Automated Author ProfileXu, Jun
National Astronomical Observatories, Beijing, China
Xu, Jun
Current S-Index
Sum of Dataset Indices for all datasets
Average Dataset Index per Dataset
Average Dataset Index per dataset
Total Datasets
Total datasets for this author
Average FAIR Score
Average FAIR Score per dataset
Total Citations
Total citations to the author's datasets
Total Mentions
Total mentions of the author's datasets
S-Index Interpretation
The S-Index (Sharing Index) is a comprehensive metric that represents the cumulative impact of all your datasets. It is calculated as the sum of Dataset Index scores across all your claimed datasets.
What it means:
- A higher S-index indicates greater overall impact of your datasets relative to typical datasets in their fields of research
- The S-Index grows as you add more datasets or as existing datasets gain more citations and mentions
- It provides a single number to track your research data impact over time
Current S-Index: 0.2 (sum of 1 dataset Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
Most millisecond pulsars are extremely stable. This stability allows such pulsars to be used for numerous applications such as searching for gravitational waves or for developing a pulsar-based time standard. In general, millisecond pulsars are located at high Galactic latitudes, whereas most pulsar surveys are carried out near the Galactic plane. Searching for radio pulsars in gamma-ray sources has been proven to be an effective means to discover new millisecond pulsars. We propose to search for pulsars in 195 southern Fermi sources (Dec
Authors
- Xu, Jun ;
- Manchester, Dick ;
- Hobbs, George ;
- Han, Jinlin ;
- Han, Jun