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<h1> XAMI-model: XMM-Newton optical Artefact Mapping for astronomical Instance segmentation </h1>
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Check the **[XAMI model](https://github.com/ESA-Datalabs/XAMI-model)**
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## Model Checkpoints
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| Model Name | Link |
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| YOLOv8 |[yolov8_segm](https://huggingface.co/iulia-elisa/XAMI/blob/main/yolo_weights/best.pt) |
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| MobileSAM |[sam_vit](https://huggingface.co/iulia-elisa/XAMI/blob/main/sam_weights/sam_0_best.pth) |
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| XAMI |[xami_model](https://huggingface.co/iulia-elisa/XAMI/blob/main/yolo_sam_final.pth) |
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## 💫 Introduction
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The code uses images from the XAMI dataset (available on [Github](https://github.com/ESA-Datalabs/XAMI-dataset) and [HuggingFace🤗](https://huggingface.co/datasets/iulia-elisa/XAMI-dataset)). The images represent observations from the XMM-Newton's Opical Monitor (XMM-OM). Information about the XMM-OM can be found here:
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<h1> XAMI-model: XMM-Newton optical Artefact Mapping for astronomical Instance segmentation </h1>
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</div>
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🚀 Check the **[XAMI model](https://github.com/ESA-Datalabs/XAMI-model)** which uses this dataset.
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<!-- ## Model Checkpoints
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| Model Name | Link |
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| YOLOv8 |[yolov8_segm](https://huggingface.co/iulia-elisa/XAMI/blob/main/yolo_weights/best.pt) |
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| MobileSAM |[sam_vit](https://huggingface.co/iulia-elisa/XAMI/blob/main/sam_weights/sam_0_best.pth) |
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| XAMI |[xami_model](https://huggingface.co/iulia-elisa/XAMI/blob/main/yolo_sam_final.pth) |
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-->
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## 💫 Introduction
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The code uses images from the XAMI dataset (available on [Github](https://github.com/ESA-Datalabs/XAMI-dataset) and [HuggingFace🤗](https://huggingface.co/datasets/iulia-elisa/XAMI-dataset)). The images represent observations from the XMM-Newton's Opical Monitor (XMM-OM). Information about the XMM-OM can be found here:
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