QSO Hosts and Environments at [CLC][ITAL]z[/ITAL][/CLC] = 0.9–4.2: [ITAL]JHK[/ITAL] Images with Adaptive OpticsJ. B. Hutchings, Eric Steinbring, D. Crampton et al.|The Astronomical Journal|1999Cited by 42
Maunakea spectroscopic explorer design development from feasibility concept to baseline designKei Szeto, Kai Zhang, Will Saunders et al.|Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE|2016Cited by 24
Characterizing the Adaptive Optics Off‐Axis Point‐Spread Function. I. A Semiempirical Method for Use in Natural Guide Star ObservationsEric Steinbring, James R. Graham, S. M. Faber et al.|Publications of the Astronomical Society of the Pacific|2002Cited by 24
Radio Galaxies at<i>z</i>= 1.1 to 3.8: Adaptive Optics Imaging and Archival<i>Hubble Space Telescope</i>DataEric Steinbring, J. B. Hutchings, D. Crampton|The Astrophysical Journal|2002Cited by 16
Resolution of a<i>z</i>= 1 QSO with Adaptive OpticsJ. B. Hutchings, Eric Steinbring, D. Crampton et al.|Publications of the Astronomical Society of the Pacific|1998Cited by 9