L. Deharveng
- Astronomy and Astrophysics top 1%
- Stellar, planetary, and galactic studies 36
- Astrophysics and Star Formation Studies 31
- Galaxies: Formation, Evolution, Phenomena 10
- Astro and Planetary Science 4
- Astrophysical Phenomena and Observations 4
- Instrumentation top 5%
- Astronomy and Astrophysical Research 11
- Spectroscopy top 5%
- Molecular Spectroscopy and Structure 5
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- Astronomical Observations and Instrumentation 5
L. Deharveng
36 papers receiving 1.5k citations
Peers
Comparison fields: 5 of 32
- Astronomy and Astrophysics 1.5k
- Instrumentation 81
- Spectroscopy 297
- Fluid Flow and Transfer Processes 32
- Atmospheric Science 91
Countries citing papers authored by L. Deharveng
This map shows the geographic impact of L. Deharveng'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 L. Deharveng with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites L. Deharveng more than expected).
Fields of papers citing papers by L. Deharveng
This network shows the impact of papers produced by L. Deharveng. 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 L. Deharveng. The network helps show where L. Deharveng may publish in the future.
Co-authorship network
The 25 scholars most cited alongside L. Deharveng, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.
All Works
| # | Work | ||
|---|---|---|---|
| 1 | 2017 | 19 | |
| 2 | 2015 | 39 | |
| 3 | 2010 | 201 | |
| 4 | 2009 | 97 | |
| 5 | 2009 | 52 | |
| 6 | 2008 | 56 | |
| 7 | 2007 | 103 | |
| 8 | 2006 | 94 | |
| 9 | 2004 | 5 | |
| 10 | 2003 | 7 | |
| 11 | 2003 | 69 | |
| 12 | 2002 | 14 | |
| 13 | 2001 | 19 | |
| 14 | 2001 | 13 | |
| 15 | 2000 | 41 | |
| 16 | H II regions in NGC 300. | 1988 | 1 |
| 17 | The Relation between Reddening and Extinction for Galactic and Extragalactic HII Regions | 1986 | 1 |
| 18 | Absolute H-alpha and H-beta photometry of LMC HII regions. | 1985 | 1 |
| 19 | Dynamics of the supergiant shell LMC 2 in the Large Magellanic Cloud. | 1982 | 1 |
| 20 | Optical study of the Carina nebula. | 1975 | 0 |
About L. Deharveng
L. Deharveng is a scholar working on Instrumentation, Astronomy and Astrophysics and Spectroscopy, having authored 40 papers that have together received 1.6k indexed citations. Recurring topics across this work include Stellar, planetary, and galactic studies (36 papers), Astrophysics and Star Formation Studies (31 papers), Astronomy and Astrophysical Research (11 papers), Galaxies: Formation, Evolution, Phenomena (10 papers), Molecular Spectroscopy and Structure (5 papers), Astronomical Observations and Instrumentation (5 papers), Astro and Planetary Science (4 papers) and Astrophysical Phenomena and Observations (4 papers). The work is most often cited by research in Astronomy and Astrophysics (1.5k citations), Instrumentation (81 citations) and Spectroscopy (297 citations). L. Deharveng has collaborated with scholars based in France, Germany and Italy. Frequent co-authors include A. Zavagno, J. Caplan, M. Pomarès, D. Russeil, R. Costero, L. D. Anderson, F. Schüller, B. Leflóch, J. Brand and F. Massi. Their work appears in journals such as Astronomy and Astrophysics, Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal, Proceedings of the International Astronomical Union and A&A.
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.