B. E. Morgado

933 total citations
16 papers, 79 citations indexed

About

B. E. Morgado is a scholar working on Astronomy and Astrophysics, Atmospheric Science and Ecology. According to data from OpenAlex, B. E. Morgado has authored 16 papers receiving a total of 79 indexed citations (citations by other indexed papers that have themselves been cited), including 15 papers in Astronomy and Astrophysics, 3 papers in Atmospheric Science and 2 papers in Ecology. Recurrent topics in B. E. Morgado's work include Astro and Planetary Science (13 papers), Stellar, planetary, and galactic studies (11 papers) and Solar and Space Plasma Dynamics (3 papers). B. E. Morgado is often cited by papers focused on Astro and Planetary Science (13 papers), Stellar, planetary, and galactic studies (11 papers) and Solar and Space Plasma Dynamics (3 papers). B. E. Morgado collaborates with scholars based in Brazil, France and Spain. B. E. Morgado's co-authors include A. R. Gomes-Júnior, M. Assafin, R. Vieira-Martins, J. I. B. Camargo, A. Dias-Oliveira, G. Benedetti-Rossi, F. Braga-Ribas, B. Sicardy, J. Desmars and A. H. Andrei and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and Philosophical Transactions of the Royal Society A Mathematical Physical and Engineering Sciences.

In The Last Decade

B. E. Morgado

15 papers receiving 76 citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
B. E. Morgado Brazil 5 71 13 6 5 4 16 79
A. Dias-Oliveira Brazil 5 66 0.9× 15 1.2× 6 1.0× 4 0.8× 3 0.8× 6 67
A. R. Gomes-Júnior Brazil 6 77 1.1× 16 1.2× 11 1.8× 5 1.0× 4 1.0× 12 80
G. Benedetti-Rossi Brazil 7 89 1.3× 16 1.2× 6 1.0× 3 0.6× 4 1.0× 15 92
Luis Riverol Italy 3 57 0.8× 7 0.5× 3 0.5× 6 1.2× 9 2.3× 7 62
M. Hankins United States 6 74 1.0× 6 0.5× 13 2.2× 2 0.4× 2 0.5× 23 83
David Grant United Kingdom 6 64 0.9× 8 0.6× 20 3.3× 6 1.2× 5 1.3× 9 76
S. Bondar Russia 5 51 0.7× 9 0.7× 15 2.5× 6 1.2× 7 1.8× 13 57
Matías Jones Chile 5 57 0.8× 8 0.6× 23 3.8× 5 1.0× 4 1.0× 7 64
Jahmour J. Givans United States 6 46 0.6× 6 0.5× 5 0.8× 5 1.0× 10 2.5× 9 62
P. M. Kilmartin New Zealand 4 75 1.1× 16 1.2× 10 1.7× 4 0.8× 3 0.8× 23 79

Countries citing papers authored by B. E. Morgado

Since Specialization
Citations

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

Fields of papers citing papers by B. E. Morgado

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by B. E. Morgado. 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 B. E. Morgado. The network helps show where B. E. Morgado may publish in the future.

Co-authorship network of co-authors of B. E. Morgado

This figure shows the co-authorship network connecting the top 25 collaborators of B. E. Morgado. A scholar is included among the top collaborators of B. E. Morgado based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with B. E. Morgado. B. E. Morgado is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

16 of 16 papers shown
1.
Braga-Ribas, F., B. Sicardy, B. E. Morgado, et al.. (2025). Centaur 29P/Schwassmann–Wachmann 1 and its near-nucleus environment from a stellar occultation. Philosophical Transactions of the Royal Society A Mathematical Physical and Engineering Sciences. 383(2291). 20240189–20240189. 2 indexed citations
2.
Assafin, M., B. Sicardy, J. L. Ortiz, et al.. (2025). Physical characteristics of Jupiter's Trojan (1437) Diomedes from a tri-chord stellar occultation in 2020 and dimensionless three-dimensional model. Philosophical Transactions of the Royal Society A Mathematical Physical and Engineering Sciences. 383(2291). 20240187–20240187. 1 indexed citations
3.
Gomes-Júnior, A. R., et al.. (2025). Characterizing longitude variation on Chariklo's main ring. Philosophical Transactions of the Royal Society A Mathematical Physical and Engineering Sciences. 383(2291). 20240199–20240199. 1 indexed citations
4.
Assafin, M., et al.. (2023). The 2021 mutual phenomena involving the Galilean satellites of Jupiter and the inner satellite Thebe. Monthly Notices of the Royal Astronomical Society. 526(4). 6145–6154. 2 indexed citations
5.
Rodríguez, Adrián, et al.. (2023). Dynamical characterization of the 6/1 mean motion resonance between Quaoar’s ring and Weywot. Monthly Notices of the Royal Astronomical Society. 525(3). 3376–3383. 4 indexed citations
6.
Gomes-Júnior, A. R., B. E. Morgado, G. Benedetti-Rossi, et al.. (2022). SORA: Stellar occultation reduction and analysis. Monthly Notices of the Royal Astronomical Society. 511(1). 1167–1181. 9 indexed citations
7.
Braga-Ribas, F., D. Souami, J. Desmars, et al.. (2022). Occultation portal: A web-based platform for data collection and analysis of stellar occultations. Monthly Notices of the Royal Astronomical Society. 515(1). 1346–1357.
8.
Barbosa, Domingos, Bruno Coelho, Sonia Antón, et al.. (2021). Radio astronomy and Space science in Azores: Enhancing the Atlantic VLBI infrastructure cluster. Advances in Space Research. 68(7). 3064–3078. 1 indexed citations
9.
Benedetti-Rossi, G., P. Santos-Sanz, J. L. Ortiz, et al.. (2020). The 2019 October 22nd multi-chord stellar occultation by (84922) 2003 VS2. 1 indexed citations
10.
Assafin, M., B. E. Morgado, R. Vieira-Martins, et al.. (2019). Mutual approximations between the five main moons of Uranus. Monthly Notices of the Royal Astronomical Society. 490(3). 3464–3475. 6 indexed citations
11.
Braga-Ribas, F., R. Vieira-Martins, B. Sicardy, et al.. (2019). Database on detected stellar occultations by small outer Solar System objects. Journal of Physics Conference Series. 1365(1). 12024–12024. 5 indexed citations
12.
Morgado, B. E., R. Vieira-Martins, M. Assafin, et al.. (2019). The 2014–2015 Brazilian mutual phenomena campaign for the Jovian satellites and improved results for the 2009 events. Planetary and Space Science. 179. 104736–104736. 4 indexed citations
13.
Gomes-Júnior, A. R., M. Assafin, J. Desmars, et al.. (2016). New orbits of irregular satellites designed for the predictions of stellar occultations up to 2020, based on thousands of new observations. Monthly Notices of the Royal Astronomical Society. 462(2). 1351–1358. 4 indexed citations
14.
Morgado, B. E., M. Assafin, R. Vieira-Martins, et al.. (2016). Astrometry of mutual approximations between natural satellites. Application to the Galilean moons. Monthly Notices of the Royal Astronomical Society. 460(4). 4086–4097. 15 indexed citations
15.
Gomes-Júnior, A. R., M. Assafin, R. Vieira-Martins, et al.. (2015). Astrometric positions for 18 irregular satellites of giant planets from 23 years of observations. Astronomy and Astrophysics. 580. A76–A76. 20 indexed citations
16.
Morgado, B. E., et al.. (2014). Kepler's ellipse, Cassini's oval and the trajectory of planets. European Journal of Physics. 35(2). 25009–25009. 4 indexed citations

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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