[{"run_id":"20261014T203208-0851c9a1","observed_at":"2026-10-14 17:50:09.728220+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"0e5a89bc1cc440848b7fef4ff92fe23cc1c11c713f55095232709950ad3aa7a6","record_version_id":"cfbee353e0cc267d7b2eca168bb40855df4f9548bdbd9b0d6af16ee13ed5069f","job_id":"enrich-49752a259f17fab0f49665b3","output_id":"cce436bc3d28ea7fe82c8bb5b6f029f5a063c7f8ea7f4b522823e69b936ff943","section":"requirements","status":"valid","value_json":"{\"nodes\":[{\"children\":[],\"condition\":\"Graduate/professional standing\",\"course\":null,\"evidence\":\"Graduate/professional standing\",\"id\":\"r1\",\"kind\":\"condition\"}],\"notes\":[],\"root\":\"r1\",\"status\":\"parsed\"}","candidate_json":null,"error":null,"model":"Qwen/Qwen3.8-27B","model_revision":"1d4bf0f2ff6012fd82039f2fa52739d0dd7c60c0","selected_for_release":true},{"run_id":"20261014T203208-0851c9a1","observed_at":"2026-10-14 17:50:09.728220+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"0e5a89bc1cc440848b7fef4ff92fe23cc1c11c713f55095232709950ad3aa7a6","record_version_id":"cfbee353e0cc267d7b2eca168bb40855df4f9548bdbd9b0d6af16ee13ed5069f","job_id":"enrich-49752a259f17fab0f49665b3","output_id":"cce436bc3d28ea7fe82c8bb5b6f029f5a063c7f8ea7f4b522823e69b936ff943","section":"search_profile","status":"valid","value_json":"{\"activity_tags\":[],\"assumed_background\":[],\"search_phrases\":[\"galaxy evolution\",\"dark matter halos\",\"stellar initial mass function\",\"supermassive black holes\",\"active galactic nuclei\",\"reionization\"],\"skills_taught\":[{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"official_learning_outcomes\",\"outcome_index\":1,\"quote\":\"Summarize relevant observational techniques and their limitations.\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Summarizing observational techniques and their limitations\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"official_learning_outcomes\",\"outcome_index\":2,\"quote\":\"Articulate the physical and mathematical assumptions that underpin models of dark matter halo collapse and growth.\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Articulating physical and mathematical assumptions for dark matter halo models\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"official_learning_outcomes\",\"outcome_index\":3,\"quote\":\"Describe and/or mathematically model the core astrophysical processes that drive the evolution of the baryonic component of galaxies.\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Describing and modeling astrophysical processes in galaxy evolution\"}],\"summary\":{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"title\",\"quote\":\"GALAXIES\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"},{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"Properties of present day galaxies, including the Milky Way, the growth and evolution of dark matter halos, star formation and the stellar initial mass function, supermassive black holes and active galactic nuclei, groups and clusters of galaxies, galaxy evolution, reionization, and the first galaxies.\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Covers properties of present-day galaxies, dark matter halos, star formation, supermassive black holes, active galactic nuclei, galaxy groups/clusters, evolution, reionization, and first galaxies.