activity
20102026
most citedDiscovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager

559 citations · 5.8k across the 113 of their papers we have counts for

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Showing 2012Show all

5 papers · 1 filter

astro-ph.SR2012★ 112 cited

Subaru Imaging of Asymmetric Features in a Transitional Disk in Upper Scorpius

S. Mayama, J. Hashimoto, T. Muto +52

We report high-resolution (0.07 arcsec) near-infrared polarized intensity images of the circumstellar disk around the star 2MASS J16042165-2130284 obtained with HiCIAO mounted on t…

astro-ph.EP2012★ 153 cited

First Light LBT AO Images of HR 8799 bcde at 1.65 and 3.3 Microns: New Discrepancies between Young Planets and Old Brown Dwarfs

Andrew J. Skemer, Philip M. Hinz, Simone Esposito +45

As the only directly imaged multiple planet system, HR 8799 provides a unique opportunity to study the physical properties of several planets in parallel. In this paper, we image a…

astro-ph.SR2012★ 50 cited

High Resolution Images of Orbital Motion in the Orion Trapezium Cluster with the LBT Adaptive Optics System

L. M. Close, A. Puglisi, J. R. Males +28

The new 8.4m LBT adaptive secondary AO system, with its novel pyramid wavefront sensor, was used to produce very high Strehl (75% at 2.16 microns) near infrared narrowband (Br gamm…

astro-ph.EP2012★ 133 cited

The missing cavities in the SEEDS polarized scattered light images of transitional protoplanetary disks: a generic disk model

R. Dong, R. Rafikov, Z. Zhu +53

Transitional circumstellar disks around young stellar objects have a distinctive infrared deficit around 10 microns in their Spectral Energy Distributions (SED), recently measured…

astro-ph.SR2012★ 54 cited

The Gray Needle: Large Grains in the HD 15115 Debris Disk from LBT/PISCES/Ks and LBTI/LMIRcam/L' Adaptive Optics Imaging

Timothy J. Rodigas, Philip M. Hinz, Jarron Leisenring +52

We present diffraction-limited \ks band and \lprime adaptive optics images of the edge-on debris disk around the nearby F2 star HD 15115, obtained with a single 8.4 m primary mirro…