G. J. Schwarz
About
In The Last Decade
G. J. Schwarz
28 papers receiving 503 citations
Peers
Comparison fields: 5 of 12
- Astronomy and Astrophysics 506
- Nuclear and High Energy Physics 196
- Geophysics 54
- Computational Mechanics 41
- Radiation 17
Countries citing papers authored by G. J. Schwarz
This map shows the geographic impact of G. J. Schwarz'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 G. J. Schwarz with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. J. Schwarz more than expected).
Fields of papers citing papers by G. J. Schwarz
This network shows the impact of papers produced by G. J. Schwarz. 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 G. J. Schwarz. The network helps show where G. J. Schwarz may publish in the future.
Co-authorship network of co-authors of G. J. Schwarz
This figure shows the co-authorship network connecting the top 25 collaborators of G. J. Schwarz. A scholar is included among the top collaborators of G. J. Schwarz 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 G. J. Schwarz. G. J. Schwarz is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 23 | |
| 2 | Super-soft X-ray emission on day 6.4 from nova LMC N1968-12a strongly suggests a very high mass white dwarf | 1 |
| 3 | 19 | |
| 4 | Nova V5668 Sgr (N Sgr 2015 no. 2) enters the super-soft X-ray phase | 1 |
| 5 | 21 | |
| 6 | The slowly rising X-ray flux of Nova V5668 Sgr (N Sgr 2015 no. 2) | 1 |
| 7 | 27 | |
| 8 | Nova SMC 2012: a probable 20.4 hour period detected by Swift in the UV and X-ray | 1 |
| 9 | Confirmation of the Swift 54-second period and detection of a strong C V absorption edge in a deep XMM-Newton observation of V339 Del | 2 |
| 10 | 13 | |
| 11 | 37 | |
| 12 | Swift detection of UV and super-soft X-ray emission in Nova LMC 2012 | 1 |
| 13 | 18 | |
| 14 | 6 | |
| 15 | Swift detection of super soft X-ray emission in Nova V2468 Cygni | 1 |
| 16 | Swift super soft X-ray detection in Nova V1213 Centauri | 2 |
| 17 | Swift detection of Super Soft X-ray emission in nova CSS081007:030559+054715 | 1 |
| 18 | Swift detects a large flux increase and a probable period of 1.77 days in the X-ray and UV emission of the nova CSS081007:030559+054715 | 1 |
| 19 | 50 | |
| 20 | The Effects of Metallicity on Hydrodynamic Studies of the Nova Outburst | 0 |
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.