Paul Etzel

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Slide2: 

MLO Facilities Not shown: 30,000 Gallon Reservoir Pump House Hydrant Stations HPWREN Pole

Science Drivers Exploit the Time Domain: 

Science Drivers Exploit the Time Domain Nova Surveys in Local Group Galaxies Synoptic Observations of Variable Stars (Interacting Binaries, Cataclysmic Variables, Multi-Wavelength Campaigns, Black-Hole Binaries) Star Cluster Photometry Extrasolar Planetary Transits Supernovae Searches in Near-IR Discovery of New Variable Stars

Science Drivers Targets of Opportunity: 

Science Drivers Targets of Opportunity Bright Novae Eruptions of X-ray Binaries Supernovae Relatively bright Microlensing Events Gamma-Ray Bursts Asteroid Occultations Deep Impact Mission (July 2005) http://mintaka.sdsu.edu/faculty/wfw/DEEPIMPACT/index.html

Slide5: 

Also Astronomical Consultants and Equipment, Inc. (ACE)

Slide6: 

CMA, Inc.

ULTRA 40-inch OTA @ CMA ULTRA Telescope Mount @ ACE: 

ULTRA 40-inch OTA @ CMA ULTRA Telescope Mount @ ACE Optical Tube Assembly on test stand with filter-guider box & CCD camera. ULTRA will be run over the Internet via HPWREN from SDSU & KU

New ULTRA 20.5-foot Dome: 

New ULTRA 20.5-foot Dome Photo credit: Monika Braun Rendering of ULTRA Telescope installed in new dome (ACE).

NSF PREST Award: 

NSF PREST Award Refurbish Optical System of “Illinois” 40-inch (nearing completion) Upgrade Telescope Control System (Dec 2006) Upgrade Dome, and Direct Imaging Capabilities (Jan/Feb 2007) Allow Remote Observing – HPWREN Guest Observer Program (20% time allocation, some service observing)

MLO 40-inch with Spectrograph: 

MLO 40-inch with Spectrograph Other Instruments: 2K2 CCD Camera, dual filter wheel, 10 positions each (0.4 “/pixel) 2562 NIRIM Camera (possible upgrade) 10242 High-Speed CCD Camera (<0.1 msec readout) Automated Photometer