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co/datasets/ByteDance-Seed/Multi-SWE-bench"},"canonical_setting_json":{"kind":"string","value":"{\"higher_is_better\": true, \"judge\": \"execution-based patch validation\", \"metric_type\": \"pct\", \"multimodal_input\": false, \"notes\": \"Official sources are the ByteDance-Seed/Multi-SWE-bench HuggingFace dataset
from the top result below
https://huggingface.co/datasets/microsoft/benchpress-score-matrix
\", \"range\": [0, 100], \"sampling\": \"pass@1; public harness default maxTurns=20\", \"tools\": \"agentic MCP servers in the official containerized harness\", \"version\": \"MCP-Atlas public 500-task HuggingFace release\"}"},"in_paper_matrix":{"kind":"bool","value":true,"string":"true"}}},{"rowIdx":9,"cells":
https://huggingface.co/papers?q=reflective%20essays
Students\nlearn from teachers about the subject material, while teachers learn from\nstudents about how to refine their instruction
https://huggingface.co/papers?q=companion
The binary system with a hot companion (O-, B- and A-type star)\nis identified by detecting the ultraviolet (UV) excess in the observed spectral\nenergy distribution (SED) ranging from ultraviolet to mid-infrared after\nsubtracting the model SED of RSG since RSGs are very weak in the UV band