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README.md
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@@ -136,7 +136,7 @@ The features we extract for each repository are illustrated in the example below
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- **retrieval_date**: date when the repo was scraped from GitHub
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We start by retrieving repositories with more than **900** stars using **two-month tumbling windows**. If we hit the **1000** repository limit per window (for a personal GitHub account), we shorten the
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search space to a **one-month window** and restart the iteration. Otherwise, the window advances by two months. Once the
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Although the creation date window can be reduced even further (week or day level), a one-month window was enough for our needs. After retrieving the repositories, we extract all the files with a
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*.java* extension.
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@@ -216,7 +216,7 @@ Thus, given the increased **complexity** and **size** of Java files, we consider
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Furthermore, **k = 9** was shown to be a safe choice for [large research articles](http://infolab.stanford.edu/~ullman/mmds/book.pdf), however, for our needs, 7-shingles strike a balance between accuracy and
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computational efficiency, crucial for handling the **Java-Stack v2’s size** of over **222 M** files. This choice provides better computational efficiency by reducing the number of comparisons while maintaining a manageable shingle space.
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Lastly, we use a **Jaccard similarity threshold** of **0.7**, which proved to be efficient for both [SantaCoder](https://arxiv.org/abs/2301.03988) and [StarCoder](https://arxiv.org/abs/2305.06161) models. Such a high threshold
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reduces false positives, leading to fewer unnecessary comparisons and lower computational overhead.
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Instead of removing near-duplicates, we introduce a new feature to our dataset, called *near_dups_stkv2_idx*. This feature is a list of IDs of the near-duplicate files from the Java-Stack v2 corresponding to the current file in our dataset.
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The table below shows the number of files removed by each preprocessing method and the final number of files we are left with in the end (excluding near-duplicates).
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- **retrieval_date**: date when the repo was scraped from GitHub
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We start by retrieving repositories with more than **900** stars using **two-month tumbling windows**. If we hit the **1000** repository limit per window (for a personal GitHub account), we shorten the
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search space to a **one-month window** and restart the iteration. Otherwise, the window advances by two months. Once the timeframe until April 2024 is covered, we reduce the star search space: between **900** and **100** stars, we decrease the interval by **50** (e.g. search between [900, 850]), between **100** and **10** stars, we decrease the interval by **10**, and for the last **10** stars, we decrease by **1**. Figure 1 showcases the distribution of repositories with up to **500** stars. Since most repositories fall within the **0-100 star range**, using the **creation date** and **star count** filters helps us avoid API limits and scrape more data by narrowing the search space.
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Although the creation date window can be reduced even further (week or day level), a one-month window was enough for our needs. After retrieving the repositories, we extract all the files with a
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*.java* extension.
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Furthermore, **k = 9** was shown to be a safe choice for [large research articles](http://infolab.stanford.edu/~ullman/mmds/book.pdf), however, for our needs, 7-shingles strike a balance between accuracy and
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computational efficiency, crucial for handling the **Java-Stack v2’s size** of over **222 M** files. This choice provides better computational efficiency by reducing the number of comparisons while maintaining a manageable shingle space.
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Lastly, we use a **Jaccard similarity threshold** of **0.7**, which proved to be efficient for both [SantaCoder](https://arxiv.org/abs/2301.03988) and [StarCoder](https://arxiv.org/abs/2305.06161) models. Such a high threshold
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reduces false positives, leading to fewer unnecessary comparisons and lower computational overhead. Moreover, this standard threshold value has been shown to be [robust for duplicate detection](https://dl.acm.org/doi/10.1145/3359591.3359735).
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Instead of removing near-duplicates, we introduce a new feature to our dataset, called *near_dups_stkv2_idx*. This feature is a list of IDs of the near-duplicate files from the Java-Stack v2 corresponding to the current file in our dataset.
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The table below shows the number of files removed by each preprocessing method and the final number of files we are left with in the end (excluding near-duplicates).
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