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nasa-v3-mmlupro-10097 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 10097 | licensed_benchmark_import | mmlu-pro:test:10097 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "How do scientists know that the majority of meteorites come from the asteroid belt?", "context": [], "choices": {"A": "The spectra of some meteorites are similar to the spectra of asteroids in the asteroid belt.", "B": "The chemical composition of meteorites is identical to the composition of asteroids from... | {"checks": [{"path": "answer", "kind": "exact", "expected": "A", "critical": true, "weight": 1}], "reference_response": {"answer": "A"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "10097", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/... | {} |
nasa-v3-mmlupro-10100 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 10100 | licensed_benchmark_import | mmlu-pro:test:10100 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Suppose you live on the Moon. How long is a day (i.e. from sunrise to sunrise)?", "context": [], "choices": {"A": "12 Earth hours", "B": "365 Earth days", "C": "about 18 years", "D": "48 Earth hours", "E": "1 Earth hour", "F": "a year", "G": "24 hours", "H": "7 Earth days", "I": "about 50 years", "J": "29 E... | {"checks": [{"path": "answer", "kind": "exact", "expected": "J", "critical": true, "weight": 1}], "reference_response": {"answer": "J"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "10100", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/... | {} |
nasa-v3-mmlupro-10102 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 10102 | licensed_benchmark_import | mmlu-pro:test:10102 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "The distance between the Earth and the star Altair is one million times greater than the distance between the Earth and the Sun. How far is Altair from the Earth?", "context": [], "choices": {"A": "9.3 x 1010 meters", "B": "1.5 x 1014 meters", "C": "1.5 x 1013 meters", "D": "9.3 x 1017 meters", "E": "9.3 x ... | {"checks": [{"path": "answer", "kind": "exact", "expected": "J", "critical": true, "weight": 1}], "reference_response": {"answer": "J"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "10102", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/... | {} |
nasa-v3-mmlupro-10208 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 10208 | licensed_benchmark_import | mmlu-pro:test:10208 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "When traveling north from the United States into Canada you’ll see the North Star (Polaris) getting _________.", "context": [], "choices": {"A": "Higher in the sky", "B": "More to the East", "C": "Closer", "D": "Changing color", "E": "More to the West", "F": "Further away", "G": "Brighter", "H": "Lower in t... | {"checks": [{"path": "answer", "kind": "exact", "expected": "A", "critical": true, "weight": 1}], "reference_response": {"answer": "A"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "10208", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/... | {} |
nasa-v3-mmlupro-10211 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 10211 | licensed_benchmark_import | mmlu-pro:test:10211 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "What element is most common among the Jovian Planets?", "context": [], "choices": {"A": "Neon", "B": "Nitrogen", "C": "Helium", "D": "Carbon", "E": "Argon", "F": "Methane", "G": "Oxygen", "H": "Silicon", "I": "Hydrogen", "J": "Iron"}, "response_schema": {"type": "object", "properties": {"answer": {"type": "... | {"checks": [{"path": "answer", "kind": "exact", "expected": "I", "critical": true, "weight": 1}], "reference_response": {"answer": "I"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "10211", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/... | {} |
nasa-v3-mmlupro-10295 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 10295 | licensed_benchmark_import | mmlu-pro:test:10295 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "You observe the visible spectrum of a star viewed through a cloud of cool hydrogen gas.", "context": [], "choices": {"A": "You see the star’s blackbody spectrum with emission lines due to hydrogen.", "B": "You see only the star’s blackbody spectrum.", "C": "You see only emission lines characteristic of heli... | {"checks": [{"path": "answer", "kind": "exact", "expected": "G", "critical": true, "weight": 1}], "reference_response": {"answer": "G"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "10295", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/... | {} |
nasa-v3-mmlupro-9044 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9044 | licensed_benchmark_import | mmlu-pro:test:9044 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "What is the significance of the 1:2:4 resonance in the Jupiter's moons system?", "context": [], "choices": {"A": "It causes the three moons to always be in a straight line.", "B": "It causes Io to rotate on its axis faster than it orbits Jupiter", "C": "It creates a gap with no asteriods between the orbits.... | {"checks": [{"path": "answer", "kind": "exact", "expected": "I", "critical": true, "weight": 1}], "reference_response": {"answer": "I"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9044", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9045 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9045 | licensed_benchmark_import | mmlu-pro:test:9045 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "We were first able to accurately measure the diameter of Pluto from:", "context": [], "choices": {"A": "Lunar-based observations made during NASA's Apollo missions", "B": "The Voyager 2 spacecraft flyby in the 1980s", "C": "Observations made by the Chandra X-ray Observatory", "D": "brightness measurements m... | {"checks": [{"path": "answer", "kind": "exact", "expected": "D", "critical": true, "weight": 1}], "reference_response": {"answer": "D"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9045", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9046 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9046 | licensed_benchmark_import | mmlu-pro:test:9046 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "What about asteroids makes them stand out in sky surveys searching for them?", "context": [], "choices": {"A": "They reflect enough of the sun's light to make them brighter than most background stars", "B": "Asteroids rotate at a high speed, making them stand out", "C": "Asteroids are larger than most celes... | {"checks": [{"path": "answer", "kind": "exact", "expected": "D", "critical": true, "weight": 1}], "reference_response": {"answer": "D"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9046", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9047 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9047 | licensed_benchmark_import | mmlu-pro:test:9047 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Approximately how far away is the Andromeda Galaxy?", "context": [], "choices": {"A": "5 million light years", "B": "2.5 million light years", "C": "2.1 million light years", "D": "1.9 million light years", "E": "3.2 million light years", "F": "4 million light years", "G": "1.7 million light years", "H": "3... | {"checks": [{"path": "answer", "kind": "exact", "expected": "B", "critical": true, "weight": 1}], "reference_response": {"answer": "B"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9047", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9048 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9048 | licensed_benchmark_import | mmlu-pro:test:9048 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "What is the source of the material that causes meteor showers?", "context": [], "choices": {"A": "Large meteorites disintegrate in the Earth's atmosphere, creating smaller particles that cause a meteor shower.", "B": "Near-Earth asteroids gradually disintegrate and spread out along their orbital paths. When... | {"checks": [{"path": "answer", "kind": "exact", "expected": "J", "critical": true, "weight": 1}], "reference_response": {"answer": "J"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9048", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9165 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9165 | licensed_benchmark_import | mmlu-pro:test:9165 