\"},\"topics\":[{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"the growth and evolution of dark matter halos\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Dark matter halo growth and evolution\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"star formation and the stellar initial mass function\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Star formation and stellar initial mass function\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"supermassive black holes and active galactic nuclei\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Supermassive black holes and active galactic nuclei\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"galaxy evolution, reionization, and the first galaxies\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Galaxy evolution, reionization, and first galaxies\"}]}","candidate_json":null,"error":null,"model":"Qwen/Qwen3.8-27B","model_revision":"1d4bf0f2ff6012fd82039f2fa52739d0dd7c60c0","selected_for_release":true},{"run_id":"20261014T203208-0851c9a1","observed_at":"2026-10-14 17:50:09.728220+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"0e5a89bc1cc440848b7fef4ff92fe23cc1c11c713f55095232709950ad3aa7a6","record_version_id":"cfbee353e0cc267d7b2eca168bb40855df4f9548bdbd9b0d6af16ee13ed5069f","job_id":"enrich-49752a259f17fab0f49665b3","output_id":"cce436bc3d28ea7fe82c8bb5b6f029f5a063c7f8ea7f4b522823e69b936ff943","section":"student_experience","status":"insufficient_evidence","value_json":"{\"status\":\"insufficient_evidence\",\"themes\":[]}","candidate_json":null,"error":null,"model":"Qwen/Qwen3.8-27B","model_revision":"1d4bf0f2ff6012fd82039f2fa52739d0dd7c60c0","selected_for_release":true},{"run_id":"20261014T203208-0851c9a1","observed_at":"2026-10-14 17:50:09.728220+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"0e5a89bc1cc440848b7fef4ff92fe23cc1c11c713f55095232709950ad3aa7a6","record_version_id":"cfbee353e0cc267d7b2eca168bb40855df4f9548bdbd9b0d6af16ee13ed5069f","job_id":"enrich-49752a259f17fab0f49665b3","output_id":"cce436bc3d28ea7fe82c8bb5b6f029f5a063c7f8ea7f4b522823e69b936ff943","section":"student_summary","status":"valid","value_json":"{\"context_hash\":\"60e57862f1da1e2a4485ec05524b516cc45031a4fe5d225f2fa60f542e46032a\",\"course_id\":\"ASTRON 730\",\"current_instructors\":[],\"difficulty_workload\":[],\"errors\":[],\"historical_context\":[],\"message\":\"No course-specific reviews available\",\"offered\":false,\"profile_hash\":\"3f5110430805ccdd533c0c072df62d68a8a5f5441c4530bbdb15d419a199a09c\",\"quick_take\":[{\"citations\":[{\"course_id\":\"ASTRON 730\",\"run_id\":\"20261014T203208-0851c9a1\",\"source_record\":{\"entity_id\":\"11370584-5ddd-3329-9175-3bf7e462c60c\",\"file\":\"tables/observations.parquet\",\"kind\":\"grades\",\"source\":\"madgrades\"},\"table\":\"grades_latest\",\"term_id\":\"1222\",\"type\":\"grade\"},{\"course_id\":\"ASTRON 730\",\"run_id\":\"20261014T203208-0851c9a1\",\"source_record\":{\"entity_id\":\"11370584-5ddd-3329-9175-3bf7e462c60c\",\"file\":\"tables/observations.parquet\",\"kind\":\"grades\",\"source\":\"madgrades\"},\"table\":\"grades_latest\",\"term_id\":\"1242\",\"type\":\"grade\"},{\"course_id\":\"ASTRON 730\",\"run_id\":\"20261014T203208-0851c9a1\",\"source_record\":{\"entity_id\":\"11370584-5ddd-3329-9175-3bf7e462c60c\",\"file\":\"tables/observations.parquet\",\"kind\":\"grades\",\"source\":\"madgrades\"},\"table\":\"grades_latest\",\"term_id\":\"1262\",\"type\":\"grade\"}],\"text\":\"Recent recorded grades — Fall 2021: 3.75 GPA, 80.0% A/AB (n=10 letter grades); Fall 2023: 3.55 GPA, 90.5% A/AB (n=21 letter grades); Fall 2025: 3.60 GPA, 70.0% A/AB (n=10 letter grades).\"}],\"student_experience\":[],\"task_hash\":\"9dea82ef7f2113a5605c1c6030c4f9b19967eb742cc93a78268fb92357d29f5c\",\"teaching_history\":[],\"term_id\":\"1274\",\"term_name\":\"2027 Sprng\",\"version\":3}","candidate_json":null,"error":null,"model":"Qwen/Qwen3.8-27B","model_revision":"1d4bf0f2ff6012fd82039f2fa52739d0dd7c60c0","selected_for_release":true},{"run_id":"20260906T231458-5fdd2fff","observed_at":"2026-09-06 