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: system_prompt
    dtype: string
  - name: conversation
    list:
    - name: content
      dtype: string
    - name: role
      dtype: string
  - name: gen_conv_model_name
    dtype: string
  - name: generations
    sequence: string
  - name: distilabel_metadata
    struct:
    - name: raw_output_chat_generation_2
      dtype: string
  - name: generations_model_names
    sequence: string
  splits:
  - name: train
    num_bytes: 1602941
    num_examples: 100
  download_size: 796068
  dataset_size: 1602941
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-v6-instructy

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-v6-instructy/raw/main/pipeline.yaml"
```

or explore the configuration:

```console
distilabel pipeline info --config "https://huggingface.co/datasets/distilabel-internal-testing/fine-preferences-magpie-v6-instructy/raw/main/pipeline.yaml"
```

## Dataset structure

The examples have the following structure per configuration:


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

```json
{
    "conversation": [
        {
            "content": "What is the interstellar medium?",
            "role": "user"
        },
        {
            "content": "The interstellar medium, or ISM, refers to the material that fills the space between stars in a galaxy. It\u0027s a complex mixture of various gases, including hydrogen, helium, and heavier elements, as well as dust particles. The ISM plays a crucial role in the formation of new stars and planets, as it provides the raw material for these processes.\n\nThink of the ISM as a vast, diffuse cloud that permeates the galaxy, with regions of varying density and composition. It\u0027s not just a passive backdrop for star formation, though \u2013 the ISM also interacts with stars and other celestial objects, influencing their evolution and behavior.\n\nIn the context of spiral galaxies like our own Milky Way, the ISM is particularly important, as it helps regulate the flow of energy and matter within the galaxy. It\u0027s a dynamic, constantly evolving environment that\u0027s shaped by a variety of processes, including supernovae explosions, stellar winds, and the formation of new stars.",
            "role": "assistant"
        },
        {
            "content": "What are the effects of a Gamma Ray Burst (GRB) on the interstellar medium?",
            "role": "user"
        },
        {
            "content": "Gamma Ray Bursts (GRBs) are incredibly powerful explosions that can have a profound impact on the interstellar medium (ISM). When a GRB occurs, it releases an enormous amount of energy, which can heat the surrounding gas to extremely high temperatures, often exceeding 10 million degrees Kelvin.\n\nThis intense heat can create a massive bubble of hot, ionized gas that expands rapidly into the surrounding ISM. As this bubble grows, it can sweep up and displace significant amounts of gas and dust, creating a large, shell-like structure that can reach sizes of up to several kiloparsecs (kpc) in diameter.\n\nThe effects of a GRB on the ISM can be quite dramatic. For one, the explosion can create a \"hole\" in the ISM, evacuating a large region of gas and dust. This can have a significant impact on the local star formation process, as the ISM is the raw material from which new stars are born.\n\nAdditionally, the momentum imparted to the ISM during the explosion can be substantial, causing the bubble to \"snowplow\" through the surrounding material and potentially triggering the formation of new stars or affecting the motion of nearby stars and gas clouds.\n\nIt\u0027s worth noting that GRBs are thought to be responsible for creating some of the giant shells and holes observed in the ISM of spiral galaxies, which can be difficult to explain using traditional models of star formation and supernovae explosions.",
            "role": "assistant"
        },
        {
            "content": "What is the significance of the energy released by a GRB?",
            "role": "user"
        }
    ],
    "distilabel_metadata": {
        "raw_output_chat_generation_2": "The energy released by a Gamma Ray Burst (GRB) is truly staggering and has significant implications for our understanding of the universe. Here are some reasons why:\n\n1. **Most energetic events in the universe**: GRBs are the most powerful explosions in the universe, releasing enormous amounts of energy in the form of gamma rays, X-rays, and other forms of electromagnetic radiation. The total energy released can be as high as 10^54 erg, which is roughly 100 times the energy released by a typical supernova.\n2. **Cosmic rays and high-energy particles**: The energy released by a GRB can accelerate particles to incredible energies, producing cosmic rays that can travel across vast distances. These particles can interact with the interstellar medium, influencing the formation of stars and planets.\n3. **Impact on the intergalactic medium**: The energy released by a GRB can ionize and heat the intergalactic medium (IGM), the diffuse gas that fills the vast spaces between galaxies. This can affect the formation of galaxies and the distribution of matter in the universe.\n4. **Probes of the distant universe**: Because GRBs are so luminous, they can be seen at vast distances, making them useful probes of the distant universe. By studying the light curves and spectra of GRBs, astronomers can learn about the properties of the IGM, the distribution of matter, and the expansion history of the universe.\n5. **Effects on the local universe**: The energy released by a GRB can also have significant effects on the local universe. For example, it can ionize and displace gas in the Milky Way\u0027s disk, affecting the formation of stars and planets in our own galaxy.\n6. **Triggering star formation**: The energy released by a GRB can compress and shock nearby molecular clouds, triggering the formation of new stars. This process can lead to the creation of multiple generations of stars, influencing the chemical evolution of galaxies.\n7. **Insights into extreme physics**: GRBs offer a unique window into extreme physical processes, such as relativistic jets, black hole formation, and neutron star mergers. By studying GRBs, astronomers can gain insights into these exotic phenomena.\n\nIn summary, the energy released by a GRB is a significant aspect of these events, with far-reaching implications for our understanding of the universe, from the formation of stars and galaxies to the properties of the intergalactic medium and the distant universe."
