size_categories:n<1K format:parquet modality:tabular modality:text library:datasets library:pandas library:mlcroissant library:polars library:distilabel region:us synthetic distilabel rlaif
---
size_categories: n<1K
dataset_info:
  features:
  - name: text
    dtype: string
  - name: id
    dtype: string
  - name: dump
    dtype: string
  - name: url
    dtype: string
  - name: file_path
    dtype: string
  - name: language
    dtype: string
  - name: language_score
    dtype: float64
  - name: token_count
    dtype: int64
  - name: score
    dtype: float64
  - name: int_score
    dtype: int64
  - name: generated_system_prompt
    dtype: string
  - name: distilabel_metadata
    struct:
    - name: raw_output_chat_generation_2
      dtype: string
  - name: gen_conv_model_name
    dtype: string
  - name: system_prompt
    dtype: string
  - name: conversation
    list:
    - name: content
      dtype: string
    - name: role
      dtype: string
  - name: generations
    sequence: string
  - name: generations_model_names
    sequence: string
  splits:
  - name: train
    num_bytes: 1568042
    num_examples: 100
  download_size: 839829
  dataset_size: 1568042
configs:
- config_name: default
  data_files:
  - split: train
    path: data/train-*
tags:
- synthetic
- distilabel
- rlaif
---

<p align="left">
  <a href="https://github.com/argilla-io/distilabel">
    <img src="https://raw.githubusercontent.com/argilla-io/distilabel/main/docs/assets/distilabel-badge-light.png" alt="Built with Distilabel" width="200" height="32"/>
  </a>
</p>

# Dataset Card for fine-preferences-magpie-generated-system-prompt-v0

This dataset has been created with [distilabel](https://distilabel.argilla.io/).



## Dataset Summary

This dataset contains a `pipeline.yaml` which can be used to reproduce the pipeline that generated it in distilabel using the `distilabel` CLI:

```console
distilabel pipeline run --config "https://huggingface.co/datasets/distilabel-internal-testing/fine-preferences-magpie-generated-system-prompt-v0/raw/main/pipeline.yaml"
```

or explore the configuration:

```console
distilabel pipeline info --config "https://huggingface.co/datasets/distilabel-internal-testing/fine-preferences-magpie-generated-system-prompt-v0/raw/main/pipeline.yaml"
```

## Dataset structure

The examples have the following structure per configuration:


