| |
Angel, R. |
| Volume |
Paper Title |
Page Number |
Authors |
| 133 |
Sensitivity of an Active Space Telescope to Faint Sources and Extra-solar Planets |
172 |
Angel, R.; Woolf, N. |
| 164 |
Testing NGST Segment Technology in a 3.5-m Space Telescope |
234 |
Burge, J.; Angel, R. |
| 194 |
Flat mirror optics to study extra-solar terrestrial planets from space |
389 |
Angel, R.; Burge, J.; Woolf, N. |
| 195 |
Design for an 8-m Telescope with a 3 Degree Field at f/1.25: The Dark Matter Telescope |
81 |
Angel, R.; Lesser, M.; Sarlot, R.; Dunham, E. |
| 195 |
Adaptive Optics High Resolution Spectroscopy: Present Status and Future Direction (Poster) |
568 |
Ge, J.; Ciarlo, D.; Kuzmenko, P.; Alcock, C.; Macintosh, B.; Cook, K.; Max, C.; Angel, R.; Woolf, N.; Lloyd-Hart, M.; Najita, J. |
| 232 |
The Large-aperture Synoptic Survey Telescope. |
347 |
Tyson, A.; Angel, R. |
| 280 |
A wide field telescope optimized for multiple object spectroscopy or adaptive optics imaging |
97 |
Burge, J.; Angel, R. |
| 291 |
A Large, Serviceable HST Successor |
263 |
Angel, R.; Codona, J. L. |
| 294 |
Imaging Extrasolar Planets from the Ground |
543 |
Angel, R. |
|
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