10.83 5.89 7.30 9.33 7.64 8.36 15.49 9.55 100.00 0.32s GPU, GTX 2080Ti
H. Jiang, D. Sun, V. Jampani, Z. Lv, E. Learned-Miller and J. Kautz: SENSE: A Shared Encoder Network for Scene-Flow Estimation. The IEEE International Conference on Computer Vision (ICCV) 2019.
28 OSF 2018 code 4.11 11.12 5.28 5.01 17.28 7.06 5.38 17.61 7.41 6.68 24.59 9.66 100.00 390 s 1 core @ 2.5 Ghz (Matlab + C/C++)
M. Menze, C. Heipke and A. Geiger: Object Scene Flow. ISPRS Journal of Photogrammetry and Remote Sensing (JPRS) 2018.
29 SSF 3.55 8.75 4.42 4.94 17.48 7.02 5.63 14.71 7.14 7.18 24.58 10.07 100.00 5 min 1 core @ 2.5 Ghz (Matlab + C/C++)
Z. Ren, D. Sun, J. Kautz and E. Sudderth: Cascaded Scene Flow Prediction using Semantic Segmentation. International Conference on 3D Vision (3DV) 2017.
30 OSF code 4.54 12.03 5.79 5.45 19.41 7.77 5.62 18.92 7.83 7.01 26.34 10.23 100.00 50 min 1 core @ 2.5 Ghz (C/C++)
M. Menze and A. Geiger: Object Scene Flow for Autonomous Vehicles. Conference on Computer Vision and Pattern Recognition (CVPR) 2015.
31 DWARF 3.20 3.94 3.33 6.21 9.38 6.73 9.80 13.37 10.39 11.72 18.06 12.78 100.00 0.14s - 1.43s TitanXP - JetsonTX2
F. Aleotti, M. Poggi, F. Tosi and S. Mattoccia: Learning end-to-end scene flow by distilling single tasks knowledge. Thirty-Fourth AAAI Conference on Artificial Intelligence (AAAI-20) 2020.
32 SFF++
This method makes use of multiple (>2) views.
4.27 12.38 5.62 7.31 18.12 9.11 10.63 17.48 11.77 12.44 25.33 14.59 100.00 78 s 4 cores @ 3.5 Ghz (C/C++)
R. Schuster, O. Wasenmüller, C. Unger, G. Kuschk and D. Stricker: SceneFlowFields++: Multi-frame Matching, Visibility Prediction, and Robust Interpolation for Scene Flow Estimation. International Journal of Computer Vision (IJCV) 2019.
33 DTF_PWOC
This method makes use of multiple (>2) views.
3.91 8.57 4.68 6.25 14.03 7.55 10.78 19.99 12.31 12.42 25.74 14.64 100.00 0.38 s RTX 2080 Ti
R. Schuster, C. Unger and D. Stricker: A Deep Temporal Fusion Framework for Scene Flow Using a Learnable Motion Model and Occlusions. IEEE Winter Conference on Applications of Computer Vision (WACV) 2021.
34 Self-SuperFlow-ft 3.81 8.92 4.66 7.13 16.27 8.65 10.65 19.44 12.12 12.33 26.73 14.73 100.00 0.13 s GTX 1080 Ti
K. Bendig, R. Schuster and D. Stricker: Self-SuperFlow: Self-supervised Scene Flow Prediction in Stereo Sequences. International Conference on Image Processing (ICIP) 2022.
35 FSF+MS
This method makes use of the epipolar geometry.
This method makes use of multiple (>2) views.
5.72 11.84 6.74 7.57 21.28 9.85 8.48 25.43 11.30 11.17 33.91 14.96 100.00 2.7 s 4 cores @ 3.5 Ghz (C/C++)
T. Taniai, S. Sinha and Y. Sato: Fast Multi-frame Stereo Scene Flow with Motion Segmentation. IEEE Conference on Computer Vision and Pattern Recognition (CVPR 2017) 2017.
