QHY CCD QHY410C

ΔΙΑΘΕΣΙΜΟ ΣΕ 10 ΗΜΕΡΕΣ ΜΕ ΠΑΡΑΓΓΕΛΙΑ

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Περιγραφή

QHY410C uses Sony’s latest back-illuminated, full
frame color sensor. The IMX410 is equipped with the sensor that used in
the Nikon Z6, and Sony A7III. In addition to BSI, the IMX410 also has
larger 5.94 um pixels giving it increases sensitivity of extended
objects in low light. The IMX410 is expected to be Sony’s most sensitive
full frame color sensor for astrophotography.

QHY410C has 1GB DDRIII buffer to cache the image and avoid the risk
of a frame loss. This avoids problems of a busy USB port when there are
other peripherals using the same port as the camera.

BSI

One benefit of the back-illuminated CMOS
structure is improved full well capacity. In a typical front-illuminated
sensor, photons from the target entering the photosensitive layer of
the sensor must first pass through the metal wiring that is embedded
just above the photosensitive layer. The wiring structure reflects some
of the photons and reduces the efficiency of the sensor.

In the back- illuminated sensor the light
is allowed to enter the photosensitive surface from the reverse side. In
this case the sensor’s embedded wiring structure is below the
photosensitive layer. As a result, more incoming photons strike the
photosensitive layer and more electrons are generated and captured in
the pixel well. This ratio of photon to electron production is called
quantum efficiency. The higher the quantum efficiency the more efficient
the sensor is at converting photons to electrons and hence the more
sensitive the sensor is to capturing an image of something dim.

TRUE RAW Data

In the DSLR implementation there is a RAW
image output, but typically it is not completely RAW. Some evidence of
noise reduction and hot pixel removal is still visible on close
inspection. This can have a negative effect on the image for astronomy
such as the “star eater” effect. However, QHY Cameras offer TRUE RAW
IMAGE OUTPUT and produces an image comprised of the original signal
only, thereby maintaining the maximum flexibility for post-acquisition
astronomical image processing programs and other scientific imaging
applications.

Anti-Dew Technology

Based on almost 20-year cooled camera
design experience, The QHY cooled camera has implemented the fully dew
control solutions. The optic window has built-in dew heater and the
chamber is protected from internal humidity condensation. An electric
heating board for the chamber window can prevent the formation of dew
and the sensor itself is kept dry with our silicon gel tube socket
design for control of humidity within the sensor chamber.

Cooling

In addition to dual stage TE cooling, QHYCCD implements proprietary technology in hardware to control the dark current noise.

Χαρακτηριστικά

Model QHY410C
Sensor SONY IMX410
Mono/Color Color
Sensor illumination type BSI
Pixel Size 5.94um*5.94um
Effective Pixel Area 6072* 4044
Effective Pixels 24.5 MP
Sensor Size Full Frame

36mm* 24mm

Full well capacity 120ke-
AD Sample Depth 14bit (Output as 16bit and 8bit)
Full Frame Rate 14 FPS @8BIT

7 FPS @16BIT

Readout Noise 3.75e- @low gain

1.1e- @high gain

Dark Current 0.01e /pix/s @0C

0.002e /pix/s @-20C

Exposure Time Range 100us-3600sec
Unity Gain 90(low gain)

40 (high gain)

Amp Glow Zero Amp
Shutter Type Electric Rolling Shutter
Computer Interface USB3.0
Built-in Image Buffer 1 GB
Cooling System Dual Stage TEC cooler(about -35C below ambient)
Optic Window Type AR+AR High Quality Multi-Layer Anti-Reflection Coating (For color camera user need to add a UV/IR filter in the light path)
Anti-Dew Heater Yes
Telescope Interface M54/0.75
Back Focal Length 17.5mm
Weight 785g
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