N. Seymour

11.0k total citations
109 papers, 2.2k citations indexed

About

N. Seymour is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, N. Seymour has authored 109 papers receiving a total of 2.2k indexed citations (citations by other indexed papers that have themselves been cited), including 104 papers in Astronomy and Astrophysics, 42 papers in Nuclear and High Energy Physics and 26 papers in Instrumentation. Recurrent topics in N. Seymour's work include Galaxies: Formation, Evolution, Phenomena (88 papers), Astrophysics and Cosmic Phenomena (42 papers) and Radio Astronomy Observations and Technology (42 papers). N. Seymour is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (88 papers), Astrophysics and Cosmic Phenomena (42 papers) and Radio Astronomy Observations and Technology (42 papers). N. Seymour collaborates with scholars based in Australia, United States and United Kingdom. N. Seymour's co-authors include C. De Breuck, J. Vernet, Daniel Stern, A. Galametz, Dominika Wylezalek, N. A. Hatch, M. J. Jarvis, A. Rettura, G. Drouart and S. A. Stanford and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

N. Seymour

102 papers receiving 2.0k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
N. Seymour Australia 29 2.1k 768 671 63 36 109 2.2k
S. Bardelli Italy 24 1.8k 0.9× 671 0.9× 687 1.0× 71 1.1× 24 0.7× 83 1.9k
Tom A. Barlow United States 18 1.6k 0.8× 370 0.5× 461 0.7× 65 1.0× 30 0.8× 20 1.6k
Aura Obreja Germany 26 1.5k 0.7× 310 0.4× 792 1.2× 47 0.7× 22 0.6× 52 1.6k
Suvendra Dutta United States 10 1.3k 0.6× 349 0.5× 546 0.8× 43 0.7× 36 1.0× 11 1.4k
L. Christensen Germany 30 2.8k 1.3× 742 1.0× 758 1.1× 47 0.7× 53 1.5× 115 2.9k
C. D. Impey United States 24 2.1k 1.0× 939 1.2× 596 0.9× 29 0.5× 45 1.3× 54 2.1k
Varoujan Gorjian United States 18 1.9k 0.9× 395 0.5× 653 1.0× 20 0.3× 33 0.9× 51 1.9k
M. N. Bremer United Kingdom 27 2.1k 1.0× 684 0.9× 855 1.3× 33 0.5× 46 1.3× 96 2.1k
M. Béthermin France 26 2.1k 1.0× 294 0.4× 888 1.3× 45 0.7× 21 0.6× 81 2.1k
Jacqueline Hodge Germany 29 2.4k 1.1× 377 0.5× 703 1.0× 22 0.3× 29 0.8× 67 2.4k

