Science Publications

Employing ShaneAO Data

Hirsch, Lea, et al. "SOFIA/FORCAST AND SPITZER/IRAC IMAGING OF THE ULTRACOMPACT H II REGION W3 (OH) AND ASSOCIATED PROTOSTARS IN W3." The Astrophysical Journal 757.2 (2012): 113.

Alyse Hirsch, Lea, et al. "Stellar Multiples Among the KOIs." AAS/Division for Extreme Solar Systems Abstracts. Vol. 3. 2015.

Gautier, Thomas N., et al. "High Resolution Active Optics Observations from the Kepler Follow-up Observation Program." American Astronomical Society Meeting Abstracts# 223. Vol. 223. 2014.

Bordwell, Baylee, et al. "FIRST, a fibered aperture masking instrument: Results of the Lick observing campaign." American Astronomical Society Meeting Abstracts. Vol. 225. 2015.

Butner, Harold M., et al. "The Search for Possible Stellar Companions of DEBRIS Candidate Stars: An Update." American Astronomical Society Meeting Abstracts# 219. Vol. 219. 2012.

Rodriguez, David R., et al. "Stellar Multiplicity in the DEBRIS disk sample."American Astronomical Society Meeting Abstracts. Vol. 225. 2015.

Rodriguez, David R., et al. "Stellar multiplicity and debris discs: an unbiased sample." Monthly Notices of the Royal Astronomical Society 449.3 (2015): 3160-3170. [8]

Everett, Mark E., et al. "High-resolution multi-band imaging for validation and characterization of small Kepler planets." The Astronomical Journal 149.2 (2015): 55. [9]

Wolfgang, Angie, and G. P. Laughlin. "Implications for Planet Formation and Evolution Processes from AO Imaging of Kepler Planet Candidate Host Stars." American Astronomical Society Meeting Abstracts# 221. Vol. 221. 2013.

Wolfgang, Angie. "The Power of a Planet Population: Kepler's Super-Earth Compositions, Mass-Radius Relation, and Host Star Multiplicity." American Astronomical Society Meeting Abstracts. Vol. 225. 2015.

Lépine, Sébastien, et al. "An Astrometric Companion to the Nearby Metal-Poor, Low-Mass Star LHS 1589Based on observations performed with the Laser Guide Star Adaptive Optics system at the Lick Observatory, operated by the University of California system. Based on observations conducted at the MDM observatory, operated jointly by the University of Michigan, Dartmouth College, the Ohio State University, Columbia University, and the University of Ohio." The Astrophysical Journal 668.1 (2007): 507. [4]

Malz, A. I., R. Rich, and S. Lepine. "Low-mass Binaries in the Galactic Halo Resolved by Adaptive Optics." American Astronomical Society Meeting Abstracts# 213. Vol. 213. 2009.