Automated Organization ProfileKonkoly Observatory, Monash University
Konkoly Observatory, Monash University
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: 2.1 (sum of 2 datasets Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
Title: Aluminium-26 From Massive Binary Stars II: ROTATING SINGLE STARS UP TO CORE-COLLAPSE AND THEIR IMPACT ON THE EARLY SOLAR SYSTEM
Authors: Brinkman H.E., den Hartogh J. W., Doherty C.L., Pignatari M., Lugaro M.
================================================================================
Description of contents: A .tar.gz package containing three files with the complete set
of yields from the models presented in this paper. YieldsNR.txt contains the yields for the
non-rotating models and Yields150.txt and Yields300.txt the yields for the models
rotating at an initial velocity of 150 and 300 km/s, respectively. ================================================================================
Authors
- Brinkman, Hannah Elisabeth ;
- Den Hartogh, J. W. ;
- Doherty, C. L. ;
- Pignatari, M. ;
- Lugaro, M.
Title: Aluminium-26 From Massive Binary Stars II: ROTATING SINGLE STARS UP TO CORE-COLLAPSE AND THEIR IMPACT ON THE EARLY SOLAR SYSTEM
Authors: Brinkman H.E., den Hartogh J. W., Doherty C.L., Pignatari M., Lugaro M.
================================================================================
Description of contents: A .tar.gz package containing three files with the complete set
of yields from the models presented in this paper. YieldsNR.txt contains the yields for the
non-rotating models and Yields150.txt and Yields300.txt the yields for the models
rotating at an initial velocity of 150 and 300 km/s, respectively. ================================================================================
Authors
- Brinkman, Hannah Elisabeth ;
- Den Hartogh, J. W. ;
- Doherty, C. L. ;
- Pignatari, M. ;
- Lugaro, M.