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SBIG STL-11000M Monochrome CCD Camera - Class 2
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Information on the SBIG STL-11000M Class 2 Monochrome CCD Camera

Introducing a Class 2 Version of the STL-11000M!

Since its introduction, the SBIG STL11000M, 35mm format, 11 Megapixel CCD Camera has been used in the hands of some of the best astrophotographers in the world to produce some of the most stunning astrophotos ever produced by amateur astronomers. When the KAI-11000M CCD was first introduced by Kodak the monochrome version was only available in a Class 1. More recently, the monochrome CCD was made available by Kodak in a Class 2 with significantly improved cosmetic specifications compared to the color version. The monochrome Class 2 CCD allows no more than 2 column defects (out of 4008). It should be noted that a column defect does not mean that an entire column is defective. It means that there are greater than a threshold number of bright or dark pixels within a certain range along one column. In many cases these cannot be seen. Even when they are visible in the image, most current software packages designed for CCD image acquisition and processing, such as CCDOPS and CCDSoftV5, have column repair functions that will easily fix any visible effects of a bright or dark column in an image.

After testing several Class 2 monochrome CCDs, and being pleased with the results, SBIG decided to make a special buy of this sensor in order to offer this 35mm format multi-megapixel camera for the lowest price possible. OPT and SBIG are proud to make this SBIG STL11000M monochrome camera available at this price, including the standard built-in 657 x 495 pixel self-guiding CCD and the standard built-in 5 position filter wheel. With the exception of the CCD, this new SBIG STL-11000M CCD camera is identical to all other model STL cameras and is compatible with all STL accessories such as the new 8-position filter wheel and AO-L Adaptive Optics.

About the new Research Line of SBIG CCD cameras...

The Research Line of cameras is an all new camera design that has been over two years in the making. SBIG's design team has combined the best features and ideas from past designs and updated their current high speed electronics and USB interface to handle these large format CCDs (up to 35mm format with 11 megapixels).

New features include a dual head self-guiding option, simplified power requirements and an internal 2" filter wheel for overall system cost and weight reduction. These large format cameras are designed to offer more features at a lower price than other previously available cameras. SBIG's goal was to produce a high performance imaging system that included large area detectors, flexible self-guiding options and a large format filter wheel all at a lower price than competing cameras alone. We believe they have achieved that goal.

DUAL HEAD, TRIPLE SENSOR, SELF-GUIDING

The best of both worlds. SBIG has expanded the self-guiding capabilities in the Research cameras by adding the option of a remote guiding head.

Prototype remote guiding head for the large format cameras with t-thread front plate and screw in nose piece. Remote head contains TC-237 CCD, TE cooling and shutter. Head accepts 1.25" and 2" nosepieces, t-thread attachments and camera lens adapters

With the remote guiding head attached, there are two, software selectable, TC-237 CCDs available for self-guiding under any conditions in addition to the main imaging CCD.

KAF-1001E CCD and internal TC-237 tracking CCD mounted in the sealed CCD chamber of prototype camera body

One guiding CCD is located next to the imaging CCD in SBIG's patented design, similar to the self-guiding arrangement in their ST line of cameras. The remote guiding CCD is in a small separate head that attaches to the main camera body by a short cable. There is no separate power supply or communication cable required. The remote head contains its own TE cooler and shutter. With the optional remote guiding head attached to the main camera body, self-guiding is accomplished by selecting either the internal TC-237 tracking CCD or the remote TC237 CCD using the camera control software. The benefits of this flexibility are obvious. Internal guiding eliminates the need for a guide scope and separate autoguider. It also eliminates the problem of differential deflection of the guide scope or differential motion of the primary mirror relative to the guide scope. However, some users prefer to use an external guider when imaging through dark infrared band or narrow band filters, or for RGB color imaging in regions of the sky with sparse guide stars. The remote guiding head may be used in an off-axis guiding accessory or attached to a separate guide scope. There is only one small cable between the remote head and the main camera body. The remote head can be left connected and the user may freely switch between the internal or the remote TC-237 for self-guiding. All the guiding functions are controlled by the same camera software that normally controls the internal guider. Below are pictures of a prototype camera and remote head attached to 5" refractor and 8" SCT.