23:14:58.172943+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"ce21b7b91a359b9ff65ab62e21293cd0840490c6aa0f47f8d82405c21d41209c","record_version_id":"e2caddc3b2abf7bab4406d0d4de7b281b110f2568f9b59510d71f0d1cfabd16f","job_id":"enrich-5291a20b802b9bbbe22b24cb","output_id":"d18796ca2fb9249b222f7ba16a57bedce02c0a31e8cace3c8d76a66ba55ad5cc","section":"requirements","status":"invalid","value_json":null,"candidate_json":"{\"nodes\":[{\"children\":[],\"condition\":null,\"course\":null,\"evidence\":\"Graduate/professional standing\",\"id\":\"n0\",\"kind\":\"condition\"}],\"notes\":[],\"root\":\"n0\",\"status\":\"parsed\"}","error":"Non-course conditions must preserve verbatim source text","model":"nvidia/Qwen3.6-35B-A3B-NVFP4","model_revision":"1355db6a052410cfd62085d94b58866fd0f2c3c5","selected_for_release":false},{"run_id":"20260906T231458-5fdd2fff","observed_at":"2026-09-06 23:14:58.172943+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"ce21b7b91a359b9ff65ab62e21293cd0840490c6aa0f47f8d82405c21d41209c","record_version_id":"e2caddc3b2abf7bab4406d0d4de7b281b110f2568f9b59510d71f0d1cfabd16f","job_id":"enrich-5291a20b802b9bbbe22b24cb","output_id":"d18796ca2fb9249b222f7ba16a57bedce02c0a31e8cace3c8d76a66ba55ad5cc","section":"search_profile","status":"valid","value_json":"{\"assumed_background\":[],\"search_phrases\":[\"galaxy evolution\",\"dark matter halos\",\"active galactic nuclei\",\"star formation\",\"reionization\"],\"skills_taught\":[],\"summary\":{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"Properties of present day galaxies, including the Milky Way, the growth and evolution of dark matter halos, star formation and the stellar initial mass function, supermassive black holes and active galactic nuclei, groups and clusters of galaxies, galaxy evolution, reionization, and the first galaxies.\"}],\"text\":\"ASTRON 730 covers the properties, evolution, and components of present-day galaxies, including dark matter, star formation, and active nuclei.\"},\"topics\":[{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"Properties of present day galaxies, including the Milky Way\"}],\"text\":\"Properties of present-day galaxies and the Milky Way\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"the growth and evolution of dark matter halos\"}],\"text\":\"Growth and evolution of dark matter halos\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"star formation and the stellar initial mass function\"}],\"text\":\"Star formation and the stellar initial mass function\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"supermassive black holes and active galactic nuclei\"}],\"text\":\"Supermassive black holes and active galactic nuclei\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"groups and clusters of galaxies\"}],\"text\":\"Groups and clusters of galaxies\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"galaxy evolution, reionization, and the first galaxies\"}],\"text\":\"Galaxy evolution, reionization, and the first galaxies\"}]}","candidate_json":null,"error":null,"model":"nvidia/Qwen3.6-35B-A3B-NVFP4","model_revision":"1355db6a052410cfd62085d94b58866fd0f2c3c5","selected_for_release":false},{"run_id":"20260906T231458-5fdd2fff","observed_at":"2026-09-06 23:14:58.172943+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"ce21b7b91a359b9ff65ab62e21293cd0840490c6aa0f47f8d82405c21d41209c","record_version_id":"e2caddc3b2abf7bab4406d0d4de7b281b110f2568f9b59510d71f0d1cfabd16f","job_id":"enrich-5291a20b802b9bbbe22b24cb","output_id":"d18796ca2fb9249b222f7ba16a57bedce02c0a31e8cace3c8d76a66ba55ad5cc","section":"student_experience","status":"insufficient_evidence","value_json":"{\"status\":\"insufficient_evidence\",\"themes\":[]}","candidate_json":null,"error":null,"model":"nvidia/Qwen3.6-35B-A3B-NVFP4","model_revision":"1355db6a052410cfd62085d94b58866fd0f2c3c5","selected_for_release":false},{"run_id":"20260907T155543-ce3781c4","observed_at":"2026-09-07 