However, the timely design, fabrication & deployment of NGAO are essential to ... NIR Imager with low wavefront error & high sensitivity. Required for all key ...
Don't use OSIRIS. Saves engineering cost of feeding OSIRIS. No visible imager ... Reduced switchyard opto-mechanics see above on OSIRIS and vis imager ...
NGAO is ready to become a real project: Ready to begin system design phase ... Need to take advantage of expertise & resources at CIT, UC & WMKO in system design ...
Protoplanetary Disk found Encircling Mira B Michael Ireland - Caltech Co-authors: John Monnier (U. Michigan), Peter Tuthill (U. Sydney), Richard Cohen (Keck Observatory)
NGAO System Design Phase. Update. Peter Wizinowich, Rich Dekany, Don ... Report 6 submitted to ... Norbert Hubin (ESO, Chair) Nick Scoville (Caltech) Gary ...
... as delivering stable high Strehl ratio infrared images in moderate field-of ... of the scientific advances in high-resolution imaging are currently thought to be. ...
Review new data on the telescope static and dynamic wavefront errors. ... E. Johansson and G. Chanan, 'Summary of WFS/FDC Vibration Tests', KOAN 199, 2000. ...
Includes conceptual design (with options), initial cost ... Who is doing what, and what % of time is each person devoting to NGAO? Details in project plan. ...
Galaxy assembly & star formation history. Nearby Active Galactic Nuclei ... 'The proposed schedule and budget estimate have been carried out with sound methodology' ...