SkyEye62AM Deep Sky Camera

Professional deep sky astrophotography camera featuring Sony IMX455 full-frame monochrome CMOS sensor with 61-megapixel ultra-high resolution, precise temperature control, ultra-low read noise, and zero amp-glow characteristics, delivering exceptional performance for deep sky object imaging.

SkyEye62AM Deep Sky Camera Product Image

Function Description

The SkyEye62AM features a full-frame image sensor, precise temperature control, ultra-low read noise, and zero amp-glow characteristics, making it ideal for deep sky object photography. Its exceptional performance and versatile applications provide users with an extraordinary astrophotography experience.

SkyEye62AM Features:

  • IMX455 Monochrome CMOS Image Sensor
  • Resolution: 61 Megapixels (9568×6380)
  • 3.76μm Square Pixels
  • Full Frame (35.976mm × 23.989mm)
  • 16-bit ADC
  • 512MB DDR3 Cache
  • G Sensitivity: 435.5mV, 1/30s
  • Zero Amp-Glow
  • Ultra-Low Noise: 0.9 to 1.95 e⁻ (Low Noise Mode)
  • Supports Low Noise Mode/High Frame Rate Mode (Up to 6.2 FPS full pixel at 8-bit output)
  • Supports HCG/LCG Mode
  • Maximum SNR: 47.1 dB (Low Noise Mode)
  • Dynamic Range: 88.3 dB (Low Noise Mode)
  • Cooling difference up to 30℃ below ambient temperature for short exposures / up to 35℃ below ambient temperature for long exposures

Core Features

61MP
Ultra-High Pixels
9568×6380 Resolution
51 ke⁻
Full Well Capacity
Up to 111ke⁻ in LCG Mode
0.9 e⁻
Ultra-Low Read Noise
Ultimate Low Noise Mode Performance
> 80%
Peak Quantum Efficiency
Excellent Photoelectric Conversion
88.3 dB
Dynamic Range
Low Noise Mode Performance
-35℃
Cooling Difference
Two-Stage TEC Deep Cooling

Technology Advantages

Full Frame 61-Megapixel Sensor

SkyEye62AM features the Sony IMX455 monochrome sensor with 61-megapixel ultra-high resolution (9568×6380) and a full-frame size of 35.976mm × 23.989mm. The 3.76μm pixel size ensures excellent light gathering capability while maintaining high resolution. The full-frame sensor guarantees an extremely large field of view, making it the ideal choice for capturing large nebulae, galaxies, and wide-field deep sky objects.

Sony IMX455 Spectral Response Curve

The SkyEye62AM sensor has a G sensitivity of 435.5mV at 1/30s. Its quantum efficiency peak exceeds 80% and maintains excellent response throughout the visible and near-infrared ranges. With an AR anti-reflection filter installed, its spectral response range is 380-1100nm. The sensor's high quantum efficiency ensures clear image capture even in low-light conditions, making it particularly suitable for photographing faint deep sky objects.

IMX455 Spectral Sensitivity Characteristics Curve

16-bit ADC and Flexible ROI

SkyEye62AM outputs native 16-bit ADC, providing 65,536 grayscale levels capable of capturing extremely fine brightness variations. This high bit depth is crucial for deep sky photography, enabling simultaneous recording of the bright core and faint outer details of nebulae. The camera supports hardware ROI, with smaller ROI sizes achieving higher frame rates.

Frame Rates at Different Resolutions/Data Bits/Data Transfer Interfaces

Resolution 16-bit Output 8-bit Output
USB3.0 USB2.0 USB3.0 USB2.0
9568×6380 3.1 0.4 6.2 0.7
9568×6380 (Low Noise Mode) 1.9 0.4 6.2 0.7
4784×3190 9.4 1.5 18.8 2.9
3184×2124 27.8 3.3 55 6.6

Unit: Frames per Second (FPS)

512MB DDR3 Cache Technology

SkyEye62AM features 512MB (4Gb) DDR3 cache, helping maintain data transmission stability and effectively reducing amp-glow phenomena, as image data can be buffered without rushing to send data to the receiving end.

DDR3 Cache Module Diagram

Pixel Binning Technology

SkyEye62AM supports digital pixel binning from 1×1 to 8×8 (stacking or averaging methods) and hardware pixel binning from 1×1 to 3×3 (averaging method). Hardware pixel binning is much more efficient than software pixel binning.

HCG/LCG Dual Mode Conversion Gain

SkyEye62AM supports HCG and LCG mode conversion. In LCG mode, its full well capacity can reach 111ke⁻.

Zero Amp-Glow Design

SkyEye62AM is carefully designed to achieve zero amp-glow photography. It's easy to see that images captured by SkyEye62AM exhibit no amp-glow phenomena.

Zero Amp-Glow Comparison Image

Ultra-Low Noise Read Mode

SkyEye62AM's read noise is as low as 0.9 - 1.95 e⁻ (Low Noise Mode). This is impressive, as SkyEye62AM features a low noise mode, which means users can select low noise mode to achieve even lower read noise at the cost of reduced frame rate.

Precision Cooling System

Two-Stage TEC Deep Cooling Technology

SkyEye62AM's cooling system is a two-stage thermoelectric cooling (TEC) system with controllable electric fan-assisted heat dissipation. The TEC system is controlled by PID algorithm, allowing precise adjustment to target temperature with 0.1°C deviation. Operating temperature can be adjusted to specific values, with effective cooling difference reaching up to 35℃ below ambient temperature. This efficient cooling system ensures the stability of ultra-low noise mode and camera image quality.

