Aura Obreja

2.2k citations
52 papers · 1.6k indexed · h-index 26

Aura Obreja

51 papers receiving 1.5k citations

Peers

Aura Obreja
Comparison fields: 5 of 42
  • Instrumentation 792
  • Astronomy and Astrophysics 1.5k
  • Nuclear and High Energy Physics 310
  • Radiation 45
  • Statistical and Nonlinear Physics 47
Replace Gergö Popping with:
Gergö Popping Germany
Renske Smit United Kingdom
L. Michel-Dansac France
Mathilde Jauzac United Kingdom
Jacqueline Hodge Germany
M. Kuhlen United States
E. Pérez‐Montero Spain
Marc Rafelski United States
Michele Cirasuolo United Kingdom
W. R. Oegerle United States
Aura Obreja relative to Gergö Popping Germany Gergö Popping's profile →
Citations per field
00.5×6.4×
Gergö Popping · 1×
Citations per year

Countries citing papers authored by Aura Obreja

Since Specialization
Citations

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

Fields of papers citing papers by Aura Obreja

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network

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

All Works

20 of 20 papers shown
#Work
1 20251
2 20248
3 20243
4 202310
5 20235
6 202325
7 202214
8 202038
9 202028
10 201927
11 201949
12 201919
13 20199
14 201914
15
gsf: galactic structure finder
20181
16 2018102
17 201843
18 20173
19 201758
20
A two-phase scenario for bulge assembly in ΛCDM cosmologies
201330

About Aura Obreja

Aura Obreja is a scholar working on Instrumentation, Astronomy and Astrophysics and Nuclear and High Energy Physics, having authored 52 papers that have together received 1.6k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (46 papers), Astronomy and Astrophysical Research (35 papers), Stellar, planetary, and galactic studies (24 papers), Astrophysics and Star Formation Studies (14 papers), Gamma-ray bursts and supernovae (8 papers), Cosmology and Gravitation Theories (6 papers), Astrophysical Phenomena and Observations (5 papers) and Radio Astronomy Observations and Technology (3 papers). The work is most often cited by research in Instrumentation (792 citations), Astronomy and Astrophysics (1.5k citations) and Nuclear and High Energy Physics (310 citations). Aura Obreja has collaborated with scholars based in Germany, United Arab Emirates and Spain. Frequent co-authors include Andrea V. Macciò, Aaron A. Dutton, Tobias Buck, Chris B. Brook, Arianna Di Cintio, Avishai Dekel, Gregory S. Stinson, Xi Kang, Liang Wang and R. Domı́nguez-Tenreiro. Their work appears in journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

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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