This repository contains code to compute depth from a single image. It accompanies our paper:
Towards Robust Monocular Depth Estimation: Mixing Datasets for Zero-shot Cross-dataset Transfer
René Ranftl, Katrin Lasinger, David Hafner, Konrad Schindler, Vladlen Koltun
and our preprint:
Vision Transformers for Dense Prediction
René Ranftl, Alexey Bochkovskiy, Vladlen Koltun
For the latest release MiDaS 3.1, a technical report and video are available.
MiDaS was trained on up to 12 datasets (ReDWeb, DIML, Movies, MegaDepth, WSVD, TartanAir, HRWSI, ApolloScape, BlendedMVS, IRS, KITTI, NYU Depth V2) with
multi-objective optimization.
The original model that was trained on 5 datasets (MIX 5
in the paper) can be found here.
The figure below shows an overview of the different MiDaS models; the bubble size scales with number of parameters.
1) Pick one or more models and download the corresponding weights to the weights
folder:
MiDaS 3.1
MiDaS 3.0: Legacy transformer models dpt_large_384 and dpt_hybrid_384
MiDaS 2.1: Legacy convolutional models midas_v21_384 and midas_v21_small_256
1) Set up dependencies:
```shell
conda env create -f environment.yaml
conda activate midas-py310
```
For the Next-ViT model, execute
git submodule add https://github.com/isl-org/Next-ViT midas/external/next_vit
For the OpenVINO model, install
pip install openvino
1) Place one or more input images in the folder input
.
2) Run the model with
python run.py --model_type <model_type> --input_path input --output_path output
where <model_type>
is chosen from dpt_beit_large_512, dpt_beit_large_384,
dpt_beit_base_384, dpt_swin2_large_384, dpt_swin2_base_384,
dpt_swin2_tiny_256, dpt_swin_large_384, dpt_next_vit_large_384,
dpt_levit_224, dpt_large_384, dpt_hybrid_384,
midas_v21_384, midas_v21_small_256, openvino_midas_v21_small_256.
3) The resulting depth maps are written to the output
folder.
1) By default, the inference resizes the height of input images to the size of a model to fit into the encoder. This
size is given by the numbers in the model names of the accuracy table. Some models do not only support a single
inference height but a range of different heights. Feel free to explore different heights by appending the extra
command line argument --height
. Unsupported height values will throw an error. Note that using this argument may
decrease the model accuracy.
2) By default, the inference keeps the aspect ratio of input images when feeding them into the encoder if this is
supported by a model (all models except for Swin, Swin2, LeViT). In order to resize to a square resolution,
disregarding the aspect ratio while preserving the height, use the command line argument --square
.
If you want the input images to be grabbed from the camera and shown in a window, leave the input and output paths away and choose a model type as shown above:
python run.py --model_type <model_type> --side
The argument --side
is optional and causes both the input RGB image and the output depth map to be shown
side-by-side for comparison.
1) Make sure you have installed Docker and the NVIDIA Docker runtime.
2) Build the Docker image:
```shell
docker build -t midas .
```
3) Run inference:
```shell
docker run --rm --gpus all -v $PWD/input:/opt/MiDaS/input -v $PWD/output:/opt/MiDaS/output -v $PWD/weights:/opt/MiDaS/weights midas
```
This command passes through all of your NVIDIA GPUs to the container, mounts the
input
and output
directories and then runs the inference.
The pretrained model is also available on PyTorch Hub
See README in the tf
subdirectory.
Currently only supports MiDaS v2.1.
See README in the mobile
subdirectory.
See README in the ros
subdirectory.
Currently only supports MiDaS v2.1. DPT-based models to be added.
We provide a zero-shot error $\epsilon_d$ which is evaluated for 6 different datasets (see paper). Lower error values are better. $\color{green}{\textsf{Overall model quality is represented by the improvement}}$ (Imp.) with respect to MiDaS 3.0 DPTL-384. The models are grouped by the height used for inference, whereas the square training resolution is given by the numbers in the model names. The table also shows the number of parameters (in millions) and the frames per second for inference at the training resolution (for GPU RTX 3090):
MiDaS Model | DIW WHDR | Eth3d AbsRel | Sintel AbsRel | TUM δ1 | KITTI δ1 | NYUv2 δ1 | $\color{green}{\textsf{Imp.}}$ % | Par.M | FPS |
---|---|---|---|---|---|---|---|---|---|
Inference height 512 | |||||||||
v3.1 BEiTL-512 | 0.1137 | 0.0659 | 0.2366 | 6.13 | 11.56* | **1.86*** | $\color{green}{\textsf{19}}$ | 345 | 5.7 |
v3.1 BEiTL-512$\tiny{\square}$ | 0.1121 | 0.0614 | 0.2090 | 6.46 | **5.00*** | 1.90* | $\color{green}{\textsf{34}}$ | 345 | 5.7 |
