S. D. Bates

3.1k total citations · 1 hit paper
16 papers, 1.2k citations indexed

About

S. D. Bates is a scholar working on Astronomy and Astrophysics, Oceanography and Geophysics. According to data from OpenAlex, S. D. Bates has authored 16 papers receiving a total of 1.2k indexed citations (citations by other indexed papers that have themselves been cited), including 16 papers in Astronomy and Astrophysics, 6 papers in Oceanography and 3 papers in Geophysics. Recurrent topics in S. D. Bates's work include Pulsars and Gravitational Waves Research (16 papers), Geophysics and Gravity Measurements (6 papers) and Gamma-ray bursts and supernovae (6 papers). S. D. Bates is often cited by papers focused on Pulsars and Gravitational Waves Research (16 papers), Geophysics and Gravity Measurements (6 papers) and Gamma-ray bursts and supernovae (6 papers). S. D. Bates collaborates with scholars based in United Kingdom, United States and Germany. S. D. Bates's co-authors include Andrea Possenti, M. Krämer, B. W. Stappers, M. Burgay, M. J. Keith, S. Johnston, M. Bailes, L. Levin, W. van Straten and N. D. R. Bhat and has published in prestigious journals such as Science, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

S. D. Bates

14 papers receiving 1.2k citations

Hit Papers

A Population of Fast Radio Bursts at Cosmological Distances 2013 2026 2017 2021 2013 100 200 300 400 500
What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the same subfield and year (this is the minimum needed to enter the top 1%, not the average within it), or reaches the top citation threshold in at least one of its specific research topics.

  1. A Population of Fast Radio Bursts at Cosmological Distances
    2013 577 citations D. Thornton, B. W. Stappers et al. Science profile →

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
S. D. Bates United Kingdom 12 1.2k 303 133 114 58 16 1.2k
V. I. Kondratiev Russia 16 906 0.8× 321 1.1× 166 1.2× 76 0.7× 73 1.3× 41 967
R. Karuppusamy Germany 19 956 0.8× 242 0.8× 119 0.9× 153 1.3× 110 1.9× 56 984
G. Desvignes Germany 17 940 0.8× 251 0.8× 118 0.9× 169 1.5× 76 1.3× 47 959
L. Levin United Kingdom 12 1.4k 1.2× 376 1.2× 256 1.9× 152 1.3× 116 2.0× 35 1.5k
K. Stovall United States 16 1.1k 0.9× 347 1.1× 238 1.8× 174 1.5× 96 1.7× 35 1.1k
F. A. Jenet United States 12 867 0.7× 207 0.7× 208 1.6× 141 1.2× 70 1.2× 20 906
R. P. Breton United Kingdom 21 1.7k 1.4× 257 0.8× 262 2.0× 216 1.9× 74 1.3× 67 1.7k
Ralph P. Eatough Germany 18 803 0.7× 303 1.0× 81 0.6× 96 0.8× 65 1.1× 39 865
S. Milia United Kingdom 7 837 0.7× 196 0.6× 81 0.6× 56 0.5× 40 0.7× 12 867
J. Kijak Poland 14 650 0.5× 287 0.9× 93 0.7× 78 0.7× 71 1.2× 45 664

Countries citing papers authored by S. D. Bates

Since Specialization
Citations

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

Fields of papers citing papers by S. D. Bates

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of S. D. Bates

This figure shows the co-authorship network connecting the top 25 collaborators of S. D. Bates. A scholar is included among the top collaborators of S. D. Bates 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. D. Bates. S. D. Bates 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.
Keith, M. J., A. Jameson, W. van Straten, et al.. (2024). The High Time Resolution Universe Pulsar Survey - I. System configuration and initial discoveries. Figshare. 1 indexed citations
2.
3.
Levin, L., M. Bailes, S. D. Bates, et al.. (2024). Radio emission evolution, polarimetry and multifrequency single pulse analysis of the radio magnetar PSRJ1622-4950. Figshare. 1 indexed citations
4.
Martinez, José, K. Stovall, P. C. C. Freire, et al.. (2015). PULSAR J0453+1559: A DOUBLE NEUTRON STAR SYSTEM WITH A LARGE MASS ASYMMETRY. The Astrophysical Journal. 812(2). 143–143. 166 indexed citations
5.
Lorimer, D. R., et al.. (2015). A search for rotating radio transients and fast radio bursts in the Parkes high-latitude pulsar survey. Monthly Notices of the Royal Astronomical Society. 455(2). 2207–2215. 43 indexed citations
6.
Keane, E. F., Bhaswati Bhattacharyya, M. Krämer, et al.. (2015). A Cosmic Census of Radio Pulsars with the SKA. UvA-DARE (University of Amsterdam). 40–40. 57 indexed citations
7.
Bates, S. D., et al.. (2014). PsrPopPy: an open-source package for pulsar population simulations. Monthly Notices of the Royal Astronomical Society. 439(3). 2893–2902. 62 indexed citations
8.
Levin, L., M. Bailes, Benjamin R. Barsdell, et al.. (2013). The High Time Resolution Universe Pulsar Survey –VIII. The Galactic millisecond pulsar population. Monthly Notices of the Royal Astronomical Society. 434(2). 1387–1397. 43 indexed citations
9.
Thornton, D., B. W. Stappers, M. Bailes, et al.. (2013). A Population of Fast Radio Bursts at Cosmological Distances. Science. 341(6141). 53–56. 577 indexed citations breakdown →
10.
Tiburzi, C., S. Johnston, M. Bailes, et al.. (2013). The High Time Resolution Universe survey – IX. Polarimetry of long-period pulsars. Monthly Notices of the Royal Astronomical Society. 436(4). 3557–3572. 11 indexed citations
11.
Burke-Spolaor, Sarah, S. Johnston, M. Bailes, et al.. (2012). The High Time Resolution Universe Pulsar Survey - V. Single-pulse energetics and modulation properties of 315 pulsars. Monthly Notices of the Royal Astronomical Society. 423(2). 1351–1367. 62 indexed citations
12.
Bates, S. D., M. Bailes, N. D. R. Bhat, et al.. (2011). The Discovery of 5 Millisecond Pulsars in the High Time Resolution Universe Survey. AIP conference proceedings. 23–27.
13.
Bailes, M., S. D. Bates, V. Bhalerao, et al.. (2011). Transformation of a Star into a Planet in a Millisecond Pulsar Binary. Science. 333(6050). 1717–1720. 89 indexed citations
14.
Burke-Spolaor, Sarah, M. Bailes, S. Johnston, et al.. (2011). The High Time Resolution Universe Pulsar Survey - III. Single-pulse searches and preliminary analysis. Monthly Notices of the Royal Astronomical Society. 416(4). 2465–2476. 55 indexed citations
15.
Bates, S. D., M. Bailes, N. D. R. Bhat, et al.. (2011). The High Time Resolution Universe Pulsar Survey - II. Discovery of five millisecond pulsars. Monthly Notices of the Royal Astronomical Society. 416(4). 2455–2464. 28 indexed citations
16.
Bates, S. D., S. Johnston, D. R. Lorimer, et al.. (2010). A 6.5-GHz multibeam pulsar survey. Monthly Notices of the Royal Astronomical Society. 411(3). 1575–1584. 40 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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