Rotational Phase Analysis
Rotational Phase Analysis is a computational method in gamma-ray timing that determines the periodic emission patterns of rotating celestial sources by aligning detected photons to a rotational ephemeris, thereby enabling phase-resolved spectral and temporal studies.
109
Publications
3K
Citations
330
Authors
149
Institutions
Publications per year
2017–2026
12
Parents
109
Yifan Zhou, Dániel Apai, Ben W. P. Lew et al. · The Astronomical Journal · 2017 · 97 citations · Full text
Natural Sciences, Astronomy, Physics +17
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149
Dalhousie University
Halifax, Canada
8 h-index
17 publications
468 citations

Centre National de la Recherche Scientifique
Paris, France
7 h-index
24 publications
491 citations
University of Arizona
Tucson, United States
5 h-index
14 publications
761 citations
University of Oxford
Oxford, United Kingdom
4 h-index
9 publications
220 citations
Herzberg Institute of Astrophysics
Victoria, Canada
3 h-index
9 publications
203 citations
Northumbria University
Newcastle upon Tyne, United Kingdom
3 h-index
4 publications
248 citations

Armagh Observatory & Planetarium
Armagh, United Kingdom
3 h-index
9 publications
546 citations

University of British Columbia
Vancouver, Canada
3 h-index
6 publications
157 citations
1–8 of 149
48 publications · 1.1K citations
21
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8 publications · 156 citations
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8 publications · 299 citations
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6 publications · 231 citations
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AJ · 6 publications · 194 citations
6
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