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "What is not true of Jupiter's magnetic field?", "context": [], "choices": {"A": "it is directly influenced by the Sun's magnetic field", "B": "it switches polarity every 11 years", "C": "it is about 20000 times stronger than Earth's magnetic field", "D": "it is weaker on the planet's dark side", "E": "it ca... | {"checks": [{"path": "answer", "kind": "exact", "expected": "B", "critical": true, "weight": 1}], "reference_response": {"answer": "B"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9165", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9167 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9167 | licensed_benchmark_import | mmlu-pro:test:9167 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "How do astronomers think Jupiter generates its internal heat?", "context": [], "choices": {"A": "the gravitational pull from its moons", "B": "heat produced by its magnetic field", "C": "by contracting changing gravitational potential energy into thermal energy", "D": "heat absorption from the Sun", "E": "n... | {"checks": [{"path": "answer", "kind": "exact", "expected": "C", "critical": true, "weight": 1}], "reference_response": {"answer": "C"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9167", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9253 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9253 | licensed_benchmark_import | mmlu-pro:test:9253 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "From laboratory measurements we know that a particular spectral line formed by hydrogen appears at a wavelength of 486.1 nanometers (nm). The spectrum of a particular star shows the same hydrogen line appearing at a wavelength of 485.9 nm. What can we conclude?", "context": [], "choices": {"A": "The star's ... | {"checks": [{"path": "answer", "kind": "exact", "expected": "J", "critical": true, "weight": 1}], "reference_response": {"answer": "J"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9253", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9255 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9255 | licensed_benchmark_import | mmlu-pro:test:9255 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Most people use C°(degree Celsius) to measure everyday temperatures. Astronomers prefer to use K (Kelvin) to measure temperatures. Approximately how many Kelvin are 25 C°?", "context": [], "choices": {"A": "350 Kelvin", "B": "250 Kelvin", "C": "200 Kelvin", "D": "300 Kelvin", "E": "375 Kelvin", "F": "275 Ke... | {"checks": [{"path": "answer", "kind": "exact", "expected": "D", "critical": true, "weight": 1}], "reference_response": {"answer": "D"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9255", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9256 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9256 | licensed_benchmark_import | mmlu-pro:test:9256 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "What do meteorites reveal about the solar system?", "context": [], "choices": {"A": "They reveal that the solar system was once part of a larger galaxy.", "B": "They reveal that all planets in the solar system once had life.", "C": "They reveal that the age of the solar system is approximately 4.6 billion y... | {"checks": [{"path": "answer", "kind": "exact", "expected": "C", "critical": true, "weight": 1}], "reference_response": {"answer": "C"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9256", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9258 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9258 | licensed_benchmark_import | mmlu-pro:test:9258 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Calculate the ratio of the solar radiation flux on Mercury's surface for perihelion (0.304 AU) versus aphelion (0.456 AU).", "context": [], "choices": {"A": "6:5", "B": "2:1", "C": "9:4", "D": "4:1", "E": "3:2", "F": "5:4", "G": "5:6", "H": "8:3", "I": "7:3", "J": "1:2"}, "response_schema": {"type": "object... | {"checks": [{"path": "answer", "kind": "exact", "expected": "C", "critical": true, "weight": 1}], "reference_response": {"answer": "C"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9258", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9261 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9261 | licensed_benchmark_import | mmlu-pro:test:9261 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Why can't we see the Sun's corona except during total solar eclipses?", "context": [], "choices": {"A": "We can't see magnetic fields", "B": "The corona is blocked by the Earth's atmosphere", "C": "The corona is hidden by the Sun's photosphere", "D": "The corona is made up mostly of charged particles which ... | {"checks": [{"path": "answer", "kind": "exact", "expected": "F", "critical": true, "weight": 1}], "reference_response": {"answer": "F"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9261", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9262 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9262 | licensed_benchmark_import | mmlu-pro:test:9262 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "The second cosmic velocity (or escape velocity) is the speed required by an object to escape the gravitational field of a celestial body with mass M and radius R. Which formula correctly calculates this velocity? (G: gravitational constant)", "context": [], "choices": {"A": "v = 2sqrt(GM/R)", "B": "v = sqrt... | {"checks": [{"path": "answer", "kind": "exact", "expected": "C", "critical": true, "weight": 1}], "reference_response": {"answer": "C"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9262", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9359 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9359 | licensed_benchmark_import | mmlu-pro:test:9359 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "A sand bag has a mass of 5kg and weight 50N on Earth. What is the mass and weight of this sand bag on a planet with half the gravity compared to Earth?", "context": [], "choices": {"A": "Mass 5kg weight 75N", "B": "Mass 5kg weight 25N", "C": "Mass 2.5kg weight 12.5N", "D": "Mass 5kg weight 100N", "E": "Mass... | {"checks": [{"path": "answer", "kind": "exact", "expected": "B", "critical": true, "weight": 1}], "reference_response": {"answer": "B"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9359", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9362 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9362 | licensed_benchmark_import | mmlu-pro:test:9362 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "The two moons of Mars are called ...", "context": [], "choices": {"A": "Deimos and Triton", "B": "Phobos and Demos", "C": "Triton and Deimos", "D": "Phobos and Deimos", "E": "Tritos and Desmos", "F": "Phobos and Mars II", "G": "Phobos and Tritos", "H": "Phobos and Triton", "I": "Tritos and Deimos", "J": "De... | {"checks": [{"path": "answer", "kind": "exact", "expected": "D", "critical": true, "weight": 1}], "reference_response": {"answer": "D"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9362", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9364 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9364 | licensed_benchmark_import | mmlu-pro:test:9364 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Find the best approximation for the surface temperature of the Sun:", "context": [], "choices": {"A": "9000 K", "B": "5000 K", "C": "6000 K", "D": "14000 K", "E": "8000 K", "F": "12000 K", "G": "7000 K", "H": "11000 K", "I": "13000 K", "J": "10000 K"}, "response_schema": {"type": "object", "properties": {"a... | {"checks": [{"path": "answer", "kind": "exact", "expected": "C", "critical": true, "weight": 1}], "reference_response": {"answer": "C"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9364", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9477 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9477 | licensed_benchmark_import | mmlu-pro:test:9477 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Why is the sky blue?", "context": [], "choices": {"A": "Because the Earth's magnetic field causes the sky to appear blue.", "B": "Because the human eye is more sensitive to blue light.", "C": "Because the Earth's atmosphere contains a large amount of blue pigment.", "D": "Because the atmosphere preferential... | {"checks": [{"path": "answer", "kind": "exact", "expected": "D", "critical": true, "weight": 