David L. Lambert
About
In The Last Decade
David L. Lambert
392 papers receiving 13.1k citations
Hit Papers
Peers
Comparison fields: 5 of 118
- Astronomy and Astrophysics 12.2k
- Instrumentation 3.5k
- Nuclear and High Energy Physics 1.8k
- Atomic and Molecular Physics, and Optics 1.3k
- Spectroscopy 1.1k
Countries citing papers authored by David L. Lambert
This map shows the geographic impact of David L. Lambert'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 David L. Lambert with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites David L. Lambert more than expected).
Fields of papers citing papers by David L. Lambert
This network shows the impact of papers produced by David L. Lambert. 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 David L. Lambert. The network helps show where David L. Lambert may publish in the future.
Co-authorship network of co-authors of David L. Lambert
This figure shows the co-authorship network connecting the top 25 collaborators of David L. Lambert. A scholar is included among the top collaborators of David L. Lambert 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 David L. Lambert. David L. Lambert is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 3 | |
| 2 | 11 | |
| 3 | 8 | |
| 4 | 4 | |
| 5 | 15 | |
| 6 | 5 | |
| 7 | The chemical abundances of open clusters: NGC 752, NGC 1817, NGC 2360 and NGC 2506 | 1 |
| 8 | 17 | |
| 9 | Emission-line spectra of XX Ophiuchi in 1996 and 1997 | 2 |
| 10 | Abundance analyses of cool extreme helium stars | 24 |
| 11 | Boron abundance of the Orion B-star HD 35299 : B III as a test of non-LTE | 1 |
| 12 | The spectrum of the cool R Coronae Borealis variable Z Ursae Minoris at minimum | 2 |
| 13 | The lithium isotope ratio in metal-poor stars. | 2 |
| 14 | 25 | |
| 15 | Frontiers of stellar evolution | 52 |
| 16 | Is LR SCO and RCB star | 2 |
| 17 | Frontiers in Stellar Evolution | 3 |
| 18 | 1 | |
| 19 | ABUNDANCES OF THE ELEMENTS IN THE SOLAR PHOTOSPHERE. III. SILICON. | 1 |
| 20 | Radiation pressure and the composition of the solar corona. | 1 |
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.