15:55:43.033547+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"ce21b7b91a359b9ff65ab62e21293cd0840490c6aa0f47f8d82405c21d41209c","record_version_id":"e2caddc3b2abf7bab4406d0d4de7b281b110f2568f9b59510d71f0d1cfabd16f","job_id":"enrich-5590a4969e0a630fe46a86e8","output_id":"7ef97fff95e8e842ce8b86ce2743fd9e760f1674d07906b6090f30d662e31983","section":"requirements","status":"valid","value_json":"{\"nodes\":[{\"children\":[],\"condition\":\"Graduate/professional standing\",\"course\":null,\"evidence\":\"Graduate/professional standing\",\"id\":\"n0\",\"kind\":\"condition\"}],\"notes\":[],\"root\":\"n0\",\"status\":\"parsed\"}","candidate_json":null,"error":null,"model":"nvidia/Qwen3.6-35B-A3B-NVFP4","model_revision":"1355db6a052410cfd62085d94b58866fd0f2c3c5","selected_for_release":false},{"run_id":"20260907T155543-ce3781c4","observed_at":"2026-09-07 15:55:43.033547+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"ce21b7b91a359b9ff65ab62e21293cd0840490c6aa0f47f8d82405c21d41209c","record_version_id":"e2caddc3b2abf7bab4406d0d4de7b281b110f2568f9b59510d71f0d1cfabd16f","job_id":"enrich-5590a4969e0a630fe46a86e8","output_id":"7ef97fff95e8e842ce8b86ce2743fd9e760f1674d07906b6090f30d662e31983","section":"search_profile","status":"valid","value_json":"{\"assumed_background\":[],\"search_phrases\":[\"galaxy evolution\",\"dark matter halos\",\"active galactic nuclei\",\"star formation\",\"reionization\"],\"skills_taught\":[],\"summary\":{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"Properties of present day galaxies, including the Milky Way, the growth and evolution of dark matter halos, star formation and the stellar initial mass function, supermassive black holes and active galactic nuclei, groups and clusters of galaxies, galaxy evolution, reionization, and the first galaxies.\"}],\"text\":\"ASTRON 730 covers the properties, evolution, and components of present-day galaxies, including dark matter, star formation, and active nuclei.\"},\"topics\":[{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"Properties of present day galaxies, including the Milky Way\"}],\"text\":\"Properties of present-day galaxies and the Milky Way\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"the growth and evolution of dark matter halos\"}],\"text\":\"Growth and evolution of dark matter halos\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"star formation and the stellar initial mass function\"}],\"text\":\"Star formation and the stellar initial mass function\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"supermassive black holes and active galactic nuclei\"}],\"text\":\"Supermassive black holes and active galactic nuclei\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"groups and clusters of galaxies\"}],\"text\":\"Groups and clusters of galaxies\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"galaxy evolution, reionization, and the first galaxies\"}],\"text\":\"Galaxy evolution, reionization, and the first galaxies\"}]}","candidate_json":null,"error":null,"model":"nvidia/Qwen3.6-35B-A3B-NVFP4","model_revision":"1355db6a052410cfd62085d94b58866fd0f2c3c5","selected_for_release":false},{"run_id":"20260907T155543-ce3781c4","observed_at":"2026-09-07 15:55:43.033547+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"ce21b7b91a359b9ff65ab62e21293cd0840490c6aa0f47f8d82405c21d41209c","record_version_id":"e2caddc3b2abf7bab4406d0d4de7b281b110f2568f9b59510d71f0d1cfabd16f","job_id":"enrich-5590a4969e0a630fe46a86e8","output_id":"7ef97fff95e8e842ce8b86ce2743fd9e760f1674d07906b6090f30d662e31983","section":"student_experience","status":"insufficient_evidence","value_json":"{\"status\":\"insufficient_evidence\",\"themes\":[]}","candidate_json":null,"error":null,"model":"nvidia/Qwen3.6-35B-A3B-NVFP4","model_revision":"1355db6a052410cfd62085d94b58866fd0f2c3c5","selected_for_release":false},{"run_id":"20261014T203208-0851c9a1","observed_at":"2026-10-14 