1}], "reference_response": {"answer": "D"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9477", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9479 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9479 | licensed_benchmark_import | mmlu-pro:test:9479 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "According to the Solar Nebular theory what are asteroids and comets?", "context": [], "choices": {"A": "They are the shattered remains of collisions between planets.", "B": "They are chunks of rock or ice that condensed long after the planets and moons had formed.", "C": "They are solidified lava from the e... | {"checks": [{"path": "answer", "kind": "exact", "expected": "D", "critical": true, "weight": 1}], "reference_response": {"answer": "D"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9479", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9677 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9677 | licensed_benchmark_import | mmlu-pro:test:9677 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Why does the plasma (ion) tail of a comet always point away from the Sun?", "context": [], "choices": {"A": "The ions are following Keplerian orbits that lead away from the Sun.", "B": "The conservation of the angular momentum in the tail keeps it always pointing away from the Sun.", "C": "The solar wind el... | {"checks": [{"path": "answer", "kind": "exact", "expected": "C", "critical": true, "weight": 1}], "reference_response": {"answer": "C"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9677", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9680 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9680 | licensed_benchmark_import | mmlu-pro:test:9680 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Why are there no impact craters on the surface of Io?", "context": [], "choices": {"A": "Any craters that existed have been eroded through the strong winds on Io's surface.", "B": "Io is protected by a layer of gas that prevents any objects from reaching its surface.", "C": "The gravitational pull of nearby... | {"checks": [{"path": "answer", "kind": "exact", "expected": "E", "critical": true, "weight": 1}], "reference_response": {"answer": "E"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9680", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9763 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9763 | licensed_benchmark_import | mmlu-pro:test:9763 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "What is the second most common element in the solar system?", "context": [], "choices": {"A": "Methane", "B": "Nitrogen", "C": "Oxygen", "D": "Iron", "E": "Hydrogen", "F": "Helium", "G": "Neon", "H": "Carbon", "I": "Silicon", "J": "Argon"}, "response_schema": {"type": "object", "properties": {"answer": {"ty... | {"checks": [{"path": "answer", "kind": "exact", "expected": "F", "critical": true, "weight": 1}], "reference_response": {"answer": "F"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9763", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9764 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9764 | licensed_benchmark_import | mmlu-pro:test:9764 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Which of the following most likely explains why Venus does not have a strong magnetic field?", "context": [], "choices": {"A": "It has a weak gravitational field.", "B": "It has too thick an atmosphere.", "C": "It does not have a metallic core.", "D": "Its rotation is too slow.", "E": "Its distance from the... | {"checks": [{"path": "answer", "kind": "exact", "expected": "D", "critical": true, "weight": 1}], "reference_response": {"answer": "D"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9764", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9877 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9877 | licensed_benchmark_import | mmlu-pro:test:9877 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "All of the following have been cited as evidence for the Giant Impact Hypothesis except:", "context": [], "choices": {"A": "The Moon and Earth have nearly identical isotopic compositions.", "B": "The Moon's orbit is not in the same plane as Earth's equator.", "C": "The Moon's crust is thicker on the far sid... | {"checks": [{"path": "answer", "kind": "exact", "expected": "I", "critical": true, "weight": 1}], "reference_response": {"answer": "I"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9877", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa-v3-mmlupro-9989 | 3.0.0-draft | challenge | astronomy | mcq | Astronomy — source question 9989 | licensed_benchmark_import | mmlu-pro:test:9989 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Why is Saturn almost as big as Jupiter despite its smaller mass?", "context": [], "choices": {"A": "Jupiter has more moons, which increase its gravitational pull and compress it more.", "B": "The rapid rotation of Saturn causes it to expand.", "C": "Saturn's lower gravity allows it to expand more.", "D": "S... | {"checks": [{"path": "answer", "kind": "exact", "expected": "F", "critical": true, "weight": 1}], "reference_response": {"answer": "F"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "9989", "source_category": "physics", "source_license": "MIT", "origin_subdataset": "ori_mmlu-astronomy", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/b... | {} |
nasa_v3_astronomy_differential_doppler_calibration_01 | 3.0.0-draft | challenge | astronomy | structured | Separate velocity from calibration drift | original_synthetic | nasa_v3_astronomy_differential_doppler_calibration | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional spectrometer measures a line centroid at 500.06 nm; its laboratory wavelength is 500.0 nm. Calibration shows an additive wavelength offset of +0.015 nm that must be subtracted. Centroid and offset errors are independent with standard uncertainties 0.003 and 0.004 nm. Use nonrelativistic v=c*(cor... | {"checks": [{"path": "corrected_wavelength_nm", "kind": "number", "expected": 500.045, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "radial_velocity_km_s", "kind": "number", "expected": 26.98132122000954, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "velocity_sigma_km... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_differential_doppler_calibration_02 | 3.0.0-draft | challenge | astronomy | structured | Separate velocity from calibration drift | original_synthetic | nasa_v3_astronomy_differential_doppler_calibration | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional spectrometer measures a line centroid at 500.07 nm; its laboratory wavelength is 500.0 nm. Calibration shows an additive wavelength offset of +0.017 nm that must be subtracted. Centroid and offset errors are independent with standard uncertainties 0.003 and 0.004 nm. Use nonrelativistic v=c*(cor... | {"checks": [{"path": "corrected_wavelength_nm", "kind": "number", "expected": 500.053, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "radial_velocity_km_s", "kind": "number", "expected": 31.778000547998364, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "velocity_sigma_k... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_differential_doppler_calibration_03 | 3.0.0-draft | challenge | astronomy | structured | Separate velocity from calibration drift | original_synthetic | nasa_v3_astronomy_differential_doppler_calibration | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional spectrometer measures a line centroid at 500.08 nm; its laboratory wavelength is 500.0 nm. Calibration shows an additive wavelength offset of +0.019 nm that must be subtracted. Centroid and offset errors are independent with standard uncertainties 0.003 and 0.004 nm. Use nonrelativistic v=c*(cor... | {"checks": [{"path": "corrected_wavelength_nm", "kind": "number", "expected": 500.061, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "radial_velocity_km_s", "kind": "number", "expected": 36.57467987598718, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "velocity_sigma_km... