G3M2210M User Manual

Version 1.0

Sept 2023

All materials related to this publication are subject to change without notice and its copyright totally belongs to ToupTek Photonics.

Please download the latest version from touptek-astro.com.

1 Description and Features

The G3M2210M camera possesses an exceptionally strong capability to capture infrared light (with a high QE value at 850nm). It also has a large full well capacity, high dynamic range, high sensitivity, and low readout noise among other advantages. This results in outstanding performance in planetary photography, as well as in solar and lunar photography.

The features of G3M2210M are listed below:

2 G3M2210M Specifications and Performance

2.1 Camera Specifications

Table 1 G3M2210M Technique Specifications.

Sensor SmartSens SC2210 back illuminated sensor
Diagonal 8.81 mm
Image Resolution 2.1 mega pixels (1920*1080)
Pixel Size 4µm × 4µm
Image Area 7.68mm x 4.32mm
Max FPS at Resolution (USB 3.0) 12bit
92.8 FPS @ 1920*1080
113 FPS @ 960*540
8bit
150 FPS @ 1920*1080
184 FPS @ 960*540
Max FPS at Resolution (USB 2.0) 14bit
9.2 FPS @ 1920*1080
11.3 FPS @ 960*540
8bit
15 FPS @ 1920*1080
18.4 FPS @ 960*540
Shutter Type Rolling shutter
Exposure Time 0.1ms - 500s
Gain 1x - 150x
SNR 39.3 dB
Dynamic Range 68.5 dB
Read Noise 3.2 - 0.47 e-
QE Peak >92%
Full Well 8.5ke-
ADC 12bit
DDR3 Buffer 512MB (4Gb)
Connection Port USB3.0/USB2.0
Camera Adaptor Standard 1.25" for telescope connection, and standard C adapter for industrial lens
Protect Windows IR-cut filter/AR-window
Spectral Range 380-690nm (with IR-cut filter)
Capture/Control SDK Windows/Linux/macOS/Android Multiple Platform SDK(Native C/C++, C#/VB.NET, Python, Java, DirectShow, Twain, etc.);
Recording System Still picture and movie
Camera Dimensions Diameter 37mm * height 72.4mm
Camera Weight 70 gram
Back Focus Distance 17.5mm with C adapter, 12.5 with CS adapter
Cooling: Passive cooling
Supported OS Microsoft® Windows® XP / Vista / 7 / 8 /10 (32 & 64 bit)
OSX(Mac OS X)
Linux

2.2 SmartSens SC2210 Sensitivity

The sensor G Sensitivity of G3M2210M is 20100mv/lux*s. Its spectral sensitivity is shown in Figure 1.

Figure 1 describes the Spectral Sensitivity Characteristic of the SC2210 sensor. The graph plots QE (%) on the y-axis against Wavelength (nm) on the x-axis, showing a peak sensitivity in the green light spectrum (around 500-600 nm) and decreasing sensitivity towards the infrared spectrum (around 850 nm and beyond).

2.3 12bit ADC and ROI

The G3M2210M has a built-in 12bit ADC. It also supports a 12bit output mode for hardware binning and smaller resolution. The camera supports hardware ROI (Region of Interest), where a smaller ROI size results in a higher frame rate.

Table 2 shows the frame rate of the G3M2210M in 12/8bit mode, USB3.0 / USB2.0 data transfer interface at different resolutions:

Table 2 G3M2210M Frame Rate at Different Resolution/Data Bit/Data Transfer (USB3.0/ USB2.0)
Resolution 12bit ADC 8bit ADC
USB3.0 USB2.0 USB 3.0 USB 2.0
1920*1080 92.8 9.2 150 15
960*540 113 11.3 184 18.4

2.4 DDR3 Buffer

The G3M2210M camera features a 512MB (4Gb) DDR3 buffer. This buffer helps maintain the stability of data transmission and effectively reduces amp-glow by temporarily buffering image data before sending it to the receiver.

2.5 Binning

The G3M2210M supports digital binning from 1x1 to 8x8 (stacking or averaging methods) and hardware binning from 1x1 to 2x2 (averaging method). Hardware pixel binning is significantly faster than software binning.

2.6 Conversion Gain Switch

The G3M2210M does not support HCG (High Conversion Gain) or LCG (Low Conversion Gain) mode switching.

2.7 Power System

The camera operates via a USB 3.0 interface. Upon establishing a connection with the host system using the USB 3.0 cable, the device is ready for operation.

2.8 Camera Performance Analysis

Camera performance can be evaluated using metrics such as e-/ADU, Read Noise, Full Well capacity, and Dynamic Range.

e-/ADU: Sensors convert incoming photons into electrons. Gain is the conversion factor from electrons (e-) to digital counts (ADUs), expressed as electrons per ADU (e-/ADU).

