University of California, Santa Cruz, Department of Astronomy and Astrophysics
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Affiliated Works
sorted by decreasing year, and then by display-name
- Accumulation of Giant Planet Atmospheres Around Cores of a Few Earth Masses
- Accumulation of Giant Planet Atmospheres Around 5 -- 10 M<SUB>⊕ </SUB> Cores
- Core Accretion - Gas Capture Model for Gas Giant Planet Formation
- Formation of Jupiter via Core Nucleated Accretion Within a Dissipating Protoplanetary Disk
- Climates of Oblique Exoplanets
- Joint Fitting of the Gamma-Ray Spectrum and Neutron-Capture Line Decay Profile and Normalization to Constrain Ion Acceleration in Large Flares
- Models of Jupiter's Growth Incorporating Thermal and Hydrodynamics Constraints
- Fates of Ejecta from Tethys
- Fates of ejecta from co-orbital satellites: Tethys, Telesto, and Calypso
- Using Animations to Study the Formation of Gas Giant Planets via the Core Accretion Model
- A Self-consistent Model of the Growth of Jupiter's Core
- Are there more TGFs in the RHESSI data?
- Combining Kepler and HARPS Exoplanet Occurrence Rates to Infer the Period-Mass-Radius Distribution of Super-Earths/Sub-Neptunes
- Formation of Jupiter's Core and Early Stages of Envelope Accretion
- Internal Gravity Waves modulate the apparent misalignment of Exoplanets around Hot Stars
- Double Diffusive Convection in Jupiter as a result of H/He demixing
- Temporal Characteristics of Impulsive Electron Precipitation Associated with Thunderstorm Activity
- Characterizing Exoplanets with 2-meter Class Space-based Coronagraphs
- Exoplanet detection and characterization with the WFIRST space coronagraph
- HabEx: Finding and characterizing Habitable Exoplanets with a potential future flagship astrophysics mission
- Imaging and characterizing exo-Earths at 10 microns - The TIKI project
- Sulfur and Sulfuric Acid Microphysics in the Venus Atmosphere: Implications for the Unknown UV Absorber
- Atmospheric Escape from Exoplanets
- Abiotic Oxygen on the Atmospheres of Venus-Like Exoplanets
- Outgassing Experiments on Carbonaceous Chondrites to Understand the Formation of Titan's Atmosphere
- Simultaneous Optical/NIR and Radio Observations of Uranus