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Yandu Sun

dblp:402/4171 · DBLP profile ↗
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2ranked-venue papers
0as first author
2since 2021 · last 2026
—ORCID · none

Domains — the database's venue-derived domains; a paper can count in several

Artificial intelligence and machine learning · 2 · 2 since 2021Graphics, computer vision, multimedia, augmented reality and games · 1 · 1 since 2021

Expertise — from the expertise taxonomy: the topics of the expert's papers under the CCF categories. A weight counts papers with recency: 1 for a paper about the topic, 0.3 when the topic is its context, halved every five years.

Artificial intelligence
2 papers
3D vision · 29% Learning paradigms · 17% Language models and text generation · 17%
Computer graphics and multimedia
1 paper
Rendering · 100%

Topics — the 8 heaviest of 8, each with the papers that count most for it

TopicWeightPapersLastEvidence papers
Natural language and speech › Language models and text generation › instruction tuning
continual instruction tuning
1.012026
PASs-MoE: Mitigating Misaligned Co-drift among Router and Experts via Pathway Activation Subspaces for Continual Learning · ACL (1) 2026
Machine learning › Learning paradigms
continual learning
1.012026
PASs-MoE: Mitigating Misaligned Co-drift among Router and Experts via Pathway Activation Subspaces for Continual Learning · ACL (1) 2026
Machine learning › Efficient and distributed learning › parameter-efficient fine-tuning
LoRA mixture of experts
1.012026
PASs-MoE: Mitigating Misaligned Co-drift among Router and Experts via Pathway Activation Subspaces for Continual Learning · ACL (1) 2026
Machine learning › Deep learning architectures and training
mixture of experts
1.012026
PASs-MoE: Mitigating Misaligned Co-drift among Router and Experts via Pathway Activation Subspaces for Continual Learning · ACL (1) 2026
Computer vision › 3D vision
novel view synthesis
0.912025
NexusGS: Sparse View Synthesis with Epipolar Depth Priors in 3D Gaussian Splatting · CVPR 2025
Computer vision › 3D vision › novel view synthesis
sparse view synthesis
0.912025
NexusGS: Sparse View Synthesis with Epipolar Depth Priors in 3D Gaussian Splatting · CVPR 2025
Rendering › gaussian splatting
3d gaussian splatting
0.912025
NexusGS: Sparse View Synthesis with Epipolar Depth Priors in 3D Gaussian Splatting · CVPR 2025
Computer vision › Vision and language › vision-language model
multimodal large language model
0.312026
PASs-MoE: Mitigating Misaligned Co-drift among Router and Experts via Pathway Activation Subspaces for Continual Learning · ACL (1) 2026

Methods — techniques the papers use, named apart from their topics

optical flow · 1.7epipolar depth priors · 1.7depth blending · 1.7pathway activation subspace · 1.0mixture of experts · 1.0LoRA · 1.0
YearPublicationVenuePosition
2026 PASs-MoE: Mitigating Misaligned Co-drift among Router and Experts via Pathway Activation Subspaces for Continual Learning
abstract
Continual instruction tuning (CIT) requires multimodal large language models (MLLMs) to adapt to a stream of tasks without forgetting prior capabilities.A common strategy is to isolate updates by routing inputs to different LoRA experts.However, existing LoRAbased Mixture-of-Experts (MoE) methods often jointly update the router and experts in an indiscriminate way, causing the router's preferences to co-drift with experts' adaptation pathways and gradually deviate from early-stage input-expert specialization.We term this as Misaligned Co-drift, which blurs expert responsibilities and exacerbates forgetting.To address this, we introduce the pathway activation subspace (PASs), a LoRA-induced subspace that reflects which low-rank pathway directions an input activates in each expert, providing a capability-aligned coordinate system for routing and preservation.Based on PASs, we propose a fixed-capacity PASsbased MoE-LoRA method with two components: PAS-guided Reweighting, which calibrates routing using each expert's pathway activation signals, and PAS-aware Rank Stabilization, which selectively stabilizes rank directions important to previous tasks.Experiments on a CIT benchmark show that our approach consistently outperforms a range of conventional continual learning baselines and MoE-LoRA variants in both accuracy and antiforgetting without adding parameters.Our code is publicly available at https://github.com/ yueluoshuangtian/PASs-MoE.
ZhiYan Hou, Haiyun Guo, Haokai Ma, Yandu Sun, Jinqiao Wang
ACL (1)4
2025 NexusGS: Sparse View Synthesis with Epipolar Depth Priors in 3D Gaussian Splatting
abstract
Neural Radiance Field (NeRF) and 3D Gaussian Splatting (3DGS) have noticeably advanced photo-realistic novel view synthesis using images from densely spaced camera viewpoints. However, these methods struggle in few-shot scenarios due to limited supervision. In this paper, we present NexusGS, a 3DGS-based approach that enhances novel view synthesis from sparse-view images by directly embedding depth information into point clouds, without relying on complex manual regularizations. Exploiting the inherent epipolar geometry of 3DGS, our method introduces a novel point cloud densification strategy that initializes 3DGS with a dense point cloud, reducing randomness in point placement while preventing over-smoothing and overfitting. Specifically, NexusGS comprises three key steps: Epipolar Depth Nexus, Flow-Resilient Depth Blending, and Flow-Filtered Depth Pruning. These steps leverage optical flow and camera poses to compute accurate depth maps, while mitigating the inaccuracies often associated with optical flow. By incorporating epipolar depth priors, NexusGS ensures reliable dense point cloud coverage and supports stable 3DGS training under sparse-view conditions. Experiments demonstrate that NexusGS significantly enhances depth accuracy and rendering quality, surpassing state-of-the-art methods by a considerable margin. Furthermore, we validate the superiority of our generated point clouds by substantially boosting the performance of competing methods. Project page: https://usmizuki.github.io/NexusGS/.
Yulong Zheng, Zicheng Jiang, Shengfeng He, Yandu Sun, Junyu Dong, Huaidong Zhang, Yong Du 0003
CVPR4