SBIG STT 3200 cooled CCD camera

No compromises. Our mid-sized STT Series cameras offer features and specifications found in no other astronomy camera – of any size. Drawing on all of our previous experience and the best of each of our previous designs over the years, the STT represents the culmination of everything that the amateur has asked for in an imaging system, packed into a 4.9 x 4.9 x 2.9 inch body. Standard features include: Two-stage cooling with a temperature delta greater than -50C with air only; water cooling ready; USB 2.0 and Ethernet on every camera; full frame buffer; fast low-noise readout in a fraction of a second; MAR coated sapphire chamber window; self-guiding in front

Compare these STT features with any other camera:

• Ethernet and USB 2.0
• Built-in Web Server
• Full Frame Image Buffer
• 2-Stage TE Cooling > -50C delta T with air
• Liquid Cooling Capability Standard for greater cooling
• Twin Variable Speed Fans
• High Accuracy Temperature Control
• Built-in Frost Detection
• Built-in RBI Pre-flash
• External Triggers In / Out
• Power Management System
• 12VDC Operation
• Lowest Noise 10Mhz Readout (<1 sec download)
• High Precision 8-position Filter Wheel Option
• Accepts 1.25" and 36mm filters
• Even-illumination (photometric) shutter
• Multi-coated Sapphire Chamber Window
• Optional Self-Guiding in Front of filters
• Optional Remote Guide Head
• Optional Adaptive Optics (AO-8T)
• User Rechargeable Desiccant Plug
• Status, Power and Relay Indicators
• Windows and Mac Control Software of the filters; remote guide head support; optional adaptive optics; and more

• Exceptionally High Quantum Efficiency
  

  The KAF-3200ME sensor has perhaps the highest quantum efficiency of any front-illuminated CCD sensor. This makes the STT-3200M ideal for extremely deep imaging, scientific observations, and more.

Specification: