Automated Organization ProfileClemson University, United States
Clemson University, United States
Current S-Index
Sum of Dataset Indices for all datasets
Average Dataset Index per Dataset
Average Dataset Index per dataset
Total Datasets
Total datasets in this organization
Average FAIR Score
Average FAIR Score per dataset
Total Citations
Total citations to the organization's datasets
Total Mentions
Total mentions of the organization'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: 0.6 (sum of 3 datasets Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
The detection of gamma-ray emission from the SNR/PWN B0453?685 could help us understand this system, especially if we know whether that emission is likely to arise from the PWN, the SNR, or the embedded pulsar. No pulsations have been detected from the central X-ray source that is almost certainly the neutron star birthed in the supernova, but the expected pulsed flux density is a factor of 3 or more below existing surveys. We propose deep observations that should detect pulsations if the source is analogous to other young SNR/PWN complexes. Knowing the pulsar energetics is key to understanding the current state and evolutionary history of the system, which in turn will increase our knowledge of star formation in the LMC, where only five PWNe are known to date.
Authors
- Kerr, Matthew ;
- Johnston, Simon ;
- Castro, Daniel ;
- Dai, Shi ;
- EAgle, Jordan
The detection of gamma-ray emission from the SNR/PWN B0453?685 could help us understand this system, especially if we know whether that emission is likely to arise from the PWN, the SNR, or the embedded pulsar. No pulsations have been detected from the central X-ray source that is almost certainly the neutron star birthed in the supernova, but the expected pulsed flux density is a factor of 3 or more below existing surveys. We propose deep observations that should detect pulsations if the source is analogous to other young SNR/PWN complexes. Knowing the pulsar energetics is key to understanding the current state and evolutionary history of the system, which in turn will increase our knowledge of star formation in the LMC, where only five PWNe are known to date.
Authors
- Kerr, Matthew ;
- Johnston, Simon ;
- Castro, Daniel ;
- Dai, Shi ;
- EAgle, Jordan
The detection of gamma-ray emission from the SNR/PWN B0453?685 could help us understand this system, especially if we know whether that emission is likely to arise from the PWN, the SNR, or the embedded pulsar. No pulsations have been detected from the central X-ray source that is almost certainly the neutron star birthed in the supernova, but the expected pulsed flux density is a factor of 3 or more below existing surveys. We propose deep observations that should detect pulsations if the source is analogous to other young SNR/PWN complexes. Knowing the pulsar energetics is key to understanding the current state and evolutionary history of the system, which in turn will increase our knowledge of star formation in the LMC, where only five PWNe are known to date.
Authors
- Kerr, Matthew ;
- Johnston, Simon ;
- Castro, Daniel ;
- Dai, Shi ;
- EAgle, Jordan