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_differential_doppler_calibration_04 | 3.0.0-draft | challenge | astronomy | structured | Separate velocity from calibration drift | original_synthetic | nasa_v3_astronomy_differential_doppler_calibration | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional spectrometer measures a line centroid at 500.09 nm; its laboratory wavelength is 500.0 nm. Calibration shows an additive wavelength offset of +0.020999999999999998 nm that must be subtracted. Centroid and offset errors are independent with standard uncertainties 0.003 and 0.004 nm. Use nonrelati... | {"checks": [{"path": "corrected_wavelength_nm", "kind": "number", "expected": 500.06899999999996, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "radial_velocity_km_s", "kind": "number", "expected": 41.371359203976006, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "veloc... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_diluted_transit_01 | 3.0.0-draft | nasa_work | astronomy | structured | Correct a diluted transit estimate | original_synthetic | nasa_v3_astronomy_diluted_transit | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional photometry study reports a fractional transit depth 0.004 with Gaussian standard uncertainty 0.0003. A constant contaminant contributes fraction 0.2 of total out-of-transit flux. Treat dilution and stellar radius 0.8 solar radii as exact. Ignore limb darkening and take true depth=(planet radius/... | {"checks": [{"path": "corrected_depth", "kind": "number", "expected": 0.005, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "radius_ratio", "kind": "number", "expected": 0.07071067811865475, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "planet_radius_solar", "kind": "nu... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_diluted_transit_02 | 3.0.0-draft | nasa_work | astronomy | structured | Correct a diluted transit estimate | original_synthetic | nasa_v3_astronomy_diluted_transit | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional photometry study reports a fractional transit depth 0.005 with Gaussian standard uncertainty 0.0003. A constant contaminant contributes fraction 0.25 of total out-of-transit flux. Treat dilution and stellar radius 0.9 solar radii as exact. Ignore limb darkening and take true depth=(planet radius... | {"checks": [{"path": "corrected_depth", "kind": "number", "expected": 0.006666666666666667, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "radius_ratio", "kind": "number", "expected": 0.08164965809277261, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "planet_radius_sola... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_diluted_transit_03 | 3.0.0-draft | nasa_work | astronomy | structured | Correct a diluted transit estimate | original_synthetic | nasa_v3_astronomy_diluted_transit | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional photometry study reports a fractional transit depth 0.006 with Gaussian standard uncertainty 0.0003. A constant contaminant contributes fraction 0.30000000000000004 of total out-of-transit flux. Treat dilution and stellar radius 1.0 solar radii as exact. Ignore limb darkening and take true depth... | {"checks": [{"path": "corrected_depth", "kind": "number", "expected": 0.008571428571428572, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "radius_ratio", "kind": "number", "expected": 0.09258200997725514, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "planet_radius_sola... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_diluted_transit_04 | 3.0.0-draft | nasa_work | astronomy | structured | Correct a diluted transit estimate | original_synthetic | nasa_v3_astronomy_diluted_transit | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional photometry study reports a fractional transit depth 0.007 with Gaussian standard uncertainty 0.0003. A constant contaminant contributes fraction 0.35000000000000003 of total out-of-transit flux. Treat dilution and stellar radius 1.1 solar radii as exact. Ignore limb darkening and take true depth... | {"checks": [{"path": "corrected_depth", "kind": "number", "expected": 0.01076923076923077, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "radius_ratio", "kind": "number", "expected": 0.10377490433255417, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "planet_radius_solar... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_extinction_distance_01 | 3.0.0-draft | nasa_work | astronomy | structured | Propagate magnitude uncertainty to distance | original_synthetic | nasa_v3_astronomy_extinction_distance | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "For a fictional stellar catalog, apparent magnitude m=14.0, extinction A=0.3, and absolute magnitude M=4.2. Only m has uncertainty: use endpoints m±0.1 magnitude. The distance relation is m-A-M=5*log10(d_pc)-5. Solar absolute magnitude in this same band is 4.83; relative band luminosity is 10^(0.4*(4.83-M))... | {"checks": [{"path": "distance_pc", "kind": "number", "expected": 794.3282347242813, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "lower_distance_pc", "kind": "number", "expected": 758.5775750291835, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "upper_distance_pc", "k... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_extinction_distance_02 | 3.0.0-draft | nasa_work | astronomy | structured | Propagate magnitude uncertainty to distance | original_synthetic | nasa_v3_astronomy_extinction_distance | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "For a fictional stellar catalog, apparent magnitude m=14.3, extinction A=0.35, and absolute magnitude M=4.0. Only m has uncertainty: use endpoints m±0.1 magnitude. The distance relation is m-A-M=5*log10(d_pc)-5. Solar absolute magnitude in this same band is 4.83; relative band luminosity is 10^(0.4*(4.83-M)... | {"checks": [{"path": "distance_pc", "kind": "number", "expected": 977.2372209558112, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "lower_distance_pc", "kind": "number", "expected": 933.2543007969915, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "upper_distance_pc", "k... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_extinction_distance_03 | 3.0.0-draft | nasa_work | astronomy | structured | Propagate magnitude uncertainty to distance | original_synthetic | nasa_v3_astronomy_extinction_distance | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "For a fictional stellar catalog, apparent magnitude m=14.6, extinction A=0.4, and absolute magnitude M=3.8000000000000003. Only m has uncertainty: use endpoints m±0.1 magnitude. The distance relation is m-A-M=5*log10(d_pc)-5. Solar absolute magnitude in this same band is 4.83; relative band luminosity is 10... | {"checks": [{"path": "distance_pc", "kind": "number", "expected": 1202.2644346174118, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "lower_distance_pc", "kind": "number", "expected": 1148.1536214968817, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "upper_distance_pc", ... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_extinction_distance_04 | 3.0.0-draft | nasa_work | astronomy | structured | Propagate magnitude uncertainty to distance | original_synthetic | nasa_v3_astronomy_extinction_distance | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "For a fictional stellar catalog, apparent magnitude m=14.9, extinction A=0.45, and absolute magnitude M=3.6. Only m has uncertainty: use endpoints m±0.1 magnitude. The distance relation is m-A-M=5*log10(d_pc)-5. Solar absolute magnitude in this same band is 4.83; relative band luminosity is 10^(0.4*(4.83-M)... | {"checks": [{"path": "distance_pc", "kind": "number", "expected": 1479.1083881682086, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "lower_distance_pc", "kind": "number", "expected": 1412.5375446227556, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "upper_distance_pc", ... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_photometry_noise_budget_01 | 3.0.0-draft | nasa_work | astronomy | structured | Plan repeated aperture measurements | original_synthetic | nasa_v3_astronomy_photometry_noise_budget | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional ground astronomy analysis measures source signal 820 electrons per exposure after exact background subtraction. The aperture has 18 pixels; each contributes 180 sky electrons, dark current 0.12 electrons/s for 80 s, and read noise 3.2 electrons rms. Background-estimation uncertainty is negligibl... | {"checks": [{"path": "single_exposure_variance", "kind": "number", "expected": 4417.12, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "single_exposure_snr", "kind": "number", "expected": 12.33798544088044, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "minimum_exposures... