The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where O. Le Fevre sits on this spectrum.
This scientist: 919 publications — 89th percentile
89% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 1,469 publications or more.
The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where O. Le Fevre sits on this spectrum.
This scientist: 173 D-Index — 97th percentile
97% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
O. Le Fevre was affiliated with Aix-Marseille University in France and contributed extensively to the field of physics and astronomy with a focus on astronomy and astrophysics. Their research work spanned multiple subfields, including instrumentation, nuclear and high energy physics, atomic and molecular physics and optics, as well as electrical and electronic engineering.
Le Fevre's main topics of research encompassed galaxies - including their formation, evolution, and phenomena - along with general astronomy and astrophysical research. Further areas of study involved astrophysics and star formation, gamma-ray bursts and supernovae, stellar, planetary, and galactic studies, astrophysics and cosmic phenomena, and adaptive optics and wavefront sensing.
Their publication record reflected their multidisciplinary approach, with key frequent venues including:
Among their recent notable papers were:
Le Fevre collaborated frequently with a core group of co-authors, including:
Their substantial body of work comprised 144 publications primarily centered on physics and astronomy. The scientist's contributions significantly intersected observational astrophysics and instrumentation, highlighting a blend of theoretical and practical approaches within the broader scientific community.
Y. Peng;S. J. Lilly;K. Kovac;M. Bolzonella
Ying-jie Peng;Simon J. Lilly;Katarina Kovač;Micol Bolzonella
O. Ilbert;S. Arnouts;H.J. McCracken;M. Bolzonella
R. Laureijs;J. Amiaux;S. Arduini;J.-L. Auguères
O. Ilbert;O. Ilbert;S. Arnouts;H. J. Mccracken;M. Bolzonella
S. J. Lilly;S. J. Lilly;O. Le Fèvre;F. Hammer;David Crampton;David Crampton
S.J. Lilly;O. Le Fevre;F. Hammer;David Crampton
S.J. Lilly;O. Le Fevre;A. Renzini;G. Zamorani
O. Ilbert;P. Capak;M. Salvato;H. Aussel
S. J. Lilly;O. Le Fèvre;A. Renzini;G. Zamorani
M. Polletta;M. Tajer;L. Maraschi;G. Trinchieri
C. Laigle;H. J. McCracken;O. Ilbert;B. C. Hsieh
O. Le Fevre;G. Vettolani;B. Garilli;L. Tresse
M. Polletta;M. Tajer;L. Maraschi;G. Trinchieri
O. Ilbert;H. J. McCracken;O. Le Fevre;P. Capak
A. M. Koekemoer;H. Aussel;D. Calzetti;P. Capak
D. B. Sanders;M. Salvato;H. Aussel;O. Ilbert
O. Ilbert;O. Ilbert;M. Salvato;E. Le Floc'h;H. Aussel
L. Guzzo;M. Pierleoni;B. Meneux;E. Branchini
A. M. Koekemoer;H. Aussel;D. Calzetti;P. Capak
If you think any of the details on this page are incorrect, let us know.
