Automated Organization ProfileDepartment of Physics and Astronomy, Seoul National University, Gwanak-gu, Seoul, 151-742, Republic of Korea
Department of Physics and Astronomy, Seoul National University, Gwanak-gu, Seoul, 151-742, Republic of Korea
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: 3.6 (sum of 2 datasets Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
MESA input files for the models presented in the paper "Stripped-Envelope Stars in Different Metallicity Environments I. Evolutionary Phases, Classification and Populations". The files included here can reproduce both the stellar models discussed in the paper (he_star_model.zip), as well as the initial helium star models (initial_model.zip). Some models used different numerical parameters to achieve convergence to core collapse. A table (MESA_params.dat) is included here with the specific models that have parameters that differ from the standard ones, and the value used for the parameters used in these models. To reproduce a model from this list, the parameters must be changed in the inlist_project file contained in he_star_model.zip. Also included is a table (lifetimes.dat) containing values of different parameters used in each simulation, as well as the data obtained from these models, used to create Figs. 4 and 5.
Authors
- Aguilera-Dena, David R. ;
- Langer, Norbert ;
- Antoniadis, John ;
- Pauli, Daniel ;
- Dessart, Luc ;
- Gräfener, Götz ;
- Yoon, Sung-Chul
MESA input files for the models presented in the paper "Stripped-Envelope Stars in Different Metallicity Environments I. Evolutionary Phases, Classification and Populations". The files included here can reproduce both the stellar models discussed in the paper (he_star_model.zip), as well as the initial helium star models (initial_model.zip). Some models used different numerical parameters to achieve convergence to core collapse. A table (MESA_params.dat) is included here with the specific models that have parameters that differ from the standard ones, and the value used for the parameters used in these models. To reproduce a model from this list, the parameters must be changed in the inlist_project file contained in he_star_model.zip. Also included is a table (lifetimes.dat) containing values of different parameters used in each simulation, as well as the data obtained from these models, used to create Figs. 4 and 5.
Authors
- Aguilera-Dena, David R. ;
- Langer, Norbert ;
- Antoniadis, John ;
- Pauli, Daniel ;
- Dessart, Luc ;
- Gräfener, Götz ;
- Yoon, Sung-Chul