Training-Free Model Ensemble for Single-Image Super-Resolution via Strong-Branch Compensation
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Abstract (arXiv)
Single-image super-resolution has progressed from deep convolutional baselines to stronger Transformer and state-space architectures, yet the corresponding performance gains typically come with higher training cost, longer engineering iteration, and heavier deployment burden. In many practical settings, multiple pretrained models with partially complementary behaviors are already available, and the binding constraint is no longer architectural capacity but how effectively their outputs can be combined without additional training. Rather than pursuing further architectural redesign, this paper proposes a training-free output-level ensemble framework. A dual-branch pipeline is constructed in which a Hybrid attention network with TLC inference provides stable main reconstruction, while a MambaIRv2 branch with geometric self-ensemble supplies strong compensation for high-frequency detail recovery. The two branches process the same low-resolution input independently and are fused in the image space via a lightweight weighted combination, without updating any model parameters or introducing an additional trainable module. As our solution to the NTIRE 2026 Image Super-Resolution (× 4) Challenge, the proposed design consistently improves over the base branch and slightly exceeds the pure strong branch in PSNR at the best operating point under a unified DIV2K bicubic × 4 evaluation protocol. Ablation studies confirm that output-level compensation provides a low-overhead and practically accessible upgrade path for existing super-resolution systems.
Key facts. Cited by 6 papers in the map (data through 7 Oct 2026). Builds on 58 of its 76 references that are in the map. First posted on arXiv 13 Apr 2026.
Builds on
58 of 76 references.
References · 58
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38 more
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50 most cited of 58 All 58 (JSON)
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Citing papers per year: 2026: 6.
6 papers.
- 2026RAWild: Sensor-Agnostic RAW Object Detection via Physics-Guided Curve and Grid Modelingcited by 3
- 2026FluxFlow: Conservative Flow-Matching for Astronomical Image Super-Resolutioncited by 2
- 2026ELoG-GS: Dual-Branch Gaussian Splatting with Luminance-Guided Enhancement for Extreme Low-light 3D Reconstructioncited by 1
- 2026Dehaze-then-Splat: Generative Dehazing with Physics-Informed 3D Gaussian Splatting for Smoke-Free Novel View Synthesiscited by 1
- 2026FujinSplat: Seeing Through Smoke with RAW-Domain Gaussian Splattingcited by 0
- 2026ASTRA-SR: Atmospheric Seeing and Turbulence Restoration for Astronomical Image Super-Resolutioncited by 0
- 2026ASTRA-SR: Atmospheric Seeing and Turbulence Restoration for Astronomical Image Super-Resolution22 Sep 2026
- 2026FujinSplat: Seeing Through Smoke with RAW-Domain Gaussian Splatting5 Sep 2026
- 2026RAWild: Sensor-Agnostic RAW Object Detection via Physics-Guided Curve and Grid Modeling7 May 2026
- 2026FluxFlow: Conservative Flow-Matching for Astronomical Image Super-Resolution5 May 2026
- 2026Dehaze-then-Splat: Generative Dehazing with Physics-Informed 3D Gaussian Splatting for Smoke-Free Novel View Synthesis15 Apr 2026
- 2026ELoG-GS: Dual-Branch Gaussian Splatting with Luminance-Guided Enhancement for Extreme Low-light 3D Reconstruction14 Apr 2026