<details><summary> Configuration: default </summary><hr>

```json
{
    "conversation": [
        {
            "content": "What do you know about gamma-ray bursts?",
            "role": "user"
        },
        {
            "content": "Gamma-ray bursts (GRBs) are incredibly powerful and explosive events that occur in the universe. They are the most energetic events known, releasing as much energy as an entire galaxy in a matter of seconds! They are thought to occur when massive stars collapse or when neutron stars or black holes merge.\n\nGRBs are characterized by a sudden and intense release of gamma radiation, which is the most energetic form of electromagnetic radiation. This radiation is so powerful that it can be detected from millions of light-years away, making GRBs visible from great distances.\n\nOne of the fascinating things about GRBs is their potential impact on their surroundings. The energy released by a GRB can heat up the surrounding gas to incredibly high temperatures, potentially creating massive shells and holes in the interstellar medium. This can have a significant effect on the structure and evolution of galaxies.\n\nWould you like to know more about the potential effects of GRBs on galaxies?",
            "role": "assistant"
        },
        {
            "content": "What kind of shells and holes are we talking about here?",
            "role": "user"
        },
        {
            "content": "The shells and holes I mentioned are actually massive structures that can form in the interstellar medium (ISM) of galaxies. The ISM is the material that fills the space between stars, including gas and dust.\n\nWhen a GRB occurs, it can release an enormous amount of energy into the surrounding ISM. This energy can heat up the gas to incredibly high temperatures, causing it to expand rapidly and create a bubble or shell. These shells can be enormous, stretching for thousands of light-years across.\n\nIn some cases, the energy released by the GRB can be so great that it can actually blow a hole through the ISM, creating a cavity or void in the galaxy. These holes can be just as large as the shells, and can have a significant impact on the surrounding galaxy.\n\nIt\u0027s worth noting that these shells and holes are not just theoretical constructs - they have actually been observed in some galaxies. In fact, some galaxies have been found to have multiple shells and holes, which are thought to have been created by repeated GRB events.\n\nWould you like to know more about how these shells and holes might form, or what they can tell us about the galaxies they\u0027re found in?",
            "role": "assistant"
        },
        {
            "content": "What do you think is the most interesting aspect of gamma-ray bursts?",
            "role": "user"
        }
    ],
    "distilabel_metadata": {
        "raw_output_chat_generation_2": "There are many fascinating aspects of gamma-ray bursts (GRBs), but if I had to choose one, I\u0027d say it\u0027s their potential to serve as \"cosmic probes\" of the universe.\n\nGRBs are so powerful that they can be seen from enormous distances, allowing us to study the universe in ways that would be impossible otherwise. Because they\u0027re so bright, they can be used to probe the intergalactic medium (IGM), the diffuse gas that fills the vast spaces between galaxies.\n\nAs the gamma rays from a GRB travel through the IGM, they interact with the gas and dust, leaving a signature that can be detected by telescopes. By analyzing this signature, astronomers can learn about the composition, density, and temperature of the IGM, as well as the distribution of matter and energy in the universe.\n\nIn essence, GRBs act as \"flashlights\" that shine through the universe, illuminating the dark matter and dark energy that make up about 95% of the universe\u0027s mass-energy budget. This allows us to study the universe\u0027s large-scale structure, the formation of galaxies, and even the properties of dark matter and dark energy themselves.\n\nAdditionally, GRBs can also be used to study the extreme physics of black holes, neutron stars,"
    },
    "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",
    "gen_conv_model_name": "meta-llama/Meta-Llama-3-70B-Instruct",
    "generated_system_prompt": "Generate a multi-turn conversation between a user and an AI assistant based on the provided document.\n\n## 1. Preparation\nRead and understand the provided document, but do not mention the document in the conversation.\n\n## 2. Interaction Structure and Roles\nThe conversation will involve a user and an AI assistant. The user will ask questions or make statements, and the AI assistant will respond accordingly.\n\n## 3. User Task Characteristics\nThe user is curious and may ask follow-up questions based on the AI assistant\u0027s responses.\n\n## 4. AI Assistant Characteristics\nThe AI assistant is knowledgeable about the topic discussed in the document and can provide clear and concise explanations.\n\n## 5. Engagement\nThe conversation should be natural and engaging, with the AI assistant responding in a friendly and helpful tone.\n\n## 6. General Guidelines\nThe conversation should be informative and accurate, and should not mention the document or any specific details about it. The AI assistant should provide explanations and answers based on the topic, without referencing the document itself.",
    "generations": [
