M. Rejkuba

7.1k citations
170 papers · 4.1k indexed · h-index 37

M. Rejkuba

153 papers receiving 3.9k citations

Peers

M. Rejkuba
Comparison fields: 5 of 60
  • Instrumentation 2.2k
  • Astronomy and Astrophysics 4.0k
  • Nuclear and High Energy Physics 275
  • Computational Mechanics 159
  • Atomic and Molecular Physics, and Optics 167
Replace M. Catelan with:
M. Catelan Chile
Ata Sarajedini United States
Kim A. Venn Canada
I. Soszyński Poland
Kareem El-Badry United States
A. Pietrinferni Italy
Richard de Grijs China
Eline Tolstoy Netherlands
M. Bellazzini Italy
S. T. Hodgkin United Kingdom
M. Rejkuba relative to M. Catelan Chile M. Catelan's profile →
Citations per field
00.5×1.7×
M. Catelan · 1×
Citations per year

Countries citing papers authored by M. Rejkuba

Since Specialization
Citations

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

Fields of papers citing papers by M. Rejkuba

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network

The 25 scholars most cited alongside M. Rejkuba, 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. Rejkuba Line = papers co-authored together M. Rejkuba links everyone, so they are left out of the graph.

All Works

20 of 20 papers shown
#Work
1 20256
2 20240
3 202317
4
The Cen A galaxy group: Dynamical mass and missing baryons
202215
5 201924
6 201961
7 201824
8 201816
9 20188
10 201721
11
201721
12 201415
13 201465
14 20142
15 20134
16 20129
17 201059
18 200882
19 200620
20 200125

About M. Rejkuba

M. Rejkuba is a scholar working on Instrumentation, Astronomy and Astrophysics and Atomic and Molecular Physics, and Optics, having authored 170 papers that have together received 4.1k indexed citations. Recurring topics across this work include Stellar, planetary, and galactic studies (135 papers), Astronomy and Astrophysical Research (105 papers), Astrophysics and Star Formation Studies (64 papers), Galaxies: Formation, Evolution, Phenomena (64 papers), Gamma-ray bursts and supernovae (20 papers), Adaptive optics and wavefront sensing (18 papers), Astrophysical Phenomena and Observations (11 papers) and Astronomical Observations and Instrumentation (11 papers). The work is most often cited by research in Instrumentation (2.2k citations), Astronomy and Astrophysics (4.0k citations) and Nuclear and High Energy Physics (275 citations). M. Rejkuba has collaborated with scholars based in Germany, Chile and Italy. Frequent co-authors include D. Minniti, M. Zoccali, O. A. González, E. Valenti, A. Renzini, L. Greggio, M. Hilker, Rodrigo Tobar, M. Schultheis and Helmut Jerjen. Their work appears in journals such as Science, SHILAP Revista de lepidopterología and The Astrophysical Journal.

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.

Explore authors with similar magnitude of impact

Rankless by CCL
2026