The Gemini Planet Imager: from science to design to construction

By B. Macintosh, J. Graham, D. Palmer, R. Doyon, J. Dunn, D. Gavel, J. Larkin, B. Oppenheimer, L. Saddlemyer, A. Sivaramakrishnan and 6 more. Astronomical Telescopes + Instrumentation, 2008

297 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics

View Paper: https://www.semanticscholar.org/paper/3db4c362abf006da79b1da1d6bdcacea68903b87

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In Aerospace Engineering

1. N. Madhusudhan
2. Adam Burrows
3. T. Robinson

In Astronomy and Astrophysics

1. N. Madhusudhan
2. Adam Burrows
3. M. Marley
4. Jon Fortney
5. T. Robinson
6. D. Apai
7. B. Bowler
8. T. Currie

In Atomic and Molecular Physics, and Optics

1. M. Marley
2. L. Pueyo
3. J. Larkin
4. Adam Burrows
5. Remi Soummer
6. N. Madhusudhan
7. T. Robinson
8. D. Apai

Citations in the corpus

• A COMBINED SUBARU/VLT/MMT 1–5 μm STUDY OF PLANETS ORBITING HR 8799: IMPLICATIONS FOR ATMOSPHERIC PROPERTIES, MASSES, AND FORMATION (2011, background): “Integral field spectrographs on Gemini Planet Imager (GPI MacIntosh et al. 2008) and SPHERE (Beuzit et al. 2008) will sample the 1–2.5 µm SED region with exceptional sensitivity and thus provide a detailed comparison between observed and predicted atmospheric properties of all planets.”
• On the Cool Side: Modeling the Atmospheres of Brown Dwarfs and Giant Planets (2014, background): “…that are expected to be discovered by the Gemini Planet Imager (GPI) and the Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) surveys for young planets (Macintosh et al. 2008; Beuzit et al. 2008), CO may be the dominant carbon bearing species until temperatures as low as about 600 K.”
• DETECTION AND CHARACTERIZATION OF EXOPLANETS AND DISKS USING PROJECTIONS ON KARHUNEN–LOÈVE EIGENIMAGES (2012, background): “Direct imaging results will significantly expand in the near future with a new generation ground-based instruments being implemented (Macintosh et al. 2008; Beuzit et al. 2008; Hinkley et al. 2011; Hodapp et al. 2008).”
• MODEL ATMOSPHERES FOR MASSIVE GAS GIANTS WITH THICK CLOUDS: APPLICATION TO THE HR 8799 PLANETS AND PREDICTIONS FOR FUTURE DETECTIONS (2011, background): “…programs currently underway – e.g. IDPS and Gemini/NICI (Marois et al. 2011, in progress; Liu et al. 2010) – and upcoming programs like GPI and SPHERE (MacIntosh et al. 2008; Beuzit et al. 2008) will likely image many new planets with a wide range of ages and masses, which translate into a wide…”