17:50:09.728220+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"0e5a89bc1cc440848b7fef4ff92fe23cc1c11c713f55095232709950ad3aa7a6","record_version_id":"cfbee353e0cc267d7b2eca168bb40855df4f9548bdbd9b0d6af16ee13ed5069f","job_id":"enrich-6556a505c10f448d98d02466","output_id":"fce5b58becd2fa2b7ccb1f6da0361e63f3757080deb35fd4d38d34bf2238ece7","section":"requirements","status":"valid","value_json":"{\"nodes\":[{\"children\":[],\"condition\":\"Graduate/professional standing\",\"course\":null,\"evidence\":\"Graduate/professional standing\",\"id\":\"r1\",\"kind\":\"condition\"}],\"notes\":[],\"root\":\"r1\",\"status\":\"parsed\"}","candidate_json":null,"error":null,"model":"Qwen/Qwen3.8-27B","model_revision":"1d4bf0f2ff6012fd82039f2fa52739d0dd7c60c0","selected_for_release":false},{"run_id":"20261014T203208-0851c9a1","observed_at":"2026-10-14 17:50:09.728220+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"0e5a89bc1cc440848b7fef4ff92fe23cc1c11c713f55095232709950ad3aa7a6","record_version_id":"cfbee353e0cc267d7b2eca168bb40855df4f9548bdbd9b0d6af16ee13ed5069f","job_id":"enrich-6556a505c10f448d98d02466","output_id":"fce5b58becd2fa2b7ccb1f6da0361e63f3757080deb35fd4d38d34bf2238ece7","section":"search_profile","status":"valid","value_json":"{\"activity_tags\":[],\"assumed_background\":[],\"search_phrases\":[\"galaxy evolution\",\"dark matter halos\",\"stellar initial mass function\",\"supermassive black holes\",\"active galactic nuclei\",\"reionization\"],\"skills_taught\":[{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"official_learning_outcomes\",\"outcome_index\":1,\"quote\":\"Summarize relevant observational techniques and their limitations.\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Summarizing observational techniques and their limitations\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"official_learning_outcomes\",\"outcome_index\":2,\"quote\":\"Articulate the physical and mathematical assumptions that underpin models of dark matter halo collapse and growth.\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Articulating physical and mathematical assumptions for dark matter halo models\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"official_learning_outcomes\",\"outcome_index\":3,\"quote\":\"Describe and/or mathematically model the core astrophysical processes that drive the evolution of the baryonic component of galaxies.\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Describing and modeling astrophysical processes in galaxy evolution\"}],\"summary\":{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"title\",\"quote\":\"GALAXIES\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"},{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"Properties of present day galaxies, including the Milky Way, the growth and evolution of dark matter halos, star formation and the stellar initial mass function, supermassive black holes and active galactic nuclei, groups and clusters of galaxies, galaxy evolution, reionization, and the first galaxies.\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Covers properties of present-day galaxies, dark matter halos, star formation, supermassive black holes, active galactic nuclei, galaxy groups/clusters, evolution, reionization, and first galaxies.