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--- |
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license: openrail++ |
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language: |
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- en |
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tags: |
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- stable-diffusion |
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- stable-diffusion-diffusers |
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- text-to-image |
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widget: |
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- text: "Hubble snaps images of the birthplace of stars within a cluster: The dust and gas expand within the cluster due to the powerful influence of baby stars. With these new images comes improved detail and a clearer view for astronomers to study how early stars are born and change over time." |
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example_title: Baby Stars |
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- text: "Hubble captures the death of a star: Old stars, nearing the end of their life, collapse under the weight of their own gravity and the outer layers explode as a 'supernova'. In this image Hubble captures the moments after collapse, where the star has exploded and left an empty void in its place, where a new black hole has emerged." |
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example_title: Old Stars |
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- text: "Hubble image of galaxies colliding: The distorted spirals of two distant galaxies colliding are captured here in a new image from the NASA/ESA Hubble Space Telescope. The typically symmetric spirals common in spiral galaxies appear significantly warped, as the shape of both galaxies is torn apart by their gravitational pulls." |
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example_title: Galaxies Collide |
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- text: "Pink-tinted plumes in the Large Magellanic Cloud: The aggressively pink plumes seen in this image are extremely uncommon, with purple-tinted currents and nebulous strands reaching out into the surrounding space." |
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example_title: Pink Plumes |
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- text: "The stellar plasma of Wolf 359: The red dwarf star Wolf 359 from the constellation Leo is captured in extreme detail in a new image from the NASA/ESA Hubble Space Telescope. Wolf 359, classified as a M6 red dwarf, has certain peculiar qualities indicated by an unusual ejection of plasma. The Hubble telescope was able to capture one such event" |
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example_title: Wolf 359 |
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thumbnail: "" |
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inference: true |
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datasets: |
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- Supermaxman/esa-hubble |
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--- |
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# Hubble Diffusion v2: Stable Diffusion v2.1 fine tuned on ESA Hubble Deep Space Images & Captions |
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Put in a detailed text prompt and generate high-quality Hubble Deep Space Images! Now with Stable Diffusion 2.1! |
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> Hubble captures the death of a star: Old stars, nearing the end of their life, collapse under the |
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> weight of their own gravity and the outer layers explode as a 'supernova'. In this image Hubble |
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> captures the moments after collapse, where the star has exploded and left an empty void in its |
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> place, where a new black hole has emerged. |
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![old.png](https://github.com/Supermaxman/HubbleDiffuser/blob/f0020b338dc13adfbac9b9e2dfa647a37df5026a/examples/hubble-diffusion-2/old.png?raw=true) |
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> Pink-tinted plumes in the Large Magellanic Cloud: |
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> The aggressively pink plumes seen in this image are extremely uncommon, |
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> with purple-tinted currents and nebulous strands reaching out into the surrounding space. |
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![pink.png](https://github.com/Supermaxman/HubbleDiffuser/blob/f0020b338dc13adfbac9b9e2dfa647a37df5026a/examples/hubble-diffusion-2/pink.png?raw=true) |
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> Hubble snaps images of the birthplace of stars within a cluster: |
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> The dust and gas expand within the cluster due to the powerful influence of baby stars. |
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> With these new images comes improved detail and a clearer view for astronomers to |
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> study how early stars are born and change over time. |
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![baby.png](https://github.com/Supermaxman/HubbleDiffuser/blob/f0020b338dc13adfbac9b9e2dfa647a37df5026a/examples/hubble-diffusion-2/baby.png?raw=true) |
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> Hubble image of galaxies colliding: The distorted spirals of two distant galaxies colliding are |
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> captured here in a new image from the NASA/ESA Hubble Space Telescope. The typically symmetric |
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> spirals common in spiral galaxies appear significantly warped, as the shape of both galaxies is torn |
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> apart by their gravitational pulls. |
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![collide.png](https://github.com/Supermaxman/HubbleDiffuser/blob/f0020b338dc13adfbac9b9e2dfa647a37df5026a/examples/hubble-diffusion-2/collide.png?raw=true) |
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> The stellar plasma of Wolf 359: The red dwarf star Wolf 359 from the constellation Leo is captured in extreme detail in a new image from the NASA/ESA Hubble Space Telescope. |
