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 A. M. Lagrange sits on this spectrum.
This scientist: 567 publications — 65th percentile
65% 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 A. M. Lagrange sits on this spectrum.
This scientist: 106 D-Index — 65th percentile
65% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
A. M. Lagrange is affiliated with Grenoble Alpes University in France and has contributed extensively to research in the field of Physics and Astronomy. Their work focuses predominantly on subfields such as Astronomy and Astrophysics, Instrumentation, Computational Mechanics, and Aerospace Engineering. The scientist's research topics include stellar, planetary, and galactic studies, astronomy and astrophysical research, astro and planetary science, astrophysics and star formation studies, astronomical observations and instrumentation, gamma-ray bursts and supernovae, as well as calibration and measurement techniques.
The scientist has published numerous articles, with notable papers including:
A. M. Lagrange frequently collaborates with other researchers. The most frequent co-authors include G. Chauvin, J. H. Girard, A. Vigan, S. Desidera, and Emily Rickman. The scientist's published work appears primarily in the following venues:
The balance of publications across these respected journals and repositories indicates an active participation in the dissemination of research within their fields of study. The scientist's work integrates observational data, instrumentation advances, and theoretical research to address questions related to planetary systems, stellar characteristics, and broader astrological phenomena. Their output over recent years points to ongoing investigations involving high-precision radial velocity measurements and astrometric analyses.
R. Schödel;T. Ott;R. Genzel;R. Hofmann
G. Chauvin;A. M. Lagrange;C. Dumas;B. Zuckerman
A.-M. Lagrange;M. Bonnefoy;G. Chauvin;D. Apai
G. Chauvin;A.-M. Lagrange;C. Dumas;B. Zuckerman
A.-M. Lagrange;D. Gratadour;G. Chauvin;T. Fusco
Rainer Lenzen;Markus Hartung;Wolfgang Brandner;Gert Finger
M. Keppler;M. Benisty;A. Müller;Th. Henning
J.-L. Beuzit;A. Vigan;D. Mouillet;K. Dohlen
D. Mouillet;J. D. Larwood;J. C. B. Papaloizou;A. M. Lagrange
M. Keppler;M. Benisty;M. Benisty;A. Müller;Th. Henning
J. Rameau;G. Chauvin;A.-M. Lagrange;A. Boccaletti
G. Chauvin;A. M. Lagrange;M. Bonavita;B. Zuckerman
G. Chauvin;A-M Lagrange;B Zuckerman;C Dumas
M. Desort;A.-M. Lagrange;F. Galland;S. Udry
J.-L. Beuzit;J.-L. Beuzit;A. Vigan;D. Mouillet;K. Dohlen
J. C. Augereau;R. P. Nelson;A. M. Lagrange;J. C. B. Papaloizou
G. Chauvin;S. Desidera;A. M. Lagrange;A. Vigan
A. Müller;M. Keppler;Th. Henning;M. Samland
G. Chauvin;G. Chauvin;S. Desidera;A. M. Lagrange;A. Vigan
G. Chauvin;A.-M. Lagrange;H. Beust;M. Bonnefoy
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