Surface Brightness Fluctuations
Surface Brightness Fluctuations is a photometric distance measurement method that relies on the variance in pixel-to-pixel brightness of a galaxy's resolved stellar population to estimate its distance by quantifying the apparent fluctuations in surface brightness caused by the discrete distribution of stars.
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2017–2026
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Sbf
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369
Detailed Structural Decomposition of Galaxy Images
Chien Y. Peng, Luis C. Ho, Chris Impey et al. · The Astronomical Journal · 2002 · 2.8K citations · Full text
Natural Sciences, Astronomy, Physics +12
The absolute magnitudes of Type IA supernovae
M. M. Phillips · The Astrophysical Journal · 1993 · 2.1K citations
Natural Sciences, Astronomy, Physics +10
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University of Hawaii System
Honolulu, United States
29 h-index
55 publications
8.3K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
27 h-index
96 publications
12.7K citations
California Institute of Technology
Pasadena, United States
21 h-index
49 publications
6.6K citations
University of Arizona
Tucson, United States
19 h-index
37 publications
8.6K citations

Kitt Peak National Observatory
Tucson, United States
19 h-index
32 publications
7.6K citations

Australian National University
Canberra, Australia
19 h-index
27 publications
3.5K citations

Johns Hopkins University
Baltimore, United States
18 h-index
27 publications
3.4K citations
University of California, Berkeley
Berkeley, United States
18 h-index
27 publications
1.8K citations
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ApJ · 128 publications · 13.4K citations
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AJ · 40 publications · 5.4K citations
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