36 PWOC-3D code 4.19 9.82 5.13 7.21 14.73 8.46 12.40 15.78 12.96 14.30 22.66 15.69 100.00 0.13 s GTX 1080 Ti
R. Saxena, R. Schuster, O. Wasenmüller and D. Stricker: PWOC-3D: Deep Occlusion-Aware End-to-End Scene Flow Estimation. Intelligent Vehicles Symposium (IV) 2019.
37 CSF 4.57 13.04 5.98 7.92 20.76 10.06 10.40 25.78 12.96 12.21 33.21 15.71 99.99 80 s 1 core @ 2.5 Ghz (C/C++)
Z. Lv, C. Beall, P. Alcantarilla, F. Li, Z. Kira and F. Dellaert: A Continuous Optimization Approach for Efficient and Accurate Scene Flow. European Conf. on Computer Vision (ECCV) 2016.
38 SceneFFields 5.12 13.83 6.57 8.47 21.83 10.69 10.58 24.41 12.88 12.48 32.28 15.78 100.00 65 s 4 cores @ 3.7 Ghz (C/C++)
R. Schuster, O. Wasenmüller, G. Kuschk, C. Bailer and D. Stricker: SceneFlowFields: Dense Interpolation of Sparse Scene Flow Correspondences. IEEE Winter Conference on Applications of Computer Vision (WACV) 2018.
39 Self-scale-flow-nerf 1.48 3.46 1.81 8.07 10.52 8.47 13.08 15.45 13.47 15.17 20.18 16.01 100.00 0.2 s 1 core @ 2.5 Ghz (C/C++)
40 PR-Sceneflow code 4.74 13.74 6.24 11.14 20.47 12.69 11.73 24.33 13.83 13.49 31.22 16.44 100.00 150 s 4 core @ 3.0 Ghz (Matlab + C/C++)
C. Vogel, K. Schindler and S. Roth: Piecewise Rigid Scene Flow. ICCV 2013.
41 SPS+FF++ code 5.47 12.19 6.59 13.06 20.83 14.35 15.91 20.27 16.64 18.98 29.51 20.73 100.00 36 s 1 core @ 3.5 Ghz (C/C++)
R. Schuster, O. Wasenmüller and D. Stricker: Dense Scene Flow from Stereo Disparity and Optical Flow. ACM Computer Science in Cars Symposium (CSCS) 2018.
42 Anonymous 4.07 9.41 4.96 12.75 14.42 13.02 17.91 18.08 17.93 21.07 25.08 21.74 100.00 0.1 s GPU @ 2.5 Ghz (Python)
43 Mono-SF 14.21 26.94 16.32 16.89 33.07 19.59 11.40 19.64 12.77 19.79 39.57 23.08 100.00 41 s 1 core @ 3.5 Ghz (Matlab + C/C++)
F. Brickwedde, S. Abraham and R. Mester: Mono-SF: Multi-View Geometry meets Single-View Depth for Monocular Scene Flow Estimation of Dynamic Traffic Scenes. Proc. of International Conference on Computer Vision (ICCV) 2019.
44 SGM+SF 5.15 15.29 6.84 14.10 23.13 15.60 20.91 25.50 21.67 23.09 34.46 24.98 100.00 45 min 16 core @ 3.2 Ghz (C/C++)
H. Hirschmüller: Stereo Processing by Semiglobal Matching and Mutual Information. PAMI 2008.
M. Hornacek, A. Fitzgibbon and C. Rother: SphereFlow: 6 DoF Scene Flow from RGB-D Pairs. CVPR 2014.
45 MonoComb 17.89 21.16 18.44 22.34 25.85 22.93 5.84 8.67 6.31 27.06 33.55 28.14 100.00 0.58 s RTX 2080 Ti
R. Schuster, C. Unger and D. Stricker: MonoComb: A Sparse-to-Dense Combination Approach for Monocular Scene Flow. ACM Computer Science in Cars Symposium (CSCS) 2020.