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_photometry_noise_budget_02 | 3.0.0-draft | nasa_work | astronomy | structured | Plan repeated aperture measurements | original_synthetic | nasa_v3_astronomy_photometry_noise_budget | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional ground astronomy analysis measures source signal 950 electrons per exposure after exact background subtraction. The aperture has 20 pixels; each contributes 195 sky electrons, dark current 0.12 electrons/s for 90 s, and read noise 3.2 electrons rms. Background-estimation uncertainty is negligibl... | {"checks": [{"path": "single_exposure_variance", "kind": "number", "expected": 5270.8, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "single_exposure_snr", "kind": "number", "expected": 13.08534979651902, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "minimum_exposures"... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_photometry_noise_budget_03 | 3.0.0-draft | nasa_work | astronomy | structured | Plan repeated aperture measurements | original_synthetic | nasa_v3_astronomy_photometry_noise_budget | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional ground astronomy analysis measures source signal 1080 electrons per exposure after exact background subtraction. The aperture has 22 pixels; each contributes 210 sky electrons, dark current 0.12 electrons/s for 100 s, and read noise 3.2 electrons rms. Background-estimation uncertainty is negligi... | {"checks": [{"path": "single_exposure_variance", "kind": "number", "expected": 6189.280000000001, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "single_exposure_snr", "kind": "number", "expected": 13.727886830072377, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "minimu... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_photometry_noise_budget_04 | 3.0.0-draft | nasa_work | astronomy | structured | Plan repeated aperture measurements | original_synthetic | nasa_v3_astronomy_photometry_noise_budget | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional ground astronomy analysis measures source signal 1210 electrons per exposure after exact background subtraction. The aperture has 24 pixels; each contributes 225 sky electrons, dark current 0.12 electrons/s for 110 s, and read noise 3.2 electrons rms. Background-estimation uncertainty is negligi... | {"checks": [{"path": "single_exposure_variance", "kind": "number", "expected": 7172.5599999999995, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "single_exposure_snr", "kind": "number", "expected": 14.287237868464274, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "minim... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_redshift_resolution_01 | 3.0.0-draft | challenge | astronomy | structured | Evaluate observed-line separation | original_synthetic | nasa_v3_astronomy_redshift_resolution | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional source has two lines at rest wavelengths 500.0 and 500.3 nm and redshift z=0.1. The spectrometer has resolving power R=2100, defined by instrumental FWHM=observed central wavelength/R. For this task only, call the pair resolved if observed separation is at least 1.5 instrumental FWHM. Return obs... | {"checks": [{"path": "observed_center_nm", "kind": "number", "expected": 550.165, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "observed_separation_nm", "kind": "number", "expected": 0.3300000000000125, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "instrumental_fwhm_n... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_redshift_resolution_02 | 3.0.0-draft | challenge | astronomy | structured | Evaluate observed-line separation | original_synthetic | nasa_v3_astronomy_redshift_resolution | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional source has two lines at rest wavelengths 500.0 and 500.3 nm and redshift z=0.15000000000000002. The spectrometer has resolving power R=2300, defined by instrumental FWHM=observed central wavelength/R. For this task only, call the pair resolved if observed separation is at least 1.5 instrumental ... | {"checks": [{"path": "observed_center_nm", "kind": "number", "expected": 575.1724999999999, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "observed_separation_nm", "kind": "number", "expected": 0.3450000000000131, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "instrumen... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_redshift_resolution_03 | 3.0.0-draft | challenge | astronomy | structured | Evaluate observed-line separation | original_synthetic | nasa_v3_astronomy_redshift_resolution | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional source has two lines at rest wavelengths 500.0 and 500.3 nm and redshift z=0.2. The spectrometer has resolving power R=2500, defined by instrumental FWHM=observed central wavelength/R. For this task only, call the pair resolved if observed separation is at least 1.5 instrumental FWHM. Return obs... | {"checks": [{"path": "observed_center_nm", "kind": "number", "expected": 600.18, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "observed_separation_nm", "kind": "number", "expected": 0.36000000000001364, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "instrumental_fwhm_n... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa_v3_astronomy_redshift_resolution_04 | 3.0.0-draft | challenge | astronomy | structured | Evaluate observed-line separation | original_synthetic | nasa_v3_astronomy_redshift_resolution | formula_checked_domain_expert_review_pending | not_run | false | {"prompt": "A fictional source has two lines at rest wavelengths 500.0 and 500.3 nm and redshift z=0.25. The spectrometer has resolving power R=2700, defined by instrumental FWHM=observed central wavelength/R. For this task only, call the pair resolved if observed separation is at least 1.5 instrumental FWHM. Return ob... | {"checks": [{"path": "observed_center_nm", "kind": "number", "expected": 625.1875, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "observed_separation_nm", "kind": "number", "expected": 0.3750000000000142, "atol": 1e-12, "rtol": 0.001, "critical": true, "weight": 1}, {"path": "instrumental_fwhm_... | [] | {"method": "assistant_written_problem_family_and_explicit_reference_calculation", "exact_model_identity": "not_independently_verified", "external_authoring_api_calls": 0, "related_parameter_variants": 4, "independent_human_review": false} |
nasa-v3-mmlupro-2847 | 3.0.0-draft | challenge | biology | mcq | Biology — source question 2847 | licensed_benchmark_import | mmlu-pro:test:2847 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "What are the typical periods in the unfolding of abehavioral act?", "context": [], "choices": {"A": "Cue, Desire, Fulfillment", "B": "Arousal, Behavior, Consequence", "C": "Stimulus, Habituation, Extinction", "D": "Appetitive behavior, Consummatory act, Quiescence", "E": "Perception, Decision, Movement", "F... | {"checks": [{"path": "answer", "kind": "exact", "expected": "D", "critical": true, "weight": 1}], "reference_response": {"answer": "D"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "2847", "source_category": "biology", "source_license": "MIT", "origin_subdataset": "stemez-Biology", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/blob/... | {} |
nasa-v3-mmlupro-2900 | 3.0.0-draft | challenge | biology | mcq | Biology — source question 2900 | licensed_benchmark_import | mmlu-pro:test:2900 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "The cells of humans and most animals have become adapted to surviving only within a relatively small range of hydrogen ion concentrations. What is the role of the kidneys in regulating hydrogen ion concentration?", "context": [], "choices": {"A": "The kidneys filter out hydrogen ions and recycle them into o... | {"checks": [{"path": "answer", "kind": "exact", "expected": "B", "critical": true, "weight": 1}], "reference_response": {"answer": "B"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "2900", "source_category": "biology", "source_license": "MIT", "origin_subdataset": "stemez-Biology", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/blob/... | {} |