Countries citing papers authored by N. Seymour

Since Specialization
Citations

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

Fields of papers citing papers by N. Seymour

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of N. Seymour

This figure shows the co-authorship network connecting the top 25 collaborators of N. Seymour. A scholar is included among the top collaborators of N. Seymour 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 N. Seymour. N. Seymour 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
1.
Wu, Linhui, Fu‐Guo Xie, Q. Zheng, et al.. (2025). MWA and VLA Observations of Diffuse Radio Lobes in M87. The Astrophysical Journal. 988(1). 28–28.
2.
Whittam, I. H., M. J. Jarvis, E. J. Murphy, et al.. (2025). Evidence for inverse Compton scattering in high-redshift Lyman-break galaxies. Monthly Notices of the Royal Astronomical Society. 543(1). 507–517.
3.
Caccianiga, A., A. Moretti, J. W. Broderick, et al.. (2024). Multi-wavelength properties of three new radio-powerful z ∼ 5.6 quasi-stellar objects discovered from RACS. Astronomy and Astrophysics. 692. A241–A241. 3 indexed citations
4.
Caccianiga, A., A. Moretti, J. W. Broderick, et al.. (2024). Comprehensive view of az  ∼  6.5 radio-loud quasi-stellar object: From the radio to the optical/NIR to the X-ray band. Astronomy and Astrophysics. 687. A242–A242. 5 indexed citations
5.
Wong, O. Ivy, L. Rudnick, Stanislav S. Shabala, et al.. (2024). Radio Galaxy Zoo data release 1: 100185 radio source classifications from the FIRST and ATLAS surveys. Monthly Notices of the Royal Astronomical Society. 536(4). 3488–3506. 3 indexed citations
6.
Wong, O. Ivy, K. Lee-Waddell, N. Seymour, et al.. (2023). WALLABY pre-pilot survey: Radio continuum properties of the Eridanus supergroup. Publications of the Astronomical Society of Australia. 40. 3 indexed citations
7.
D’Silva, Jordan C. J., Simon P. Driver, Claudia del P. Lagos, et al.. (2023). GAMA/DEVILS: cosmic star formation and AGN activity over 12.5 billion years. Monthly Notices of the Royal Astronomical Society. 524(1). 1448–1463. 11 indexed citations
8.
Goyal, A., K. Małek, Timothy J. Galvin, et al.. (2022). Low-frequency Radio Continuum Imaging and SED Modeling of 11 LIRGs: Radio-only and FUV to Radio Bands. The Astrophysical Journal. 938(2). 152–152. 8 indexed citations
9.
Hurley‐Walker, N., et al.. (2022). Wide-band spectral variability of peaked spectrum sources. Monthly Notices of the Royal Astronomical Society. 512(4). 5358–5373. 7 indexed citations
10.
Seymour, N., et al.. (2021). A calibration and imaging strategy at 300 MHz with the Murchison Widefield Array (MWA). Publications of the Astronomical Society of Australia. 38. 4 indexed citations
11.
Mei, S., P. Salomé, F. Combes, et al.. (2020). Massive molecular gas reservoir around the central AGN in the CARLA J1103 + 3449 cluster at z = 1.44. Astronomy and Astrophysics. 641. A22–A22. 5 indexed citations
12.
Noirot, Gaël, Daniel Stern, S. Mei, et al.. (2018). HST grism confirmation of 16 structures at 1.4 < z < 2.8 from the Clusters Around Radio-Loud AGN (CARLA) survey. Oxford University Research Archive (ORA) (University of Oxford). 32 indexed citations
13.
Kapińska, A. D., Ivan A. Terentev, O. Ivy Wong, et al.. (2017). Radio Galaxy Zoo: A Search for Hybrid Morphology Radio Galaxies. The Astronomical Journal. 154(6). 253–253. 36 indexed citations
14.
Gullberg, B., C. De Breuck, M. D. Lehnert, et al.. (2016). The mysterious morphology of MRC0943-242 as revealed by ALMA and MUSE. Springer Link (Chiba Institute of Technology). 10 indexed citations
15.
Gullberg, B., M. D. Lehnert, C. De Breuck, et al.. (2016). ALMA finds dew drops in the dusty spider’s web. Astronomy and Astrophysics. 591. A73–A73. 28 indexed citations
16.
Gaensler, B. M., I. Agudo, Takuya Akahori, et al.. (2015). Broadband Polarimetry with the Square Kilometre Array: A Unique Astrophysical Probe. Radboud Repository (Radboud University). 103–103. 10 indexed citations
17.
Dannerbauer, H., J. Kurk, C. De Breuck, et al.. (2014). An excess of dusty starbursts related to the Spiderweb galaxy. Springer Link (Chiba Institute of Technology). 42 indexed citations
18.
Drouart, G., C. De Breuck, J. Vernet, et al.. (2012). Jet and torus orientations in high redshift radio galaxies. Astronomy and Astrophysics. 548. A45–A45. 29 indexed citations
19.
Ogle, Patrick, et al.. (2012). PKS 1138-26電波銀河の原始星団における超発光性星形成銀河およびz=2.16での極端な発光性の温かい水素分子の放出. The Astrophysical Journal. 751. 1–13. 1 indexed citations
20.
Seymour, N.. (2007). Disentangling the evolution of starburst and AGN populations in deep radio surveys. 363. 1 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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