G3M678M User Manual

Version 1.0

September 2023

Product Overview

The G3M678M camera offers high infrared band light-capturing capability with a very high QE value at 850nm. It also features high full-well capacity, high dynamic range, and low read noise, making it suitable for planetary, solar, and lunar photography.

Key features of the G3M678M include:

Specifications and Performance

Camera Specifications

Parameter Value
Sensor Sony IMX678 Monochrome Back-illuminated Sensor
Diagonal Length 8.47 mm
Image Resolution 8.3 Megapixels (3840*2160)
Pixel Size 2.0 µm x 2.0 µm
Image Area 7.7 mm x 4.3 mm
Max Frame Rate (USB 3.0) 12-bit: 24 fps @ 3840*2160, 70 fps @ 1920*1080
8-bit: 47 fps @ 3840*2160, 70 fps @ 1920*1080
Max Frame Rate (USB 2.0) 12-bit: 1.9 fps @ 3840*2160, 3.9 fps @ 1920*1080
8-bit: 3.8 fps @ 3840*2160, 7.9 fps @ 1920*1080
Shutter Type Rolling Shutter
Exposure Time 0.1 ms – 1000 s
Gain 1x – 100x
Signal-to-Noise Ratio 41 dB
Dynamic Range 74 dB
Read Noise 0.5 – 2.55 e-
QE Peak >83%
Full Well Capacity 11.6ke-
ADC 12-bit
DDR3 Memory 512 MB (4Gb)
Data Transfer Port USB3.0/USB2.0
Camera Interface 1.25-inch adapter for 1.25-inch telescopes, C-mount adapter for industrial C-mount lenses
Protection Window IR-Cut filter / Anti-reflection coating
Spectral Response Range 380-1100 nm (with AR coating)
Camera Control SDK Windows/Linux/macOS/Android SDK (Native C/C++, C#/VB.NET, Python, Java, DirectShow, Twain)
Shooting Mode Still capture and video mode
Camera Size Diameter 37 mm * Height 72.4 mm
Camera Weight 70 g
Back Focus 17.5 mm with C-mount, 12.5 mm with CS-mount
Cooling Passive cooling
Supported OS Microsoft Windows XP/Vista/7/8/10 (32 & 64-bit), macOS, Linux

Sony IMX678 Spectral Response Curve

The G3M678M has a G sensitivity of 5644mv at 1/30s. The spectral sensitivity is shown in Figure 1. Sensitivity is measured using a standard test lens CM500S (t=1.0mm) as an IR-CUT filter and an F8.0 aperture. If the image is measured at F5.6, the result may be twice the current value.

Figure 1: IMX678 Spectral Sensitivity Characteristics

12-bit ADC and ROI

The G3M678M is a native 12-bit ADC. It also features a 12-bit output mode with 2x2 binning for lower resolution. The camera also supports hardware ROI, where smaller ROI sizes result in higher frame rates.

Table 2 shows the frame rates for the G3M678M in 12/8-bit modes at different resolutions and USB3.0/USB2.0 data transfer interfaces.

Resolution 12-bit ADC 8-bit ADC
USB3.0 USB2.0 USB 3.0 Interface USB 2.0 Interface
3840 * 2160 24 1.9 47 3.8
1920*1080 70 3.9 70 7.9

DDR3 Memory

The G3M678M camera has 512MB (4Gb) of DDR3 memory, which helps maintain data transfer stability and effectively reduces glow caused by temporary image data buffering, eliminating the need to rush data to the receiving end.

Pixel Binning

The G3M678M supports digital pixel binning from 1x1 to 8x8 (summation or averaging method) and hardware pixel binning from 1x1 to 2x2 (averaging method). Hardware pixel binning offers higher frame rates than software pixel binning.

Gain Switching

The G3M678M supports HCG and LCG switching.

Power System

The camera is powered via the USB 3.0 interface. Once connected to the host system via the USB 3.0 data cable, the camera is ready to operate.

Camera Performance Analysis

Camera performance can be evaluated using e-/ADU, read noise, full well capacity, and dynamic range.

e-/ADU: Sensors in cameras for visual applications convert incident photons into electrons. The gain on CCD/CMOS cameras is the conversion factor from electrons (e-) to digital signal or analog-to-digital units (ADU). Gain indicates the number of electrons required for conversion to a digital signal, or the number of electrons per ADU (e-/ADU).

