activity
20152019
most citedPerformance of the Gemini Planet Imager Non-Redundant Mask and spectroscopy of two close-separation binaries HR 2690 and HD 142527

3 citations · 3 across the 1 of their papers we have counts for

collaborators

5 papers

astro-ph.IM2019★ 3 cited

Performance of the Gemini Planet Imager Non-Redundant Mask and spectroscopy of two close-separation binaries HR 2690 and HD 142527

Alexandra Z. Greenbaum, Anthony Cheetham, Anand Sivaramakrishnan +51

The Gemini Planet Imager (GPI) contains a 10-hole non-redundant mask (NRM), enabling interferometric resolution in complement to its coronagraphic capabilities. The NRM operates bo…

astro-ph.EP2017

1 to 2.4 micron Near-IR spectrum of the Giant Planet Pictoris b obtained with the Gemini Planet Imager

Jeffrey Chilcote, Laurent Pueyo, Robert J. De Rosa +61

Using the Gemini Planet Imager (GPI) located at Gemini South, we measured the near-infrared (1.0-2.4 micron) spectrum of the planetary companion to the nearby, young star Picto…

astro-ph.SR2015

An M-dwarf star in the transition disk of Herbig HD 142527; Physical parameters and orbital elements

S. Lacour, B. Biller, A. Cheetham +29

HD 142527A is one of the most studied Herbig Ae/Be stars with a transitional disk, as it has the largest imaged gap in any protoplanetary disk: the gas is cleared from 30 to 90 AU.…

astro-ph.EP2015

Pictoris' inner disk in polarized light and new orbital parameters for Pictoris b

Maxwell A. Millar-Blanchaer, James R. Graham, Laurent Pueyo +54

We present -band observations of Pic with the Gemini Planet Imager's (GPI's) polarimetry mode that reveal the debris disk between ~0.3" (~6 AU) and ~1.7" (~33 AU), while sim…

astro-ph.EP2015

Gemini Planet Imager Observations of the AU Microscopii Debris Disk: Asymmetries within One Arcsecond

Jason J. Wang, James R. Graham, Laurent Pueyo +42

We present Gemini Planet Imager (GPI) observations of AU Microscopii, a young M dwarf with an edge-on, dusty debris disk. Integral field spectroscopy and broadband imaging polarime…