T. Urrutia

64 papers receiving 1.8k citations

Hit Papers

The data processing pipeline for the MUSE instrument2020202620222024202050100150200

Peers

T. Urrutia
Comparison fields: 5 of 72
  • Astronomy and Astrophysics 1.8k
  • Instrumentation 647
  • Nuclear and High Energy Physics 339
  • Atomic and Molecular Physics, and Optics 65
  • Psychiatry and Mental health 60
Replace A. C. Becker with:
A. C. Becker United States
J. Fischer United States
L. Rizzi Italy
Andrew W. Green Australia
A. Domínguez United States
Karl Förster United States
Mélanie Chevance Germany
Jerry Edelstein United States
B. García‐Lorenzo Spain
Marcel Zemp Switzerland
T. Urrutia relative to A. C. Becker United States A. C. Becker's profile →
Citations per field
00.5×2.5×
A. C. Becker · 1×
Citations per year

Countries citing papers authored by T. Urrutia

Since Specialization
Citations

This map shows the geographic impact of T. Urrutia'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 T. Urrutia with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. Urrutia more than expected).

Fields of papers citing papers by T. Urrutia

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of T. Urrutia

This figure shows the co-authorship network connecting the top 25 collaborators of T. Urrutia. A scholar is included among the top collaborators of T. Urrutia 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 T. Urrutia. T. Urrutia is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
#WorkIndexed citations
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5 10
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11 21
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13 43
14 14
15 58
16 47
17
Ubiquitous Giant Lyα Nebulae around the Brightest Quasars at z ∼3.5 Revealed with MUSE
96
18 52
19 13
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Dust-reddened Quasars In First And Ukidss
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About T. Urrutia

T. Urrutia is a scholar working on Instrumentation, Astronomy and Astrophysics and Nuclear and High Energy Physics, having authored 64 papers that have together received 2.0k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (49 papers), Astrophysical Phenomena and Observations (26 papers) and Astronomy and Astrophysical Research (26 papers). The work is most often cited by research in Instrumentation (647 citations), Astronomy and Astrophysics (1.8k citations) and Nuclear and High Energy Physics (339 citations). T. Urrutia has collaborated with scholars based in Germany, United States and France. Frequent co-authors include Mark Lacy, R. H. Becker, Roland Bacon, B. Husemann, Peter M. Weilbacher, L. Wisotzki, Johan Richard, O. Streicher, Aurélien Jarno and Arlette Pécontal-Rousset. Their work appears in journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

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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2026