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> Wolf 359, classified as a M6 red dwarf, has certain peculiar qualities indicated by an unusual ejection of plasma. The Hubble telescope was able to capture one such event |
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![wolf359.png](https://github.com/Supermaxman/HubbleDiffuser/blob/f0020b338dc13adfbac9b9e2dfa647a37df5026a/examples/hubble-diffusion-2/wolf359.png?raw=true) |
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## Model Details |
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- **Developed by:** Maxwell Weinzierl |
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- **Model type:** Diffusion-based text-to-image generation model |
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- **Language(s):** English |
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- **License:** [CreativeML Open RAIL++-M License](https://huggingface.co/stabilityai/stable-diffusion-2/blob/main/LICENSE-MODEL) |
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- **Model Description:** This is a model that can be used to generate and modify images based on text prompts. It is a [Latent Diffusion Model](https://arxiv.org/abs/2112.10752) that uses a fixed, pretrained text encoder ([OpenCLIP-ViT/H](https://github.com/mlfoundations/open_clip)). |
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- **Resources for more information:** [GitHub Repository](https://github.com/Stability-AI/). |
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- **Cite as:** |
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@misc{weinzierl2023sdhubble2, |
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author = {Weinzierl, Maxwell A.}, |
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title = {Hubble Diffusion v2: Stable Diffusion v2.1 fine tuned on ESA Hubble Deep Space Images & Captions}, |
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year={2023}, |
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howpublished= {\url{https://huggingface.co/Supermaxman/hubble-diffusion-2}} |
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} |
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Also, be sure to check out the prior version [Hubble Diffusion v1](https://huggingface.co/Supermaxman/hubble-diffusion-1)! |
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## Examples |
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We recommend using [🤗's Diffusers library](https://github.com/huggingface/diffusers) to run Hubble Diffusion. |
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### Usage |
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```bash |
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pip install transformers diffusers accelerate |
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``` |
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```python |
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import torch |
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from diffusers import StableDiffusionPipeline |
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model_id = "Supermaxman/hubble-diffusion-2" |
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pipe = StableDiffusionPipeline.from_pretrained(model_id, torch_dtype=torch.float16) |
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pipe = pipe.to("cuda") |
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# saves significant GPU memory for small inference cost |
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pipe.enable_attention_slicing() |
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prompt = "Hubble snaps images of the birthplace of stars within a cluster: The dust and gas expand within the cluster due to the powerful influence of baby stars. With these new images comes improved detail and a clearer view for astronomers to study how early stars are born and change over time." |
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image = pipe(prompt).images[0] |
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image |
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``` |
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![example.png](https://github.com/Supermaxman/HubbleDiffuser/blob/f0020b338dc13adfbac9b9e2dfa647a37df5026a/examples/hubble-diffusion-2/example.png?raw=true) |
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## Model description |
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Trained on [ESA Hubble Deep Space Images & Captions](https://huggingface.co/datasets/Supermaxman/esa-hubble) using [Google Colab Pro](https://colab.research.google.com/signup) with a single A100 GPU for around 33,000 steps (about 12 hours, at a cost of about $20). |
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## Links |
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- [Captioned Hubble Deep Space Scans dataset](https://huggingface.co/datasets/Supermaxman/esa-hubble) |
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- [Model weights in Diffusers format](https://huggingface.co/Supermaxman/hubble-diffusion-2) |
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- [Training code](https://github.com/Supermaxman/HubbleDiffuser) |
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- [Hubble Diffusion v1](https://huggingface.co/Supermaxman/hubble-diffusion-1) |
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Trained by [Maxwell Weinzierl](https://personal.utdallas.edu/~maxwell.weinzierl/) ([@Supermaxman1](https://twitter.com/Supermaxman1)). |
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## Citation |
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```bibtex |
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@misc{weinzierl2023sdhubble2, |
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author = {Weinzierl, Maxwell A.}, |
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title = {Hubble Diffusion v2: Stable Diffusion v2.1 fine tuned on ESA Hubble Deep Space Images & Captions}, |
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year={2023}, |
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howpublished= {\url{https://huggingface.co/Supermaxman/hubble-diffusion-2}} |
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} |
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``` |
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