An Optical Ultrahigh Resolution Spectrograph for Use with Adaptive Optics
| dc.creator | Ge, J. | |
| dc.creator | Jacobsen, B. | |
| dc.creator | Angel, J. R. P. | |
| dc.creator | Woolf, N. | |
| dc.creator | Black, J. H. | |
| dc.creator | Lloyd-Hart, M. | |
| dc.creator | Gray, P. | |
| dc.creator | Fugate, R. Q. | |
| dc.date | 1996-07-29 | |
| dc.date.accessioned | 2026-07-07T02:21:40Z | |
| dc.date.available | 2026-07-07T02:21:40Z | |
| dc.description | A prototype ultrahigh resolution spectrograph has been built with an adaptive optics telescope. It provides $250,000$ resolving power, 300 Å wavelength coverage and 0.8\% efficiency. | |
| dc.description | Review paper; 13 pages with 7 figs included. Also available from "http://qso.as.arizona.edu/~jge/projects.html" | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9607146 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9607146 | |
| dc.identifier | Adaptive Optics, Vol. 13, 1996 OSA Technical Digest Series, 122 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10589 | |
| dc.subject | Astrophysics | |
| dc.title | An Optical Ultrahigh Resolution Spectrograph for Use with Adaptive Optics | |
| dc.type | text |