ATR533M (IMX533)

Professional 1" Square Cooled Camera for Mono Deep-Sky Astrophotography

定価 $959.00
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ATR533M is a high-performance monochrome astronomy camera designed for detailed deep-sky imaging. Featuring the Sony IMX533 monochrome 1" square sensor, 9MP resolution, peak QE above 90%, ultra-low read noise, zero amp-glow design, and advanced TEC cooling, it captures fine details and faint structures in galaxies, nebulae, and star clusters.

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Compatibility / Requirements

ATR Series cooled cameras require a stable 12V 3A DC power supply. Use the supplied adapter or a lithium-ion battery with a stable 11–14V output.

Delivery and Shipping

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Warranty and Support

For setup support, software downloads and warranty service, contact ToupTek Astro support with your order information.

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Full Specifications

  • Sensor: Sony IMX533 Mono
  • Resolution: 3008 x 3008 (9MP)
  • Pixel Size: 3.76 μm
  • Full Well: 52ke- (104.6ke- @ HFW Mode)
  • ADC: 14bit
  • TEC Cooling: Two-stage TEC, -35/-45°C below ambient

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Meet ATR533M: Advanced Square-Sensor Cooled Mono Camera for Flexible Deep-Sky Imaging

Explore the beauty of the deep sky with the ToupTek ATR533M. Featuring Sony’s back-illuminated IMX533 monochrome sensor, 9MP resolution, and a square 1-inch format, this cooled astronomy camera combines high sensitivity with ultra-low read noise. Its zero amp-glow design, 14-bit ADC, and two-stage TEC cooling support clean, detailed long-exposure imaging. Pair it with LRGB or narrowband filters to capture galaxies, nebulae, and star clusters with greater control over every channel.

ATR533M cooled astronomy camera

IMX533M Sensor

IMX533 sensor illustration for ATR533M

Square 1-Inch Sensor for Balanced Framing

The Sony IMX533 monochrome sensor features a 3008 × 3008 resolution and a square imaging area. Its format offers a balanced field of view for a variety of deep-sky targets, from compact nebulae to galaxies and star clusters.

3.76 μm Pixels for Detailed Imaging

With 3.76 μm square pixels and a back-illuminated design, the IMX533 combines fine sampling with strong light sensitivity, making it well suited to capturing subtle structures in deep-sky objects.

Peak QE >90% for Greater Light Sensitivity

IMX533M sensor offers peak quantum efficiency above 90%, capturing a high proportion of incoming photons. Combined with its monochrome design, it is well suited to LRGB and narrowband imaging, helping reveal faint details in nebulae and galaxies.

Is ATR533M Right for Your Astronomy Imaging Setup?

Deep-Sky Beginners Ready to Explore Mono Imaging

If you are moving beyond a DSLR or one-shot color camera, the ATR533M offers a cooled monochrome platform for exploring LRGB and narrowband astrophotography. Pair it with a suitable telescope, filter wheel, and filters to build a versatile imaging setup.

Dedicated Deep-Sky Imagers Seeking Cleaner Data

For astrophotographers focused on faint nebulae, distant galaxies, and extended imaging sessions, the ATR533M combines ultra-low read noise, zero amp-glow design, and temperature-controlled cooling to support detailed long-exposure capture.

Astrophotographers Who Want Flexible Imaging Options

The ATR533M is primarily designed for deep-sky imaging, but it can also be used for planetary photography. Its square sensor, adjustable gain, and support for high-frame-rate and low-noise modes offer flexibility across different targets and capture workflows.

The Ghostly Cheerio Nebula by © Bruno Rota Sargi

Why Choose the ATR533M

ATR series DDR3 memory buffer

512MB DDR3 High-Speed Buffer

High-bandwidth data transmission is secured by an onboard DDR3 buffer, preventing frame dropping, minimizing USB bus traffic bottlenecks, and ensuring ultra-stable image delivery even during fast frame rates or live rendering.

ATR series zero amp-glow technology

Zero Amp-Glow Technology

The ATR series features a specialized zero amp-glow circuit design that maintains a clean, perfectly uniform sensor background across multi-minute long exposures, protecting the faintest details of delicate nebulae.

ATR series anti-condensation heating system

Anti-Condensation Heating

The ATR series optical window features an integrated smart heating system that actively measures ambient temperature and humidity. It automatically applies precise heat to prevent condensation, keeping your optical path crystal clear without introducing disruptive thermal air currents.

ATR series two-stage TEC cooling system

Two-Stage TEC Cooling

Equipped with an integrated heat dissipation structure and a high-efficiency dual-stage Thermoelectric Cooling (TEC) module with a controllable fan. It lowers the sensor temperature to 42°C below ambient, consistently maintaining a stable -5°C to -10°C even in peak summer. This allows for clean, long-exposure tracking up to 1 hour without thermal noise accumulation.

ATR533M Performance Analysis

ATR vs. SkyEye Plus

Which Series Do You Need

OSC or Mono

Choose the acquisition workflow that matches your imaging goals

What's in the Box

ATR series camera and included accessories

Back Focus Connection

Frequently Asked Questions

Can I power my guide camera through the camera's built-in USB Hub?

Yes. The ATR series cameras connect with accessories through USB data connection and stable external power, allowing users to build a complete deep-sky imaging workflow with a telescope, mount, guide camera, computer or controller, and power supply.

Does the camera include a 12V power adapter, and is it mandatory for imaging?

Yes. All ToupTek Astro DSO cooled cameras require a regulated 12V 3A DC power supply for imaging. Please use the included factory power adapter or a high-quality lithium-ion battery with a stable 11V–14V output.

Will this camera work with my existing control software?

Yes. The ATR series features robust, industry-standard ASCOM and INDI drivers. It integrates seamlessly with all major open-source and commercial astronomy suites.

How do I achieve the standard 55mm backfocus with my telescope?

Achieving the industry-standard 55mm backfocus is precise and seamless. The optical train is configured via a modular three-stage connection sequence: a 17.5mm front adapter or tilter, a 20mm filter drawer or extension tube, and a 17.5mm Off-Axis Guider (OAG). This combination yields a perfect 55mm stack distance that connects natively to M48, M54, and M68 telescope interfaces, with simple adapter options available for M42 threads and 2-inch ports.

How does the Anti-Dew Technology work?

The ATR series utilizes a multi-layer defense system. The sensor chamber is industrially sealed with dry air to prevent internal frost. Simultaneously, a built-in electronic heating strip warms the protective window to prevent external dew under humid summer nights.