Program: GS-2014B-Q-500

Abstract

Publications using this program's data

• [data] [ADS] Astrometric Confirmation and Preliminary Orbital Parameters of the Young Exoplanet 51 Eridani b with the Gemini Planet Imager
• [data] [ADS] Discovery and spectroscopy of the young jovian planet 51 Eri b with the Gemini Planet Imager
• [data] [ADS] The Orbit and Transit Prospects for β Pictoris b Constrained with One Milliarcsecond Astrometry
• [data] [ADS] Improving and Assessing Planet Sensitivity of the GPI Exoplanet Survey with a Forward Model Matched Filter
• [data] [ADS] Characterizing 51 Eri b from 1 to 5 μm: A Partly Cloudy Exoplanet
• [data] [ADS] A Model-independent Mass and Moderate Eccentricity for β Pic b
• [data] [ADS] The Gemini Planet Imager Exoplanet Survey: Giant Planet and Brown Dwarf Demographics From 10-100 AU
• [data] [ADS] First Resolved Scattered-light Images of Four Debris Disks in Scorpius-Centaurus with the Gemini Planet Imager
• [data] [ADS] Hint of curvature in the orbital motion of the exoplanet 51 Eridani b using 3 yr of VLT/SPHERE monitoring
• [data] [ADS] Detecting Planets from Direct-imaging Observations Using Common Spatial Pattern Filtering
• [data] [ADS] Direct imaging of irregular satellite discs in scattered light
• [data] [ADS] The Gemini Planet Imager View of the HD 32297 Debris Disk
• [data] [ADS] Model of the Search for Extraterrestrial Intelligence with Coronagraphic Imaging
• [data] [ADS] Debris Disk Results from the Gemini Planet Imager Exoplanet Survey's Polarimetric Imaging Campaign
• [data] [ADS] Dynamical Mass Estimates of the β Pictoris Planetary System through Gaussian Process Stellar Activity Modeling
• [data] [ADS] Precise Dynamical Masses and Orbital Fits for beta Pic β and β Pic c
• [data] [ADS] Limits on the mass and initial entropy of 51 Eri b from Gaia EDR3 astrometry
• [data] [ADS] An optimized survey strategy for the ERIS/NIX imager: searching for young giant exoplanets and very low mass brown dwarfs using the K-peak custom photometric filter
• [data] [ADS] α-deep Probabilistic Inference (α-DPI): Efficient Uncertainty Quantification from Exoplanet Astrometry to Black Hole Feature Extraction
• [data] [ADS] The Infrared Colors of 51 Eridani b: Micrometeoroid Dust or Chemical Disequilibrium?