The GPM462C camera possesses an exceptionally strong capability to capture infrared light (with a high QE value at 500nm). 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 GPM462C are listed below:
Sensor |
Sony IMX462 back illuminated sensor |
|
Diagonal |
6.39 mm |
|
Image Resolution |
2.1 mega pixels (1920*1080) |
|
Pixel Size |
2.9mm x 2.9mm |
|
Image Area |
5.57mm x 3.13mm |
|
Max FPS at Resolution |
12bit |
8bit |
8.9 FPS @ 1920*1080 |
17.8 FPS @ 1920*1080 |
|
Shutter Type |
Rolling shutter |
|
Exposure Time |
0.1ms – 1000s |
|
Gain |
1x – 500x |
|
SNR |
40.8 dB |
|
Dynamic Range |
74.1 dB |
|
Read Noise |
2.4 – 0.76 e- |
|
QE Peak |
>89% |
|
Full Well |
12.7ke- |
|
ADC |
12bit |
|
Frame Buffer |
Built-in |
|
Connection Port |
USB2.0 Type C |
|
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 window) |
|
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 |
Back Focus Distance is 8.5mm,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 |
The sensor G Sensitivity of GPM462C is 2376mv with 1/30s. Its spectral sensitivity is shown in Figure 1. The sensitivity is measured with a testing standard lens with CM500S (t = 1.0mm) as an IR-cut filter and image at F5.6.
The GPM462C has built in 12bit ADC. It also has 12bit output mode for hardware binning and smaller resolution. The camera also supports hardware ROI, and the smaller the ROI size is, the higher the frame rate is.
Bit & Interface FPS Resolution |
12bit ADC |
8bit ADC |
USB2.0 |
USB 2.0 |
|
1920*1080 |
8.9 |
17.8 |
GPM462C camera has a built-in frame buffer, which helps maintain the stability of data transmission, and effectively reduce the amp-glow caused because image data can be temporarily buffered without being sent hastily to the receiver. Ensure that each camera can still achieve its maximum frame rate when multiple cameras are operating simultaneously.
The GPM462C supports digital binning from 1x1 to 8x8 in either stacking or averaging method.
GPM462C support HCG 、LCG mode switch.
The camera operates via a USB 2.0 interface. Upon establishing a connection with the host system using the USB 2.0 cable, the device is primed for operation.
Camera performance can be evaluated with e-/ADU, Read Noise, Full Well and Dynamic Range.
e-/ADU: The sensors found in cameras used for vision applications have pixels that convert incoming photons into electrons. Gain on a CCD /CMOS camera represents the conversion factor from electrons (e-) into digital counts, or Analog-Digital Units (ADUs). Gain is expressed as the number of electrons that get converted into a digital number, or electrons per ADU (e-/ADU).
Read Noise: Read Noise is the most important reference to measure the performance of a camera. Lower read noise usually means better SNR and better quality of image. Read Noise is created within the camera electronics during the readout process as the electrons are subjected to the analog to digital conversion, amplification and processing steps that enable an image to be produced.
Full Well: The electrons are held in each pixel and are converted into electrical charge which can be measured to show the amount of light that has fallen on each pixel. The maximum electrical charge possible is termed "full well capacity". Under the same conditions such as noise and A/D converter quality, the greater full well capacity a sensor has, the wider dynamic range the sensor has. As there is a limit to the depth to which pixels can be made, the full well capacity is often proportional to the frontal area of the light gathering element of the pixel.
Dynamic Range is the ratio between the maximum output signal level and the noise floor at minimum signal amplification (noise floor which is the RMS (root mean square) noise level in a black image). The noise floor of the camera contains sensor readout noise, camera processing noise and the dark current shot noise. Dynamic range represents the camera’s ability to display/reproduce the brightest and darkest portions of the image and how many variations in between. This is technically intra-scene dynamic range. Within one image there may be a portion that is in complete black and a portion that is completely saturated.
For the GPM series camera, the Gain Value is in xxx% mode. Here xxx is used as the x axis (Gain Value) for the description of the camera performance
Read noise is the most important reference to measure the performance of a camera. Lower read noise usually means better SNR and better quality of image.
Camera setting used for performance analysis is shown below:
Sensor Analysis Data |
||||||||
Gain Value |
100 |
177 |
316 |
562 |
1000 |
1778 |
3162 |
4998 |
Rel Gain (dB) |
0.00 |
4.87 |
9.98 |
14.87 |
19.89 |
25.02 |
29.92 |
33.91 |
e-/ADU |
2.96 |
1.69 |
0.94 |
0.53 |
0.30 |
0.17 |
0.09 |
0.06 |
Read Noise (e-) |
2.4 |
2.10 |
1.84 |
1.72 |
1.62 |
1.54 |
1.48 |
1.50 |
Full Well (ke-) |
12.1 |
6.9 |
3.8 |
2.2 |
1.2 |
0.7 |
0.4 |
0.2 |
Dynamic Range (stop) |
12 |
11.68 |
11.03 |
10.32 |
9.56 |
8.78 |
8.03 |
7.35 |
Camera setting used for performance analysis is shown below:
Sensor Analysis Data |
|||||||||||
Gain Value |
100 |
177 |
316 |
562 |
1000 |
1778 |
3162 |
4998 |
|||
Rel Gain (dB) |
0 |
4.84 |
9.91 |
14.75 |
19.83 |
24.88 |
29.81 |
33.95 |
|||
e-/ADU |
1.17 |
0.67 |
0.37 |
0.21 |
0.12 |
0.07 |
0.04 |
0.02 |
|||
Read Noise (e-) |
1.08 |
0.93 |
0.85 |
0.81 |
0.75 |
0.74 |
0.71 |
0.70 |
|||
Full Well (ke-) |
4.8 |
2.8 |
1.5 |
0.9 |
0.5 |
0.3 |
0.2 |
0.1 |
|||
Dynamic Range (stop) |
12 |
11.53 |
10.81 |
10.08 |
9.34 |
8.54 |
7.77 |
7.09 |
Standard Camera Packing List |
|
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 GPM series camera with a Type-C-Mount(inner) |
D |
High-speed USB3.0 A male to C male connectors cable /2.0m |
F |
1.25-inch nosepiece |
G |
ST4 guide cable /2.0m |
H |
CS-mount ring |
The GPM series body, made from tough, alloy, ensures a heavy duty, workhorse solution. The camera is designed with a high-quality IR-CUT or AR to protect the camera sensor and block the IR elimination the reflection light. No moving parts included. These measures ensure a rugged, robust solution with an increased lifespan when compared to other industrial camera solutions.
Item |
Specification |
1 |
Directly with 1.25’’ telescope; |
2 |
GPM + 1.25’’ extender with 1.25’’ telescope |
3 |
Standard C adapter connects to industrial C-mount adapter lens. |
Item |
Specification |
1 |
A built-in ST4 auto guider port for the easy connection of the auto guider. |
2 |
USB2.0 interface, Type C |