ToupTek SkyEye24AC Full Frame Color Astro Camera User Manual
- August 16, 2024
- TOUPTEK
Table of Contents
ToupTek SkyEye24AC Full Frame Color Astro Camera
Specifications
Item | Specification |
---|---|
Sensor | Sony IMX410 Color CMOS |
Diagonal | 43.3 mm |
Image Resolution | 24 mega pixels, 6064 x 4040 |
Pixel Size | 5.94μm x 5.94μm |
Image Size | 36.02mm x 23.998mm |
Max FPS at Resolution (USB 3.0) | 8.0 FPS @ 6064 x 4040 |
Max FPS at Resolution Low Noise (USB 3.0) | 19.5 FPS @ 3024 x 2012 |
Max FPS at Resolution (USB 2.0) | 0.9 FPS @ 6064 x 4040 |
Max FPS at Resolution Low Noise (USB 2.0) | 3.7 FPS @ 3024 x 2012 |
Product Usage Instructions
Installation and Setup
Before using the SkyEye24AC camera, ensure that you have downloaded the
necessary software from touptek-astro.com. Connect
the camera to your computer using the appropriate connection port.
Post-Processing
After capturing images, transfer them to your preferred image processing
software for editing and enhancement. Adjust brightness, contrast, and colors
to achieve the desired astrophotography results.
FAQ
Q: How do I update the camera software?
A: To update the camera software, visit touptek-astro.com and download the latest version of the software compatible with
your SkyEye24AC camera.
SkyEye24AC User Manual
Version 2.1
Apr 2024
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.
Description and Features
With full frame sensor, precise temperature regulation, ultra-low readout
noise and zero amp-glow, The SkyEye24AC camera is mainly used for deep sky
photo shooting. Its extraordinary performance and extensive usage will give
you great astrophotography experience.
The features of SkyEye24AC are listed below:
- IMX 410 Color CMOS Sensor
- Resolution: 6064 x 4040
- 5.94 μm Square Pixels
- 43.3mm Full Frame Optical Format
- 14-bit ADC
- 512 Mbyte Memory Onboard
- Precise Temperature Regulation
- Zero Amp-Glow
- G Sensitivity: 572.76mV with 1/30s
- Ultra-Low Noise: 1.95 to 4.48 e- (Low Noise Mode)
- Support Low Noise Mode/ High Frame Rate Mode (15.2 FPS at all Pixel Readout 8 bit)
- Support HCG Mode/ LCG Mode
- SNR Max: 50.2 dB (Low Noise Mode)
- Dynamic Range: 87.3 dB (Low Noise Mode)
- -30C below ambient under short exposure/ -35C under long exposure time (> 1s)
SkyEye24AC Specifications and Performance
Camera Specifications
Item | Specifications |
---|---|
Sensor | Sony IMX410 Color CMOS |
Diagonal | 43.3 mm |
Image Resolution | 24 mega pixels, 6064´ 4040 |
Pixel Size | 5.94mm ´ 5.94mm |
Image Size | 36.02mm ´ 23.998mm |
Max FPS at Resolution (USB 3.0) | 14bit |
8.0 FPS @ 60644040
19.5 FPS @ 30242012
64.3 FPS @ 20161342| 16.0 FPS @ 60644040
38.8 FPS @ 30242012
114.6 FPS @ 20161342
Max FPS at Resolution Low Noise (USB 3.0)|
14bit| 8bit
4.6 FPS @ 60644040
9.7 FPS @ 30242012
32.2 FPS @ 20161342| 9.2 FPS @ 60644040
19.4 FPS @ 30242012
57.3 FPS @ 20161342
Max FPS at Resolution (USB 2.0)| 14bit| 8bit
0.9 FPS @ 60644040
3.7 FPS @ 30242012
8.3 FPS @ 20161342| 1.8 FPS @ 60644040
7.4 FPS @ 30242012
16.5 FPS @ 20161342
Max FPS at Resolution Low Noise (USB 2.0)|
14bit| 8bit
0.4 FPS @ 60644040
2.5 FPS @ 30242012
5.8 FPS @ 20161342| 0.8 FPS @ 60644040
5.0 FPS @ 30242012
11.6 FPS @ 20161342
Shutter Type| Rolling Shutter
Exposure Time| 0.1ms – 3600s
Gain| 1x – 150x
SNR| 50.2 dB
Dynamic Range| 87.3 dB (Low Noise Mode)
Read Noise(LCG)| 4.48 – 1.95 e-
Read Noise (HCG)| 0.68 – 0.3 e-
QE Peak| >80%
Full Well| 104ke- (20ke- @HCG)
ADC| 14bit
DDR3 Buffer| 512MB (4Gb)
Connection Port| USB3.0/USB2.0
Camera Adaptor| M54 ´ 0.75
Protect Windows| IR CUT
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 89 * Height 103 (mm)
Camera Weight| 0.718kg
Back Focus Distance| 17.5mm
Cooling:| Two stage TEC
Effective Cooling Temp:| -30°C below ambient under short
exposure/ -35°C under long exposure (> 1s)
---|---
Supported OS| Microsoft® Windows® XP / Vista / 7 / 8 /10 (32 & 64
bit)
OSx(Mac OS X)
Linux
Sony IMX410 Sensitivity
The sensor G sensitivity of SkyEye24AC is 572.76mV with 1/30s. Its spectral
sensitivity is shown in Figure 2
Figure 2 IMX410 Sensitivity Spectral Characteristic
it ADC and ROI
The SkyEye24AC has built in 14bit 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 faster frame rate is.
