Variable Star Photometry is a specialized method within stellar photometry that involves the precise measurement and analysis of the temporal variations in a star's brightness to characterize its intrinsic or extrinsic variability.
260
Publications
10.3K
Citations
776
Authors
329
Institutions
Publications per year
2017–2026
31
Publications
260
General catalogue of variable stars: Version GCVS 5.1
N. N. Samus’, E. V. Kazarovets, Ο. V. Durlevich et al. · Astronomy Reports · 2017 · 630 citations
Natural Sciences, Astronomy, Physics +16
1–5 of 260
Authors
776
- JR
10
h-index
- GW
9
h-index
- GC
7
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- SB
6
h-index
- AF
6
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1–5 of 776
Institutions
329
University of Toronto
Toronto, Canada
11 h-index
29 publications
514 citations
University of Vienna
Vienna, Austria
10 h-index
30 publications
834 citations
Lowell Observatory
Flagstaff, United States
9 h-index
18 publications
1.7K citations
Space Telescope Science Institute
Baltimore, United States
8 h-index
8 publications
592 citations
University of British Columbia
Vancouver, Canada
8 h-index
8 publications
178 citations
Tennessee State University
Nashville, United States
8 h-index
8 publications
152 citations
South African Radio Astronomy Observatory
Cape Town, South Africa
8 h-index
22 publications
445 citations
University of California, Berkeley
Berkeley, United States
7 h-index
23 publications
4K citations
1–8 of 329
Venues
- The Astronomical Journal
AJ · 44 publications · 2.4K citations
25
h-index
- Publications of the Astronomical Society of the Pacific
PASP · 48 publications · 1.6K citations
21
h-index
- Astronomy and Astrophysics
37 publications · 1.1K citations
21
h-index
- Monthly Notices of the Royal Astronomical Society
39 publications · 1.7K citations
20
h-index
- The Astrophysical Journal
ApJ · 22 publications · 1K citations
17
h-index
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