\"},\"topics\":[{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"the growth and evolution of dark matter halos\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Dark matter halo growth and evolution\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"star formation and the stellar initial mass function\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Star formation and stellar initial mass function\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"supermassive black holes and active galactic nuclei\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Supermassive black holes and active galactic nuclei\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"galaxy evolution, reionization, and the first galaxies\",\"source_url\":\"https://guide.wisc.edu/courses/astron/\"}],\"text\":\"Galaxy evolution, reionization, and first galaxies\"}]}","candidate_json":null,"error":null,"model":"Qwen/Qwen3.8-27B","model_revision":"1d4bf0f2ff6012fd82039f2fa52739d0dd7c60c0","selected_for_release":false},{"run_id":"20261014T203208-0851c9a1","observed_at":"2026-10-14 17:50:09.728220+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"0e5a89bc1cc440848b7fef4ff92fe23cc1c11c713f55095232709950ad3aa7a6","record_version_id":"cfbee353e0cc267d7b2eca168bb40855df4f9548bdbd9b0d6af16ee13ed5069f","job_id":"enrich-6556a505c10f448d98d02466","output_id":"fce5b58becd2fa2b7ccb1f6da0361e63f3757080deb35fd4d38d34bf2238ece7","section":"student_experience","status":"insufficient_evidence","value_json":"{\"status\":\"insufficient_evidence\",\"themes\":[]}","candidate_json":null,"error":null,"model":"Qwen/Qwen3.8-27B","model_revision":"1d4bf0f2ff6012fd82039f2fa52739d0dd7c60c0","selected_for_release":false},{"run_id":"20260906T231458-5fdd2fff","observed_at":"2026-09-06 23:14:58.172943+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"ce21b7b91a359b9ff65ab62e21293cd0840490c6aa0f47f8d82405c21d41209c","record_version_id":"e2caddc3b2abf7bab4406d0d4de7b281b110f2568f9b59510d71f0d1cfabd16f","job_id":"enrich-789789da373eecc1ff75f626","output_id":"ffbbfa8a2d14d68c56302e66697f934e324bc421f3060d31f269073438464ffe","section":"requirements","status":"valid","value_json":"{\"nodes\":[{\"children\":[],\"condition\":\"Graduate/professional standing\",\"course\":null,\"evidence\":\"Graduate/professional standing\",\"id\":\"n0\",\"kind\":\"condition\"}],\"notes\":[],\"root\":\"n0\",\"status\":\"parsed\"}","candidate_json":null,"error":null,"model":"nvidia/Qwen3.6-35B-A3B-NVFP4","model_revision":"1355db6a052410cfd62085d94b58866fd0f2c3c5","selected_for_release":false},{"run_id":"20260906T231458-5fdd2fff","observed_at":"2026-09-06 23:14:58.172943+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"ce21b7b91a359b9ff65ab62e21293cd0840490c6aa0f47f8d82405c21d41209c","record_version_id":"e2caddc3b2abf7bab4406d0d4de7b281b110f2568f9b59510d71f0d1cfabd16f","job_id":"enrich-789789da373eecc1ff75f626","output_id":"ffbbfa8a2d14d68c56302e66697f934e324bc421f3060d31f269073438464ffe","section":"search_profile","status":"valid","value_json":"{\"assumed_background\":[],\"search_phrases\":[\"galaxy evolution\",\"dark matter halos\",\"active galactic nuclei\",\"star formation\",\"reionization\"],\"skills_taught\":[],\"summary\":{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"Properties of present day galaxies, including the Milky Way, the growth and evolution of dark matter halos, star formation and the stellar initial mass function, supermassive black holes and active galactic nuclei, groups and clusters of galaxies, galaxy evolution, reionization, and the first galaxies.\"}],\"text\":\"ASTRON 730 covers the properties, evolution, and components of present-day galaxies, including dark matter, star formation, and active nuclei.\"},\"topics\":[{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"Properties of present day galaxies, including the Milky Way\"}],\"text\":\"Properties of present-day galaxies and the Milky Way\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"the growth and evolution of dark matter halos\"}],\"text\":\"Growth and evolution of dark matter halos\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"star formation and the stellar initial mass function\"}],\"text\":\"Star formation and the stellar initial mass function\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"supermassive