Metallicity Constraints
Metallicity Constraints is a scientific construct in exoplanetary science that specifies the permissible range or bounds on the abundance of elements heavier than helium in an exoplanet’s atmosphere or host star, as inferred from infrared observational data, to inform planetary formation models and atmospheric characterization.
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Galactic Chemical Evolution: Carbon through Zinc
Chiaki Kobayashi, Hideyuki Umeda, K. Nomoto et al. · The Astrophysical Journal · 2006 · 877 citations · Full text
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University of California, Santa Cruz, United States
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Centre National de la Recherche Scientifique
Paris, France
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University of California, Santa Cruz
Santa Cruz, United States
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162 publications
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Space Telescope Science Institute
Baltimore, United States
50 h-index
134 publications
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California Institute of Technology
Pasadena, United States
49 h-index
173 publications
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
44 h-index
188 publications
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University of Cambridge
Cambridge, United Kingdom
42 h-index
110 publications
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Carnegie Observatories
Pasadena, United States
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European Southern Observatory
Garching bei München, Germany
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ApJ · 343 publications · 33.6K citations
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AJ · 83 publications · 5.6K citations
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