Relative Photometry
Relative Photometry is a photometric method that determines the brightness of celestial objects by comparing their ultraviolet flux measurements to those of reference stars within the same observational frame, thereby minimizing systematic errors arising from instrumental response and atmospheric transmission variations.
68
Publications
3.9K
Citations
302
Authors
165
Institutions
Publications per year
2017–2026
8
Parents
68
R. G. Bower, J. R. Lucey, R. S. Ellis · Monthly Notices of the Royal Astronomical Society · 1992 · 826 citations · Full text
Natural Sciences, Astronomy, Physics +13
1–5 of 68
302
3
h-index
3
h-index
3
h-index
2
h-index
2
h-index
1–5 of 302
165
California Institute of Technology
Pasadena, United States
11 h-index
22 publications
698 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
11 h-index
18 publications
625 citations

Centre National de la Recherche Scientifique
Paris, France
9 h-index
14 publications
347 citations
Jet Propulsion Laboratory
Pasadena, United States
6 h-index
11 publications
964 citations
University of California, Berkeley
Berkeley, United States
6 h-index
11 publications
237 citations
South African Radio Astronomy Observatory
Cape Town, South Africa
5 h-index
23 publications
805 citations
Yale University
New Haven, United States
4 h-index
4 publications
141 citations

Pennsylvania State University
State College, United States
4 h-index
7 publications
217 citations
1–8 of 165
AJ · 14 publications · 984 citations
14
h-index
ApJ · 12 publications · 562 citations
12
h-index
10 publications · 1.2K citations
10
h-index
6 publications · 215 citations
6
h-index
PASP · 3 publications · 135 citations
3
h-index
1–5