Influence of restricted FOV and CCD binning in SH-WFS on the performance of NAOMI

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 5490, Issue PART 2, 2004, Pages 574-579

  Sochting I K ^a   Wilson, R ^b   Myers, R ^b   Longmore, A ^c   Benn, C ^d   Ostensen, R ^d   Els, S ^d   Goodsell, S ^d   Gregory, T ^d   Talbot, G ^d  

^a UNIVERSITY OF OXFORD   (United Kingdom)

^b DURHAM UNIVERSITY   (United Kingdom)

^c Science and Technology Facilities Council   (United Kingdom)

^d ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

Author keywords

Adaptive Optics; Performance Modelling; Shack Hartmann Wave Front Sensor

Indexed keywords

ASTRONOMY; ATMOSPHERIC TURBULENCE; CONDITION MONITORING; MIRRORS; OPTICAL PHASE CONJUGATION; OPTICAL RESOLVING POWER; OPTICAL TELESCOPES; PERFORMANCE; SENSORS; WAVE PROPAGATION;

DEFORMABLE MIRRORS (DM); ELECTRONIC ROOMS; PERFORMANCE MODELING; SHACK-HARTMANN WAVEFRONT SENSOR;

ADAPTIVE OPTICS;

EID: 19944373051     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.552046     Document Type: Conference Paper

References (3)

1. Benn C., et al., 2004, SPIE, this proceedings
2. Harder S., Chelli A., 2000, A&AS, 142, 119
3. Myers R., et al., 2003, SPIE, 4839, 647