This repo is the implementation of Spatio-angular Dense Network (SADenseNet) for light field reconstruction.

Efficient Light Field Reconstruction via Spatio-Angular Dense Network
Zexi Hu; Henry Wing Fung Yeung; Xiaoming Chen; Yuk Ying Chung; Haisheng Li
IEEE Transactions on Instrumentation and Measurement (2021)
[IEEE Xplore] [arXiv]

Python 3.6
Tensorflow 1.15.5 (Tensorflow 2 is not supported.)
Keras 2.3.1

Running the following command to install the required Python packages:

pip install -r requirements.txt

As the light field files are substaintially larger than regular image files, this repo using HDF5 format to store and preload the needed LF images for both training and testing.

To obtain the HDF5 files, two options are provided:

1. Download the generated HDF5 files we provided in this page and put them under the data folder.
2. Do it yourself following the instruction below.

NOTICE:

1. Beware of your disk space as the HDF5 files will be huge.
2. As the cloud storage is provided the University of Sydney, it will expire after one year and needs manual renewal. Therefore, I would encourage readers to obtain HDF5 files via Do It Yourself presented below. In spite of that, you are welcome to use the pre-computed HDF5 files or remind me to renew it again if expiration happens again.

Modify the datasets variable in prepare.py to specify which datasets to be prepared, and then following the instruction below to have raw data and configuration ready. The HDF5 files will be placed in dir_data variable in config.py.

30Scenes (Kalantari)

1. Visit the page to download the training and test sets and unzip them somewhere. As a result, there should be two folders, namely TrainingSet and TestSet.
2. In components/datasets/lytro/KalantariDataset.py, modify path_raw to the path containing the two folders mentioned in the last step.
3. If your intention is just the test set, comment out Dataset.MODE_TRAIN in list variable in components/datasets/lytro/KalantariDataset.py to save time.
4. Run python prepare.py.

Stanford Lytro Light Field Archive

1. Visit the the official website to download Occlusions and Refelctive categories, and unzip them in the same folder.
2. In components/datasets/lytro/StanfordDataset.py, modify path_raw to the unzipped folder.
3. Run python prepare.py.

EPFL

1. The original data was downloaded from the official website or the alternative website and converted from .mat files to .png files. Unfortunately, the conversion code is lost while the PNG files are kept here.
2. In components/datasets/lytro/EpflDataset.py, modify path_raw to the unzipped folder.
3. Run python prepare.py.

1. We provide the pre-trained models mentioned in the paper in the release page. Download them and put it somewhere, e.g. the models folder.
2. In config.py, change the corresponding variables in the Network section for the model you choose. The default configuration is for the full SADenseNet variant ISA_651 which provides the best performance.

Simply run the following command:

python --model /path/to/model.hdf5 --bgr --diff --mp 1

Assuming we are benchmarking on 30Scenes:

1. --mp enables multiprocessing when it is larger than 0 while you can disable it by set it to 0. Default to 1.
2. --bgr enables image rendering into PNG files in tmp/test/30Scenes.
3. --diff enables error map rendering in tmp/test/30Scenes.diff to visualize the reconstruction performance.

The result will be output to tmp/test/test_model_30Scenes.csv with PSNR, SSIM and running time for each sample:

sample,psnr,ssim,time
IMG_1085_eslf,44.03,0.9859,1.58
IMG_1086_eslf,46.95,0.9925,1.66
IMG_1184_eslf,44.04,0.9789,1.08
IMG_1187_eslf,43.77,0.9837,1.16

If you find our research helpful, please cite the paper.

@article{hu_TIM2021_SADenseNet,
  title={Efficient Light Field Reconstruction via Spatio-Angular Dense Network},
  author={Hu, Zexi and Yeung, Henry Wing Fung and Chen, Xiaoming and Chung, Yuk Ying and Li, Haisheng},
  journal={IEEE Transactions on Instrumentation and Measurement},
  volume={70},
  pages={1--14},
  year={2021},
  publisher={IEEE}
}