2D Gaussian Splatting
Reconstructs a real photograph with anisotropic 2D Gaussians (with densification) — the 2D analogue of 3D Gaussian Splatting.
Trained from scratch in Ropedia Academy — an interactive, bilingual course on embodied & spatial AI. Educational model: small and quick to train; the value is the method and a reproducible pipeline, not a leaderboard score. Try it live in the Ropedia demos Space.
At a glance
| Base model | Trained from scratch (random initialization) — no pretrained base model. |
| Task | differentiable image fitting |
| Training objective | Photometric L2 between the splatted render and the target image, with gradient-based densification. |
| Track | B · 3D & rendering |
| Notebook |
Dataset
- Name: Real photograph (astronaut)
- Type: real — public-domain image
- Size / stats: 1 RGB photo resized to 64×64; ~500 Gaussians (densified to ~650)
- Split: single image (overfit)
- Source: scikit-image data.astronaut() (NASA, public domain)
Training config
Adam (lr 0.02), 800 steps; 500 Gaussians, gradient-based densification (→ ~650); 64×64 target.
Evaluation results
| metric | value | meaning |
|---|---|---|
psnr (final) |
32.45 |
Inference example
import torch
g = torch.load("gaussians.pt", map_location="cpu") # dict: pos, logs, rot, col, op
# Re-create render() from the notebook (see "Reproduce") and call it on these tensors
# to reconstruct the fitted image.
Limitations
Educational scale. Trained quickly on CPU on small or synthetic data, so absolute numbers are not competitive with production systems — the value is the method and a reproducible pipeline. No large-scale data, no hyperparameter sweep, and no multi-seed variance is reported. Not for production use.
Overfits a single image — it does not generalize to other images; quality is capped by the Gaussian count.
Failure cases
Without densification, large flat regions stay blurry; over-large σ washes the image out.
Reproduce / train your own
One click: open the notebook in Colab → Runtime → GPU → Run all, then run its Publish to the Hugging Face Hub cell.
From a shell:
git clone https://github.com/ChaoYue0307/ropedia-academy.git && cd ropedia-academy
pip install torch numpy matplotlib scikit-learn scikit-image gymnasium
jupyter nbconvert --to notebook --execute notebooks/training/B_gaussian_splatting_2d.ipynb --output run.ipynb
# optional: override training length, e.g. STEPS=2000 (or EPISODES=600) before running
Files
figure.pnggaussians.ptmetrics.json
License
Code & weights: MIT (this repository) — educational use encouraged.
Image: astronaut test image (NASA) — public domain, shipped with scikit-image.
Citation
If you use this model or the course materials, please cite:
@misc{ropedia_academy,
title = {Ropedia Academy: an interactive course on embodied & spatial AI},
author = {Ropedia Academy},
year = {2026},
howpublished = {\url{https://chaoyue0307.github.io/ropedia-academy/}}
}
Method / original work: Kerbl et al., 3D Gaussian Splatting for Real-Time Radiance Field Rendering, SIGGRAPH 2023.
Related assets
- 🚀 Live demos: https://huggingface.co/spaces/cy0307/ropedia-demos
- 🤗 All trained models + collection: https://huggingface.co/cy0307
- 📚 Course & all labs: https://chaoyue0307.github.io/ropedia-academy/ · Labs tab
- 💻 Source / notebooks: github.com/ChaoYue0307/ropedia-academy
Part of the Ropedia Academy trained-model collection. Contributions & issues welcome on GitHub.