Large format camera attached to 5" AP refractor on Losmandy G11 mount

Large format camera attached to 8" SCT on Losmandy G11 mount. Remote guiding head with eFinder lens assembly is mounted on piggyback bracket

INTERNAL 2" FILTER CAROUSEL

An internal 5 position 2" filter carousel is integrated into the front cover of the camera body.

Five position 2" filter carousel mounted in the front cover of the large format camera body. Filter carousel accepts both 48mm threaded cells and 2" round flats

For color, UBVRI, or narrow band imaging simply add filters to the camera's carousel. There is no expensive separate 2" filter wheel to purchase. The filter carousel accepts both 50mm diameter flats and 48mm threaded filter cells. The front cover of the camera is easily removed for changing filters. Since the CCD is in a separate sealed chamber, removal of the front cover to change filters does not expose the CCD to dust or air and the desiccant does not need to be recharged after replacing the cover. Extra carousels may be purchased for quick and easy transition between filter sets. A shutter mechanism is also located inside the camera body, between the filter wheel and the sealed CCD chamber.

12VDC OPERATION

SBIG has added an internal 12VDC regulated power supply to the camera for simplified power requirements and greater tolerance of input voltage variation.

Inside the back cover - regulated 12VDC power supply, shutter motor and heat sink

When operating in the field from a 12V battery, current drain, power cord extensions and cold temperatures may cause the input voltage to drop below 12 volts. The internal regulated supply will accommodate some variation in input voltage (from about 10 volts to 18 volts) and keep the camera operating normally. This will allow for longer power cords to be used with less concern for voltage drops so long as the input voltage stays within a certain range. A set of indicator LEDs will let you know if your input voltage at the camera is getting too low for normal operation. A universal 110VAC-220VAC to 12VDC power supply is also included for operation from virtually any line voltage in the world.

INTELLIGENT

A set of five LED indicator lights on the side panel of the camera provide critical camera status information.

Rear and side view of prototype body showing connectors on bottom and five status lights on side panel

The green LED lets you know the camera is booting up and gives camera exposure status during normal operation. One red LED provides a warning if the heat sink gets too hot. This could happen, for instance, if you were running high power to the cooler and the fan failed for some reason. In this case the camera automatically reduces power to the two-stage cooler to prevent damage. One amber LED warns of an input voltage drop to 11 volts or less but the camera will continue functioning normally. The second amber LED warns of an input voltage drop to 10 volts but the camera will still continue functioning normally. The last red LED warns of an input voltage drop to 9 volts or less. In this case, the camera automatically turns off the TE cooler and continues to operate normally without cooling until the voltage drops to the point that the camera shuts down (around < 7 volts).

TWO-STAGE COOLING WITH WATER ASSIST

Behind the two-stage cooler is a large heat sink, channeled for water circulation. The heat sink design was modeled for maximum efficiency with the selected TE cooler.

The standard cooling design utilizes a very efficient two-stage TE cooler for maximum performance with large format detectors. Each camera is also liquid assist ready so that additional cooling in warm climates may be achieved by circulating water if needed. SBIG is currently testing a special magnetic levitating fan to eliminate even the smallest vibration. Preliminary tests indicate that cooling -50 Degrees C below ambient will be achieved with this system.

DELUXE ACCOMMODATIONS

Every Research Model camera will be shipped in a custom fitted Pelican brand carrying case for superior protection of your equipment.

An optional lid pocket is available from Pelican that will hold charts and manuals.

These cases are waterproof, dustproof, crushproof and have a lifetime guarantee from the manufacturer. Each Pelican case has an automatic pressure relief valve and double hinged latches for easier opening. There is ample room inside for the camera, cables, wall transformer and some accessories in the custom cut foam insert.



Please Note: SBIG drivers are compatible with 32 bit Vista, but they are not compatible with 64 bit Vista.

Save $390 on a Baader 50.8mm LRGB and 7nm H-Alpha Filter Set when you buy any new SBIG STL-series camera at the same time! See more info and instructions in the Sales tab to your left.