        " There are many fascinating aspects of gamma-ray bursts, but I think one of the most interesting is their potential role in shaping the universe.\n\nAs I mentioned earlier, GRBs are incredibly powerful events that can release massive amounts of energy into their surroundings. This energy can have a significant impact on the structure and evolution of galaxies.\n\nFor example, the shells and holes created by GRBs can affect the distribution of gas and dust in a galaxy, potentially influencing the formation of new stars. The energy released by GRBs can also heat up the surrounding gas, which can have a number of consequences for the galaxy.\n\nBut perhaps even more intriguing is the possibility that GRBs could play a role in the reionization of the universe. After the Big Bang, the universe was filled with a thick fog of neutral hydrogen gas. Over time, this gas was gradually ionized by the first stars and galaxies, a process known as reionization.\n\nIt\u0027s possible that GRBs could have contributed to this process by releasing high-energy photons that could ionize the neutral hydrogen gas. Some researchers have even suggested that GRBs could have been responsible for up to 5",
        "There are several fascinating aspects of gamma-ray bursts (GRBs), but one that stands out is their potential role in shaping the structure and evolution of galaxies. As I mentioned earlier, the energy released by a GRB can create massive shells and holes in the interstellar medium (ISM) of galaxies. These structures can have a significant impact on the galaxy\u0027s star formation, gas distribution, and overall structure.\n\nAnother interesting aspect of GRBs is their potential connection to the formation of heavy elements in the universe. When a massive star collapses into a black hole or neutron star, it can produce a GRB. This process also results in the formation of heavy elements, such as gold, platinum, and uranium. Some scientists believe that GRBs may have been responsible for the production of a significant fraction of these elements in the early universe.\n\nFinally, GRBs are also important tools for studying the universe itself. Because they are so bright and can be detected from great distances, they can be used as \"cosmic lighthouses\" to help us understand the large-scale structure of the universe and the distribution of matter in it.\n\nWould you like to know",
        "There are many fascinating aspects of gamma-ray bursts (GRBs), but if I had to choose one, I\u0027d say it\u0027s their potential to serve as \"cosmic probes\" of the universe.\n\nGRBs are so powerful that they can be seen from enormous distances, allowing us to study the universe in ways that would be impossible otherwise. Because they\u0027re so bright, they can be used to probe the intergalactic medium (IGM), the diffuse gas that fills the vast spaces between galaxies.\n\nAs the gamma rays from a GRB travel through the IGM, they interact with the gas and dust, leaving a signature that can be detected by telescopes. By analyzing this signature, astronomers can learn about the composition, density, and temperature of the IGM, as well as the distribution of matter and energy in the universe.\n\nIn essence, GRBs act as \"flashlights\" that shine through the universe, illuminating the dark matter and dark energy that make up about 95% of the universe\u0027s mass-energy budget. This allows us to study the universe\u0027s large-scale structure, the formation of galaxies, and even the properties of dark matter and dark energy themselves.\n\nAdditionally, GRBs can also be used to study the extreme physics of black holes, neutron stars,"
    ],
    "generations_model_names": [
        "mistralai/Mixtral-8x7B-Instruct-v0.1",
        "NousResearch/Nous-Hermes-2-Mixtral-8x7B-DPO",
        "meta-llama/Meta-Llama-3-70B-Instruct"
    ],
    "id": "\u003curn:uuid:e2300ad5-01dd-4e80-92b3-7ec88785cc9d\u003e",
    "int_score": 3,
    "language": "en",
    "language_score": 0.9126408100128174,
    "score": 2.765625,
    "system_prompt": "Generate a multi-turn conversation between a user and an AI assistant based on the provided document.\n\n## 1. Preparation\nRead and understand the provided document, but do not mention the document in the conversation.\n\n## 2. Interaction Structure and Roles\nThe conversation will involve a user and an AI assistant. The user will ask questions or make statements, and the AI assistant will respond accordingly.\n\n## 3. User Task Characteristics\nThe user is curious and may ask follow-up questions based on the AI assistant\u0027s responses.\n\n## 4. AI Assistant Characteristics\nThe AI assistant is knowledgeable about the topic discussed in the document and can provide clear and concise explanations.\n\n## 5. Engagement\nThe conversation should be natural and engaging, with the AI assistant responding in a friendly and helpful tone.\n\n## 6. General Guidelines\nThe conversation should be informative and accurate, and should not mention the document or any specific details about it. The AI assistant should provide explanations and answers based on the topic, without referencing the document itself.## Document\n\nPrevious abstract Next abstract\nSession 40 - The Interstellar Medium.\nDisplay session, Tuesday, June 09\nGamma 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.\nProgram listing for Tuesday",
    "text": "Previous abstract Next abstract\nSession 40 - The Interstellar Medium.\nDisplay session, Tuesday, June 09\nGamma 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.\nProgram listing for Tuesday",
    "token_count": 208,
    "url": "http://aas.org/archives/BAAS/v30n2/aas192/abs/S040015.html"
}
```

This subset can be loaded as:

```python
from datasets import load_dataset

ds = load_dataset("distilabel-internal-testing/fine-preferences-magpie-generated-system-prompt-v0", "default")
```

Or simply as it follows, since there's only one configuration and is named `default`: 

```python
from datasets import load_dataset

ds = load_dataset("distilabel-internal-testing/fine-preferences-magpie-generated-system-prompt-v0")
```


</details>
