Transit Depth Analysis
Transit Depth Analysis is a quantitative method in exoplanetary science that measures the fractional decrease in a star's observed flux during a planetary transit to infer the relative size of an exoplanet with respect to its host star.
208
Publications
15.4K
Citations
877
Authors
368
Institutions
Publications per year
2017–2026
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208
HAT-P-11b: A SUPER-NEPTUNE PLANET TRANSITING A BRIGHT K STAR IN THE<i>KEPLER</i>FIELD
G. Á. Bakos, Guillermo Torres, András Pál et al. · The Astrophysical Journal · 2010 · 424 citations · Full text
Natural Sciences, Astronomy, Physics +16
Evaporation of the planet HD 189733b observed in H I Lyman-<i>α</i>
A. Lecavelier des Étangs, D. Ehrenreich, A. Vidal‐Madjar et al. · Astronomy and Astrophysics · 2010 · 372 citations · Full text
Natural Sciences, Astronomy, Physics +15
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
30 h-index
113 publications
16.1K citations
Massachusetts Institute of Technology
Cambridge, United States
27 h-index
66 publications
5.8K citations
California Institute of Technology
Pasadena, United States
27 h-index
90 publications
7.5K citations

Centre National de la Recherche Scientifique
Paris, France
23 h-index
97 publications
11.4K citations

Ames Research Center
Mountain View, United States
22 h-index
63 publications
5.6K citations
University of California, Santa Cruz
Santa Cruz, United States
21 h-index
43 publications
6K citations
University of California, Berkeley
Berkeley, United States
21 h-index
33 publications
3.3K citations

Space Telescope Science Institute
Baltimore, United States
21 h-index
37 publications
3.3K citations
1–8 of 368
ApJ · 49 publications · 5.7K citations
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37 publications · 2.8K citations
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AJ · 29 publications · 1.3K citations
24
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25 publications · 1.6K citations
21
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18 publications · 1.2K citations
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