Laser Launch System for the LBT Richard Davies Sebastian Rabien Max Planck Institute for Extraterrestrial Physics Approaches of other observatories
J. H. Burge 3. Image motion due to optical element motion Tilt and decenter of optical components (lenses, mirrors, prisms) will cause motion of the image.
Overall Ingle and Crouch, Spectrochemical Analysis.
Http://nodens.physics.ox.ac.uk/~mcdonnell/wardPres/wardPres.html .
Telescopes of the future: SKA and SKA demonstrators Elaine Sadler, University of Sydney Aperture synthesis techniques have now been in use for over 40.
15 October 20151 Observational Astronomy Direct imaging Photometry Kitchin pp. 187-217, 276-309.
Coronal Spectro- polarimetry with the Turin Lyot-Filter Silvano Fineschi INAF – Astrophysical Observatory of Torino, Italy Future of Polarimetry - Brussels.
Laser Launch System for the LBT
Ion Traps
MIA: Miniature In-Situ Rock Analysis Requiring Minimal Preparation P.E. Clark 1, W. Farrand 2, Joseph P Martin 3, John R Marshall 4, Larry W Mason 5, Dan.
Imaging Spectropolarimetry with IBIS: evolution of a magnetic feature. Del Moro D.
Wide Field Corrector Current status / risk assessment Gary Hill and Hanshin Lee 1.
