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 Mark Halpern sits on this spectrum.
This scientist: 599 publications — 69th percentile
69% 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 Mark Halpern sits on this spectrum.
This scientist: 145 D-Index — 91st percentile
91% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
Mark Halpern is affiliated with the University of British Columbia in Canada and has made significant contributions in the field of Physics and Astronomy. Their research encompasses a broad range of topics, with a primary focus on Astronomy and Astrophysics along with notable work in Nuclear and High Energy Physics, Oceanography, Instrumentation, and Aerospace Engineering.
Their major scientific interests cover several key topics, including:
Some of the frequent publication venues for their work are:
Mark Halpern has collaborated extensively with other researchers, often coauthoring papers with:
The following is a selection of recent papers authored or coauthored by Mark Halpern demonstrating a range of interests within cosmology, astrophysics, and radio astronomy:
Mark Halpern was recognized as a Fellow of the Royal Society of Canada in 2020 by the Academy of Science, highlighting their standing within the scientific community.
D. N. Spergel;L. Verde;H. V. Peiris;E. Komatsu
Eiichiro Komatsu;J. Dunkley;J. Dunkley;M. R. Nolta;C. L. Bennett
Eiichiro Komatsu;K. M. Smith;J. Dunkley;C. L. Bennett
E. Komatsu;J. Dunkley;M. R. Nolta;C. L. Bennett
D. N. Spergel;R. Bean;R. Bean;O. Doré;O. Doré;M. R. Nolta;M. R. Nolta
D. N. Spergel;R. Bean;O. Doré;M. R. Nolta
C. L. Bennett;M. Bay;M. Halpern;G. Hinshaw
C. L. Bennett;M. Halpern;G. Hinshaw;N. Jarosik
C. L. Bennett;M. Halpern;G. Hinshaw;N. Jarosik
G. Hinshaw;D. Larson;E. Komatsu;David N. Spergel;David N. Spergel
J. Dunkley;E. Komatsu;M. R. Nolta;D. N. Spergel
G. Hinshaw;J. L. Weiland;R. S. Hill;N. Odegard
C. L. Bennett;R. S. Hill;G. Hinshaw;M. R. Nolta
C. L. Bennett;D. Larson;J. L. Weiland;N. Jarosik
J. Dunkley;J. Dunkley;Eiichiro Komatsu;M. R. Nolta;D. N. Spergel
G. Hinshaw;M. R. Nolta;C. L. Bennett;R. Bean
G. Hinshaw;J. L. Weiland;R. S. Hill;N. Odegard
D. Larson;J. Dunkley;G. Hinshaw;Eiichiro Komatsu
Peter A. R. Ade;R.W. Aikin;D. Barkats;S.J. Benton
L. Page;G. Hinshaw;E. Komatsu;M. R. Nolta
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Institut National des Sciences Appliquées de Toulouse
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