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 Gijs Nelemans sits on this spectrum.
This scientist: 657 publications — 74th percentile
74% 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 Gijs Nelemans sits on this spectrum.
This scientist: 142 D-Index — 90th percentile
90% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
Gijs Nelemans is affiliated with Radboud University in the Netherlands and focuses on research within the broad domain of Physics and Astronomy. Their scholarly work encompasses several subfields including Astronomy and Astrophysics, Instrumentation, Oceanography, General Health Professions, and Computational Mechanics.
The scientist's research topics are diverse, with a concentration on Gamma-ray bursts and supernovae, Pulsars and Gravitational Waves Research, Stellar, planetary, and galactic studies, Astro and Planetary Science, Astronomy and Astrophysical Research, Astrophysical Phenomena and Observations, and Geophysics and Gravity Measurements.
Frequent publication venues for Gijs Nelemans include arXiv (Cornell University), Astronomy and Astrophysics, Monthly Notices of the Royal Astronomical Society, Springer Link (Chiba Institute of Technology), and Zenodo (CERN European Organization for Nuclear Research).
Recent notable papers authored or coauthored by Nelemans cover a range of topics and venues:
The scientist has collaborated frequently with several coauthors including Alina Istrate, P. Groot, Fiorenzo Stoppa, Jakub Klencki, and Onno R. Pols.
B. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
A. G. A. Brown;A. Vallenari;T. Prusti
T. Prusti;J. H. J. de Bruijne;A. G. A. Brown
B. P. Abbott;R. Abbott
F. Acernese;M. Agathos;K. Agatsuma;D. Aisa
B. P. Abbott;R. Abbott
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
F. Acernese;M. Agathos;K. Agatsuma;D. Aisa
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
A. G. A. Brown;A. Vallenari;T. Prusti
B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy
B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy
B. P. Abbott;R. Abbott
B. P. Abbott;R. Abbott
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
B. P. Abbott;R. Abbott
C. Babusiaux;F. van Leeuwen;M.A. Barstow
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