    },
    "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",
    "generations": [
        " The energy released by a Gamma Ray Burst (GRB) is truly staggering. A single GRB can release as much energy as the sun will emit over its entire 10-billion-year lifetime. In fact, some GRBs have been estimated to emit as much as 10^54 joules of energy \u2013 the equivalent of more than a billion trillion (10^21) suns!\n\nThis enormous amount of energy is released in the form of gamma rays, the most energetic form of electromagnetic radiation. These gamma rays can travel vast distances across the universe, and their high energy allows them to penetrate even the densest regions of interstellar and intergalactic space.\n\nThe energy released by a GRB can have far-reaching consequences. For example, it can create a massive shockwave that propagates through the interstellar medium (ISM), heating and ionizing the surrounding gas and potentially triggering the formation of new stars.\n\nAdditionally, the intense radiation from a GRB can have a significant impact on the composition of the ISM, as it can break apart atoms and molecules, creating a hot, highly ionized plasma. This can have a profound effect on the chemistry of the ISM, as well as the physical processes that govern its behavior.\n\nFinally, the energy released by a GRB can also have cosmological implications. For example, some researchers have suggested that a particularly powerful GRB could have contributed to the reionization of the universe, which occurred during the first few hundred million years after the Big Bang. During this period, the universe transitioned from a neutral state to a highly ionized state, and GRBs could have provided a significant source of ionizing radiation to drive this process.",
        "The energy released by a Gamma Ray Burst (GRB) is truly astounding. GRBs are the most powerful explosions in the universe since the Big Bang, releasing an enormous amount of energy in a short period of time.\n\nThe energy released by a GRB is typically measured in the form of gamma rays, which are the most energetic form of electromagnetic radiation. GRBs can emit energy at a rate of up to 10^51 ergs per second, which is more than the energy produced by our Sun in its entire lifetime. In fact, a typical GRB can release more energy than our Sun will produce in the next 10 billion years.\n\nThe significance of this energy release lies in its potential to shape the structure and evolution of the universe. The intense radiation and high-energy particles emitted by a GRB can have profound effects on the surrounding interstellar medium (ISM), as we discussed earlier. These effects can include heating and ionizing the gas, triggering the formation of new stars or inhibiting it, and even affecting the motion of nearby stars and gas clouds.\n\nMoreover, the energy released by GRBs can have cosmological implications. For instance, the energy density of GRBs in the early universe (around the time of the cosmic microwave background) might have contributed to the reionization of hydrogen gas, which is a critical step in the formation of the first stars and galaxies.\n\nAdditionally, GRBs are thought to be potential sources of high-energy cosmic rays and neutrinos, which can provide valuable insights into the fundamental nature of the universe and its constituents.\n\nIn summary, the energy released by a GRB is significant because it can have a profound impact on its immediate surroundings and potentially shape the evolution of the universe as a whole. It also serves as a powerful probe of the most extreme environments and physical processes in the cosmos.",
        "The energy released by a Gamma Ray Burst (GRB) is truly staggering and has significant implications for our understanding of the universe. Here are some reasons why:\n\n1. **Most energetic events in the universe**: GRBs are the most powerful explosions in the universe, releasing enormous amounts of energy in the form of gamma rays, X-rays, and other forms of electromagnetic radiation. The total energy released can be as high as 10^54 erg, which is roughly 100 times the energy released by a typical supernova.\n2. **Cosmic rays and high-energy particles**: The energy released by a GRB can accelerate particles to incredible energies, producing cosmic rays that can travel across vast distances. These particles can interact with the interstellar medium, influencing the formation of stars and planets.\n3. **Impact on the intergalactic medium**: The energy released by a GRB can ionize and heat the intergalactic medium (IGM), the diffuse gas that fills the vast spaces between galaxies. This can affect the formation of galaxies and the distribution of matter in the universe.