P. M. McCulloch

1.5k total citations
40 papers, 768 citations indexed

About

P. M. McCulloch is a scholar working on Astronomy and Astrophysics, Oceanography and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, P. M. McCulloch has authored 40 papers receiving a total of 768 indexed citations (citations by other indexed papers that have themselves been cited), including 35 papers in Astronomy and Astrophysics, 16 papers in Oceanography and 8 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in P. M. McCulloch's work include Pulsars and Gravitational Waves Research (23 papers), Geophysics and Gravity Measurements (16 papers) and Advanced Frequency and Time Standards (6 papers). P. M. McCulloch is often cited by papers focused on Pulsars and Gravitational Waves Research (23 papers), Geophysics and Gravity Measurements (16 papers) and Advanced Frequency and Time Standards (6 papers). P. M. McCulloch collaborates with scholars based in Australia, United States and Japan. P. M. McCulloch's co-authors include P. A. Hamilton, S. P. Ellingsen, A. K. Tzioumis, J. E. Reynolds, Chris Phillips, R. P. Norris, Richard Dodson, J. E. J. Lovell, D. L. Jauncey and Francesco D’Alessandro and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

P. M. McCulloch

33 papers receiving 735 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
P. M. McCulloch Australia 13 723 234 115 105 97 40 768
L. M. Newton Australia 12 628 0.9× 84 0.4× 52 0.5× 57 0.5× 35 0.4× 28 658
Jr. Harnden F. R. United States 24 1.8k 2.4× 309 1.3× 46 0.4× 14 0.1× 123 1.3× 59 1.8k
Plamen Krastev United States 17 503 0.7× 352 1.5× 109 0.9× 31 0.3× 205 2.1× 26 767
V. A. Hughes Canada 15 561 0.8× 120 0.5× 31 0.3× 121 1.2× 25 0.3× 68 616
C. Neiner France 33 3.3k 4.5× 78 0.3× 44 0.4× 38 0.4× 64 0.7× 175 3.3k
Sourav Chatterjee United States 25 2.9k 4.0× 232 1.0× 62 0.5× 25 0.2× 168 1.7× 54 3.0k
S. H. Knowles United States 12 470 0.7× 44 0.2× 54 0.5× 81 0.8× 26 0.3× 62 569
R. Pallavicini Italy 27 2.3k 3.1× 154 0.7× 33 0.3× 43 0.4× 41 0.4× 142 2.3k
W. E. Kunkel United States 22 1.6k 2.1× 155 0.7× 26 0.2× 15 0.1× 27 0.3× 95 1.6k
C. Catala France 31 2.8k 3.8× 30 0.1× 32 0.3× 87 0.8× 72 0.7× 104 2.8k

Countries citing papers authored by P. M. McCulloch

Since Specialization
Citations

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

Fields of papers citing papers by P. M. McCulloch

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by P. M. McCulloch. 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 P. M. McCulloch. The network helps show where P. M. McCulloch may publish in the future.