Read Noise: A critical performance metric. Lower read noise generally indicates better Signal-to-Noise Ratio (SNR) and image quality. It originates from the camera electronics during the readout process, including analog-to-digital conversion, amplification, and processing.

Full Well: Represents the maximum number of electrons a pixel can hold before saturation. A larger full well capacity, under similar noise and ADC conditions, leads to a wider dynamic range. It is often proportional to the pixel's frontal area.

Dynamic Range: The ratio between the maximum output signal level and the noise floor at minimum signal amplification. It indicates the camera's ability to reproduce both the brightest and darkest portions of an image simultaneously. The noise floor includes sensor readout noise, processing noise, and dark current shot noise.

For the G3M series camera, the Gain Value is expressed in 'xxx%' mode, where 'xxx' represents the gain value on the x-axis for performance descriptions. The relationship is given by:

Rel Gain(dB) = 20 * log10[xxx(Gain Value)/100]

xxx(Gain Value) = 100 × 10(Rel Gain(dB)/20)

Lower read noise generally correlates with better SNR and image quality.

Camera settings used for performance analysis are:

Figure 2 illustrates the camera analysis data presented in Table 3.

Figure 2 displays three plots: e/ADU vs. Gain, Read Noise vs. Gain, Full Well vs. Gain, and Dynamic Range vs. Gain. The x-axis represents Gain/Gain(dB), and the y-axes show the respective performance metrics.

Table 3 Camera Analysis Data
Gain Value 100 1100 2100 3100 4100 5100 6100 7100 8100 9100 10100 11100 12100 13100 14100 15100
Rel Gain (dB) 0.00 2.87 4.99 7.48 9.93 11.85 13.48 15.61 18.04 20.5 22.43 25.32 27.48 29.93 32.44 34.19
e-/ADU 4.16 2.99 2.34 1.76 1.33 1.06 0.88 0.69 0.52 0.39 0.31 0.23 0.18 0.13 0.1 0.08
Read Noise (e-) 3.17 2.76 2.54 2.18 2.03 1.93 0.97 0.91 0.81 0.75 0.72 0.67 0.64 0.59 0.53 0.47
Full Well (ke-) 8.5 6.1 4.8 3.6 2.7 2.2 1.8 1.4 1.1 0.8 0.6 0.5 0.4 0.3 0.2 0.2
Dynamic Range
(stop)
11 11 10.88 10.69 10.39 10.14 10.87 10.6 10.37 10.06 9.8 9.44 9.44 9.13 8.85 8.45

3 Product Package and Connections

3.1 Packing List

Figure 3 shows the packing information for the G3M2210M camera.

Table 4 G3M2210M Packing List
Item Description
A Carton L:50cm W:30cm H:30cm (20pcs, 12~17Kg/carton, 0.045m³), not shown in the photo
B Gift box L:15cm W:15cm H:10cm (0.8~1.0Kg/box)
C One G3M series USB3.0 camera with 1.25" interface(outer) and C-Mount(inner)
D High-speed USB3.0 A male to B male gold-plated connectors cable /2.0m
E 2.0m guide cable
F 1.25-inch nosepiece
G CD (Driver & utilities software, Ø12cm)
H (Optional Accessory) CS-mount ring

3.2 Camera Dimension and Its Mount

Figure 4 illustrates the dimensions and mounting options for the G3M2210M camera and its 1.25" extender.

The G3M series body is constructed from tough alloy, ensuring a heavy-duty, workhorse solution. The camera is designed with a high-quality IR-CUT or AR coating to protect the camera sensor and block IR reflection. It features no moving parts, ensuring a rugged, robust solution with an increased lifespan compared to other industrial camera solutions.

Table 5 Adapter of G3M2210M
Item Specification
1 Directly with 1.25" telescope;
2 G3M + 1.25" extender with 1.25" telescope
3 Standard C adapter connects to industrial C-mount adapter lens.

3.3 Camera Outline and Interface

Figure 5 shows the camera outline and identifies its interfaces.

Table 6 Camera Outline and Interface List
Item Specification
1 A built-in ST4 auto guider port for the easy connection of the auto guider.
2 USB3.0 interface.

4 G3M2210M and Its Software

4.1 Application Installation

For software, customers can visit the official website touptek-astro.com to download the latest ToupSky software. The G3M camera is also compatible with ASCOM and DirectShow SDKs. If third-party software supports these SDKs, drivers can be downloaded from the website and installed.

ToupSky is ToupTek's Windows application for astronomy cameras. It is a professional software integrating camera control, image capture & process, image browse, and analysis functions. ToupSky offers the following features:

Windows Requirements:

Features:

Supported Camera:

4.1.1 User-friendly UI Design

ToupSky features well-arranged menus and toolbars for quick operation. It has a unique design with three sidebars (Camera, Folders, Undo/Redo) for organized classification. Operation is convenient, utilizing double-click or right-click context menus where possible. A detailed help manual is also available.

