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Catalog excerpts
![ApogeeAspen CG9000 - 1](https://img.directindustry.com/pdf/repository_di/34591/apogeeaspen-cg9000-725315_1m.jpg)
High Performance Cooled CCD Camera System ANDOR an Oxford Instruments company Typical. Applications Y Astrophotography Y Sky Surveys Y Radiology • High Resolution Sensor 9.3 Megapixel sensor with 12 mm pixels delivers an exceptionally large field of view with high resolution. • Programmable TE cooling down to 60oC below ambient Ideal for detection of weak chemiluminescence or astronomy images, enabling long exposure acquisitions with optimized signal to noise ratio. • Ethernet interface with built-in web server Remote access and control over the Internet, via standard web browser. • USB 2.0 interface Direct ‘Plug and Play’ simplicity of USB 2.0. • 16-Bit digitization High photometric accuracy. • High longevity shutter Shutter during readout and take dark reference frames - 58 mm. Specified for >5 million cycles. • Programmable I/O port Synchronization with intricate experimental set-ups. • Remote Triggering LVTTL input allows exposure to start within 25 microseconds of the rising edge of the trigger. • Focusing mode Faster readout option, ideal for focus optimisation. Array Size (pixels) Pixel Size Sensor Size Pixel Well Depth (typical) • 2 Dark Current •3 Read Noise Maximum Dynamic Range Quantum Efficiency Apogee Aspen CG9000: Compact, 9.3 Megapixel CCD Ideally suited to challenging astronomy and physical science imaging applications, the Apogee Aspen family offers a range of popular full frame CCD sensors, within a camera platform that is designed to push performance. Deep thermoelectric cooling ensures optimal sensitivity for long exposure applications. The simple convenience of a USB 2.0 interface is accompanied by an Ethernet network interface with a built-in web server. The Apogee Aspen also utilizes a new extremely high reliability shutter, specified for > 5 million shutter cycles. The Aspen CG9000 uses a very large format 9.3 megapixel full frame sensor with 12 mm pixels and anti-blooming gates. Cooling down to 60oC below ambient results in a low dark current contribution. These features make the Aspen CG9000 an ideal solution for applications requiring both a large field of view and optimal signal to noise ratio, such as astrophotography, sky surveys and radiology.
Open the catalog to page 1![ApogeeAspen CG9000 - 3](https://img.directindustry.com/pdf/repository_di/34591/apogeeaspen-cg9000-725315_3m.jpg)
High Performance Cooled CCD Camera System ANDOR an Oxford Instruments company Size of CCD Imaging Area Mechanical Drawings Mechanical Specifications Camera Housing
Open the catalog to page 3![ApogeeAspen CG9000 - 4](https://img.directindustry.com/pdf/repository_di/34591/apogeeaspen-cg9000-725315_4m.jpg)
High Performance Cooled CCD Camera System ANDOR an Oxford Instruments company CREATING THE OPTIMUM PRODUCT FOR YOU How to customize the Apogee Aspen CG9000: Step 1: Select your camera type
Open the catalog to page 4![ApogeeAspen CG9000 - 5](https://img.directindustry.com/pdf/repository_di/34591/apogeeaspen-cg9000-725315_5m.jpg)
High Performance Cooled CCD Camera System ANDOR an Oxford Instruments company Order Today Need more information? At Andor we are committed to finding the correct solution for you. With a dedicated team of technical advisors, we are able to offer you one-to-one guidance and technical support on all Andor products. For a full listing of our Footnotes 1. Figures are typical unless stated otherwise 3. Readout noise is for the entire system. It is a combination of sensor readout noise and A/D noise. 4. Quantum efficiency of the sensor at 25°C, as supplied by the sensor manufacturer. 5. Assumes...
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