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Published byMarybeth Powell Modified over 9 years ago
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Jamie Holder University of Leeds August 2005 Status and Performance of the First VERITAS Telescope
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VERITAS Telescope I 12m diameter reflector –Davies-Cotton F/1.0 –110m 2 499 PMT Camera Steel OSS Installed at Mt. Hopkins Basecamp (1275m) in January 2005
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Mechanical Performance Alt-Az mount Slew speed –0.3 /sec –1.0 /sec modified Tracking accuracy –Still evaluating –Encoders give <0.005 –Source location good
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Optical Performance 350 mirror facets –glass –aluminium coated on- site reflectivity >90% at 320nm PSF –0.09 FWHM initially –0.06 now PSF plot (with PMT size)
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Camera 499 PMTs –Photonis XP2970 –0.15 spacing –3.5 FOV PMT Gain = 2 10 5 NSB ~100 - 200 MHz No light cones yet Single photoelectron peak (5 times operating voltage)
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Trigger Each channel has programmable CFDs CFD output sent to pattern selection trigger –any 3 adjacent PMTs Trigger rate ~ 150Hz
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Data Acquisition PMT signals digitized with 500MHz sampling FADCs Data rates –24 samples/channel –13.5 kb/event –10% deadtime @ 150 Hz –4% with zero supression
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Timing Define optimum integration gate (10ns) Poster: “Exploiting VERITAS Timing Information” Holder et al.
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Results Crab Nebula observations –3.9 hours ON/OFF –19.4 s –10 s /hour Note –Engineering data –Preliminary analysis –No light cones –cf Whipple 10m (7 s /hour) Mkn 421 and Mkn 501 also detected (Poster: Cogan et al)
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Results Local Muon background –~150 GeV trigger threshold –~400 GeV analysis threshold Need Stereo! Local Muons
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Kitt Peak Site Horseshoe Canyon –1800m –KPNO Completed –Site Clearance –Power –Telescope Pads Temporary access problems
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Temporary Site 2 Telescopes at Mt. Hopkins Basecamp –88m baseline First light October 2005 Test –array trigger –array analysis 4 telescopes on Kitt Peak October 2006
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