S. E. Scott

1.4k total citations
8 papers, 554 citations indexed

About

S. E. Scott is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, S. E. Scott has authored 8 papers receiving a total of 554 indexed citations (citations by other indexed papers that have themselves been cited), including 8 papers in Astronomy and Astrophysics, 5 papers in Nuclear and High Energy Physics and 1 paper in Instrumentation. Recurrent topics in S. E. Scott's work include Galaxies: Formation, Evolution, Phenomena (8 papers), Astrophysics and Cosmic Phenomena (5 papers) and Radio Astronomy Observations and Technology (4 papers). S. E. Scott is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (8 papers), Astrophysics and Cosmic Phenomena (5 papers) and Radio Astronomy Observations and Technology (4 papers). S. E. Scott collaborates with scholars based in United Kingdom, Mexico and United States. S. E. Scott's co-authors include S. Serjeant, R. J. Ivison, M. Fox, A. W. Blain, O. Almaini, D. H. Hughes, J. A. Peacock, M. Rowan-Robinson, A. Efstathiou and Chris J. Willott and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and Figshare.

In The Last Decade

S. E. Scott

8 papers receiving 547 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
S. E. Scott United Kingdom 8 553 226 159 13 11 8 554
J. Rossa United States 10 609 1.1× 160 0.7× 148 0.9× 13 1.0× 9 0.8× 13 615
Jonathan R. Hargis United States 9 494 0.9× 250 1.1× 140 0.9× 12 0.9× 8 0.7× 16 518
C. Balkowski France 9 535 1.0× 204 0.9× 81 0.5× 15 1.2× 15 1.4× 18 546
R. Coziol Mexico 15 418 0.8× 156 0.7× 94 0.6× 7 0.5× 11 1.0× 34 427
Colin Borys United States 13 700 1.3× 253 1.1× 120 0.8× 15 1.2× 11 1.0× 19 706
Kiyoto Yabe Japan 10 467 0.8× 219 1.0× 68 0.4× 9 0.7× 11 1.0× 22 481
Nicola Mehrtens United Kingdom 6 365 0.7× 199 0.9× 63 0.4× 10 0.8× 11 1.0× 9 374
Shi Shao China 10 386 0.7× 191 0.8× 100 0.6× 10 0.8× 8 0.7× 23 412
S. Lípari Argentina 13 421 0.8× 140 0.6× 62 0.4× 18 1.4× 9 0.8× 17 428
Deborah Padgett Italy 2 410 0.7× 189 0.8× 99 0.6× 8 0.6× 6 0.5× 3 412

Countries citing papers authored by S. E. Scott

Since Specialization
Citations

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

Fields of papers citing papers by S. E. Scott

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of S. E. Scott

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

All Works

8 of 8 papers shown
1.
Scott, S. E., J. S. Dunlop, & S. Serjeant. (2006). A combined re-analysis of existing blank-field SCUBA surveys: comparative 850-mum source lists, combined number counts, and evidence for strong clustering of the bright submillimetre galaxy population on arcminute scales. Open Research Online (The Open University). 40 indexed citations
2.
Mainieri, V., I. Lehmann, S. E. Scott, et al.. (2005). Submillimetre detection of a high-redshift type 2 QSO. Monthly Notices of the Royal Astronomical Society. 356(4). 1571–1575. 22 indexed citations
3.
Kampen, E. van, Will J. Percival, M. Crawford, et al.. (2005). The extragalactic submillimetre population: predictions for the SCUBA Half-Degree Extragalactic Survey (SHADES). Monthly Notices of the Royal Astronomical Society. 359(2). 469–480. 15 indexed citations
4.
Simpson, Chris, J. S. Dunlop, S. Eales, et al.. (2004). Deep near-infrared spectroscopy of submillimetre-selected galaxies. Monthly Notices of the Royal Astronomical Society. 353(1). 179–188. 12 indexed citations
5.
Scott, S. E., M. Fox, J. S. Dunlop, et al.. (2002). The SCUBA 8-mJy survey - I. Submillimetre maps, sources and number counts. Figshare. 186 indexed citations
6.
Fox, M., A. Efstathiou, M. Rowan-Robinson, et al.. (2002). The SCUBA 8-mJy survey -- II. Multiwavelength analysis of bright submillimetre sources. Monthly Notices of the Royal Astronomical Society. 331(4). 839–852. 43 indexed citations
7.
Ivison, R. J., T. R. Greve, Ian Smail, et al.. (2002). Deep radio imaging of the SCUBA 8-mJy survey fields: submillimetre source identifications and redshift distribution. Monthly Notices of the Royal Astronomical Society. 337(1). 1–25. 200 indexed citations
8.
Lutz, D., J. S. Dunlop, O. Almaini, et al.. (2001). The extended counterpart of submm source Lockman 850.1. Astronomy and Astrophysics. 378(1). 70–75. 36 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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