E. Shaya
About
In The Last Decade
E. Shaya
67 papers receiving 2.6k citations
Peers
Comparison fields: 5 of 60
- Astronomy and Astrophysics 2.6k
- Instrumentation 931
- Nuclear and High Energy Physics 309
- Atomic and Molecular Physics, and Optics 147
- Statistical and Nonlinear Physics 67
Countries citing papers authored by E. Shaya
This map shows the geographic impact of E. Shaya'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. Shaya with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites E. Shaya more than expected).
Fields of papers citing papers by E. Shaya
This network shows the impact of papers produced by E. Shaya. 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. Shaya. The network helps show where E. Shaya may publish in the future.
Co-authorship network of co-authors of E. Shaya
This figure shows the co-authorship network connecting the top 25 collaborators of E. Shaya. A scholar is included among the top collaborators of E. Shaya 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. Shaya. E. Shaya is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 5 | |
| 2 | 10 | |
| 3 | 4 | |
| 4 | 64 | |
| 5 | Converting FITS into XML: Methods and Advantages | 2 |
| 6 | Publishing Scientific Articles in XML. | 1 |
| 7 | Specifics on a XML Data Format for Scientific Data | 3 |
| 8 | Using XML for Accessing Resources in Astronomy | 1 |
| 9 | An XML Representation of FITS - Introducing FITSML | 1 |
| 10 | XML at the ADC: Steps to a Next Generation Data Archive | 2 |
| 11 | Formatting Journal Tables in XML at the ADC | 1 |
| 12 | Star formation in NGC 6611 with ADONIS and Hubble. | 3 |
| 13 | 14 | |
| 14 | 14 | |
| 15 | Polarized CCD Imaging of the Horsehead Nebula and MonR2 | 1 |
| 16 | 12 | |
| 17 | 118 | |
| 18 | Far Infrared Observations of Titan and Iapetus | 1 |
| 19 | The Abundance of CO in Diffuse Interstellar Clouds | 1 |
| 20 | A Survey of Interstellar CI | 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.