Pulsar Timing Analysis
Pulsar Timing Analysis is a specialized methodology in gamma-ray data analysis that precisely measures the arrival times of pulsed electromagnetic radiation from rotating neutron stars to detect deviations induced by astrophysical phenomena, orbital dynamics, or gravitational waves, thereby enabling high-precision tests of fundamental physics and neutron star astrophysics.
849
Publications
57.7K
Citations
2.1K
Authors
672
Institutions
Publications per year
2017–2026
245
Parents
849
Tests of General Relativity from Timing the Double Pulsar
M. Krämer, I. H. Stairs, R. N. Manchester et al. · Science · 2006 · 1.1K citations · Full text
Natural Sciences, Astronomy, Physics +15
1–5 of 849
2.1K
Commonwealth Scientific and Industrial Research Organisation, Australia
83 publications · 11.5K citations
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42
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35
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1–5 of 2.1K
672

University of Manchester
Manchester, United Kingdom
62 h-index
419 publications
58.1K citations

Commonwealth Scientific and Industrial Research Organisation
Canberra, Australia
60 h-index
379 publications
64.8K citations
Australia Telescope National Facility
Sydney, Australia
59 h-index
350 publications
59.8K citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
53 h-index
436 publications
37.6K citations
National Radio Astronomy Observatory
Charlottesville, United States
46 h-index
172 publications
24.1K citations

McGill University
Montreal, Canada
42 h-index
161 publications
18K citations
Goddard Space Flight Center
Greenbelt, United States
42 h-index
171 publications
19.5K citations
Swinburne University of Technology
Melbourne, Australia
40 h-index
204 publications
20.3K citations
1–8 of 672
ApJ · 252 publications · 18.7K citations
73
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181 publications · 14.4K citations
61
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49 publications · 1.8K citations
26
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PRD · 30 publications · 1.5K citations
21
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27 publications · 2.8K citations
20
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