black holes and active galactic nuclei\"}],\"text\":\"Supermassive black holes and active galactic nuclei\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"groups and clusters of galaxies\"}],\"text\":\"Groups and clusters of galaxies\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"galaxy evolution, reionization, and the first galaxies\"}],\"text\":\"Galaxy evolution, reionization, and the first galaxies\"}]}","candidate_json":null,"error":null,"model":"nvidia/Qwen3.6-35B-A3B-NVFP4","model_revision":"1355db6a052410cfd62085d94b58866fd0f2c3c5","selected_for_release":false},{"run_id":"20260906T231458-5fdd2fff","observed_at":"2026-09-06 23:14:58.172943+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"ce21b7b91a359b9ff65ab62e21293cd0840490c6aa0f47f8d82405c21d41209c","record_version_id":"e2caddc3b2abf7bab4406d0d4de7b281b110f2568f9b59510d71f0d1cfabd16f","job_id":"enrich-789789da373eecc1ff75f626","output_id":"ffbbfa8a2d14d68c56302e66697f934e324bc421f3060d31f269073438464ffe","section":"student_experience","status":"insufficient_evidence","value_json":"{\"status\":\"insufficient_evidence\",\"themes\":[]}","candidate_json":null,"error":null,"model":"nvidia/Qwen3.6-35B-A3B-NVFP4","model_revision":"1355db6a052410cfd62085d94b58866fd0f2c3c5","selected_for_release":false},{"run_id":"20260907T155543-ce3781c4","observed_at":"2026-09-07 15:55:43.033547+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"ce21b7b91a359b9ff65ab62e21293cd0840490c6aa0f47f8d82405c21d41209c","record_version_id":"e2caddc3b2abf7bab4406d0d4de7b281b110f2568f9b59510d71f0d1cfabd16f","job_id":"enrich-8b774950c2b6adfdc46d1b82","output_id":"88f153a7ee051f8caab99c4760e60466f4170190ec78e5e0c09f7d922c245a55","section":"requirements","status":"valid","value_json":"{\"nodes\":[{\"children\":[],\"condition\":\"Graduate/professional standing\",\"course\":null,\"evidence\":\"Graduate/professional standing\",\"id\":\"n0\",\"kind\":\"condition\"}],\"notes\":[],\"root\":\"n0\",\"status\":\"parsed\"}","candidate_json":null,"error":null,"model":"nvidia/Qwen3.6-35B-A3B-NVFP4","model_revision":"1355db6a052410cfd62085d94b58866fd0f2c3c5","selected_for_release":false},{"run_id":"20260907T155543-ce3781c4","observed_at":"2026-09-07 15:55:43.033547+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"ce21b7b91a359b9ff65ab62e21293cd0840490c6aa0f47f8d82405c21d41209c","record_version_id":"e2caddc3b2abf7bab4406d0d4de7b281b110f2568f9b59510d71f0d1cfabd16f","job_id":"enrich-8b774950c2b6adfdc46d1b82","output_id":"88f153a7ee051f8caab99c4760e60466f4170190ec78e5e0c09f7d922c245a55","section":"search_profile","status":"valid","value_json":"{\"assumed_background\":[],\"search_phrases\":[\"galaxy evolution\",\"dark matter halos\",\"active galactic nuclei\",\"star formation\",\"reionization\"],\"skills_taught\":[],\"summary\":{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"Properties of present day galaxies, including the Milky Way, the growth and evolution of dark matter halos, star formation and the stellar initial mass function, supermassive black holes and active galactic nuclei, groups and clusters of galaxies, galaxy evolution, reionization, and the first galaxies.\"}],\"text\":\"ASTRON 730 covers the properties, evolution, and components of present-day galaxies, including dark matter, star formation, and active nuclei.