|
|
|
* The Apogee Alta U47MB-1 comes with a class 1 back-illuminated E2V CCD47-10 (1024 X 1024 pixel array) full-frame sensor with
very high quantum efficiency.
* The MB version of the Alta U47 sensor has standard grade one midband coatings.
* High resolution, high quantum efficiency, advanced cooling, and low noise make the Apogee U47 one of the most powerful
systems available.
* USB 2.0 Interface.
* The price shown is based on full payment at the time of order. Scroll down to read more about Apogee's rules regarding
pricing & pre-payment.
The Apogee Alta U47 is the most sensitive, cost-effective, back-illuminated CCD Apogee offers, and it is especially well suited
for astronomy. This CCD has 13u pixels, 1K x 1K and a very broad and high QE curve. These are the same Grade 1 Midband coated
47-10 CCDs from E2V that have been standard for the U47 since its introduction. UV coatings and Grade 0 sensors are available at
additional cost.
The U47 has a fast readout time (less than 2 seconds) and a typical noise of 6-8e- at 700Khz. High resolution, high quantum
efficiency, advanced cooling, and low noise make the U47 one of the most powerful systems available. Apogee was the first to
introduce cost-effective back-illuminated CCD technology a decade ago with the AP7, and they have done it again with the U47. Back
illuminated technology has long been the choice for professional astronomers, but has traditionally been out of reach to many with
lower budgets - until now.
The Apogee Alta U47 has a back-illuminated full frame megapixel CCD with exceptionally high quantum efficiency. The included
midband coating (U47-MB) has the highest peak in the visible; the optional broadband coating (U47-BB) has somewhat higher QE in
the near UV but lower QE across the visible. The UV-enhanced version (U47-UV) has the highest QE in the UV (See the quantum
efficiency curve)
Apogee Alta U47 Highlights
* 1024 x 1024 array, 13 x 13 micron pixels
* 2 MHz 12-bit and 700 kHz 16-bit digitization
* 32Mbyte camera memory
* USB 2.0 interface: no plug in cards or external controllers
* Programmable, intelligent cooling to 55C below ambient
* Binning up to 10 Horizontal x 1024 Vertical
* Subarray readout and fast sequencing modes
* Precision time delayed integration readout
* Programmable fan speed for low / zero vibration
* Two serial port outputs for control of peripheral devices
* General purpose programmable I/O port
* External triggering and strobe controls
* ActiveX drivers included with every system
* Field upgradeable firmware
* Fused silica windows
* Runs from single 12V supply with input voltage monitor
* Compact enclosure
* Programmable status indicators
Apogee Alta U47 Specifications
* Array Size (pixels): 1024 x 1024
* Pixel size: 13 x 13 microns
* Imaging area: 13.3 x 13.3 mm (177.2 mm2)
* Imaging diagonal: 18.83 mm
* Linear Full Well (typ.): 100,000 e-
* Dynamic Range: >83 dB
* PC Interface: USB 2.0
* Max. Cable length: 5 meters between hubs; 5 hubs maximum (max. total of 30m)
* Digital resolution: 12 bits at 2 MHz and 16 bits at 700 kHz
* System Noise (typ.): 2 counts at 2 MHz; 10 e- RMS at 700 kHz
* Pixel Binning: 1x1 to 10x1024 on-chip
* Exposure Time: 20 milliseconds to 183 minutes (2.56 microsecond increments)
* Image Sequencing: 1-65535 image sequences under software control
* Frame Sizes: Full frame, subframe, focus mode
* Cooling: Thermoelectric cooler with forced air. Maximum cooling 55° C below ambient temperature
* Temperature Stability: ±0.1° C
* Dark Current (typ.): <0.1 e-/pixel/sec (-35° C)
* Camera Head: Standard: D2; Low profile: D6. Aluminum, hard blue and black anodized. 6" x 6" x 2.5" (15 x 15 x 6.35 cm).
Weight: 3.1 lb. (1.4 kg)
* Mounting: 3.5" bolt circle, 8-32 thread. 2†24 threads per inch. Optional Nikon or Canon lens mount.
* Back focal distance: Standard: 1.025†(2.60 cm); Low profile: 0.460†(1.17 cm). [optical]
* Operating Environment: Temperature: -22° to 27°C. Relative humidity: 10 to 90% noncondensing
* Cable length: Standard: 15 ft. (4.5m)
* Power: 40W maximum power with shutter open and cooling maximum. Power supplied by AC/DC “brick†supply with
international AC input plug. Alternate 12V input for user’s source.
* Shutter Standard: Melles Griot 43 mm. Low profile: no shutter.
* Remote Triggering: LVTTL input to camera allows exposure start within 25 microseconds of rising edge of trigger.In order to take advantage of the discounted pricing advertised on Woodland Hills Telescope's website, Apogee
requires payment in full at the time of order. This pre-payment is required regardless of whether the camera is readily available
or there is a lead-time, since WHCT is required to pay the full amount due when we place your order.
If you'd like to order this camera without prepaying, that's not a problem, but the price will be a bit higher. To find out what
the price would be, you can call WHCT at 1-888-427-8766 or email our
, and we will provide pricing and lead times, if any.
|