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20022017
most citedClosest Star Seen Orbiting the Supermassive Black Hole at the Centre of the Milky Way

1.2k citations · 4.2k across the 51 of their papers we have counts for

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15 papers · 1 filter

astro-ph.IM2014★ 10 cited

Astrometric Calibration of the Gemini NICI Planet-Finding Campaign

Thomas L. Hayward, Beth A. Biller, Michael C. Liu +6

We describe the astrometric calibration of the Gemini NICI Planet-Finding Campaign. The Campaign requires a relative astrometric accuracy of 20 mas across multi-year time…

astro-ph.IM2014★ 2 cited

On-sky low order non-common path correction of the GPI Calibration Unit

Markus Hartung, Bruce Macintosh, Paul Langlois +12

The Gemini Planet Imager (GPI) entered on-sky commissioning phase, and had its First Light at the Gemini South telescope in November 2013. Meanwhile, the fast loops for atmospheric…

astro-ph.IM2014★ 7 cited

On-sky vibration environment for the Gemini Planet Imager and mitigation effort

Markus Hartung, Tom Hayward, Les Saddlemyer +20

The Gemini Planet Imager (GPI) entered on-sky commissioning and had its first-light at the Gemini South (GS) telescope in November 2013. GPI is an extreme adaptive optics (XAO), hi…

astro-ph.IM2014

Effects of differential wavefront sensor bias drifts on high contrast imaging

Naru Sadakuni, Bruce A. Macintosh, David W. Palmer +11

The Gemini Planet Imager (GPI) is a new facility, extreme adaptive optics (AO), coronagraphic instrument, currently being integrated onto the 8-meter Gemini South telescope, with t…

astro-ph.IM2014★ 6 cited

Characterization of the Atmospheric Dispersion Corrector of the Gemini Planet Imager

Pascale Hibon, Sandrine Thomas, Jennifer Dunn +18

An Atmospheric Dispersion Corrector (ADC) uses a double-prism arrangement to nullify the vertical chromatic dispersion introduced by the atmosphere at non-zero zenith distances. Th…

astro-ph.IM2014★ 19 cited

The Integral Field Spectrograph for the Gemini Planet Imager

James E. Larkin, Jeffrey K. Chilcote, Theodore Aliado +31

The Gemini Planet Imager (GPI) is a complex optical system designed to directly detect the self-emission of young planets within two arcseconds of their host stars. After suppressi…