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TS-Optics MONO AstroKamera 571MP Sony IMX571 sensor D-28.3mm

Cooled MONO APS-C USB 3.0 astronomical camera with a powerful Sony CMOS sensor for astrophotography

♦ Powerful two-stage Peltier cooling up to 40°C below ambient temperature

♦ Sony IMX571 APS-C format b/w with back-illuminated sensor

♦ High resolution with 3.76 µm pixels

♦ 16-bit ADC: dynamic range like a CCD sensor

♦ No more amp glow due to Zero-Ampglow circuitry

♦ Telescope side connection: female thread M42x0.75

♦ Working distance of only 17.5 mm from the internal thread T2 (M42x0.75)

♦ Built-in AR protection filter with IR pass

♦ DDR3 Buffer 512MB for more stable data transfer

♦ Grouping is supported

♦ Unlike the third picture, no extra desiccant or CD is included.

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Entrega entre 8 y 10 días laborables
Entrega entre 8 y 10 días laborables

Latest generation MONO TS 2600MP astronomical camera

The camera with the powerful Sony IMX571 sensor enables astrophotography at a very high level. This cooled CMOS sensor no longer has amplifier flare and can be used for all areas of astrophotography. Due to the high resolution of the sensor, fine details show up even at shorter focal lengths.

Another advantage is the sensational sensitivity to light. The QE of 91% thanks to the BACK ILLUMINATION technology already allows deep astrophotography with short exposure times. This makes the camera very suitable for deep sky photography.

Back lighting technology:

Sony's back-illuminated CMOS image sensor improves sensitivity and noise reduction, key factors in improving image quality, by changing the basic pixel structure from front to back exposure. The advantages of CMOS image sensors, such as low power consumption and high operating speed, have been retained.

Postexposure improves light capture while increasing the amount of light. This makes significantly shorter exposure times possible and leads to an improved quantum efficiency of 80%.

Sony has developed a unique photodiode structure and on-chip lens optimized for back-illuminated structures, resulting in higher sensitivity and lower non-light random noise by reducing noise, dark current, and defective pixels compared to traditional structure with front lighting.

No amp glow:

Conventional CMOS sensors produce a faint source of infrared light during operation, which can often be seen in the corners of uncalibrated images as a telltale sign of "amplifier brightness." Because this camera's sensor uses zero brightness circuitry, you don't have to worry about "amperage brightness" even when using high-gain, long-exposure images.

Optimum support before and after the purchase by Teleskop-Service

Thanks to many years of experience, we can offer you the best possible advice and also an excellent after-sales service. We can perform almost all services in-house. For a professional service, we also have a clean room, where we can carry out repairs, cleaning, etc. excluding dust.

Connection to correctors with M48 thread and 55 mm working distance with filter change

Most refractor field flatteners or coma correctors have a 55mm working distance and an M48x0.75 thread on the camera side. Here is an interesting suggestion for the connection. The camera has a 17.5mm back focus from the internal T2 thread. The adapters are from the camera to the corrector:

1. TSFSLM48T2 - Filter box with T2 connector on the camera side and M48 thread on the telescope side.

2. TSVF220 - 20mm M48 Extension

A total of 55.5mm back focus - 0.5mm well compensates for the filter glass path - precision landing!

Sensor: CMOS Mono Sensor IMX571
Size: 23.5 x 15.7 mm - diagonal 28.3 mm
Pixel size: 3.8 µm
Number of pixels: 6224 x 4168 - 26 MP
Bit depth: 16
Frames per second: 7 frames at full resolution
Cooling: Peltier cooling up to 40 °C below ambient temperature
Power supply: 12 V 3 A
Interfaces: USB 3.0 and USB 2.0
Supported operating systems: Windows from Win7
Dimension: Diameter 80 mm - Lenght 100 mm
Connection telescope side: T2 internal thread (M42x0,75)
Back focus: 17.5 mm (distance sensor to internal thread)

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