Science with the ADOPT system on Mount Wilson

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 3126, Issue , 1997, Pages 321-329

  Shelton, Chris ^a   Schneider, Thomas ^a   Baliunas, Sallie ^a  

^a UNIVERSITY OF ARIZONA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

OPTICAL FILTERS; OPTICAL RESOLVING POWER; OPTICAL TELESCOPES; PLANETS; SPECTROSCOPY;

ASTEROIDS;

ADAPTIVE OPTICS;

EID: 0031289220     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.290174     Document Type: Conference Paper

References (15)

1. Bulk density of asteroid 243 Ida from the orbit of its satellite, Dactyl
2. The coronagraph at the diffraction limit, the detection of faint sources
3. Direct detection of extra-solar planets by imaging - Definition of the background
4. First tests of the Cassegrain adaptive optics system of the Mount Wilson 100-inch telescope
5. Binary star orbits from speckle interferometry VIII. Orbit of 37 close visual systems
6. Chromospheric variation in main sequence stars. II
7. The effects of pulsation-extended atmospheres on the apparent diameters of Mira variables
8. A spectrographic study of Mira Ceti
9. First Hubble Space Telescope observations of Mira AB wind-accreting binary system
10. Performance of the Canada-France-Hawaii telescope adaptive optics bonnette
11. Denominator-free control algorithms for adaptive optics
12. Adaptive optics spectroscopy: Theory and observation