nasa-v3-mmlupro-2908 | 3.0.0-draft | challenge | biology | mcq | Biology — source question 2908 | licensed_benchmark_import | mmlu-pro:test:2908 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Why is a moss plant restricted to a height of less thanabout 15 cm?", "context": [], "choices": {"A": "Moss plants lack photosynthetic capabilities", "B": "Inefficiency of the rhizoids in absorbing water and minerals and the absence of True vascular and supporting tissues restricts a moss plant to a height ... | {"checks": [{"path": "answer", "kind": "exact", "expected": "B", "critical": true, "weight": 1}], "reference_response": {"answer": "B"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "2908", "source_category": "biology", "source_license": "MIT", "origin_subdataset": "stemez-Biology", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/blob/... | {} |
nasa-v3-mmlupro-2915 | 3.0.0-draft | challenge | biology | mcq | Biology — source question 2915 | licensed_benchmark_import | mmlu-pro:test:2915 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Why does one experience difficulty in breathing at high altitudes ?", "context": [], "choices": {"A": "At high altitudes, the amount of hemoglobin in blood decreases", "B": "At high altitudes, the body's respiratory rate decreases, leading to reduced oxygen intake", "C": "At high altitudes, the air is less ... | {"checks": [{"path": "answer", "kind": "exact", "expected": "F", "critical": true, "weight": 1}], "reference_response": {"answer": "F"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "2915", "source_category": "biology", "source_license": "MIT", "origin_subdataset": "stemez-Biology", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/blob/... | {} |
nasa-v3-mmlupro-2947 | 3.0.0-draft | challenge | biology | mcq | Biology — source question 2947 | licensed_benchmark_import | mmlu-pro:test:2947 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "What is the physiological purpose of shivering?", "context": [], "choices": {"A": "Shivering is a method the body uses to relieve pain.", "B": "Shivering is a tactic to ward off predators by appearing agitated.", "C": "Shivering is a way to burn excess calories", "D": "Shivering is a response to fear or anx... | {"checks": [{"path": "answer", "kind": "exact", "expected": "F", "critical": true, "weight": 1}], "reference_response": {"answer": "F"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "2947", "source_category": "biology", "source_license": "MIT", "origin_subdataset": "stemez-Biology", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/blob/... | {} |
nasa-v3-mmlupro-2965 | 3.0.0-draft | challenge | biology | mcq | Biology — source question 2965 | licensed_benchmark_import | mmlu-pro:test:2965 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "Besides temperature, what other physical conditions must be taken into account for the growth of bacteria?", "context": [], "choices": {"A": "Levels of oxygen, acidity or alkalinity of the medium", "B": "Temperature changes, light exposure", "C": "Atmospheric pressure, noise levels", "D": "Nitrogen levels, ... | {"checks": [{"path": "answer", "kind": "exact", "expected": "A", "critical": true, "weight": 1}], "reference_response": {"answer": "A"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "2965", "source_category": "biology", "source_license": "MIT", "origin_subdataset": "stemez-Biology", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/blob/... | {} |
nasa-v3-mmlupro-2994 | 3.0.0-draft | challenge | biology | mcq | Biology — source question 2994 | licensed_benchmark_import | mmlu-pro:test:2994 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "The soils of which of the following biomes has the highest rate of leaching and cycling of nutrients?", "context": [], "choices": {"A": "Wetlands", "B": "Tropical rain forest", "C": "Alpine", "D": "Desert", "E": "Chaparral", "F": "Temperate deciduous forest", "G": "Savanna", "H": "Tundra", "I": "Grasslands"... | {"checks": [{"path": "answer", "kind": "exact", "expected": "B", "critical": true, "weight": 1}], "reference_response": {"answer": "B"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "2994", "source_category": "biology", "source_license": "MIT", "origin_subdataset": "ori_mmlu-college_biology", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU... | {} |
nasa-v3-mmlupro-3041 | 3.0.0-draft | challenge | biology | mcq | Biology — source question 3041 | licensed_benchmark_import | mmlu-pro:test:3041 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "What are the difficulties in the classification of tissuesof higherplants?", "context": [], "choices": {"A": "Plant tissues can be fully characterized based on their evolutionary heritage", "B": "Plant tissues are distinguished only by their cellular composition without considering their function", "C": "Al... | {"checks": [{"path": "answer", "kind": "exact", "expected": "G", "critical": true, "weight": 1}], "reference_response": {"answer": "G"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "3041", "source_category": "biology", "source_license": "MIT", "origin_subdataset": "stemez-Biology", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/blob/... | {} |
nasa-v3-mmlupro-3057 | 3.0.0-draft | challenge | biology | mcq | Biology — source question 3057 | licensed_benchmark_import | mmlu-pro:test:3057 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "In order for the Hardy-Weinberg law to operate with respect to a population of organisms, each of the following conditions must be met EXCEPT:", "context": [], "choices": {"A": "Genes are exchanged with other populations.", "B": "Population size is large.", "C": "Natural selection does not take place.", "D"... | {"checks": [{"path": "answer", "kind": "exact", "expected": "A", "critical": true, "weight": 1}], "reference_response": {"answer": "A"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "3057", "source_category": "biology", "source_license": "MIT", "origin_subdataset": "ori_mmlu-college_biology", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU... | {} |
nasa-v3-mmlupro-3082 | 3.0.0-draft | challenge | biology | mcq | Biology — source question 3082 | licensed_benchmark_import | mmlu-pro:test:3082 | inherited_answer_not_independently_reviewed | not_run | false | {"prompt": "What controls the process of molting incrustacea?", "context": [], "choices": {"A": "Water temperature alone without hormonal influence", "B": "The age of the crustacean", "C": "Environmental factors", "D": "Social interactions with other crustaceans", "E": "Diet of the crustacean", "F": "The salinity level... | {"checks": [{"path": "answer", "kind": "exact", "expected": "H", "critical": true, "weight": 1}], "reference_response": {"answer": "H"}, "human_review_required": true, "explanation_criteria": []} | [{"source_dataset": "TIGER-Lab/MMLU-Pro", "source_revision": "b189ec765aa7ed75c8acfea42df31fdae71f97be", "source_split": "test", "source_item_id": "3082", "source_category": "biology", "source_license": "MIT", "origin_subdataset": "stemez-Biology", "source_url": "https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro/blob/... | {} |
NASA Ground Work Eval: v3 development draft
This research bank asks whether models can produce correct scientific and engineering answers under a recorded evaluation protocol. Its intended use is to compare capability, cost, and specific failure modes in work relevant to NASA ground personnel. It is not an official NASA dataset, an operational mission model, or evidence of measured workforce benefit.
What is in this version?
There are 1,000 development instances across 20 selected science and engineering prerequisite topics:
| Origin and intended collection | Instances | Labeled problem families |
|---|---|---|
| Attributed MMLU-Pro questions, challenge collection | 600 | 600 source identities |
| New synthetic NASA-motivated work, natural-work collection | 232 | 58 |
| New synthetic NASA-motivated work, challenge collection | 168 | 42 |
| Total | 1,000 | 700 |
Each new family has four related parameter cases. This is not 1,000 independently constructed questions. Source identities also do not guarantee that imported questions are scientifically independent. All difficulty labels are design intentions, not calibrated measurements. Many new tasks supply the governing equations explicitly; this draft does not establish extreme or frontier-level difficulty.