Inference height 384 | |||||||||
v3.1 BEiTL-512 | 0.1245 | 0.0681 | 0.2176 | 6.13 | 6.28* | **2.16*** | $\color{green}{\textsf{28}}$ | 345 | 12 |
v3.1 Swin2L-384$\tiny{\square}$ | 0.1106 | 0.0732 | 0.2442 | 8.87 | **5.84*** | 2.92* | $\color{green}{\textsf{22}}$ | 213 | 41 |
v3.1 Swin2B-384$\tiny{\square}$ | 0.1095 | 0.0790 | 0.2404 | 8.93 | 5.97* | 3.28* | $\color{green}{\textsf{22}}$ | 102 | 39 |
v3.1 SwinL-384$\tiny{\square}$ | 0.1126 | 0.0853 | 0.2428 | 8.74 | 6.60* | 3.34* | $\color{green}{\textsf{17}}$ | 213 | 49 |
v3.1 BEiTL-384 | 0.1239 | 0.0667 | 0.2545 | 7.17 | 9.84* | 2.21* | $\color{green}{\textsf{17}}$ | 344 | 13 |
v3.1 Next-ViTL-384 | 0.1031 | 0.0954 | 0.2295 | 9.21 | 6.89* | 3.47* | $\color{green}{\textsf{16}}$ | 72 | 30 |
v3.1 BEiTB-384 | 0.1159 | 0.0967 | 0.2901 | 9.88 | 26.60* | 3.91* | $\color{green}{\textsf{-31}}$ | 112 | 31 |
v3.0 DPTL-384 | 0.1082 | 0.0888 | 0.2697 | 9.97 | 8.46 | 8.32 | $\color{green}{\textsf{0}}$ | 344 | 61 |
v3.0 DPTH-384 | 0.1106 | 0.0934 | 0.2741 | 10.89 | 11.56 | 8.69 | $\color{green}{\textsf{-10}}$ | 123 | 50 |
v2.1 Large384 | 0.1295 | 0.1155 | 0.3285 | 12.51 | 16.08 | 8.71 | $\color{green}{\textsf{-32}}$ | 105 | 47 |
Inference height 256 | |||||||||
v3.1 Swin2T-256$\tiny{\square}$ | 0.1211 | 0.1106 | 0.2868 | 13.43 | **10.13*** | **5.55*** | $\color{green}{\textsf{-11}}$ | 42 | 64 |
v2.1 Small256 | 0.1344 | 0.1344 | 0.3370 | 14.53 | 29.27 | 13.43 | $\color{green}{\textsf{-76}}$ | 21 | 90 |
Inference height 224 | |||||||||
v3.1 LeViT224$\tiny{\square}$ | 0.1314 | 0.1206 | 0.3148 | 18.21 | **15.27*** | **8.64*** | $\color{green}{\textsf{-40}}$ | 51 | 73 |
* No zero-shot error, because models are also trained on KITTI and NYU Depth V2\ $\square$ Validation performed at square resolution, either because the transformer encoder backbone of a model does not support non-square resolutions (Swin, Swin2, LeViT) or for comparison with these models. All other validations keep the aspect ratio. A difference in resolution limits the comparability of the zero-shot error and the improvement, because these quantities are averages over the pixels of an image and do not take into account the advantage of more details due to a higher resolution.\ Best values per column and same validation height in bold
The improvement in the above table is defined as the relative zero-shot error with respect to MiDaS v3.0 DPTL-384 and averaging over the datasets. So, if $\epsilon_d$ is the zero-shot error for dataset $d$, then the $\color{green}{\textsf{improvement}}$ is given by $100(1-(1/6)\sum_d\epsilond/\epsilon{d,\rm{DPT_{L-384}}})$%.
Note that the improvements of 10% for MiDaS v2.0 → v2.1 and 21% for MiDaS v2.1 → v3.0 are not visible from the improvement column (Imp.) in the table but would require an evaluation with respect to MiDaS v2.1 Large384 and v2.0 Large384 respectively instead of v3.0 DPTL-384.
Zoom in for better visibility
Test configuration
Speed: 22 FPS
MiDaS is used in the following other projects from Intel Labs:
Please cite our paper if you use this code or any of the models:
@ARTICLE {Ranftl2022,
author = "Ren\'{e} Ranftl and Katrin Lasinger and David Hafner and Konrad Schindler and Vladlen Koltun",
title = "Towards Robust Monocular Depth Estimation: Mixing Datasets for Zero-Shot Cross-Dataset Transfer",
journal = "IEEE Transactions on Pattern Analysis and Machine Intelligence",
year = "2022",
volume = "44",
number = "3"
}
If you use a DPT-based model, please also cite:
@article{Ranftl2021,
author = {Ren\'{e} Ranftl and Alexey Bochkovskiy and Vladlen Koltun},
title = {Vision Transformers for Dense Prediction},
journal = {ICCV},
year = {2021},
}
Please cite the technical report for MiDaS 3.1 models:
@article{birkl2023midas,
title={MiDaS v3.1 -- A Model Zoo for Robust Monocular Relative Depth Estimation},
author={Reiner Birkl and Diana Wofk and Matthias M{\"u}ller},
journal={arXiv preprint arXiv:2307.14460},
year={2023}
}
For ZoeDepth, please use
@article{bhat2023zoedepth,
title={Zoedepth: Zero-shot transfer by combining relative and metric depth},
author={Bhat, Shariq Farooq and Birkl, Reiner and Wofk, Diana and Wonka, Peter and M{\"u}ller, Matthias},
journal={arXiv preprint arXiv:2302.12288},
year={2023}
}
and for LDM3D
@article{stan2023ldm3d,
title={LDM3D: Latent Diffusion Model for 3D},
author={Stan, Gabriela Ben Melech and Wofk, Diana and Fox, Scottie and Redden, Alex and Saxton, Will and Yu, Jean and Aflalo, Estelle and Tseng, Shao-Yen and Nonato, Fabio and Muller, Matthias and others},
journal={arXiv preprint arXiv:2305.10853},
year={2023}
}
Our work builds on and uses code from timm and Next-ViT. We'd like to thank the authors for making these libraries available.
MIT License