Dimitar Sasselov
About
In The Last Decade
Dimitar Sasselov
225 papers receiving 7.3k citations
Hit Papers
Peers
Comparison fields: 5 of 130
- Astronomy and Astrophysics 6.6k
- Instrumentation 1.9k
- Atomic and Molecular Physics, and Optics 759
- Nuclear and High Energy Physics 437
- Atmospheric Science 420
Countries citing papers authored by Dimitar Sasselov
This map shows the geographic impact of Dimitar Sasselov'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 Dimitar Sasselov with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Dimitar Sasselov more than expected).
Fields of papers citing papers by Dimitar Sasselov
This network shows the impact of papers produced by Dimitar Sasselov. 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 Dimitar Sasselov. The network helps show where Dimitar Sasselov may publish in the future.
Co-authorship network of co-authors of Dimitar Sasselov
This figure shows the co-authorship network connecting the top 25 collaborators of Dimitar Sasselov. A scholar is included among the top collaborators of Dimitar Sasselov 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 Dimitar Sasselov. Dimitar Sasselov is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 11 | |
| 2 | 10 | |
| 3 | 21 | |
| 4 | 120 | |
| 5 | MOST photometry and DDO spectroscopy of the eclipsing (white dwarf + red dwarf) binary V471 Tau | 7 |
| 6 | Nonradial p-modes in the G9.5 giant [epsilon] Ophiuchi? Pulsation model fits to MOST photometry | 8 |
| 7 | An Isotopically Homogeneous Region of the Inner Terrestrial Planet Region (Mercury to Earth): Evidence from E Chondrites and Implications for Giant Moon-Forming Impact Scenarios | 5 |
| 8 | 2 | |
| 9 | RECFAST: Calculate the Recombination History of the Universe | 2 |
| 10 | 11 | |
| 11 | Hf-W Chronometry and the Timing of the Giant Moon-forming Impact on Earth | 1 |
| 12 | Super-Earths' Evolution: Towards Habitability | 1 |
| 13 | 39 | |
| 14 | Laser Simulation of High P-T Planetary Processes | 2 |
| 15 | EXPERIMENTAL STUDY OF HIGH-ENERGY PROCESSING OF PROTOPLANETARY MATERIALS: | 3 |
| 16 | Pulsating stars: recent developments in theory and observation | 14 |
| 17 | Surface Imaging by Microlensing | 0 |
| 18 | Opportunities for stellar surface imaging via gravitational microlensing | 1 |
| 19 | Intercontinental simultaneous survey of the unique Cepheid HR 7308 in photometry and radial velocity | 3 |
| 20 | Variable F-Type Supergiants Far above the Galactic Plane | 2 |
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.