Émile Biémont
About
In The Last Decade
Émile Biémont
240 papers receiving 4.3k citations
Peers
Comparison fields: 5 of 67
- Atomic and Molecular Physics, and Optics 3.2k
- Mechanics of Materials 1.6k
- Astronomy and Astrophysics 1.3k
- Spectroscopy 824
- Nuclear and High Energy Physics 711
Countries citing papers authored by Émile Biémont
This map shows the geographic impact of Émile Biémont'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 Émile Biémont with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Émile Biémont more than expected).
Fields of papers citing papers by Émile Biémont
This network shows the impact of papers produced by Émile Biémont. 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 Émile Biémont. The network helps show where Émile Biémont may publish in the future.
Co-authorship network of co-authors of Émile Biémont
This figure shows the co-authorship network connecting the top 25 collaborators of Émile Biémont. A scholar is included among the top collaborators of Émile Biémont 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 Émile Biémont. Émile Biémont is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 19 | |
| 2 | Spectroscopie atomique. Instrumentation et structures atomiques | 1 |
| 3 | Ritmi del tempo, astronomia e calendari | 0 |
| 4 | Experimental M1 Transition Rates in Highly Charged Krypton Ions | 2 |
| 5 | Rythmes du temps, Astronomie et Calendriers | 2 |
| 6 | 157 | |
| 7 | Météores et effets lumineux dans l'atmosphère terrestre | 0 |
| 8 | Interesting Lines in the Infrared Solar Spectrum. II. Unblended Lines between 1.0 and 1.8µm | 4 |
| 9 | Forbidden transitions of astrophysical interest in the 5pk (k=1-5) configurations | 24 |
| 10 | Radiative Lifetime Measurements in Dy II and the Solar Abundance of Dysprosium | 3 |
| 11 | Accurate F values of astrophysical interest for neutral carbon | 20 |
| 12 | n < 2 Allowed Transitions in Neutral Sulfur within in the Visible and Infrared Spectral Ranges | 5 |
| 13 | Electric Dipole Transitions in Atomic Oxygen and the lifetimes of the 2p3(4S°)3s5S° and 3S° States | 15 |
| 14 | Oscillator strengths for the gallium-like ions Br V - In XIX | 1 |
| 15 | Interesting lines in the infrared solar spectrum between 1.49 and 1.8 microns | 5 |
| 16 | The nickel spectrum in the infrared - Application to the solar spectrum | 5 |
| 17 | Identification on chromium lines in the infrared solar spectrum based on new interferometric measurements | 5 |
| 18 | Radiative lifetimes for Pd I and the solar abundance of palladium | 2 |
| 19 | New lifetime measurements for Nb I and Rh I and the solar photospheric abundances of Nb and Rh. | 1 |
| 20 | Theoretical F values for sodium-like ions (11 <= Z <= 26) | 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.