SBIG Seeing Monitor, 765x510 Pixel Array, 6.9x4.3mm (0.27x0.16") CCD, 150mm Focal Length

SKU: SBSEEINGM

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SBIG Seeing Monitor, 765 x 510 Pixel Array Specifications

  • CCD

    Kodak KAF-0402ME

  • Pixel Array

    765 x 510 pixels

  • CCD Size

    6.9 x 4.3 mm

  • Total Pixels

    390000

  • Pixel Size

    9 x 9 microns

  • Full Well Capacity

    Approx. 100,000 e-

  • Dark Current

    Approx. 1e½/pixel/sec at 0deg. C

  • Dark Current Doubling Temp

    Approx. 6 deg. C

  • Exposure

    0.04 to 3600 seconds,10ms resolution

  • Correlated Double Sampling

    Yes

  • A/D Converter

    16 bits

  • A/D Gain

    1.5e- unbinned
    2.0e- binned 2x2, 3x3

  • Read Noise

    13.8e RMS Typical

  • Binning Modes

    1 x 1, 2 x 2, 3 x 3

  • Pixel Digitization Rate

    Up to 800.000 pixels per second with USB 2.0

  • Full Frame Download

    <1 second

  • Lens Focal Length

    150mm

  • Lens Focal Ratio

    f/5.6

  • Field of View

    2.6 x 1.7 degrees

  • Cooling

    Ambient

  • Power

    12VDC, 1A without cooling on, 3A with cooling enabled (power supply included)

  • Computer Interface

    USB 2.0
    (USB 1.1 compatible)

  • Computer Compatibility

    Windows 32 bit and 64 bit

  • Dimensions

    Enclosure: 6 x 8 x 10" (15.24 x 20.32 x 25.4cm)

  • Weight

    17lbs (7.7kg)

About SBIG Seeing Monitor, 765 x 510 Pixel Array

The SBIG Seeing Monitor determines the quality of seeing each night. This can be useful in helping to decide whether to take certain kinds of images, or whether to image at all. If you happen to be at the observatory you can sometimes just look through an eyepiece and see whether the night "looks" good or not. But customers are mimicking professional observatory installations with remote observing sites and fully automated observing systems. Remote can mean anything from a few meters to a few thousand kilometers. No matter where one observes, it is often a time consuming matter to get ready for a nights imaging session. It would be convenient to know before hand what kind of results one could expect. Even if the expectation is that the night's seeing would be no better than several arc seconds, the type of imaging one decided to set up for could be changed to make the best use of the conditions available for that evening.

The Seeing Monitor lens is a 150 mm f/5.3 lens mounted to the ST-402, all contained inside a weatherproof box. The box also contains a USB extender and a 12 VDC power supply for the camera. The window in the top of the box is clear. The window is heated to prevent condensation on the outside. The USB extender allows operation up to 150 feet (50 meters) from the controlling PC. The lens and box is permanently pointed at Polaris by the user. It is assumed the user will mount posts in the ground outside his observatory or home for this purpose. Roof mounting is not recommended because small vibrations from the building may affect the monitor's measurements.

SBIG Seeing Monitor, 765 x 510 Pixel Array Features

  • The SBIG Seeing Monitor gives the serious astrophotographer the ultimate edge by recording every detail of the sky's conditions
  • Know exactly what your surrounding sky conditions are before you spend hours imaging
  • The SBIG SMC is hyper sensitive and readings are done quickly - every 5 milliseconds - so you can be sure of highly accurate results
  • Included software auto-calculates results into an easily readable format
  • Allows for up to 150 foot long USB connections to operating computer

Key Features

  • Know exactly what your surrounding sky conditions are before you spend hours imaging
  • Included software auto-calculates results into an easily readable format
  • Allows for up to 150 foot long USB connections to operating computer

What's in the box:

  • SBIG Seeing Monitor
  • Power Supply
  • SBIG Warranty