Astro Physics collaboration network
Dataset information
Dataset information
Arxiv ASTRO-PH (Astro Physics) collaboration network is from the e-print arXiv and covers scientific collaborations between authors papers submitted to Astro Physics category. If an author i co-authored a paper with author j, the graph contains a undirected edge from i to j. If the paper is co-authored by k authors this generates a completely connected (sub)graph on k nodes.
The data covers papers in the period from January 1993 to April 2003 (124 months). It begins within a few months of the inception of the arXiv, and thus represents essentially the complete history of its ASTRO-PH section.
| Dataset statistics | |
|---|---|
| Nodes | 18772 |
| Edges | 198110 |
| Nodes in largest WCC | 17903 (0.954) |
| Edges in largest WCC | 197031 (0.995) |
| Nodes in largest SCC | 17903 (0.954) |
| Edges in largest SCC | 197031 (0.995) |
| Average clustering coefficient | 0.6306 |
| Number of triangles | 1351441 |
| Fraction of closed triangles | 0.1345 |
| Diameter (longest shortest path) | 14 |
| 90-percentile effective diameter | 5 |
Source (citation)
- J. Leskovec, J. Kleinberg and C. Faloutsos. Graph Evolution: Densification and Shrinking Diameters. ACM Transactions on Knowledge Discovery from Data (ACM TKDD), 1(1), 2007.
Files
| File | Description |
|---|---|
| ca-AstroPh.txt.gz | Collaboration network of Arxiv Astro Physics category |