C. de Bérgh
About
In The Last Decade
C. de Bérgh
125 papers receiving 4.0k citations
Peers
Comparison fields: 5 of 56
- Astronomy and Astrophysics 3.5k
- Atmospheric Science 1.7k
- Spectroscopy 726
- Global and Planetary Change 581
- Ecology 428
Countries citing papers authored by C. de Bérgh
This map shows the geographic impact of C. de Bérgh'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 C. de Bérgh with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. de Bérgh more than expected).
Fields of papers citing papers by C. de Bérgh
This network shows the impact of papers produced by C. de Bérgh. 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 C. de Bérgh. The network helps show where C. de Bérgh may publish in the future.
Co-authorship network of co-authors of C. de Bérgh
This figure shows the co-authorship network connecting the top 25 collaborators of C. de Bérgh. A scholar is included among the top collaborators of C. de Bérgh 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 C. de Bérgh. C. de Bérgh 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 Tenuous Atmospheres of Pluto and Triton Explored by CRIRES on the VLT | 7 |
| 2 | 1 | |
| 3 | Spectroscopy and Photometry of Jupiter Trojans V1.0 | 1 |
| 4 | Surface composition of Rhea from reflectance spectra, 0.2 to 3.6 μm. | 3 |
| 5 | ISOPHOT observations of the Pluto-Charon system: Pluto's thermal lightcurve | 3 |
| 6 | The Abundance of CO in the Deep Troposphere of Titan from Near-Infrared Observations at the IRTF | 1 |
| 7 | Breakthroughs in Groundbased Infrared Spectroscopy of Planets | 1 |
| 8 | Determination of the Temperature of Nitrogen on Pluto from Spectral Measurements | 1 |
| 9 | Detection of Nitrogen and Carbon Monoxide on the Surface of Pluto | 3 |
| 10 | Intense Localized Near-Infrared Oxygen Airglow on the Venus Night Side | 1 |
| 11 | High-Resolution Spectroscopy of Venus's Night Side in the 2.3, 1.7, and 1.1-1.3μm Windows | 1 |
| 12 | Tentative Detection of CO and CO 2 Ices on Triton | 6 |
| 13 | Composition of the Deep Atmosphere of Venus from High-Resolution Nightside Spectra | 2 |
| 14 | Ground-based High Resolution Spectroscopy of Venus near 3. 6 Microns | 2 |
| 15 | Detection of CO infrared emission lines in spectra of Venus | 7 |
| 16 | Detection of HDO in the Atmosphere of Mars: Its Abundance and the Value of D/H | 1 |
| 17 | The Troposphere of Titan Probed by Ground-Based Spectroscopy at 1.6 microns | 2 |
| 18 | Carbon monoxide in the atmosphere of Titan: search and discovery. | 1 |
| 19 | Laboratory Spectra of CH 4 at Low Temperature for an Improved Determination of the 12C/13C ratio in Jupiter and Saturn | 1 |
| 20 | The C/H and 12 CH 4 / 13 CH 4 ratios in the atmospheres of Jupiter and Saturn from 0.1 cm -1 resolution nearinfrared spectra. | 5 |
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.