46 Self-SuperFlow 5.78 19.76 8.11 19.88 30.03 21.57 22.70 28.55 23.67 26.31 40.72 28.71 100.00 0.13 s GTX 1080 Ti
K. Bendig, R. Schuster and D. Stricker: Self-SuperFlow: Self-supervised Scene Flow Prediction in Stereo Sequences. International Conference on Image Processing (ICIP) 2022.
47 PCOF-LDOF 6.31 19.24 8.46 19.09 30.54 20.99 14.34 38.32 18.33 25.26 49.39 29.27 100.00 50 s 1 core @ 3.0 Ghz (C/C++)
M. Derome, A. Plyer, M. Sanfourche and G. Le Besnerais: A Prediction-Correction Approach for Real-Time Optical Flow Computation Using Stereo. German Conference on Pattern Recognition 2016.
48 PCOF + ACTF 6.31 19.24 8.46 19.15 36.27 22.00 14.89 60.15 22.43 25.77 67.75 32.76 100.00 0.08 s GPU @ 2.0 Ghz (C/C++)
M. Derome, A. Plyer, M. Sanfourche and G. Le Besnerais: A Prediction-Correction Approach for Real-Time Optical Flow Computation Using Stereo. German Conference on Pattern Recognition 2016.
49 Multi-Mono-SF-ft
This method makes use of multiple (>2) views.
code 21.60 28.22 22.71 25.47 31.72 26.51 12.41 18.20 13.37 31.18 42.68 33.09 100.00 0.06 s NVIDIA GTX 1080 Ti
J. Hur and S. Roth: Self-Supervised Multi-Frame Monocular Scene Flow. CVPR 2021.
50 SGM&FlowFie+ 11.93 20.57 13.37 27.02 31.71 27.80 22.83 22.75 22.82 32.26 40.12 33.57 81.24 29 s 1 core @ 3.5 Ghz (C/C++)
R. Schuster, C. Bailer, O. Wasenmüller and D. Stricker: Combining Stereo Disparity and Optical Flow for Basic Scene Flow. Commercial Vehicle Technology Symposium (CVTS) 2018.
51 Self-Mono-SF-ft code 20.72 29.41 22.16 23.83 32.29 25.24 15.51 17.96 15.91 31.51 45.77 33.88 100.00 0.09 s NVIDIA GTX 1080 Ti
J. Hur and S. Roth: Self-Supervised Monocular Scene Flow Estimation. CVPR 2020.
52 RAFT-MSF 18.10 36.82 21.21 24.98 40.19 27.51 17.98 20.33 18.37 31.59 51.97 34.98 100.00 0.18 s GPU @ 2.5 Ghz (Python)
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53 SGM+C+NL code 5.15 15.29 6.84 28.77 25.65 28.25 34.24 42.46 35.61 38.21 50.95 40.33 100.00 4.5 min 1 core @ 2.5 Ghz (C/C++)
H. Hirschmüller: Stereo Processing by Semiglobal Matching and Mutual Information. PAMI 2008.
D. Sun, S. Roth and M. Black: A Quantitative Analysis of Current Practices in Optical Flow Estimation and the Principles Behind Them. IJCV 2013.
54 3DG-DVO 7.62 11.44 8.26 21.56 20.84 21.44 34.04 50.52 36.78 37.94 56.97 41.11 100.00 0.04 s GPU @ 1.5 Ghz (Python)
55 SGM+LDOF code 5.15 15.29 6.84 29.58 23.48 28.56 40.81 31.92 39.33 43.99 42.09 43.67 100.00 86 s 1 core @ 2.5 Ghz (C/C++)
H. Hirschmüller: Stereo Processing by Semiglobal Matching and Mutual Information. PAMI 2008.
T. Brox and J. Malik: Large Displacement Optical Flow: Descriptor Matching in Variational Motion Estimation. PAMI 2011.
56 Multi-Mono-SF
This method makes use of multiple (>2) views.
