Ground-based Photometry
Ground-Based Photometry is a measurement technique in observational astronomy that quantifies the brightness of celestial sources using instruments located on Earth’s surface, distinguished by its reliance on atmospheric transmission and correction for local environmental and artificial light contamination.
347
Publications
20.4K
Citations
2.3K
Authors
599
Institutions
Publications per year
2017–2026
119
Parents
347
1–5 of 347
2.3K
21
h-index
Center for Astrophysics Harvard & Smithsonian, United States
23 publications · 882 citations
21
h-index
21
h-index
Center for Astrophysics Harvard & Smithsonian, United States
22 publications · 744 citations
19
h-index
18
h-index
1–5 of 2.3K
599
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
33 h-index
183 publications
8K citations

Space Telescope Science Institute
Baltimore, United States
32 h-index
62 publications
8.5K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
31 h-index
148 publications
6K citations
Massachusetts Institute of Technology
Cambridge, United States
29 h-index
244 publications
8.9K citations
Princeton University
Princeton, United States
28 h-index
71 publications
2.8K citations

Ames Research Center
Mountain View, United States
28 h-index
127 publications
5.1K citations

Centre National de la Recherche Scientifique
Paris, France
26 h-index
150 publications
11.8K citations
California Institute of Technology
Pasadena, United States
26 h-index
80 publications
4.5K citations
1–8 of 599
ApJ · 57 publications · 5.8K citations
36
h-index
62 publications · 3.4K citations
32
h-index
AJ · 50 publications · 2.2K citations
31
h-index
56 publications · 2.8K citations
31
h-index
PASP · 11 publications · 1.4K citations
10
h-index
1–5