Co-authorship network of co-authors of P. M. McCulloch

This figure shows the co-authorship network connecting the top 25 collaborators of P. M. McCulloch. A scholar is included among the top collaborators of P. M. McCulloch 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 P. M. McCulloch. P. M. McCulloch 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.
Lovell, J. E. J., Lucia McCallum, P. M. McCulloch, et al.. (2013). The AuScope geodetic VLBI array. Journal of Geodesy. 87(6). 527–538. 32 indexed citations
2.
Cimò, Giuseppe, et al.. (2004). PKS 0405-385. International Astronomical Union Circular. 6418. 2.
3.
Donovan, Jennifer L., A. N. Lommen, Zaven Arzoumanian, et al.. (2004). Correlations Between X-ray and Radio Pulses in Vela. eCite Digital Repository (University of Tasmania). 1. 335.
4.
Tingay, S. J., D. L. Jauncey, J. E. Reynolds, et al.. (2000). The Parsec-Scale Structure and Evolution of the Nearby Fanaroff-Riley Type II Radio Galaxy Pictor A. The Astronomical Journal. 119(4). 1695–1700. 20 indexed citations
5.
Lovell, J. E. J., D. L. Jauncey, A. K. Tzioumis, et al.. (2000). First results of VSOP imaging of strong GPS sources. Advances in Space Research. 26(4). 715–718. 1 indexed citations
6.
Norris, R. P., P. J. Diamond, S. P. Ellingsen, et al.. (1998). Methanol Masers as Tracers of Circumstellar Disks. The Astrophysical Journal. 508(1). 275–285. 78 indexed citations
7.
Ommen, T. D. van, Francesco D’Alessandro, P. A. Hamilton, & P. M. McCulloch. (1997). Polarimetric observations of southern pulsars at 800 and 950 MHz. Monthly Notices of the Royal Astronomical Society. 287(2). 307–327. 37 indexed citations
8.
Jones, Dayton L., R. A. Preston, D. W. Murphy, et al.. (1996). Interstellar Broadening of Images in the Gravitational Lens PKS 1830−211. The Astrophysical Journal. 470(1). L23–L25. 14 indexed citations
9.
Deshpande, A. A., Francesco D’Alessandro, & P. M. McCulloch. (1996). Application of ‘CLEAN’ in the power spectral analysis of non-uniformly sampled pulsar timing data. Journal of Astrophysics and Astronomy. 17(1-2). 7–16. 4 indexed citations
10.
Deshpande, A. A., et al.. (1995). New HI absorption measurements towards six pulsars. Figshare. 23. 512. 1 indexed citations
11.
Tingay, S. J., D. L. Jauncey, R. A. Preston, et al.. (1995). Relativistic motion in a nearby bright X-ray source. Nature. 374(6518). 141–143. 172 indexed citations
12.
Sacco, B., G. Gerardi, T. Mineo, et al.. (1990). Observation of the VELA pulsar, PSR 0833-45, at 0.2-6.0 MeV with the FIGARO II experiment. The Astrophysical Journal. 349. L21–L21. 3 indexed citations
13.
Ferris, R. H., P. Turner, P. A. Hamilton, & P. M. McCulloch. (1980). The Llanherne VHF Radio Telescope. Publications of the Astronomical Society of Australia. 4(1). 26–28. 3 indexed citations
14.
McCulloch, P. M., P. A. Hamilton, R. N. Manchester, & J. G. Ables. (1978). Polarization characteristics of southern pulsars - II. 640-MHz observations. Monthly Notices of the Royal Astronomical Society. 183(4). 645–676. 36 indexed citations
15.
Hamilton, P. A., P. M. McCulloch, J. G. Ables, & M. M. Komesaroff. (1977). Polarization characteristics of southern pulsars - I. 400-MHz observations. Monthly Notices of the Royal Astronomical Society. 180(1). 1–18. 21 indexed citations
16.
McCulloch, P. M.. (1975). Long Term Variations in Jupiter’s 11 cm Radio Emission. Publications of the Astronomical Society of Australia. 2(6). 340–342. 1 indexed citations
17.
Komesaroff, M. M., J. G. Ables, D. J. Cooke, P. A. Hamilton, & P. M. McCulloch. (1973). Results and implications of a recent search for high-dispension pulsars. 15. 169. 1 indexed citations
18.
Hamilton, P. A., P. M. McCulloch, J. G. Ables, M. M. Komesaroff, & D. J. Cooke. (1973). A New Search Method for Pulsars. 15. 163. 1 indexed citations
19.
McCulloch, P. M.. (1968). Interpretation of the Radio Rotation Period of Jupiter in Terms of the Cyclotron Theory. Australian Journal of Physics. 21(3). 409–414. 1 indexed citations
20.
Komesaroff, M. M. & P. M. McCulloch. (1967). THE RADIO ROTATION PERIOD OF JUPITER.. 1(3). 39–254. 10 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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