Welcome to the University of Michigan – Dearborn Observatory Founded 2007.
Wide Field Imaging Not really a novice RV lifestyle forced change in 2009 Light weight and portable equipment Ideal for wide field imaging with camera.
By Kevin Saunders. tml tml.
Bhattacharya phys455
Webcams and CCTV Cameras: Affordable Imaging Tools for the Amateur Astronomer Giles Hammond Institute for Gravitational Research University of Glasgow.
Detector Monitoring as part of VLT Science and Data Flow Operations
NGC 6217 in DSI mode with F658N Mosaic before new superbias why we don’t release images until after SMOV! ACS CCD monitoring and pipeline calibration review.
Denoising photographs using dark frames optimized by quadratic programming Manuel Gomez-Rodriguez * Jens Kober † Bernhard Schölkopf † † Max Planck Institute.
The DWARF project: Vidojevica Vince Oliver, Astronomical observatory of Belgrade
CCD testing Enver Alagoz 12 April 2010. CCD testing goals CCD testing is to learn how to – do dark noise characterization – do gain measurements – determine.