Table 2 SkyEye24AC Frame Rate at Different Resolution/Data Bit/Data
Transfer(USB3.0/ USB2.0)
DDR3 Buffer
SkyEye24AC camera has a 512MB (4Gb) DDR3 buffer, which helps maintain the
stability of data transmission, and effectively reducing the amp-glow caused
because image data can be temporarily buffered without being sent hastily to
the receiver.
Binning
The SkyEye24AC supports digital binning from 11 to 8 in either stacking or
averaging method, and hardware binning from 11 to 33 in averaging method.
Hardware pixel binning is much faster than software binning.
Conversion Gain Switch
SkyEye24AC supports HCG and LCG mode switch. Under HCG mode, the readout noise
could reach 0.3 e- at maximum gain setting.
Power and Cooling System for Precise Temperature Regulation
The cooling system of SkyEye24AC is two-stage Thermoelectric Cooling (TEC)
with controllable electric fan assisting heat dissipation. The working
temperature can be regulated to specific number, and effective temperature
drop can be -35C from ambient temperature. Such efficient cooling system
guarantees the stability of ultra-low noise mode and quality of the camera
image.
The TEC system is controlled by PID algorithm, which allows the TEC to be
precisely regulated towards the target temperature with 0.1C deviation.
Zero Amp-Glow
The SkyEye24AC has been carefully designed and is able to achieve zero amp-
glow photo shooting. Figure 3 Amp-glow. and Figure 4 show the different
cameras at 20C and 5-minute exposure time with and without amp-glow. One can
find that SkyEye24AC captured image has zero amp-glow.
Camera Performance Analysis
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 SkyEye 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
??? ????(??) = 20 ∗ ???10[???(???? ?????)/100] ???(???? ?????) = 100 × 10(???
????(??)/20
SkyEye24AC has a significantly low read noise: 4.48 – 0.68e-. It is more
impressive that this camera comes with low noise mode, which means users could
get even lower readout noise by selecting low noise mode while the frame rate
only drops a little as sacrifice.
Camera setting used for performance analysis in
HCG mode is as follow:
- Full resolution
- RAW 14 Bit mode
- Temperature: -5
Table 3 Sensor Analysis Data in HCG Mode
SensorAnalysis Data
Gain Value| 100| 158| 251| 398| 630| 1000| 1584| 2511| 3981| 6309|
10000| 15000
Rel Gain (dB)| 0.00| 4.17| 8.17| 12.16| 16.03| 20.12| 24.09|
28.02| 32.02| 35.95| 39.78| 42.56
e- /ADU| 1.22| 0.77| 0.49| 0.31| 0.2| 0.12| 0.08| 0.05| 0.03| 0.02|
0.01| 0.01
Read Noise Normal (e-)| 0.68| 0.62| 0.62| 0.61| 0.59| 0.57|
0.55| 0.52| 0.49| 0.42| 0.39| 0.3
Full Well (ke-)| 20| 12.7| 8.81| 5.05| 3.2| 2.02| 1.28| 0.8|
0.51| 0.32| 0.21| 0.15
DR (stop)| 14| 14| 13.66| 13.02| 12.41| 11.78| 11.18| 10.61| 10.02|
9.54| 9.08| 8.97
Camera setting used for performance analysis in LCG mode is as follow:
- Full resolution
- RAW 14 bit mode
- Temperature: -5
Table 4 Sensor Analysis Data in LCG Mode
SensorAnalysis Data
Gain Value| 100| 158| 251| 398| 630| 1000| 1584| 2511| 3981| 6309|
10000| 15000
Rel Gain| 0.00| 3.95| 7.97| 11.96| 15.93| 19.93| 23.92| 27.87|
31.92| 35.87| 39.78| 42.69
e- /ADU| 6.33| 4.02| 2.53| 1.6| 1.01| 0.64| 0.4| 0.26| 0.16| 0.1|
0.06| 0.05
Read Noise (e-)| 4.48| 4.12| 4.3| 4.16| 3.96| 3.8| 3.62| 3.5|
3.36| 3.14| 2.55| 1.95
Full Well(ke-)| 104| 65.8| 41.5| 26.2| 16.6| 10.5| 6.61| 4.19| 2.63|
1.67| 1.06| 0.76
DR(stop)| 14| 13.96| 13.24| 12.62| 12.03| 11.43| 10.83| 10.22| 9.61|
9.05| 8.70| 8.61
Product Package and Connections
packing List
Standard Package
A| 3-A safety equipment case: L:26.2cm W:24.0cm H:12.4cm (1pcs, 3.9Kg/ box)
B| SkyEye camera (M54Fx0.75 mount)
C| Power adapter: input: AC 100~240V 50Hz/F60Hz, output: DC 12V 3A
D| High-Speed USB3.0 A male to B male gold-plated connectors cable /1.5m
E| CD (Driver & utilities software, Ø12cm)
F| Hex wrench H 2.0
G| M54M-M48F 21mm extender
