distilabel-internal-testing/fine-preferences-test-6
收藏数据集卡片：fine-preferences-test-6
数据集概述
该数据集包含一个 pipeline.yaml 文件，可用于在 distilabel 中重现生成该数据集的管道。
数据集结构
数据集的示例具有以下结构：
配置：default
json { "context": "Previous abstract Next abstract Session 40 - The Interstellar Medium. Display session, Tuesday, June 09 Gamma Ray Burst (GRB) explosions can make kpc-size shells and holes in the interstellar media (ISM) of spiral galaxies if much of the energy heats the local gas to above 10^7 K. Disk blowout is probably the major cause for energy loss in this case, but the momentum acquired during the pressurized expansion phase can be large enough that the bubble still snowplows to a kpc diameter. This differs from the standard model for the origin of such shells by multiple supernovae, which may have problems with radiative cooling, evaporative losses, and disk blow-out. Evidence for giant shells with energies of \sim10^53 ergs are summarized. Some contain no obvious central star clusters and may be GRB remnants, although sufficiently old clusters would be hard to detect. The expected frequency of GRBs in normal galaxies can account for the number of such shells. Program listing for Tuesday", "conversation": [ { "content": "Whatu0027s the most powerful explosion in the universe?", "role": "User" }, { "content": "Thatu0027s a great question! The most powerful explosion in the universe is likely a Gamma Ray Burst, or GRB. Theyu0027re incredibly energetic events that can release as much as 10^53 ergs of energy.", "role": "Assistant" }, { "content": "What kind of damage can a GRB do to a galaxy?", "role": "User" }, { "content": "A GRB can create enormous shells and holes in the interstellar medium of a galaxy, potentially even blowing out the entire disk. This can have a huge impact on the galaxyu0027s structure and evolution.", "role": "Assistant" }, { "content": "How does a GRB compare to a supernova?", "role": "User" }, { "content": "While both are incredibly powerful, a GRB is much more energetic than a supernova. A GRB can release hundreds of times more energy than a supernova, making it a much more significant event in the life of a galaxy.", "role": "Assistant" }, { "content": "Are GRBs common in the universe?", "role": "User" }, { "content": "Actually, GRBs are relatively rare in the universe. However, theyu0027re thought to occur in normal galaxies at a rate that could account for the number of giant shells we observe.", "role": "Assistant" }, { "content": "Can we see the remnants of a GRB in a galaxy?", "role": "User" }, { "content": "Yes, itu0027s possible to see the remnants of a GRB in a galaxy. In fact, some giant shells have been observed that may be the remnants of a GRB, although it can be difficult to detect the central star cluster if itu0027s very old.", "role": "Assistant" }, { "content": "How do astronomers detect these giant shells?", "role": "User" } ], "distilabel_metadata": { "raw_output_generate_conv_with_context_0": "User: Whatu0027s the most powerful explosion in the universe? Assistant: Thatu0027s a great question! The most powerful explosion in the universe is likely a Gamma Ray Burst, or GRB. Theyu0027re incredibly energetic events that can release as much as 10^53 ergs of energy. User: What kind of damage can a GRB do to a galaxy? Assistant: A GRB can create enormous shells and holes in the interstellar medium of a galaxy, potentially even blowing out the entire disk. This can have a huge impact on the galaxyu0027s structure and evolution. User: How does a GRB compare to a supernova? Assistant: While both are incredibly powerful, a GRB is much more energetic than a supernova. A GRB can release hundreds of times more energy than a supernova, making it a much more significant event in the life of a galaxy. User: Are GRBs common in the universe? Assistant: Actually, GRBs are relatively rare in the universe. However, theyu0027re thought to occur in normal galaxies at a rate that could account for the number of giant shells we observe. User: Can we see the remnants of a GRB in a galaxy? Assistant: Yes, itu0027s possible to see the remnants of a GRB in a galaxy. In fact, some giant shells have been observed that may be the remnants of a GRB, although it can be difficult to detect the central star cluster if itu0027s very old. User: How do astronomers detect these giant shells?" }, "dump": "CC-MAIN-2013-20", "file_path": "s3://commoncrawl/crawl-data/CC-MAIN-2013-20/segments/1368696381249/warc/CC-MAIN-20130516092621-00000-ip-10-60-113-184.ec2.internal.warc.gz", "id": "u003curn:uuid:e2300ad5-01dd-4e80-92b3-7ec88785cc9du003e", "int_score": 3, "language": "en", "language_score": 0.9126408100128174, "model_name": "meta-llama/Meta-Llama-3-70B-Instruct", "score": 2.765625, "token_count": 208, "url": "http://aas.org/archives/BAAS/v30n2/aas192/abs/S040015.html" }
加载数据集
可以使用以下代码加载数据集：
python from datasets import load_dataset
ds = load_dataset("distilabel-internal-testing/fine-preferences-test-6")
