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Code for paper "From Crowd to Herd Counting: How to Precisely Detect and Count African Mammals using Aerial Imagery and Deep Learning?"

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HerdNet

License: MIT Open In Colab

Code for paper "From Crowd to Herd Counting: How to Precisely Detect and Count African Mammals using Aerial Imagery and Deep Learning?"

Model Architecture

Detection Examples

License

HerdNet is available under the MIT License and is thus open source and freely available. For a complete list of package dependencies with copyright and license info, please look at the file packages.txt

Citation

If you use this code in your work, please cite our paper:

@article{
    title = {From crowd to herd counting: How to precisely detect and count African mammals using aerial imagery and deep learning?},
    journal = {ISPRS Journal of Photogrammetry and Remote Sensing},
    volume = {197},
    pages = {167-180},
    year = {2023},
    issn = {0924-2716},
    doi = {https://doi.org/10.1016/j.isprsjprs.2023.01.025},
    url = {https://www.sciencedirect.com/science/article/pii/S092427162300031X},
    author = {Alexandre Delplanque and Samuel Foucher and Jérôme Théau and Elsa Bussière and Cédric Vermeulen and Philippe Lejeune}
    }

Pretrained Models

Models were trained separatly for each of the two datasets. These pre-trained models follow the (CC BY-NC-SA-4.0) license and are available for academic research purposes only, no commercial use is permitted.

Model Params Dataset Environment Species F1score MAE¹ RMSE² AC³ Download
HerdNet 18M Ennedi 2019 Desert, xeric shrubland and grassland Camel, donkey, sheep and goat 73.6% 6.1 9.8 15.8% PTH file
HerdNet 18M Delplanque et al. (2022) Tropical forest, savanna, tropical shrubland and grassland Buffalo, elephant, kob, topi, warthog, waterbuck 83.5% 1.9 3.6 7.8% PTH file

¹MAE, Mean Absolute Error; ²RMSE, Root Mean Square Error; ³AC, Average Confusion between species.

Note that these metrics have been computed on full-size test images.

Installation

Create and activate the conda environment

conda env create -f environment.yml
conda activate herdnet

Install the code

python setup.py install

Create a Weights & Biases account and then log in

wandb login

Dataset Format

A CSV file which must contain the header images,x,y,labels for points, or images,x_min,y_min,x_max,y_max,y,labels for bounding boxes. Each row should represent one annotation, with at least, the image name (images), the object location within the image (x, y) for points, and (x_min, y_min, x_max, y_max) for bounding boxes and its label (labels):

Point dataset:

images,x,y,labels
Example.JPG,517,1653,2
Example.JPG,800,1253,1
Example.JPG,78,33,3
Example_2.JPG,896,742,1
...

Bounding box dataset:

images,x_min,y_min,x_max,y_max,labels
Example.JPG,530,1458,585,1750,4
Example.JPG,95,1321,152,1403,2
Example.JPG,895,478,992,658,1
Example_2.JPG,47,253,65,369,1
...

An image containing n objects is therefore spread over n lines.

Quick Start

Open In Colab

Set the seed for reproducibility

from animaloc.utils.seed import set_seed

set_seed(9292)

Create point datasets

import albumentations as A

from animaloc.datasets import CSVDataset
from animaloc.data.transforms import MultiTransformsWrapper, DownSample, PointsToMask, FIDT

patch_size = 512
num_classes = 4
down_ratio = 2

train_dataset = CSVDataset(
    csv_file = '/path/to/train/data.csv',
    root_dir = '/path/to/train/data',
    albu_transforms = [
        A.VerticalFlip(p=0.5), 
        A.Normalize(p=1.0)
        ],
    end_transforms = [MultiTransformsWrapper([
        FIDT(num_classes=num_classes, down_ratio=down_ratio),
        PointsToMask(radius=2, num_classes=num_classes, squeeze=True, down_ratio=int(patch_size//16))
        ])]
    )

val_dataset = CSVDataset(
    csv_file = '/path/to/val/data.csv',
    root_dir = '/path/to/val/data',
    albu_transforms = [A.Normalize(p=1.0)],
    end_transforms = [DownSample(down_ratio=down_ratio, anno_type='point')]
    )

Create dataloaders

from torch.utils.data import DataLoader

train_dataloader = DataLoader(
    dataset = train_dataset,
    batch_size = 4,
    shuffle = True
    )

val_dataloader = DataLoader(
    dataset = val_dataset,
    batch_size = 1,
    shuffle = False
    )

Instanciate HerdNet

from animaloc.models import HerdNet

herdnet = HerdNet(num_classes=num_classes, down_ratio=down_ratio).cuda()

Define the losses for training HerdNet

from torch import Tensor
from animaloc.models import LossWrapper
from animaloc.train.losses import FocalLoss
from torch.nn import CrossEntropyLoss

weight = Tensor([0.1, 1.0, 1.0, 1.0]).cuda()

losses = [
    {'loss': FocalLoss(reduction='mean'), 'idx': 0, 'idy': 0, 'lambda': 1.0, 'name': 'focal_loss'},
    {'loss': CrossEntropyLoss(reduction='mean', weight=weight), 'idx': 1, 'idy': 1, 'lambda': 1.0, 'name': 'ce_loss'}
    ]

herdnet = LossWrapper(herdnet, losses=losses)

