Acton Princeton Instruments Pixis 1024 UV/NIR Spectroscopy Astronomy Camera

Description

Acton Princeton Instruments Pixis 1024 UV/NIR Spectroscopy Astronomy Camera
no power supply included
mounting plate is included, we can take it off if not needed.
Please Note the following:
Actual Picture of Unit
No accessories provided unless pictured.
If you have any questions regarding this item, please contact me _before_ bidding.
Manufacturer information (not our description)
The PIXIS: 1024 series of cameras from Princeton Instruments (PI) are fully integrated, low noise cameras with 1024 x 1024 resolution designed for quantitative scientific imaging applications from UV to NIR. Based on PI’s exclusive XP cooling technology, PIXIS are the only cameras that offer cooling down to -90°C, with an all-metal, hermetically sealed design and the industry’s only lifetime vacuum guarantee. High QE and ultra low-noise electronics make the PIXIS: 1024 series of cameras ideal for demanding, low light applications such as astronomy, Bose-Einstein Condensate (BEC), solar cell inspection, chemiluminescence and fluorescence imaging. The exclusive B_eXcelon and BR_eXcelon technologies of the PIXIS:1024 deliver the highest sensitivity in the UV-NIR range while suppressing the etaloning that occurs in standard back illuminated CCDs. Dual speed operation at 100kHz or 2MHz enables these cameras to be used both for steady state as well as fast kinetics studies.
FEATURE BENEFITS Back-illuminated, deep depletion CCD with eXcelon® technology (BR_eXcelon) Highest QE in the UV and NIR range; High QE in the NIR range; Eliminates etaloning. Back-illuminated, eXcelon® technology (B_eXcelon) Lower dark charge than back-illuminated deep depletion CCDs; Extremely low etaloning. 1024 x 1024 imaging array, 13 mm x 13 mm pixels Scientific grade CCD High spatial resolution. Low noise, few defects, linear response. All-metal, hermetic vacuum seals; Lifetime vacuum guarantee No out-gassing (as in epoxy seals) which can compromise vacuum performance; Worry free operation. Deep cooling Low dark noise allows detection of faint signals; CoolCUBE II, a compact room temperature coolant circulator, is available for vibration sensitive environments. Single fused silica vacuum window Minimizes reflection losses from UV to IR; No optical losses due to multiple optical surfaces; Optional AR coating and wedge windows available. Optional UV phosphor coatings Enhances sensitivity throughout the UV to below 200 nm. TTL input and output, and shutter control External control and triggering. Low noise electronics Best performance for low light level applications. Dual digitizers Dual-speed digitization allows complete freedom to select between “slow operation” for low noise and highest SNR or “fast operation” for rapid image acquisition. Software selectable system gains Flexibility to optimize signal-to-noise ratio and dynamic range. Kinetics Custom readout mode offers microsecond resolution. USB2.0 data interface Plug-and-play operation with desktops or laptops; Optional fiber optic interface for remote operation. Optional: LightField® (for Windows 8/7, 64-bit) Or WinView/Spec (for Windows 8/7/XP, 32-bit) Flexible software packages for data acquisition, display and analysis; LightField offers intuitive, cutting edge user interface, IntelliCal® and more. PICAM (64-bit) / PVCAM (32-bit) software development kits (SDKs)) Compatible with Windows 8/7/XP, and Linux; Universal programming interfaces for easy custom programmin
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WAREHOUSE LOCATION
F-1-3