The Gemini Planet Imager

By B. Macintosh, J. Graham, D. Palmer, R. Doyon, D. Gavel, J. Larkin, B. Oppenheimer, L. Saddlemyer, J. K. Wallace, B. Bauman and 9 more. SPIE Astronomical Telescopes + Instrumentation, 2006

170 citations recorded by the source corpus.

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

View Paper: https://www.semanticscholar.org/paper/1e2808519c99a68474497bdfa58c8e30aa6c7798

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Jon Fortney
2. M. Marley
3. N. Madhusudhan
4. Adam Burrows
5. D. Saumon
6. A. Showman
7. B. Bowler
8. Th. Henning

In Atomic and Molecular Physics, and Optics

1. M. Marley
2. Jon Fortney
3. D. Saumon
4. K. Lodders
5. Adam Burrows
6. D. Spiegel
7. Th. Henning
8. L. Pueyo

Citations in the corpus

• Magellan Adaptive Optics Imaging of PDS 70: Measuring the Mass Accretion Rate of a Young Giant Planet within a Gapped Disk (2018, background): “With rapidly advancing instrumentation (e.g., Macintosh et al. 2006, Close et al. 2008, Beuzit et al. 2008) it is now possible to place (often powerful) constraints on massive planets interior to gapped disks around nearby young stars.”
• FUNDAMENTAL LIMITATIONS OF HIGH CONTRAST IMAGING SET BY SMALL SAMPLE STATISTICS (2014, background): “This is particularly relevant in the wake of the golden age of high contrast imaging, with many new systems and upgrades coming online (e.g. SPHERE (Kasper et al. 2012), GPI (Macintosh et al. 2014), and recent NACO upgrades (Mawet et al. 2013; Absil et al. 2013)), as well as a series of ground-based”
• Synthetic Spectra and Colors of Young Giant Planet Atmospheres: Effects of Initial Conditions and Atmospheric Metallicity (2008, background): “Work on suppressing the glare of potential parent stars has proceeded to the point where contrast ratios of 10−5 can now typically be achieved on the telescope, and 10−7 is on the horizon (Macintosh et al. 2006; Dohlen et al. 2006).”
• SPECTRAL AND PHOTOMETRIC DIAGNOSTICS OF GIANT PLANET FORMATION SCENARIOS (2011, background): “Examples of such campaigns include the Gemini Planet Imager (GPI; Macintosh et al. 2006; McBride et al. 2011), the NearInfrared Coronagraphic Imager on Gemini South (NICI; Liu et al. 2010), the Spectro-Polarimetric High-contrast Exoplanet REsearch instrument on the Very Large Telescope (SPHERE;…”