Specifications Summary 1. Array Size (pixels) Pixel Well Depth (typical) 94,000 e - Dark Current 2. Read Noise 3
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1 Apogee Alta Series System Features 1 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 45 o C below ambient Ideal for detection of weak chemiluminescence or astronomy images, enabling long exposure acquisitions with optimized signal to noise ratio. USB 2.0 interface Direct Plug and Play simplicity of USB Bit digitization High photometric accuracy. High longevity shutter Shutter during readout and take dark reference frames - 63 mm. 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. Precision locking filter wheels optional Choose from a range of Apogee family filter wheels with up to 17 positions. Andor OEM optimisation Compact and robust, Andor integration support, Andor quality enhancement, Andor post-sale support. Now also supported by Andor SDK Apogee Alta F9000: Compact, 9.3 Megapixel CCD Ideal for OEM and astronomy applications, the Apogee Alta family has been a mainstream of high end imaging for many years, offering a wide range of full frame and interline CCDs. A USB 2.0 interface offers the convenience of simple, robust connection to PC. The Alta F9000 uses a very large format 9.3 megapixel full frame sensor with anti-blooming gates, ideal for applications requiring large field of view, such as astrophotography, sky surveys and radiology. Cooling down to 45 o C below ambient results in a low dark current contribution. These features combine to make the Alta F9000 an ideal solution for applications requring both a large field of view and optimal signal to noise ratio, such as astrophotography, sky surveys and radiology. Specifications Summary 1 Array Size (pixels) Pixel Size Sensor Size 3056 x 3056 (9.3 Megapixel) 12 x 12 mm 36.7 x 36.7 mm (1345 mm 2 ) 51.9 mm diagonal Pixel Well Depth (typical) 94,000 e - Dark Current 2 Read Noise e - /pixel/sec 16.1 e MHz) Maximum Dynamic Range 75.3 db (5839:1) Quantum Efficiency 1
2 SPECIFICATIONS Technical Specifications 1 Sensor Type Active pixels Sensor Size Pixel Size KAF (ON Semiconductor) 3056 x 3056 W x H (9.3 Megapixel) 36.7 x 36.7 mm (1345 mm 2 ) 51.9 mm diagonal 12 x 12 mm Pixel Well Depth 94,000 e - Read Noise 3 Pixel Binning Quantum Efficiency 4 Cooling Temperature Stability Dark Current 3 Blemish Specification 16.1 e- Mhz) 1 x 1 to 8 x 3056 on chip Maximum cooling up to 45 C below ambient temperature; -20 C at 25 C ambient Thermoelectric cooler with forced air. +/- 0.1 o C e - /pixel/sec Grade S as per sensor manufacturer definition Anti-blooming factor >100x Maximum Dynamic Range 75.3 db (5839:1) Linearity Better than 99% Frame Rate (fps) 5 Frame Sizes Digital Resolution Camera Window 0.29 Full frame (@2.90 MHz) 0.61 Full frame (@6.37 MHz, focusing mode) Full frame, sub-frame 16-bit UV-grade fused silica General Specifications Interface Options USB 2.0 Remote Triggering Peripheral communications Image Sequencing Exposure Time Operating System Support LVTTL trigger input, expose strobe output 8 pin mini-din I/O connector 1 to image sequences under software control 100 milliseconds to 183 minutes (2.56 microsecond increments) Windows, Linux 2
3 Quantum Efficiency (QE) Curve 5 Size of CCD Imaging Area 36.7 x 36.7 mm Mechanical Drawings Connections Power USB Status LEDs I/O Connector Mechanical Specifications Camera Housing Aluminum, hard anodized (D07) Camera Head Size 7 x7 x2.55 (17.8x17.8x6.48 cm) Back Focal Distance Mounting Shutter Weight (2.56 cm) [optical] bolt circle TPI thread. Optional Nikon F-mount or Canon EOS/EF or FD mount. 63 mm shutter. 4.2 lb. (1.9 kg) 3
