Instructions to use nvidia/RADIO with libraries, inference providers, notebooks, and local apps. Follow these links to get started.
- Libraries
- Transformers
How to use nvidia/RADIO with Transformers:
# Use a pipeline as a high-level helper from transformers import pipeline pipe = pipeline("image-feature-extraction", model="nvidia/RADIO", trust_remote_code=True)# Load model directly from transformers import AutoModel model = AutoModel.from_pretrained("nvidia/RADIO", trust_remote_code=True, dtype="auto") - Notebooks
- Google Colab
- Kaggle
| {} | |
| # AM-RADIO: Reduce All Domains Into One | |
| Mike Ranzinger, Greg Heinrich, Jan Kautz, Pavlo Molchanov | |
| [NVIDIA Research](https://www.nvidia.com/en-us/research/) | |
| \[[Paper](https://arxiv.org/abs/2312.06709)\]\[[BibTex](#citing-radio)\] | |
| ## Pretrained Models | |
| Refer to `model_results.csv` for model versions and their metrics. | |
| ### HuggingFace Hub | |
| In order to pull the model from HuggingFace, you need to be logged in: | |
| ```Bash | |
| huggingface-cli login | |
| ``` | |
| Then you can pull the model from a Python script: | |
| ```Python | |
| from transformers import AutoModel | |
| model = AutoModel.from_pretrained("nvidia/RADIO", trust_remote_code=True) | |
| ``` | |
| Alternatively, you can specify an access token: | |
| ```Python | |
| access_token = "<YOUR ACCESS TOKEN" | |
| model = AutoModel.from_pretrained("nvidia/RADIO", trust_remote_code=True, token=access_token) | |
| ``` | |
| ### Usage | |
| RADIO will return a tuple with two tensors. The `summary` is similar to the `cls_token` in ViT and is meant to represent the general concept of the entire image. It has shape $(B,C)$ with $B$ being the batch dimension, and $C$ being some number of channels. The `spatial_features` represent more localized content which should be suitable for dense tasks such as semantic segmentation, or for integration into an LLM. It has shape $(B,T,D)$ with $T$ being the flattened spatial tokens, and $D$ being the channels for spatial features. Note that $C \neq D$ in general. | |
| Converting to a spatial tensor format can be done using the downsampling size of the model, combined with the input tensor shape. For 'radio_v1', the patch size is 14. | |
| ```Python | |
| from einops import rearrange | |
| spatial_features = rearrange(spatial_features, 'b (h w) d -> b d h w', h=x.shape[-2] // patch_size, w=x.shape[-1] // patch_size) | |
| ``` | |
| The resulting tensor will have shape $(B,D,H,W)$, as is typically seen with computer vision models. | |
| ### RADIOv1 Notes | |
| We have trained this model to be flexible in input dimension. It supports inputs with both width and height in the range $[14, 1008]$ as long as both axes are divisible by 14. We have found that summarization tokens work best at $H=W=378$ (although the range $[192, 448]$ works well). For spatial tasks, we used $H=W=518$ to perform linear probing for semantic segmentation, and may perform better for more high-resolution tasks. Going up to $1008$, the model may need additional fine tuning at that resolution for best results. | |
| It is not required that $H=W$ although we have not specifically trained or testing the model in this setting. | |
| ## Training | |
| _Coming Soon_ | |
| ## License | |
| RADIO code and weights are released under the [NSCLv1 License](LICENSE). | |
| ## Citing RADIO | |
| If you find this repository useful, please consider giving a star and citation: | |
| ``` | |
| @misc{ranzinger2023amradio, | |
| title={AM-RADIO: Agglomerative Model -- Reduce All Domains Into One}, | |
| author={Mike Ranzinger and Greg Heinrich and Jan Kautz and Pavlo Molchanov}, | |
| year={2023}, | |
| eprint={2312.06709}, | |
| archivePrefix={arXiv}, | |
| primaryClass={cs.CV} | |
| } | |
| ``` |