Pulse Profile Modeling is a computational method in X-ray timing analysis that characterizes the periodic emission patterns of compact astrophysical objects by statistically reconstructing the phase-resolved intensity variations of their pulsed signals.
220
Publications
12.7K
Citations
837
Authors
367
Institutions
Publications per year
2017–2026
47
Parents
Publications
220
1–5 of 220
Authors
837
- AL
6
h-index
- LS
6
h-index
- SM
6
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- SB
6
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- SG
5
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1–5 of 837
Institutions
367
Columbia University
New York, United States
16 h-index
18 publications
3.9K citations
University of Amsterdam
Amsterdam, The Netherlands
15 h-index
47 publications
4K citations
Goddard Space Flight Center
Greenbelt, United States
12 h-index
30 publications
15.4K citations
Centre National de la Recherche Scientifique
Paris, France
11 h-index
17 publications
6K citations
Commonwealth Scientific and Industrial Research Organisation
Canberra, Australia
10 h-index
29 publications
1.1K citations
United States Naval Research Laboratory
Washington, United States
10 h-index
25 publications
7.3K citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
10 h-index
18 publications
1.6K citations
University of Manchester
Manchester, United Kingdom
10 h-index
21 publications
960 citations
1–8 of 367
Venues
- The Astrophysical Journal
ApJ · 50 publications · 2.9K citations
29
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- Monthly Notices of the Royal Astronomical Society
33 publications · 1.1K citations
21
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- Astronomy and Astrophysics
15 publications · 623 citations
15
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- Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment
9 publications · 241 citations
9
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- The Astrophysical Journal Letters
7 publications · 3.3K citations
7
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1–5