B. E. Woodgate
About
In The Last Decade
B. E. Woodgate
147 papers receiving 2.8k citations
Peers
Comparison fields: 5 of 65
- Astronomy and Astrophysics 2.7k
- Instrumentation 385
- Nuclear and High Energy Physics 355
- Atomic and Molecular Physics, and Optics 200
- Spectroscopy 183
Countries citing papers authored by B. E. Woodgate
This map shows the geographic impact of B. E. Woodgate'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 B. E. Woodgate with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. E. Woodgate more than expected).
Fields of papers citing papers by B. E. Woodgate
This network shows the impact of papers produced by B. E. Woodgate. 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 B. E. Woodgate. The network helps show where B. E. Woodgate may publish in the future.
Co-authorship network of co-authors of B. E. Woodgate
This figure shows the co-authorship network connecting the top 25 collaborators of B. E. Woodgate. A scholar is included among the top collaborators of B. E. Woodgate 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 B. E. Woodgate. B. E. Woodgate is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | The Goddard Integral Field Spectrograph at Apache Point Observatory: Current Status and Progress Towards Photon Counting | 0 |
| 2 | PISCES Development and Status: An Integral Field Spectrograph for the High Contrast Imaging Testbed | 0 |
| 3 | UV Imaging Detectors: High-QE EBCMOS Enabling New Science Missions | 1 |
| 4 | HST/STIS Coronagraphic Imaging of the Disk of DM Tauri | 1 |
| 5 | 30 | |
| 6 | Discovery of a Lyα Galaxy Near the Damped Lyα System at z = 2.3 towards the QSC PHL 957 | 1 |
| 7 | Fabry-Perot Imaging of Absorbers towards QSO 0836 + 113 | 2 |
| 8 | Forbidden Oxygen Emission from Galaxies Surrounding QSO 3C275.1 at z=0.55 | 1 |
| 9 | The Hubble Space Telescope Imaging Spectrograph | 0 |
| 10 | The Space Telescope Imaging Spectrograph (STIS) | 2 |
| 11 | Fabry-Perot Images of Extragalactic Superbubbles | 1 |
| 12 | The MIT spectroscopy investigations on AXAF and the study of supernova remnants | 2 |
| 13 | A Second Chance for Solar Max | 1 |
| 14 | Center-to-Limb Variation of Transition Region Redshift | 1 |
| 15 | Upflows Immediately Prior to the Impulsive Phase of Solar Flares | 2 |
| 16 | 52 | |
| 17 | Steady Flows in the Solar Transition Region Observed with the UVSP Experiment on SMM | 1 |
| 18 | Detection of the Fe XIV Coronal Line at 5303 Å in the Cygnus Loop | 1 |
| 19 | 12 | |
| 20 | 20 |
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.