about
The Pale Orange Dot: The Spectrum and Habitability of Hazy Archean EarthNonphotosynthetic pigments as potential biosignaturesFalse Negatives for Remote Life Detection on Ocean-Bearing Planets: Lessons from the Early Earth.Correlations Between Life-Detection Techniques and Implications for Sampling Site Selection in Planetary Analog Missions.Modeling pN2 through Geological Time: Implications for Planetary Climates and Atmospheric Biosignatures.The Habitability of Proxima Centauri b: Environmental States and Observational Discriminants.Exoplanet Biosignatures: A Review of Remotely Detectable Signs of Life.Exoplanet Biosignatures: Understanding Oxygen as a Biosignature in the Context of Its Environment.Exoplanet Biosignatures: At the Dawn of a New Era of Planetary Observations.Identifying planetary biosignature impostors: spectral features of CO and O_4_ resulting from abiotic O_2_/O_3_ProductionPale Orange Dots: The Impact of Organic Haze on the Habitability and Detectability of Earthlike Exoplanets
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description
researcher ORCID ID = 0000-0002-2949-2163
@en
wetenschapper
@nl
name
Edward Schwieterman
@ast
Edward Schwieterman
@en
Edward Schwieterman
@es
Edward Schwieterman
@nl
type
label
Edward Schwieterman
@ast
Edward Schwieterman
@en
Edward Schwieterman
@es
Edward Schwieterman
@nl
prefLabel
Edward Schwieterman
@ast
Edward Schwieterman
@en
Edward Schwieterman
@es
Edward Schwieterman
@nl
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0000-0002-2949-2163