Showing 181–200 of 900 results
/ Date/ Name
Jun 6, 2025Astra: Toward General-Purpose Mobile Robots via Hierarchical Multimodal LearningJun 5, 2025MINT-CoT: Enabling Interleaved Visual Tokens in Mathematical Chain-of-Thought ReasoningJun 3, 2025Measurement of the branching fractions of the Cabibbo-favored decays $Λ_{c}^{+}\toΛK_{S}^{0}K^{+}$ and $Λ_{c}^{+}\toΞ^{0}K_{S}^{0}π^{+}$ and search for $Λ_{c}^{+}\toΣ^{0} K_{S}^{0}K^{+}$Jun 2, 2025EarthMind: Leveraging Cross-Sensor Data for Advanced Earth Observation Interpretation with a Unified Multimodal LLMMay 31, 2025Spectral Hardening Reveals Afterglow Emergence in Long-Duration Fast X-ray Transients: A Case Study of GRB 250404A/EP250404aMay 30, 2025Characterization of Hamamatsu R11410-23 Photomultiplier Tubes and Performance in the PandaX-4T DetectorMay 29, 2025Argus: Vision-Centric Reasoning with Grounded Chain-of-ThoughtMay 29, 2025The ambiguous AT2022rze: Changing-look AGN mimicking a supernova in a merging galaxy systemMay 28, 2025ForceVLA: Enhancing VLA Models with a Force-aware MoE for Contact-rich ManipulationMay 27, 2025Pangu Pro MoE: Mixture of Grouped Experts for Efficient SparsityMay 22, 2025NTIRE 2025 challenge on Text to Image Generation Model Quality AssessmentMay 21, 2025Hunyuan-TurboS: Advancing Large Language Models through Mamba-Transformer Synergy and Adaptive Chain-of-ThoughtMay 16, 2025GenoArmory: A Unified Evaluation Framework for Adversarial Attacks on Genomic Foundation ModelsMay 13, 2025Strain Induced Robust Skyrmion lattice at Room Temperature in van der Waals FerromagnetMay 12, 2025Why is the Star Formation Rate Proportional to Dense Gas Mass?May 11, 2025Seed1.5-VL Technical ReportMay 7, 2025Final Moments III: Explosion Properties and Progenitor Constraints of CSM-Interacting Type II SupernovaeMay 7, 2025Pangu Ultra MoE: How to Train Your Big MoE on Ascend NPUsMay 5, 2025Redshift Assessment Infrastructure Layers (RAIL): Rubin-era photometric redshift stress-testing and at-scale productionMay 5, 2025Measurement of the time-integrated $CP$ asymmetry in $D^0\toπ^0π^0$ decays at Belle II