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Joanna Bulger

Researcher at National Institutes of Natural Sciences, Japan

Publications -  97
Citations -  4654

Joanna Bulger is an academic researcher from National Institutes of Natural Sciences, Japan. The author has contributed to research in topics: Gemini Planet Imager & Debris disk. The author has an hindex of 35, co-authored 93 publications receiving 4053 citations. Previous affiliations of Joanna Bulger include European Southern Observatory & University of Hawaii at Manoa.

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Discovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager

Bruce Macintosh, +94 more
- 02 Oct 2015 - 
TL;DR: Using the Gemini Planet Imager, a Jupiter-like planet is discovered orbiting the ~20-million-year-old star 51 Eridani at a projected separation of 13 astronomical units and has a methane signature and is probably the smallest exoplanet that has been directly imaged.
Journal ArticleDOI

Discovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager

Bruce Macintosh, +94 more
TL;DR: In this paper, the Gemini Planet Imager was used to detect a planet orbiting the star 51 Eridani at a projected separation of 13 astronomical units, with a spectrum with strong methane and water vapor absorption.
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The Gemini Planet Imager Exoplanet Survey: Giant Planet and Brown Dwarf Demographics from 10 to 100 au

Eric L. Nielsen, +73 more
TL;DR: Nielsen et al. as discussed by the authors presented a statistical analysis of the first 300 stars observed by the Gemini Planet Imager Exoplanet Survey (GPEES) to infer the underlying distributions of substellar companions with respect to their mass, semimajor axis, and host stellar mass.
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The Gemini Planet Imager Exoplanet Survey: Giant Planet and Brown Dwarf Demographics From 10-100 AU

TL;DR: In this paper, a statistical analysis of the first 300 stars observed by the Gemini Planet Imager Exoplanet Survey (GPIES) includes six detected planets and three brown dwarfs; from these detections and their contrast curves, infer the underlying distributions of substellar companions with respect to their mass, semi-major axis, and host stellar mass.
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Characterizing 51 Eri b from 1 to 5 μm: A Partly Cloudy Exoplanet

Abhijith Rajan, +65 more
TL;DR: In this paper, the authors proposed a method to detect exoplanets using the ESI program for GPI related to NASA's Exoplanets Research Program (XRP) and NExSS (NExSS).