Figure 6 shows the ToupSky interface and its video window, displaying camera controls and a preview of captured imagery.

Figure 7 displays the ToupSky browse window, used for viewing captured images.

4.1.2 Professional Camera Control Panel

The ToupSky software provides a comprehensive control panel with the following functions:

Function Description
Capture & Resolution Set live and snap resolution; capture images or record video.
Exposure & Gain Auto exposure (preset target) and manual exposure (inputtable time); up to 5x gain.
Color Balance Advanced single-click white balance; manual adjustment of temperature and tint.
Color Adjustment Hue, saturation, brightness, contrast, gamma initialization adjustment.
Frame Rate Adjustable frame rate for different computer configurations.
Flip Correct sample direction by selecting "horizontal" or "vertical".
Sampling Bin mode for low noise video; Skip mode for sharper/smoother video. Supports video stream histogram extension, negative/positive switching, gray calibration, and clarity adjustment for focusing.
Bit Depth Switch between 8-bit and 12-bit. 8-bit is standard Windows format; 12-bit offers higher image quality at moderate FPS.
ROI Region of Interest. Set ROI on the video window using handles. Mouse adjustment of ROI size. Apply to set video to ROI size; Defaults returns to original size.
Dark Field Correction Enable Dark Field Correction by capturing a dark field image first. The 'Enable' button becomes clickable after capture. Unchecking disables the correction.
Cooling Set TE-Cooling target temperature and fan On/Off.
Parameters Load, save, overwrite, import, export self-defined parameters (including calibration, exposure, and color settings).

4.1.3 Practical Functions with Good Results

ToupSky offers practical functions for enhanced imaging:

Function Category Description
Video functions Video broadcast, time lapse capture, video record, video stream grid, image stitch, video scale bar, date display, etc.
Image Processing and Enhancement Denoise, sharpen, color toning, deinterlace, various filtering algorithms, mathematical morphology, range, binary, pseudo color, surface plot, and line profile adjustments.
Image Stacking Utilizes advanced image matching technology. Stacks recorded video frames, correcting for shifting, rotation, and scaling to reduce image noise and improve fidelity.

Figure 8 illustrates the concept of image stacking, where multiple input images are combined to produce a final stacked image.

4.1.4 Powerful Compatibility

Category Details
Video Interface Supports Twain, DirectShow, SDK Package (Native C++, C#/VB.NET)
Operating System Compatible with Microsoft® Windows® XP / Vista / 7 / 8 /10 (32 & 64 bit), macOS, Linux
Language Support Unlimited language support, including Simplified Chinese, Traditional Chinese, English, Russian, German, French, Polish, and Turkish.

4.1.5 Hardware Requirement

PC Requirements
Component Specification
CPU Intel Core 2 2.8GHz or higher
Memory 2GB or more
USB port USB3.0/USB2.0 port
Display 17" or larger
Other CD-ROM

4.2 G3M2210M and Dshow

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

Supported OS: Windows:

Supported Camera:

4.3 G3M2210M and the 3rd Party Software

4.3.1 Support Software

Supported Software List
No. Software Version WDM ASCOM Native
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) ✔️ /

4.3.2 ASCOM Platform

All AstroCam telescope camera drivers require the ASCOM platform, which is available for free. You can download the ASCOM package from: ascom-standards.org/Downloads/Index.htm.

4.3.3 PHD Guiding

A popular free guiding software. Visit openphdguiding.org for more information. ToupTek's telescope cameras support Native/ASCOM/WDM drivers for video operation.

4.3.4 Nebulosity

A popular cooled camera control and image processing software directly supported via ASCOM.

4.3.5 MetaGuide

Autoguiding software with a novel method to avoid atmospheric agitation. The latest version supports GCMOS01200KPB and the guide port. More information can be found at: astrogeeks.com/Bliss/MetaGuide/.

4.3.6 MAXIMDL

A famous, full-functional CCD Control/Image Process software, popular in the US.

4.3.7 AstroArt

A famous, full-functional CCD Control/Image Process software, popular in Europe.

4.3.8 FireCapture

Great free planetary capture software. Supports part of the AstroCam series telescope cameras.

4.3.9 SharpCAP

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

4.3.10 Registax

A popular free planetary stacking and processing software.

4.3.11 AstroStack

A planetary stacking and process software.

4.3.12 DeepSky Stacker

A free deep sky image stacking and processing software.

5 Service

For software upgrades, please refer to "Download" on the official website: https://touptek-astro.com/.

For customers purchasing cameras from a local dealer, please contact your dealer for more inquiries.

For technical support, please contact via email at: karas@Touptek-astro.com.

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