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High-Resolution Speckle Imaging at Gemini-North: Exoplanets and Beyond

Resource type
Authors/contributors
Title
High-Resolution Speckle Imaging at Gemini-North: Exoplanets and Beyond
Abstract
Using our state-of-the-art 2-channel speckle imaging instrument, we have recently obtained diffraction-limited optical images at the 8-m Gemini-N telescope. The primary science goal was to search for faint (delta_mag = 4-6 mag) and nearby (<0.05") stellar companions around potential planet hosting stars as part of the small small exoplanet validation for the NASA Kepler and ESA CoRoT missions. As a demonstration of the instrument capabilities on Gemini, we achieved an angular resolution of ~20 mas which yielded the highest resolution ground-based optical image of the Pluto-Charon system ever obtained. Our instrument is likely to return to Gemini-N in mid-2013 for observations by general community programs
Date
2013-01-01
Meeting Name
American Astronomical Society, AAS Meeting
Citation Key
howellHighResolutionSpeckleImaging2013
Accessed
11/8/23, 7:55 PM
Short Title
High-Resolution Speckle Imaging at Gemini-North
Extra
Conference Name: American Astronomical Society Meeting Abstracts #221 ADS Bibcode: 2013AAS...22114208H
Citation
Howell, S. B., Horch, E., Everett, M. E., & Ciardi, D. (2013, January 1). High-Resolution Speckle Imaging at Gemini-North: Exoplanets and Beyond. American Astronomical Society, AAS Meeting. https://ui.adsabs.harvard.edu/abs/2013AAS...22114208H