The Apogee Alta U16M CCD Camera employs a Kodak KAF-16803 full frame sensor with microlensing and anti-blooming gates.Features the D07 body and is great for applications requiring large fields of view, like sky surveys and radiology

Alta U Series cameras are available with a wide variety of sensors, including: Back-illuminated sensors with very high quantum efficiency, some with sensitivity in the deep UV; Interline transfer sensors with fast electronic shuttering and inherent anti-blooming; front-illuminated CCDs with high sensitivity in the near-IR without etaloning.

So many improvements in such a small package: No more external controllers, plug-in cards, or frame grabbers. Dual digitization for high precision plus high speed focus. On-board camera memory for fast local sequences and no worries about transfer interruptions. Time delayed integration for imaging far beyond the size of the sensor. A single 12V power input for optional battery-powered operation. In addition, the Apogee Alta U Series cameras have dual digitization, 12 and 16 bit. The 12 bit mode is intended primarily as a focus mode.

The Alta U230 uses a very large format 4-megapixel back-illuminated sensor, ideal for applications requiring large field of view, such as sky surveys and radiology.

The Apogee F9000 Monochrome CCD camera from Apogee is an astro-imaging camera consisting of a Kodak KAF-51000 sensor, advanced fan cooling options, USB 2.0 computer interface connection, as well as a 63mm shutter.

The Apogee Alta F42 CCD Camera has a back-illuminated full frame 4 megapixel EV2 CCD42-40 sensor with very high quantum efficiency. Midband, broadband, and UV-enhanced versions of the CCD are available.

The Apogee Alta F2 is a front illuminated microlensed monochrome CCD camera with Quantum Efficiency of 45% at 400nm. It comes with a fan cooling method in which the observor can cool down to 55°C below ambient temperature, but also can be upgraded with a liquid cooling option as well upon request.