The 20 topics are astronomy, optics, classical mechanics, engineering thermodynamics, electromagnetics, electrical circuits, communications, fluid mechanics, heat transfer, transport phenomena, machine design, general chemistry, physical chemistry, biology, genetics, scientific mathematics, differential equations, statistics, computer science, and machine learning/security. Each has 30 imports and 20 synthetic instances. These are selected prerequisite strata, not a complete taxonomy of NASA's Earth science, planetary science, aeronautics, human research, or supporting occupations. Supporting-personnel workflows and executable repository repairs need further development; they are not established by a large question count.
The collection field keeps nasa_work and challenge separately scored within one dataset. The origin field separately identifies imports versus original synthetic cases. Report both axes; do not turn their mixture into one NASA-competence percentage.
The problem this benchmark is trying to solve
Generic examination benchmarks can test broad knowledge or reasoning without establishing whether a model produces a usable analysis, respects data provenance, handles uncertainty, or reduces the effort required to check its work. Our earlier v1 pilot illustrated this gap: 90 of 108 questions passed for all 11 tested models. High scores on those development questions were weak evidence for model selection, particularly when the remaining failures included JSON formatting and API problems.
The intended distinction here is to request inspectable work products: corrected measurements, uncertainty calculations, resource estimates, bounded engineering decisions, dataset-quality operations, and reproducible intermediate quantities. The new tasks include correlated uncertainty, calibration publication dates, missing-value/quality-bit semantics, numerical stability, conservation, false-positive base rates, and competing constraints. Values and experimental situations are synthetic.
NASA's Evaluation Policy, NPD1210.7 describes rigor, relevance, utility, independence and transparency. NASA's 2024 advisory-council AI briefing provides a historical management perspective on useful agency applications. The NASA technical memorandum on LLM assurance arguments is research, not agency leadership policy. Our task design is an interpretation of these sources, not NASA's approval or a claim that these calculations operationalize every agency requirement.
Independent expert review, realistic files and workflows, a genuinely protected holdout, and human-only versus AI-assisted studies remain necessary to establish scientific validity and workplace value.
How this relates to existing benchmarks
| Benchmark | What we use or learn | What we do not claim |
|---|---|---|
| MMLU-Pro | 600 pinned, attributed source questions; multiple-choice foundation coverage | A paraphrase becomes a new independent question, or a familiar source is uncontaminated |
| GPQA | Expert science reasoning and independent review are useful design principles | We downloaded, rewrote, or redistributed GPQA examples; its official gate asks users not to reveal examples online |
| SciCode | Eligible source bank for a future executable scientific-coding collection | Downloaded question/test files alone establish a verified, runnable grader; no SciCode tasks are scored in v3 yet |
| AA-LCR | Long-document evidence handling and versioned reference corrections | Its question license automatically licenses all underlying source documents |
| AstaBench | Real scientific work, explicit agent protocols, cost/performance comparisons | Our short numerical cases are equivalent to end-to-end research projects |
MMLU-Pro's dataset is declared MIT by its card and paper; its code repository has a separate Apache-2.0 license. Original source labels, revision, row identifiers and notices are retained. MMLU-Pro's authors describe the underlying STEM website material as open-licensed, but this project could not independently retrieve that website's original license. This limitation is recorded in the source register and attribution notice. Source answers have not undergone independent domain-expert adjudication here. Rewording would not resolve either uncertain answer quality or training contamination. This release preserves source wording so that changes and origins remain auditable.
No license has been selected for the user's original research. This repository begins as a private development draft. Source material keeps its respective applicable terms. The source license must not be treated as a blanket license for the entire collection.
Examples and answer structure
Imported MMLU-Pro astronomy item 9364 (nasa-v3-mmlupro-9364) asks for the best approximation to the Sun's surface temperature. Its 10 supplied options include 6000 K; the inherited correct label is C in the stored option order. This is a foundation check, not evidence of frontier-level difficulty. The original dataset, item ID, revision and option order accompany the stored row.
The new data-processing task nasa_v3_computer_science_quality_mask_00 supplies values [10, -9999, 20, 30, 40], flags [0, 0, 1, 2, 0], and weights [1, 2, 3, 4, 2]. It defines -9999 as missing, bit 0 as invalid, and bit 1 as advisory. Correct processing retains zero-based indices 0, 3, and 4, with weight sum 7 and weighted mean (10×1 + 30×4 + 40×2)/7 = 30. The requested work product is:
{
"retained_count": 3,
"retained_weight_sum": 7,
"weighted_mean": 30.0,
"retained_index_sum": 7
}
This tests a common failure: deleting advisory-only data or allowing fill values into a weighted mean. The expected values follow the supplied synthetic semantics; they do not assert a particular NASA product's quality conventions.
The uncertainty task nasa_v3_statistics_correlated_replicates_00 specifies 20 measurements with individual standard deviation 2 and pairwise correlation 0.1. It asks for the mean's variance, standard error, effective sample size, and the naive independent-measurement standard error. The correct values are approximately 0.58, 0.7615773, 6.8965517, and 0.4472136, respectively. The variance is (2²/20)×[1 + (20−1)×0.1] = 0.58; the other quantities follow from its square root, 20/[1 + 19×0.1], and 2/√20. This tests whether repeated correlated observations are incorrectly treated as independent evidence.
Scoring
The imported items have between 3 and 10 choices (548 of 600 have 10). Uniform random guessing has an expected accuracy of approximately 10.76% on this selected import bank. This baseline does not apply to multi-field numerical tasks. See answer-structure audit.
- Multiple choice: compare the selected label to the inherited key. A bare correct label is recorded as correct content but invalid JSON format.
- Numerical work: check every requested quantity against the stated reference calculation and task-specific tolerance. New floating-point values generally allow relative error 0.1%; small absolute allowances are capped to avoid accepting zero for tiny nonzero quantities. Integer counts and Boolean decisions are exact. Inspect each row for its actual tolerance.
- Full task success: all critical answer checks plus the requested response format must pass. Partial credit reports the fraction of weighted checks passed.
- Keep scientific-content errors, format errors, incomplete responses, transport errors and missing responses separate.
- These checks do not establish the truth of unrequested prose, citation entailment, or an expert's acceptance of a complete deliverable.
human_review_requiredremains true andfully_acceptedremains unknown.
The reference-output acceptance and mutation tests validate evaluator behavior. They do not independently prove that every reference answer is scientifically correct. See the mechanical validation and scientific review records.
The content parser can also recover one unambiguous JSON object embedded in prose or a Markdown fence. Such an answer can receive content credit while still failing the requested format. Multiple candidate objects and duplicate keys are rejected. This parser change is recorded in the pilot's rescoring provenance; original responses and original run scores are retained.
