E. M. Ratti
About
In The Last Decade
E. M. Ratti
12 papers receiving 178 citations
Peers
Comparison fields: 5 of 10
- Astronomy and Astrophysics 182
- Nuclear and High Energy Physics 68
- Geophysics 26
- Biomedical Engineering 19
- Computational Mechanics 15
Countries citing papers authored by E. M. Ratti
This map shows the geographic impact of E. M. Ratti'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 E. M. Ratti with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites E. M. Ratti more than expected).
Fields of papers citing papers by E. M. Ratti
This network shows the impact of papers produced by E. M. Ratti. 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 E. M. Ratti. The network helps show where E. M. Ratti may publish in the future.
Co-authorship network of co-authors of E. M. Ratti
This figure shows the co-authorship network connecting the top 25 collaborators of E. M. Ratti. A scholar is included among the top collaborators of E. M. Ratti 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 E. M. Ratti. E. M. Ratti is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Title | Journal | Authors | Indexed citations |
|---|---|---|---|---|
| 1 | Optical spectroscopy of the quiescent counterpart to EXO 0748−676: a Black Widow scenario? | E. M. Ratti | 10 | |
| 2 | IGR J19308+0530: Roche lobe overflow on to a compact object from a donor 1.8 times as massive | Monthly Notices of the Royal Astronomical Society Letters | E. M. Ratti, M. A. P. Torres et al. | 6 |
| 3 | VLT/FORS2 observations of four high-luminosity ULX candidates★ | Monthly Notices of the Royal Astronomical Society | Marianne Heida, P. G. Jonker et al. | 5 |
| 4 | THE NATURE OF THE BRIGHT ULX X-2 IN NGC 3921: ACHANDRAPOSITION ANDHSTCANDIDATE COUNTERPART | The Astrophysical Journal | P. G. Jonker, Marianne Heida et al. | 20 |
| 5 | CXOGBS J174444.7−260330: a new long orbital period cataclysmic variable in a low state★ | Monthly Notices of the Royal Astronomical Society | E. M. Ratti, C. T. Britt et al. | 11 |
| 6 | On the harmonics of the low-frequency quasi-periodic oscillation in GRS 1915+105 | Monthly Notices of the Royal Astronomical Society | E. M. Ratti, T. Belloni et al. | 6 |
| 7 | Multiwavelength campaign on Mrk 509 | Astronomy and Astrophysics | K. C. Steenbrugge, J. S. Kaastra et al. | 8 |
| 8 | X-ray and radio observations of the re-brightening event in MAXI J1659-152 | ATel | J. C. A. Miller‐Jones, P. G. Jonker et al. | 1 |
| 9 | Multiwavelength campaign on Mrk 509 VII. Relative abundances of the warm absorber | arXiv (Cornell University) | K. C. Steenbrugge, J. S. Kaastra et al. | 9 |
| 10 | An accurate position for the black hole candidate XTE J1752−223: re-interpretation of the VLBI data | Monthly Notices of the Royal Astronomical Society | J. C. A. Miller‐Jones, P. G. Jonker et al. | 37 |
| 11 | Chandra localization and optical/near-infrared follow-up of Galactic X-ray sources | eSpace (Curtin University) | E. M. Ratti, C. Bassa et al. | 27 |
| 12 | Rossi XTE monitoring of 4U 1636-53 - I. Long-term evolution and kHz quasi-periodic oscillations | Monthly Notices of the Royal Astronomical Society | T. Belloni, J. Homan et al. | 44 |
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.