code 27.48 47.30 30.78 32.39 44.56 34.41 18.13 26.59 19.54 40.29 62.78 44.04 100.00 0.06 s NVIDIA GTX 1080 Ti
J. Hur and S. Roth: Self-Supervised Multi-Frame Monocular Scene Flow. CVPR 2021.
57 DWBSF 19.61 22.69 20.12 35.72 28.15 34.46 40.74 31.16 39.14 46.42 40.76 45.48 100.00 7 min 4 cores @ 3.5 Ghz (C/C++)
C. Richardt, H. Kim, L. Valgaerts and C. Theobalt: Dense Wide-Baseline Scene Flow From Two Handheld Video Cameras. 3DV 2016.
58 Self-Mono-SF code 31.22 48.04 34.02 34.89 43.59 36.34 23.26 24.93 23.54 46.68 63.82 49.54 100.00 0.09 s NVIDIA GTX 1080 Ti
J. Hur and S. Roth: Self-Supervised Monocular Scene Flow Estimation. CVPR 2020.
59 GCSF code 11.64 27.11 14.21 32.94 35.77 33.41 47.38 41.50 46.40 52.92 56.68 53.54 100.00 2.4 s 1 core @ 2.5 Ghz (C/C++)
J. Cech, J. Sanchez-Riera and R. Horaud: Scene Flow Estimation by growing Correspondence Seeds. CVPR 2011.
60 VSF code 27.31 21.72 26.38 59.51 44.93 57.08 50.06 45.40 49.28 67.69 62.93 66.90 100.00 125 min 1 core @ 2.5 Ghz (C/C++)
F. Huguet and F. Devernay: A Variational Method for Scene Flow Estimation from Stereo Sequences. ICCV 2007.
61 Stereo-RSSF code 56.60 73.05 59.34 58.86 74.41 61.45 70.68 73.60 71.17 76.21 81.62 77.11 9.26 2.5 s 8 core @ 2.5 Ghz (Matlab)
E. Salehi, A. Aghagolzadeh and R. Hosseini: Stereo-RSSF: stereo robust sparse scene-flow estimation. The Visual Computer 2023.
Table as LaTeX | Only published Methods




Related Datasets

  • HCI/Bosch Robust Vision Challenge: Optical flow and stereo vision challenge on high resolution imagery recorded at a high frame rate under diverse weather conditions (e.g., sunny, cloudy, rainy). The Robert Bosch AG provides a prize for the best performing method.
  • Image Sequence Analysis Test Site (EISATS): Synthetic image sequences with ground truth information provided by UoA and Daimler AG. Some of the images come with 3D range sensor information.
  • Middlebury Stereo Evaluation: The classic stereo evaluation benchmark, featuring four test images in version 2 of the benchmark, with very accurate ground truth from a structured light system. 38 image pairs are provided in total.
  • Daimler Stereo Dataset: Stereo bad weather highway scenes with partial ground truth for freespace
  • Make3D Range Image Data: Images with small-resolution ground truth used to learn and evaluate depth from single monocular images.
  • Lubor Ladicky's Stereo Dataset: Stereo Images with manually labeled ground truth based on polygonal areas.
  • Middlebury Optical Flow Evaluation: The classic optical flow evaluation benchmark, featuring eight test images, with very accurate ground truth from a shape from UV light pattern system. 24 image pairs are provided in total.

Citation

When using this dataset in your research, we will be happy if you cite us:
@article{Menze2018JPRS,
  author = {Moritz Menze and Christian Heipke and Andreas Geiger},
  title = {Object Scene Flow},
  journal = {ISPRS Journal of Photogrammetry and Remote Sensing (JPRS)},
  year = {2018}
}
@inproceedings{Menze2015ISA,
  author = {Moritz Menze and Christian Heipke and Andreas Geiger},
  title = {Joint 3D Estimation of Vehicles and Scene Flow},
  booktitle = {ISPRS Workshop on Image Sequence Analysis (ISA)},
  year = {2015}
}



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