M. W. E. Smith

14.8k citations
2 papers · 128 indexed · h-index 2

Impact in

    • Cosmology and Gravitation Theories
    • Radio Astronomy Observations and Technology
    • Galaxies: Formation, Evolution, Phenomena
    • Gamma-ray bursts and supernovae
    • Superconducting and THz Device Technology
    • Astrophysics and Cosmic Phenomena
    • Dark Matter and Cosmic Phenomena
    • Neutrino Physics Research

Papers in

    • Dark Matter and Cosmic Phenomena 1
    • Astrophysics and Cosmic Phenomena 1
    • Radio Astronomy Observations and Technology 1
    • Gamma-ray bursts and supernovae 1
    • Cosmology and Gravitation Theories 1
    • Pulsars and Gravitational Waves Research 1

M. W. E. Smith

2 papers receiving 121 citations

Peers

M. W. E. Smith
Comparison fields: 5 of 16
  • Astronomy and Astrophysics 117
  • Nuclear and High Energy Physics 79
  • Statistical and Nonlinear Physics 9
  • Instrumentation 2
  • Oceanography 7
Replace D. Contreras with:
D. Contreras Canada
Utkarsh Kumar Israel
J. Raux France
Robert Benkel United Kingdom
Bogdan Dănilă Romania
O. Sergijenko Ukraine
D. I. Novikov Russia
Masroor C. Pookkillath Japan
N. Chandrachani Devi India
R. Valentim Brazil
M. W. E. Smith relative to D. Contreras Canada D. Contreras's profile →
Citations per field
00.5×1.5×1.8×
D. Contreras · 1×
Citations per year

Countries citing papers authored by M. W. E. Smith

Since Specialization
Citations

This map shows the geographic impact of M. W. E. Smith'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 M. W. E. Smith with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. W. E. Smith more than expected).

Fields of papers citing papers by M. W. E. Smith

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by M. W. E. Smith. 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 M. W. E. Smith. The network helps show where M. W. E. Smith may publish in the future.

Co-authors

The 23 scholars most cited alongside M. W. E. Smith, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.

Border = papers with M. W. E. Smith Line = papers co-authored together M. W. E. Smith links everyone, so they are left out of the graph.

All Works

2 of 2 papers shown

About M. W. E. Smith

M. W. E. Smith is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics, Infectious Diseases, Organic Chemistry and Surgery, having authored 2 papers that have together received 128 indexed citations. Recurring topics across this work include Dark Matter and Cosmic Phenomena (1 paper), Radio Astronomy Observations and Technology (1 paper), Astrophysics and Cosmic Phenomena (1 paper), Gamma-ray bursts and supernovae (1 paper), Cosmology and Gravitation Theories (1 paper) and Pulsars and Gravitational Waves Research (1 paper). The work is most often cited by research in Astronomy and Astrophysics (117 citations), Nuclear and High Energy Physics (79 citations), Statistical and Nonlinear Physics (9 citations), Instrumentation (2 citations) and Oceanography (7 citations). M. W. E. Smith has collaborated with scholars based in United States and Germany. Frequent co-authors include E. M. Leitch, C. Pryke, J. E. Carlstrom, J. M. Kovac, N. W. Halverson, P. Mészáros, Shan Gao, G. Tešić, S. Coutu and Abe Falcone. Their work appears in journals such as The Astrophysical Journal and Astroparticle Physics.

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.

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