Read Noise: Read noise is the most important reference for measuring camera performance. Lower read noise generally means better signal-to-noise ratio and better image quality. Read noise is generated within the camera's electronics during readout, as electrons pass through analog-to-digital conversion, amplification, and processing steps to produce an image.

Full Well Capacity: Electrons are retained in each pixel and converted into charge, which can be measured to display the amount of light falling on each pixel. The maximum possible charge is called the "full well capacity." Under the same conditions of noise and A/D converter quality, the larger the sensor's full well capacity, the higher the sensor's dynamic range. Due to limitations in pixel depth, the full well capacity is generally proportional to the front area of the pixel's light-gathering element.

Dynamic Range: This is the ratio of the maximum output signal level to the background noise (background noise, i.e., the RMS noise level in a black image) when the signal is amplified at its minimum. The camera's background noise includes sensor read noise, camera processing noise, and dark current shot noise. Dynamic range represents the camera's ability to display/reproduce the brightest and darkest parts of a scene, and the variation between them. Technically, this is the dynamic range of the scene. In a single image, there may be a completely black area and a completely saturated area.

For the G3M series cameras, the gain value is in the xxx% mode. Here, xxx is used to describe the x-axis (gain value) of the camera's performance:

Gain (dB) = 20 * log10 (Gain Value / 100)

Read Noise (e-) = 100 * 10^(Gain Value / 20)

Read noise is the most important reference for measuring camera performance. Lower read noise generally means better SNR and better image quality.

Camera settings for performance analysis are as follows:

Figure 2 shows the curves for the camera analysis data in Table 3.

Figure 2: G3M678M e/ADU, Read Noise, Full Well, and Dynamic Range

Camera Analysis Data

Camera analysis data is shown in Table 3:

Gain Value 100 177 316 562 1000 1778 3162 5623 10000 15000
Logarithmic Gain (dB) 0.00 4.82 9.95 14.78 19.87 24.96 29.81 34.87 39.96 43.53
e-/ADU 2.85 1.62 0.89 0.51 0.28 0.16 0.09 0.05 0.03 0.02
Read Noise (e-) 2.55 1.39 1.38 1.17 1.07 0.92 0.77 0.86 0.85 0.9
Full Well Capacity (ke-) 11.7 6.7 3.7 2.1 1.2 0.6 0.4 0.2 0.1 0.07
Dynamic Range (stop) 12 12 11.37 10.8 10.08 9.45 8.91 7.91 7.1 6.45

The camera settings for performance analysis are as follows:

Figure 3 shows the curves for the camera analysis data in Table 3.

Figure 3: G3M678M e/ADU, Read Noise, Full Well, and Dynamic Range

Camera Analysis Data

Camera analysis data is shown in Table 4:

Gain Value 100 177 316 562 1000 1778 3162 5623 10000 15000
Logarithmic Gain (dB) 0 5.12 10.23 15 20.09 25.22 29.91 34.96 39.95 43.07
e-/ADU 0.64 0.36 0.2 0.11 0.06 0.04 0.02 0.01 0.01 0
Read Noise (e-) 0.54 0.45 0.44 0.4 0.38 0.36 0.36 0.36 0.38 0.39
Full Well Capacity (ke-) 2.6 1.5 0.8 0.5 0.3 1.4 0.08 0.05 0.03 0.02
Dynamic Range (stop) 12 11.67 10.86 10.21 9.43 8.63 7.86 7.04 6.15 5.62

Product Packaging and Connection

Packing List

Figure 1: G3M678M Packaging Information

Table 1: G3M678M Packing List

Item Description
A Outer Box: Length 50cm, Width 30cm, Height 30cm (20 units/box, 12-17kg/box, 0.045 cubic meters/box). Not shown in the photo.
B Inner Box: Length 15cm, Width 15cm, Height 10cm (Approx. 0.8-1.0kg per finished product box).
C G3M Series Camera with standard C-mount interface
D 2-meter USB3.0 high-speed cable (Type-A to Type-B)
E 2-meter ST4 guide scope cable
F 1.25-inch extension tube
G CD (Driver and utility software, Ø12cm)

Camera Dimensions and Mounting Bracket

Figure 2: G3M678M Dimensions and Mounting Bracket

The G3M series camera body is made of a sturdy alloy, ensuring a robust and durable camera structure. The camera is equipped with an IR-CUT or AR anti-reflection coated glass to protect the sensor and block infrared light while preventing reflection. There are no moving parts inside the camera. This design makes the camera more rugged and extends its lifespan compared to other industrial camera solutions.