Train et validate HerdNet

from torch.optim import Adam
from animaloc.train import Trainer
from animaloc.eval import PointsMetrics, HerdNetStitcher, HerdNetEvaluator

work_dir = 'path/to/working/directory'

lr = 1e-4
weight_decay = 1e-3
epochs = 100

optimizer = Adam(params=herdnet.parameters(), lr=lr, weight_decay=weight_decay)

metrics = PointsMetrics(radius=5, num_classes=num_classes)

stitcher = HerdNetStitcher(
    model=herdnet, 
    size=(patch_size,patch_size), 
    overlap=160, 
    down_ratio=down_ratio, 
    reduction='mean'
    )

evaluator = HerdNetEvaluator(
    model=herdnet, 
    dataloader=val_dataloader, 
    metrics=metrics, 
    stitcher=stitcher, 
    work_dir=work_dir, 
    header='validation'
    )

trainer = Trainer(
    model=herdnet,
    train_dataloader=train_dataloader,
    optimizer=optimizer,
    num_epochs=epochs,
    evaluator=evaluator,
    work_dir=work_dir
    )

trainer.start(warmup_iters=100, checkpoints='best', select='max', validate_on='f1_score')

Use pretrained model

from animaloc.models import HerdNet, LossWrapper, load_model

herdnet = HerdNet(num_classes=4, down_ratio=2)
herdnet = LossWrapper(herdnet, losses=[])
herdnet = load_model('path/to/the/file.pth')

Tools

Creating Patches

To train a model, such as HerdNet, it is often useful to extract patches from the original full-size images, especially if you have a GPU with limited memory. To do so, you can use the patcher.py tool:

python tools/patcher.py root height width overlap dest [-csv] [-min] [-all]

For help, run:

python tools/patcher.py -h

Starting a Training Session

A training session can easily be launched using the train.py tool. This tool uses Hydra framework. You simply need to modify the basic config file and then run:

python tools/train.py

You can also create your own config file. Save it first into the configs/train folder and then run:

python tools/train.py train=<your config name>

Click here to see how to write a training config file.

You can also make multiple different configurations runs or modify some parameters directly from the command line (see the doc).

Starting a Testing Session

A testing session can easily be launched using the test.py tool. This tool uses Hydra framework again. You simply need to modify the basic config file and then run:

python tools/test.py

You can also create your own config file. Save it first into the configs/test folder and then run:

python tools/test.py test=<your config name>

Click here to see how to write a testing config file.

Visualizing Ground Truth (and Detections)

You can view your ground truth and your model's detections by using the view.py tool. This tool uses FiftyOne. You simply need to specify a root directory that contains your images (root), your CSV file containing the ground truth (gt) and optionaly a CSV file containing model's detections (-dets). See dataset format below for your CSV files format.

python tools/view.py root gt [-dets]

Making Inference with a PTH File

You can get HerdNet detections from new images using the infer.py tool. To use it, you will need a .pth file obtained using this code, which also contains the label-species correspondence (classes) as well as the mean (mean) and std (std) values for normalization (see the code snippet below to add this information in your .pth file). This tool exports the detections in .csv format, the plots of the detections on the images, and thumbnails of the detected animals. All this is saved in the same folder as the one containing the images (i.e. -root). You can adjust the size of the thumbnails by changing the -ts argument (defaults to 256), the frequency of the prints by changing the -pf argument (defaults to 10), as well as the computing device by changing the -device argument (defaults to cuda).

python tools/infer.py root pth [-ts] [-pf] [-device]

For help, run:

python tools/infer.py -h

Code snippet to add the required information in the pth file:

import torch

pth_file = torch.load('path/to/the/file.pth')
pth_file['classes'] = {1:'species_1', 2:'species_2', ...}
pth_file['mean'] = [0.485, 0.456, 0.406]
pth_file['std'] = [0.229, 0.224, 0.225] 
torch.save(pth_file, 'path/to/the/file.pth')

Colab Demo

Here is a Google Colab demo based on the UAV nadir dataset used in the paper:

Delplanque, A., Foucher, S., Lejeune, P., Linchant, J. and Théau, J. (2022), Multispecies detection and identification of African mammals in aerial imagery using convolutional neural networks. Remote Sens Ecol Conserv, 8: 166-179. https://doi.org/10.1002/rse2.234.

Code Versioning

The code used in the paper is the one corresponding to the tag v0.1.0. The 'main' branch contains the latest stable version with fixed bugs and new features, it is recommended to use this branch for your development. The file CHANGELOG.md contains the details of the commits for each version of the code.

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Code for paper "From Crowd to Herd Counting: How to Precisely Detect and Count African Mammals using Aerial Imagery and Deep Learning?"

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