Two-Stage TEC Cooling System Structure Diagram

TEC Cooling Structure

Adopts two-stage semiconductor cooling chip series design, where the first stage directly cools the sensor and the second stage efficiently conducts heat to the heat dissipation system.

Anti-Dew Heating System Working Principle Diagram

Anti-Dew Heating System

The camera front end is equipped with an intelligent anti-dew heating system that automatically monitors environmental humidity and temperature, activating heating when necessary to prevent optical window condensation.

Technical Specifications

Core Performance Parameters

Maximum Frame Rate (USB 3.0) 16-bit: 3.1 FPS @ 9568×6380
16-bit: 1.9 FPS @ 9568×6380 (Low Noise Mode)
8-bit: 6.2 FPS @ 9568×6380
8-bit: 55 FPS @ 3184×2124
Read Noise Standard Mode: 2.8 - 0.97 e⁻
Low Noise Mode: 1.95 - 0.9 e⁻
LCG Mode: 4.29 - 1.47 e⁻
Full Well Capacity 51ke⁻ (HCG Mode)
111ke⁻ (LCG Mode)
Peak Quantum Efficiency >80%
Dynamic Range 88.3 dB (Low Noise Mode)
Signal-to-Noise Ratio 47.0 dB
Exposure Time Range 0.1ms - 3600s
Gain Range 1× - 150×
Cooling Capability Short Exposure: ΔT = -30℃
Long Exposure (>1s): ΔT = -35℃

Basic Technical Specifications

Sensor Sony IMX455 Monochrome CMOS
Image Resolution 61 Megapixels (9568×6380)
Pixel Size 3.76μm × 3.76μm
Sensor Size Full Frame (43.3mm Diagonal)
Imaging Area 35.976mm × 23.989mm
Shutter Type Rolling Shutter
ADC Bit Depth 16-bit
DDR3 Cache 512MB (4Gb)
Spectral Response Range 380-1100nm (with AR Anti-Reflection Filter)
Front Window Protection Glass AR Anti-Reflection Filter

Interface and Physical Specifications

Data Interface USB 3.0 / USB 2.0
Camera Interface M54 × 0.75 Thread
Back Focus 17.5mm / 12.5mm (Adjustable)
USB Hub USB 2.0 Hub for Accessory Connection
Power Requirements DC 12V 3A
Dimensions Diameter 89mm × Height 107mm
Weight 713g
Cooling Method Two-Stage TEC Cooling
Supported Systems Windows XP/Vista/7/8/10/11 (32&64-bit)
Mac OS X, Linux
SDK Support Native C/C++, C#/VB.NET, Python
Java, DirectShow, Twain, ASCOM, etc.

Multi-Mode Flexible Switching

SkyEye62AM supports HCG (High Conversion Gain) and LCG (Low Conversion Gain) mode conversion. In LCG mode, its full well capacity can reach 111ke⁻.

HCG Mode Performance

Camera Settings: Full Resolution, RAW 16-bit Mode, Temperature: -5℃

HCG (High Conversion Gain) mode is optimized for deep sky astrophotography. In this mode, read noise can be as low as 0.97e⁻, making it ideal for capturing faint nebulae, galaxies, and other deep sky objects. With a full well capacity of 51ke⁻ and dynamic range reaching 14.15 stops, it can simultaneously capture both the bright core and faint outer structures of celestial objects.

HCG Mode Performance Curve: Showing e/ADU, read noise, full well capacity, and dynamic range at different gains

LCG Mode Performance

Camera Settings: Full Resolution, RAW 16-bit Mode, Temperature: -5℃

LCG (Low Conversion Gain) mode provides larger full well capacity (111ke⁻), suitable for capturing high dynamic range celestial objects. Dynamic range can reach 14.7 stops, ensuring complete recording of all details from brightest to darkest.

LCG Mode Performance Curve: Showing performance parameters in low conversion gain mode

Low Noise Read Mode

Optimized for extreme low-light photography

Low noise read mode achieves ultra-low noise levels of 0.9-1.95e⁻. While the frame rate decreases to 1.9 FPS (16-bit), for deep sky photography requiring long exposures, the signal-to-noise ratio improvement from ultra-low read noise makes this sacrifice completely worthwhile.

Camera Interface & Dimensions

Flexible Back Focus Design

The upgraded SkyEye62AM with new housing has the capability to switch back focus lengths. By removing the 5mm back focus ring from the camera's front end, the camera's occupied back focus length changes from 17.5mm to 12.5mm, effectively adapting to non-standard back focus optical systems and more flexible equipment configurations.

Sensor Tilt Adjustment

SkyEye62AM has the capability to adjust sensor tilt. Three sets of screws can be used to adjust the image sensor tilt angle to make it parallel to the telescope's primary mirror surface, with each set containing one screw for pulling back and one for pushing forward.

Package Contents

Package Contents Overview

Standard Configuration Includes:

A Cardboard Packaging Box: L:21.9cm W:21.9cm H:13.6cm
B SkyEye Series Camera (M54F×0.75 Interface)
C Power Adapter: AC 100-240V 50Hz/60Hz, Output DC 12V 3A
D High-Speed USB 3.0 A-Male to B-Male Gold-Plated Connection Cable (1.5m)
E Rubber Plug
F Hex Wrench H 2.0
G M54M-M48F 21mm Extension Tube
H M48M-M48F 16.5mm Extension Tube
I M48M-M42F Adapter Ring

Note: Actual package contents are subject to the physical product. ToupTek reserves the right to make detail adjustments without affecting product performance.

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