Item Specification
1 Directly fits into a 1.25-inch telescope eyepiece holder.
2 G3M with a 1.25-inch extension tube, directly fits into a 1.25-inch telescope eyepiece holder.
3 Standard C-mount interface directly adapts to industrial C-mount lenses.

Camera Outline and Interfaces

Figure 3: Camera Outline and Interfaces

Item Specification
1 Built-in ST4 auto-guider interface for direct connection to equatorial mounts.
2 USB3.0 Type-B female port.

G3M678M and Software

ToupSky Installation

For software, customers can visit our software website at https://touptek-astro.cn to download the latest ToupSky. The G3M series cameras can also be used with ASCOM and DirectShow SDKs. If third-party software is compatible with these drivers, customers can download software drivers from our website and install them in the third-party software.

ToupSky is a Windows application for ToupTek astronomy cameras. ToupSky is a professional software that integrates camera control, image capture and processing, image browsing, and analysis functions. ToupSky has the following features:

Windows:

Features:

Supported Cameras:

User-Friendly Interface Design

ToupSky Video Window

ToupSky Browse Window

Professional Camera Control Panel

Function Description
Capture & Resolution Sets real-time and capture resolution, and captures images or records videos.
Capture & Gain Auto exposure (preset exposure target) and manual exposure (exposure time can be manually entered); Gain up to 5x.
White Balance Advanced one-key intelligent white balance setting, with manual temperature and tint adjustment.
Color Adjustment Hue, saturation, brightness, contrast, gamma initialization adjustment.
Frame Rate Adjustable frame rate for different computer configurations to ensure smooth video streaming.
Flip Select "Horizontal" or "Vertical" to correct video sampling orientation.
Binning Binning mode for low-noise video streams; Interval sampling mode for clearer, smoother video streams. Supports video stream histogram expansion, positive/negative switching, grayscale calibration, focus sharpness factor, etc.
Bit Depth Switch between 8-bit and 12-bit. 8-bit is the basic image format for Windows. 12-bit offers higher image quality but lower FPS.
ROI Region of Interest. This function allows setting ROI in the video window. When the ROI group is expanded, a dashed rectangle with "handles" will appear around the video window, which can be used to change the ROI. Adjust the ROI size using the mouse button. If the ROI is correct, click "Apply" to set the video to the ROI size; the default value will be restored to the original size.
Dark Frame Correction To enable dark frame correction, a dark frame image should be captured first. After capturing the image, the "Enable" button will be activated. Selecting it enables dark frame correction. Deselecting it disables dark frame correction.
Cooling Set the TE target cooling temperature and control the fan (On/Off).
Presets Load, save, overwrite, import, and export custom parameters for the camera control panel (including calibration information, exposure, and color settings).

Practical Functions for Good Results

Figure 4: Image Stacking

Compatibility

Interface Description
Preview Interface Supports Twain, DirectShow, Labview, SDK Package (Native C++, C#/VB.NET)
Operating System Compatible with Microsoft® Windows® XP / Vista / 7 / 8 /10 (32 & 64 bit), macOS, Linux
Multi-language Environment Currently supports Simplified Chinese, Traditional Chinese, English, Russian, German, French, Polish, and Turkish, with support for adding new languages.

Hardware Requirements

Computer Configuration Requirements
CPU Intel Core 2 2.8GHz or higher
Memory 2GB or more
USB Interface USB2.0 or higher high-speed interface
Display 17” or larger
CD-ROM Required

G3M678M and Dhow

ToupTekDshowAstroSetup (download via the blue link on the left)

DshowAstro is an interface driver that provides Dshow standard support for ToupTek USB astronomy cameras.

