M. Salaris
About
In The Last Decade
M. Salaris
10 papers receiving 264 citations
Peers
Comparison fields: 5 of 16
- Astronomy and Astrophysics 251
- Nuclear and High Energy Physics 109
- Instrumentation 78
- Radiation 33
- Atomic and Molecular Physics, and Optics 18
Countries citing papers authored by M. Salaris
This map shows the geographic impact of M. Salaris's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by M. Salaris with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Salaris more than expected).
Fields of papers citing papers by M. Salaris
This network shows the impact of papers produced by M. Salaris. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by M. Salaris. The network helps show where M. Salaris may publish in the future.
Co-authorship network of co-authors of M. Salaris
This figure shows the co-authorship network connecting the top 25 collaborators of M. Salaris. A scholar is included among the top collaborators of M. Salaris based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with M. Salaris. M. Salaris is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 2 | |
| 2 | 0 | |
| 3 | 3 | |
| 4 | 4 | |
| 5 | 0 | |
| 6 | Theoretical uncertainties in Red Giant Branch stellar models | 0 |
| 7 | What Are White Dwarfs Telling Us About the Galactic Disk and Halo | 1 |
| 8 | Atomic Diffusion in Stellar Interiors and Field Halo Subdwarfs Ages | 1 |
| 9 | Theoretical uncertainties on the evolution of HB and AGB-clump stars | 1 |
| 10 | The effective temperature scale of giant stars (F0-K5). III. Stellar radii and the calibration of convection | 2 |
| 11 | 75 | |
| 12 | 200 | |
| 13 | 1 |
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.