\"},\"topics\":[{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"Properties of present day galaxies, including the Milky Way\"}],\"text\":\"Properties of present-day galaxies and the Milky Way\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"the growth and evolution of dark matter halos\"}],\"text\":\"Growth and evolution of dark matter halos\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"star formation and the stellar initial mass function\"}],\"text\":\"Star formation and the stellar initial mass function\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"supermassive black holes and active galactic nuclei\"}],\"text\":\"Supermassive black holes and active galactic nuclei\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"groups and clusters of galaxies\"}],\"text\":\"Groups and clusters of galaxies\"},{\"evidence\":[{\"course_id\":\"ASTRON 730\",\"field\":\"description\",\"quote\":\"galaxy evolution, reionization, and the first galaxies\"}],\"text\":\"Galaxy evolution, reionization, and the first galaxies\"}]}","candidate_json":null,"error":null,"model":"nvidia/Qwen3.6-35B-A3B-NVFP4","model_revision":"1355db6a052410cfd62085d94b58866fd0f2c3c5","selected_for_release":false},{"run_id":"20260907T155543-ce3781c4","observed_at":"2026-09-07 15:55:43.033547+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"ce21b7b91a359b9ff65ab62e21293cd0840490c6aa0f47f8d82405c21d41209c","record_version_id":"e2caddc3b2abf7bab4406d0d4de7b281b110f2568f9b59510d71f0d1cfabd16f","job_id":"enrich-8b774950c2b6adfdc46d1b82","output_id":"88f153a7ee051f8caab99c4760e60466f4170190ec78e5e0c09f7d922c245a55","section":"student_experience","status":"insufficient_evidence","value_json":"{\"status\":\"insufficient_evidence\",\"themes\":[]}","candidate_json":null,"error":null,"model":"nvidia/Qwen3.6-35B-A3B-NVFP4","model_revision":"1355db6a052410cfd62085d94b58866fd0f2c3c5","selected_for_release":false},{"run_id":"20260907T155543-ce3781c4","observed_at":"2026-09-07 15:55:43.033547+00:00","course_uid":"course_b3c2a88b55c044776e0e00d2","course_id":"ASTRON 730","catalog_version_id":"ce21b7b91a359b9ff65ab62e21293cd0840490c6aa0f47f8d82405c21d41209c","record_version_id":"e2caddc3b2abf7bab4406d0d4de7b281b110f2568f9b59510d71f0d1cfabd16f","job_id":"enrich-8b774950c2b6adfdc46d1b82","output_id":"88f153a7ee051f8caab99c4760e60466f4170190ec78e5e0c09f7d922c245a55","section":"student_summary","status":"valid","value_json":"{\"context_hash\":\"e5edf5e1a0b34749f239a1e4a3977ae3091cf52a6efc407d4132a22134d2946f\",\"course_id\":\"ASTRON 730\",\"current_instructors\":[],\"difficulty_workload\":[],\"errors\":[],\"historical_context\":[],\"message\":\"No course-specific reviews available\",\"offered\":false,\"profile_hash\":\"672f506f2fc2f46a071b9777f4a92cc197b2ccdeef25590e9285146d8c7e7f90\",\"quick_take\":[{\"citations\":[{\"course_id\":\"ASTRON 730\",\"run_id\":\"20260907T155543-ce3781c4\",\"source_record\":{\"entity_id\":\"11370584-5ddd-3329-9175-3bf7e462c60c\",\"file\":\"tables/observations.parquet\",\"kind\":\"grades\",\"source\":\"madgrades\"},\"table\":\"grades_latest\",\"term_id\":\"1222\",\"type\":\"grade\"},{\"course_id\":\"ASTRON 730\",\"run_id\":\"20260907T155543-ce3781c4\",\"source_record\":{\"entity_id\":\"11370584-5ddd-3329-9175-3bf7e462c60c\",\"file\":\"tables/observations.parquet\",\"kind\":\"grades\",\"source\":\"madgrades\"},\"table\":\"grades_latest\",\"term_id\":\"1242\",\"type\":\"grade\"},{\"course_id\":\"ASTRON 730\",\"run_id\":\"20260907T155543-ce3781c4\",\"source_record\":{\"entity_id\":\"11370584-5ddd-3329-9175-3bf7e462c60c\",\"file\":\"tables/observations.parquet\",\"kind\":\"grades\",\"source\":\"madgrades\"},\"table\":\"grades_latest\",\"term_id\":\"1262\",\"type\":\"grade\"}],\"text\":\"Recent recorded grades — Fall 2021: 3.75 GPA, 80.0% A/AB (n=10 letter grades); Fall 2023: 3.55 GPA, 90.5% A/AB (n=21 letter grades); Fall 2025: 3.60 GPA, 70.0% A/AB (n=10 letter grades).\"}],\"student_experience\":[],\"task_hash\":\"74fb0997943e888960bbc9e47db8c4fd12e4292d55c20509d8d89db6a9910f68\",\"teaching_history\":[],\"term_id\":\"1272\",\"term_name\":\"2026 Fall\",\"version\":2}","candidate_json":null,"error":null,"model":"nvidia/Qwen3.6-35B-A3B-NVFP4","model_revision":"1355db6a052410cfd62085d94b58866fd0f2c3c5","selected_for_release":false}]