Supported Operating Systems: Windows:

Supported Cameras:

G3M678M and Third-Party Software

Supported Software

No. Software Version Native ASCOM WDM Others
1 PHD Guiding 2.3.0(2014)
2 Nebulosity 3.2.2(2014) ×
3 MaxIm DL 5.23(2013) ×
4 SharpCap 2.1(2014) ×
5 MetaGuide 5.2.0(2014)
6 FireCapture 2.4.05(2014)
7 Astroart 5.0(2014) ×

N.I.N.A

A powerful open-source free astronomy deep-sky imaging control system.

INDI

A popular third-party astronomy device driver, often used for Linux and MacOS systems.

ASCOM Platform

All AstroCam telescope camera drivers require the ASCOM platform to be installed.

Download ASCOM package from: http://www.ascom-standards.org/index.htm

You can download the ASCOM package from: http://ascom-standards.org/Downloads/Index.htm

PHD Guiding

Popular free guiding software: http://openphdguiding.org/

ToupTek telescope cameras support Native/ASCOM/WDM drivers for video operation.

Nebulosity

A popular cooled camera control/image processing software directly supported by ASCOM.

MetaGuide

An automatic guiding software with a novel approach to avoid atmospheric turbulence. The latest version supports GCMOS01200KPB. Guiding port: http://www.astrogeeks.com/Bliss/MetaGuide/

MAXIMDL

A well-known full-featured CCD control/image processing software, popular in the United States.

AstroArt

A well-known full-featured CCD control/image processing software, popular in Europe.

FireCapture

Great free planetary capture software. Supports some AstroCam series telescope cameras.

SharpCAP

A nice free planetary capture software that supports WDM cameras, including AstroCam series telescope cameras.

Registax

A popular free planetary stacking and processing software.

AstroStack

A planetary stacking and processing software.

DeepSky Stacker

Free deep-sky image stacking and processing software.

Service

For software upgrades, please refer to the "Download" section on our official website: https://ToupTek.com/

For customers who purchased cameras from local distributors, please contact your distributor for further inquiries.

For technical support, please contact the email address: karas@ToupTek.com.

PDF preview unavailable. Download the PDF instead.

G3M678M

Related Documents

Preview ToupTek G3M678M Astronomy Camera: User Manual and Specifications
Comprehensive user manual for the ToupTek G3M678M astronomy camera. Details specifications, features, software compatibility, and usage for astrophotography, including performance analysis and package contents.
Preview G3M2210M User Manual - ToupTek Astronomy Camera
Comprehensive user manual for the ToupTek G3M2210M astronomy camera, detailing its specifications, performance analysis, software compatibility, and usage.
Preview ATR3CMOS07100KMA User Manual - ToupTek Astronomy Camera
Comprehensive user manual for the ToupTek ATR3CMOS07100KMA astronomy camera, detailing specifications, features, software, and connections for astrophotography.
Preview SkyEye24AC User Manual: ToupTek Cooled Astronomy Camera Guide
Explore the ToupTek SkyEye24AC, a cooled full-frame astronomy camera for deep sky imaging. This manual covers its advanced features, technical specifications, software integration, and performance for astrophotographers.
Preview ToupTek ATR585C Astronomy Camera User Manual - Specifications, Features, and Software Guide
Comprehensive user manual for the ToupTek ATR585C cooled CMOS astrophotography camera. Details specifications, features, performance analysis, package contents, mechanical and electrical connections, and software compatibility with ToupSky and third-party applications.
Preview ATR533C Astronomy Camera User Manual
This user manual provides detailed information on the ATR533C astronomy camera, including its specifications, features, software, and connections. It covers technical data, performance analysis, and compatibility with various astronomy software.
Preview ToupTek GPM462M Astronomy Camera User Manual
Comprehensive user manual for the ToupTek GPM462M astronomy camera, detailing its specifications, features, performance analysis, software compatibility, and package contents.
Preview XCAM1080PHX Series Camera Help Manual
This manual provides comprehensive guidance on the ToupTek XCAM1080PHX series cameras, detailing their basic characteristics, specifications, dimensions, package contents, extension capabilities with microscopes and telescopes, software and app downloads, various application configurations (standalone, WiFi, Ethernet), user interface elements, measurement tools, and customer service information.