Storage and access
The dataset is physically stored as UTF-8 JSON Lines on the Hugging Face Hub. Each line is one record.
hub/dev.jsonl: the standard Hub view; variable nested candidate, scoring and provenance objects are JSON strings for reliable Arrow loading.data/dev.jsonl: canonical nested records for the local evaluation harness.candidate_packets/dev.jsonl: candidate-only projection plus task identifiers for transport. The harness itself sends only the approved prompt/context/choices/schema.evaluation/evaluation.py: standalone deterministic scoring code.authoring/: construction-source snapshots and provenance, not an independent human review.source_notices/: attribution and applicable original source notices.dataset_manifest.json: counts, source status, hash, and limitations.
After signing in to an account with access, load the Hub view with:
from datasets import load_dataset
import json
ds = load_dataset("MarshallDoyle/nasa-ground-work-eval-v3", split="dev")
candidate = json.loads(ds[0]["candidate_json"])
scoring = json.loads(ds[0]["scoring_json"])
Never mount this full answer-containing development repository into an evaluated agent's filesystem or retrieval tools. Private Hub visibility does not make it a holdout.
Model comparison protocol
The first v3 pilot uses a fixed, seeded, family-distinct subset with matched questions for every model, no retries and an explicit dollar ceiling. Record exact model/provider, reasoning setting, output cap, protocol, dataset hash, raw response, usage, cost and status. The planned low-cost panel includes OpenAI, Anthropic, Google, DeepSeek and Qwen. A budget-conscious pilot measures those settings; it is not a price-agnostic maximum-capability leaderboard.
No-tool requests supply no tools, specify tool_choice: none, and disable web and response-healing plugins. This is request-level control. Provider network isolation and locked account plugin overrides are not independently verified. Search-enabled comparisons need a separately fixed protocol and full tool-cost accounting; they have not been run in this release.
Answer-containing public benchmark sources may be searchable on the web. A future web-enabled score on those items would mix answer retrieval with reasoning; it must not be presented as a pure reasoning comparison. A realistic scientific-work condition should also distinguish permission to use a calculator or code from permission to search the web.
Reports should show matched-case score versus observed cost, per-topic pass/count cells, and failure types. Group related variants together when sampling or splitting. Do not use row-level binomial confidence intervals as if four variants were independent expert-authored problems. A 40-task pilot provides at most two observations per topic, which is insufficient for robust topic rankings.
Results: initial development pilot
The October 8, 2026 baseline made 195 attempted calls across five models. Provider interruptions left 38 questions attempted by every model: 19 imported multiple-choice questions and 19 original synthetic tasks. Five attempts from two partly completed question blocks are preserved but excluded from the matched comparison. No failed or refused baseline answer was retried or silently replaced. All complete responses were rescored consistently under the documented content extractor.
For the same 19 original synthetic tasks, with no external tools and an output cap of 1,536 tokens:
| Model | Delivered correct answers / attempted | Correct / evaluable answers | Reported API cost for these 19 attempts |
|---|---|---|---|
| Claude Sonnet 5.5 | 19/19 | 19/19 | $0.098810 |
| GPT-6 Luna | 18/19 | 18/19 | $0.003519 |
| Gemini 3.8 Flash | 15/19 | 15/19 | $0.041061 |
| DeepSeek V4.1 Flash | 10/19 | 10/10 | $0.020992 |
| Qwen3.8 Flash | 8/19 | 8/9 | $0.006080, plus at most $0.021375 in unresolved charges |
DeepSeek's nine missing answers in this subset hit the output limit. Qwen had eight rate-limit errors and two returned fragments with no evaluable answer. Conditional accuracy therefore does not measure dependable answer delivery. Extra prose or Markdown around otherwise correct JSON is a format failure, not automatically a scientific error. These are single attempts on a small development subset, with low reasoning settings (Qwen used its supported explicit reasoning-token setting); they do not establish the best model at maximum capability or a robust domain ranking.
A separate output-budget condition evaluated all 19 of these synthetic tasks again on DeepSeek with a 6,144-token cap, holding the other configured inference settings fixed. All 19 paired requests used the same provider (Relace), and their payloads differed only in the output cap. It delivered 16/19 correct answers, with three length-limited responses, for $0.047542. Every completed answer passed the declared content checks. This is a separately reported experimental condition; it does not replace the baseline, and one generation per condition leaves stochastic variability uncontrolled.
Across the baseline and this additional condition, reported new charges were $0.3282547365, with $0.08540294 of conservatively retained unresolved charges. The combined upper accounting bound is $0.4136576765, within the previously authorized campaign budget. Exact receipts, settings, source hashes, uncertainty about charges and comparison data accompany the result package.
Answer-quality audit
The baseline contained eight evaluable disagreements with reference keys. Six were original numerical answers; separate high-precision recalculation confirmed the references under the supplied assumptions. Two involved imported multiple-choice questions: diode item12125 omits the intended device-model assumptions; thermal-panel item11407 omits conventions required to reproduce its exact numerical key. Both need expert adjudication. This does not establish that the models' alternatives are correct. The original inherited-key scores are retained, and a separately labeled, post-hoc sensitivity analysis excludes both flagged items for every model.
The pilot samples only one of the newly authored challenge families. It therefore does not calibrate that collection's intended difficulty. Sonnet also passed all 19 synthetic tasks in the tested subset: we have not demonstrated the extremely difficult frontier benchmark envisioned for a later release. More source imports or parameter variants alone will not close that gap.
See portable baseline responses, matched comparison summary, and failed-answer review. Plotting scripts, editable data and rendered figures are included in the plotting package.
Download the editable Matplotlib/Spyder package. Open plot_v3_results.py for the model comparison or plot_v3_cap_study.py for the output-budget experiment. The package includes local data, PNG/SVG exports, CSV tables and instructions. The scripts were executed and the rendered figures inspected; Spyder's graphical application itself was not tested.
Development status
The row-level evaluation_status records the frozen pre-pilot authoring snapshot. Subsequent attempts and results belong in separate versioned result files; the evaluated questions and answers are not silently rewritten after seeing model behavior. The NASA application map records our proposed relevance and the remaining scope gaps.
All 1,000 reference responses pass the declared evaluator. A mechanical audit rejects single-field wrong-answer mutations, confirms imported answer mapping and verifies candidate projection. Assistant cross-review checks formulas and invariants, while independent human expert review remains pending. The original 400 instances were authored in this assistant session; no external question-authoring API was used and the session's exact model identity is not independently verified.
The next validity step is expert adjudication and pilot-error review, followed by genuinely new task families involving real public scientific data and executable work. Do not silently remove questions simply because a favored model fails them. Record reference corrections and score all affected models again on a new version.
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