4 CREATING THE OPTIMUM PRODUCT FOR YOU How to customize the Alta F9000: Step 1: Select your camera type Description Apogee Alta F Megapixel Full frame CCD camera Grade S sensor and 63 mm Shutter Part Code F9000-S-D07-S63 Camera Step 2: Please indicate which adapters and accessories are required Adapters & Accessories A wide range of mounting adapters and accessory options are available for the Alta. Please refer to the links below for further information on filter wheels, filters and adapters. Filter Wheels Filter wheels available with up to 17 filter positions. Please refer to Apogee Filter Wheels Filters A comprehensive selection of Astrodon filters and filters are available to complement your selected filter wheel Please refer to Apogee Filters Lens Adapters and flanges Select the required camera mounting option for your application, Please refer to Apogee Adapter Matrix from our range of lens, telescope and slip-fit faceplate adapters. Step 3: Please indicate which software you require The Alta also requires at least one of the following software options: Software Description Ordering Information Windows SDK for Apogee Please download from the Apogee Downloads Page ASCOM Camera and Filter Wheel Driver Please download from the Apogee Downloads Page Linux Driver CD Maxim DL Pro Software CD MicroManager Please see 4
5 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 local sales offices, please see: andor.com/contact Our regional headquarters are: Europe Belfast, Northern Ireland Japan Tokyo Phone +44 (28) Phone +81 (3) Fax +44 (28) Fax +81 (3) North America China Connecticut, USA Beijing Phone +1 (860) Phone +86 (10) Fax +1 (860) Fax +86 (10) Footnotes 1. Figures are typical unless stated otherwise 2. At minimum temperature 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 internal trigger mode of operation and minimum exposure time. Front page image M101, the Pinwheel Galaxy courtesy of Greg Morgan. Check out other astounding images captured with Apogee cameras at the Andor image gallery PC Requirements Operating and Storage Conditions 3.0 GHz single core or 2.4 GHz multi core processor Operating Temperature: 0 to 40ºC 2 GB RAM Relative Humidity: < 70% (non-condensing) FM40523 EMS91062 OHS MB free hard disc to install software (at least Storage Temperature: -25ºC to 50ºC 1GB recommended for data spooling) Altitude up to 2000 m USB 2.0 High Speed Host Controller capable of a sustained rate of 40MB/s Windows (XP, Vista, 7 and 8) or Linux Power Requirements V, AC 50-60Hz, or alternate 12V input from user s source. 40W maximum power consumption (shutter open and cooling maximum) ALTA F R2 5
Specifications Summary 1. Array Size (pixels) Pixel Size. Sensor Size. Dark Current 2. Pixel Well Depth (typical) e e -
AVAILABLE WITH LOW NOISE & HIGH DYNAMIC RANGE sensor options Apogee Alta Series System Features 1 High Resolution Sensors 1.0 Megapixel sensor with large 24 mm pixels deliver a large field of view with
scmos discover new ways of seeing andor.com Features and Benefits Scientific CMOS - Fast, sensitive, compact and light. Specifications Summary
Ultra Sensitive Imaging Low Light Imaging Features and Benefits Compact and light Ideal for integration into space restrictive set-ups 1.2 e - read noise Lower detection limit than any CCD 5.5 megapixel
andor.com Scientific CMOS - Fast, sensitive, compact and light Features and Benefits Specifications Summary Ultra Sensitive Imaging Low Light Imaging
Interline CCD 5.5 e - read noise Andor scmos 1.2 e - read noise Low Light Imaging Ultra Sensitive Imaging Upgrading to Zyla scmos can radically improve the performance of your fluorescence microscope Features
Neo scmos. Specifications Summary 2. Pixel size (W x H) 6.5 µm. Pixel well depth (typical) 30,000 e - Pixel readout rate (MHz) 560, 200
