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 Omar Almaini sits on this spectrum.
This scientist: 279 publications — 14th percentile
14% 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 Omar Almaini sits on this spectrum.
This scientist: 88 D-Index — 36th percentile
36% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
Omar Almaini is affiliated with the University of Nottingham in the United Kingdom and specializes in Physics and Astronomy. Their research is concentrated primarily within the subfield of Astronomy and Astrophysics, supported by work in Instrumentation, Nuclear and High Energy Physics, Statistical and Nonlinear Physics, and Global and Planetary Change. The scientist's investigations explore various key topics including Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, and phenomena such as Gamma-ray bursts and supernovae.
The research outputs by Omar Almaini are documented in leading publication venues, with frequent contributions to and collaborations published in:
Their recent scholarly articles include the following significant works:
Collaboration plays a notable role in Omar Almaini's work, with frequent co-authorship alongside several researchers. The most consistent collaborators include:
Their academic contributions focus on observational and instrumental approaches in astrophysical research, tackling questions of galaxy formation and evolution, as well as dynamic external cosmic phenomena. Through sustained publication in reputable astronomy and astrophysics journals, they contribute data and analysis relevant to early universe studies, galaxy surveys, and emission-line galaxy characterization using advanced observatories like JWST and ALMA.
Andy Lawrence;S. J. Warren;Omar Almaini;A. C. Edge
Norman A. Grogin;Dale D. Kocevski;S. M. Faber;Henry C. Ferguson
Anton M. Koekemoer;S. M. Faber;Henry C. Ferguson;Norman A. Grogin
K. Coppin;E.L. Chapin;A.M.J. Mortier;S.E. Scott
M. Moresco;A. Cimatti;R. Jimenez;L. Pozzetti
K. Coppin;E. L. Chapin;E. L. Chapin;A. M. J. Mortier;S. E. Scott
Rob Ivison;Thomas Greve;Ian Smail;James Dunlop
Rob Ivison;Thomas Greve;Ian Smail;James Dunlop
Audrey Galametz;Andrea Grazian;Adriano Fontana;Henry C. Ferguson
Audrey Galametz;Andrea Grazian;Adriano Fontana;Henry C. Ferguson
S. J. Warren;N. C. Hambly;S. Dye;O. Almaini
J.E. Geach;J.S. Dunlop;M. Halpern;Ian Smail
P. Santini;H. C. Ferguson;A. Fontana;B. Mobasher
Simon Dye;S. J. Warren;N. C. Hambly;N. J. G. Cross
Seb Oliver;Michael Rowan-Robinson;D. M. Alexander;O. Almaini
M. Cirasuolo;R. J. McLure;J. S. Dunlop;O. Almaini
J.M. Simpson;Ian Smail;A.M. Swinbank;O. Almaini
M. Cirasuolo;R. J. McLure;J. S. Dunlop;O. Almaini
S. J. Warren;N. C. Hambly;S. Dye;O. Almaini
U. Dudzevičiūtė;Ian Smail;A. M. Swinbank;S. M. Stach
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