\n4. **Probes of the distant universe**: Because GRBs are so luminous, they can be seen at vast distances, making them useful probes of the distant universe. By studying the light curves and spectra of GRBs, astronomers can learn about the properties of the IGM, the distribution of matter, and the expansion history of the universe.\n5. **Effects on the local universe**: The energy released by a GRB can also have significant effects on the local universe. For example, it can ionize and displace gas in the Milky Way\u0027s disk, affecting the formation of stars and planets in our own galaxy.\n6. **Triggering star formation**: The energy released by a GRB can compress and shock nearby molecular clouds, triggering the formation of new stars. This process can lead to the creation of multiple generations of stars, influencing the chemical evolution of galaxies.\n7. **Insights into extreme physics**: GRBs offer a unique window into extreme physical processes, such as relativistic jets, black hole formation, and neutron star mergers. By studying GRBs, astronomers can gain insights into these exotic phenomena.\n\nIn summary, the energy released by a GRB is a significant aspect of these events, with far-reaching implications for our understanding of the universe, from the formation of stars and galaxies to the properties of the intergalactic medium and the distant universe."
    ],
    "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": "You\u0027re a helpful AI assistant that responds user questions based on a document\u0027s content, without explicitly mentioning the document. \nFollow these guidelines:\n\n## 1. Preparation\n- Absorb the document\u0027s main topics, key points, and themes.\n- The conversation will be between two participants: a curious user and a knowledgeable AI assistant.\n\n## 2. Conversation Structure\n- Start with a user query related to the document\u0027s main topic, without referencing the document.\n- The AI assistant should respond using information from the document, presented as its own knowledge.\n- Alternate between user questions/comments and AI responses.\n- Cover main points from the document through this natural dialogue.\n\n## 3. User Characteristics\n- The user should ask relevant questions and express interest in the topic.\n- User messages can include follow-up questions, requests for clarification, or sharing of personal opinions.\n- The user\u0027s knowledge level can vary, allowing the AI to explain concepts when necessary.\n- Incorporate a diverse range of verbs, avoiding repetition. Ensure queries are compatible with AI model\u0027s text generation functions and are limited to 1-3 sentences. Design queries to be self-contained and standalone. Blend interrogative (e.g., \"What is the significance of x?\") and imperative (e.g., \"Detail the process of x.\") styles.\n\n## 4. AI Assistant Characteristics\n- Respond comprehensively and accurately based on the document\u0027s content.\n- Adapt explanations to the user\u0027s apparent level of understanding.\n- Offer analogies, examples, or scenarios to illustrate points when appropriate.\n- Be prepared to clarify or expand on previous statements if the user asks.\n\n## 5. Engagement\n- Maintain a helpful and engaging tone throughout the conversation.\n- The AI should encourage deeper exploration of topics through its responses.\n- Conclude the conversation with a summary or thought-provoking insight.\n\n## 6. General Guidelines\n- Ensure the conversation flows naturally and coherently.\n- The AI\u0027s knowledge should seem broad but not omniscient, reflecting the document\u0027s scope.\n- Adapt to any specific instructions provided about the conversation\u0027s focus or detail level.\n\n## 7. User Role Refinement\n- The user should primarily ask follow-up questions based on the AI\u0027s previous response.\n- User questions should build on the information just provided, showing curiosity and engagement with the topic at hand.\n- Avoid having the user abruptly introduce new topics from the document without context.\n\nRemember: Never mention or directly reference the source document in the generated conversation. The AI assistant should present information as if it\u0027s part of its general knowledge base.\n\n## Document\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\n",
    "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-v6-instructy", "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-v6-instructy")
```


</details>