Interline CCD 5.5 e - read noise Interline CCD 5.5 e - read noise Andor scmos 1 e - read noise Low Light Imaging Ultra Sensitive Imaging Andor scmos 1 e - read noise Features and Benefits TE cooling to
Specifications Summary. Active pixels 1024 x Pixel size (W x H) 13 µm x 13 µm. Active area pixel well depth (typical) 100,000 e -
Features and Benefits QE > 90% beyond 800 nm, optimized for NIR Very high detector sensitivity in near infra-red 5 MHz and 3 MHz readout speeds Rapid frame rates for high throughput cell inspection Dual
SYNCERITY TM 1024 x 256
ELEMENTAL ANALYSIS FLUORESCENCE GRATINGS & OEM SPECTROMETERS OPTICAL COMPONENTS PARTICLE CHARACTERIZATION RAMAN SPECTROSCOPIC ELLIPSOMETRY SPR IMAGING SYNCERITY TM 1024 x 256 Open-Electrode TE-Cooled CCD
Neo scmos. Specifications Summary. Pixel size (W x H) 6.5 µm. Pixel well depth (typical) 25,000 e - Pixel readout rate (MHz) 560, 400, 200
Interline CCD 5.5 e - read noise Low Light Imaging Low Light Imaging Andor scmos 1 e - read noise Features and Benefits 1 e - read noise Lower detection limit than any CCD 5.5 megapixel sensor format and
Neo scmos. Specifications Summary. Pixel size (W x H) 6.5 µm. Pixel well depth (typical) 30,000 e - Pixel readout rate (MHz) 560, 200
Interline CCD 5.5 e - read noise Low Light Imaging Ultra Sensitive Imaging Andor scmos 1 e - read noise Features and Benefits TE cooling to -40 C Minimization of dark current and pixel blemish 1 e - read
800 nm µm Spectroscopy InGaAs PDA. Specifications Summary. Active pixels 512 or Pixel well depth (typical)
Quantum efficiency (%) 100 90 80 70 60 50 40 30 Spectroscopy 20 10 0 1 1.2 1.4 1.6 1.8 2 2.2 2.4 Wavelength (µm) Features and Benefits 0.8 to 2.2 μm Operating wavelength range Peak QE of > 70% High detector
ikon-xl 230 VERY LARGE AREA ASTRONOMY CCD P P P CCD NEW
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Wavelength (nm) Specifications Summary. Active pixels 512 x 512. Pixel size (W x H) 24 µm x 24 µm
QE (%) 100 90 BV 80 70 60 50 40 FI Low Light Imaging Low Light Imaging 30 20 Bioluminescence image showing an agar plate streaked with an Escherichia Coli strain containing bioluminescence genes 10 0 200
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Features and Benefits EM sensor technology
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+5 o C YEAR VACUUM WARRANTY Low Light Imaging Ultra Sensitive Imaging -40 o C -40 o C Vacuum Cooling Lowest dark current Lowest hot pixels Fan-off capability Features and Benefits TE cooling to -40 C Minimization
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Specifications Summary. Active pixels 2048 x Active area pixel well depth 100,000 e - Maximum readout rate. Read noise 2.9 e - Maximum cooling
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Specifications Summary. Active pixels 1024 x Pixel size (W x H) 13 µm x 13 µm. Active area pixel well depth
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idus 401 Series Specifications Summary Active pixels 1024 x 127 Register well depth (typical) 1,000,000 e - Maximum spectra per sec 88
Spectroscopy Features and Benefits Peak QE of 95% High detector sensitivity TE cooling to 100 C Negligible dark current without the inconvenience of LN 2 UltraVac 1 Permanent vacuum integrity, critical
600 nm µm Spectroscopy InGaAs PDA. Specifications Summary. Active pixels 512 or Pixel well depth (typical)
Quantum efficiency (%) 100 90 80 70 60 50 40 30 Spectroscopy 20 10 0 0.6 0.8 1 1.2 1.4 1.6 1.8 Wavelength (µm) Features and Benefits 0.6 to 1.7 μm Operating wavelength range Peak QE of > 85% High detector
ikon-xl 231 VERY LARGE AREA ASTRONOMY CCD P P P P CCD NEW
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