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Astronomy
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Astrophotography
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Astronomical Cameras
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Active cooling
Active cooling
For long exposure times, many CCD cameras are cooled to reduce thermal noise and achieve higher image quality. CCD cameras are grouped into three categories:
- no cooling
- passive cooling via cooling fins
- active cooling (e.g. using a fan and Peltier element)
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yes
(1)
Connection (to the telescope)
Connection (to the telescope)
Specifies the product's connection or connection thread on the telescope connection end. The same adapter dimension must always be available on the telescope.
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T2 (M42 x 0,75)
(1)
Megapixel
Megapixel
Specifies the total number of pixels. With this handy value you can compare the resolutions of different cameras.
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> 10
(1)
Bit depth
Bit depth
The bit depth is also referred to as the dynamic range of a chip. The number of bits in a picture also determines how many different shades of grey can be displayed. The depth of the image information depends directly on it. In an image taken with 1 bit depth, you will only see black and white dots. In this case, you can hardly call it a picture. Many details that the naked eye can discern are missing. 16 bits means the presentation of more than 65.000 shades of grey.
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12
(1)
Colour camera
Colour camera
Colour cameras produce quick results, monochrome cameras capture more detail.
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yes
(1)
Pixel size
Pixel size
Specifies the edge length of the mostly square pixels that make up a camera sensor.
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< 4
(1)
Area of application
Areas of application
Information about areas of application serves as a rough orientation.
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Moon & Planets
(1)
Nebulae & galaxies
(1)
Filter wheel
Filter wheel
This refers to whether a filter wheel is integrated in the camera housing, or is included in the scope of delivery as an external filter wheel.
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no
(1)
Price
> 1,040 $
(1)
Availability
in stock
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Categories:
Astronomy
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Telescope accessories
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Astrophotography
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Cameras
Manufacturers:
Meade
Active cooling:
yes
Product series:
DSI-IV
(1)
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Meade
Camera Deep Sky Imager DSI IV Color
$ 1,450.00
ready for shipping in
24 h
