Like other self-guiding cameras in the ST series, the ST-10XME contains two CCDs. In this case, the imaging CCD is an enhanced KAF-3200ME imaging detector from Kodak with 3.2 million pixels. The guiding CCD is the TC-237H with 657 x 495 pixels.
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The Model ST-10XME is the flagship of the "ST" series of self-guiding CCD cameras from SBIG. The body is identical to the ST-7XME, ST-8XME, ST-9XME and ST-2000XM models with some slight modifications to accommodate the larger detector.
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The ST-3200ME is essentially the same camera as the ST-402ME except that the imaging CCD is over 4X larger and it has more than 8X the number of pixels. The ST-3200ME uses the KAF-3200ME CCD, the same sensor we use in the ST-10XME. This CCD is 2184 x 1472 pixels at 6.8 microns.
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SBIG's Research Series STL-4020CM CCD Camera ABG with Class 2 color CCD makes filter wheels unnecessary for most applications. The STL-4020M has 4 million total pixels in a 2k x 2k array, 15 x 15mm dimensions, a 7.4 u pixel size and an interline detector.
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SBIG's Research Series STL-4020M CCD Camera ABG. SBIG's new research class Cameras. The STL-4020M has 4 million total pixels, in a 2k x 2k array, has a 15 x 15mm Dimensions, 7.4 u Pixel Size, and a Interline detector.
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No compromises. The new mid-sized STT Series cameras offer features and specifications found in no other astro-camera - of any size.
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To meet the demands of the next generation astroimaging, SBIG introduces the next generation STXL Camera System with self-guiding integrated into a Micron-Precision Filter Wheel.
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SBIG's Research 1001E Class 2 CCD Camera NABG. SBIG's new research class Cameras. The 1001E has 1 million total pixels, in a 1k x 1k array, has a 24.5 x 24.5mm Dimensions, 24u Pixel Size, and a Full Frame detector.
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To meet the demands of the next generation astroimaging, SBIG introduces the next generation STXL Camera System with self-guiding integrated into a Micron-Precision Filter Wheel.
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With four times the field of view and four times the number of pixels, the 6.3 megapixel Research 6303XE is essentially like having four ST-8XE cameras imaging at once. The 9 micron pixels are small enough that the large field of view can be exploited with relatively modest telescopes of less than 100 inches focal length.
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The advantage of easier guiding through a separate guide scopes is often limited by differential deflection of the guide scope relative to the main optical axis due to mechanical flexure or shifting of the mirror in the main OTA. This difficulty is addressed with two new guiding techniques developed by SBIG and implemented in the STX series cameras.
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Major price reduction! WAS $11875 NOW $9995
The advantage of easier guiding through a separate guide scopes is often limited by differential deflection of the guide scope relative to the main optical axis due to mechanical flexure or shifting of the mirror in the main OTA. This difficulty is addressed with two new guiding techniques developed by SBIG and implemented in the STX series cameras.
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