H| M48M-M48F 16.5mm extender
I| M48M-M42F adapter
Camera Dimension and Its Mount
Table 6 Dimension and Mount of SkyEye24AC
Item | Specification |
---|---|
Diameter | Æ89mm |
Height | 103mm |
Mount | M54Fx0.75mm |
Camera Outline and Interface
Item | Specification |
---|---|
1 | Protective window, 39 ´ 27 ´ 1.1mm, AR window for mono camera, IR-CUT for |
color camera
2| M54F ´ 0.75 thread
3| Air inlet
4| Thermo outlet
5| USB 2.0 HUB
6| USB 3.0/ USB 2.0 port
7| DC 12V 3A power port, 5.5 ´ 2.1mm
8| LED indicators: 1) Power LED. 2) System LED. 3)TEC LED. 4)Fan LED
Camera Mechanical Connection with Adapter
The SkyEye24AC can be connected to a telescope with proper adapter, or the
camera lens. The most common adapters are already included in the package, but
we also provide some specific adaptors based on the requirement.
The female flange to the sensor is 17.5mm. User can make it to 55mm back focus
distance with the 21mm and 16.5mm extender included in the camera package.
Please check Figure 10 for details.
Item | Specification |
---|---|
Back Focal Distance | Protective window, 39 ´ 27 ´ 1.1mm, AR window for mono |
camera, IR-CUT for color camera
M54M-M48F 21mm extender| 21mm with M48Fx0.75mm for M48M´ 0.75 telescope
M48M-M48F 16.5mm extender| 16.5mm with M48Fx0.75mm for M48M´ 0.75 telescope
M48M-M42F 0mm adapter| 0mm with M48Fx0.75mm for M42F´ 0.75 telescope
Camera Mechanical Connection with Lens
Item | Specification |
---|---|
1 | Nikon F-M54 adapter |
2 | EOS EF-M54 adapter |
3 | Nikon F-Mount lens |
4 | Canon EF-Mount lens |
5 | SkyEye camera with M54Fx0.75 mount |
Camera Tilt Adjustment
SkyEye24AC has the tilt adjustment ability. There are 3 sets of screws that
can be used to tilt the sensor, making it parallel with the telescope, two
screws per set for screw in /out.
One can refer to below:
Table 10 Camera Tilt Adjustment
Steps | Operations |
---|---|
1 | Take a starred image with the camera, user can easily find out the tilt |
part in the image through the software(such as
siril、ccdinspector、astap), and then adjust one or more sets of flange adjustment screws on the camera corresponding to the imaging result.
2| Take another image after the sensor tilt adjustment, and compare it with
the previous one in the software. If the tilt issue is reduced, that means the
adjustment is correct. Otherwise, the adjustment is wrong.
3| Repeat step 2 until the stars in all corners are perfect.
Camera Electric Connection with Accessories
On the back side of SkyEye24AC, there are 3 connection ports: DC 12V/3A power
port, USB3.0/ USB2.0 port and USB-HUB.
Due to the significantly larger power consumption of IMX410, SkyEye24AC
(including the cooling system) is now booted up only by 12V/3A power supply.
USB3.0 no longer works as a power source but only as a data communication
method. The USB-HUB provides connection with other devices, which allows user
to avoid the mess of cable management. Once another device is connected
through the USB-HUB, it will be connected to PC device through the
USB3.0/USB2.0 port.
Table 11 Camera Electric Connection
Item | Specification |
---|---|
USB3.0/USb2.0 port | To computer with USB3.0/USB2.0 cable |
USB HUB for accessories
| To filter wheel with USB2.0 cable
To guiding camera with USB 2.0 cable
Power port| DC12V/3A
SkyEye24AC and Its Software
Application Installation
For software, customers are welcomed to go to our software website: https
://touptek-astro.com/downloads/ , to download the latest ToupSky. The SkyEye
can also be used with ASCOM, DirectShow SDK. If the third-party software is
compatible with these SDK, customers can also download the software driver
from our website and install the drivers into the third-party software.
ToupSky is ToupTek astronomy camera’s Windows application. ToupSky is a
professional software integrated with camera control, image capture & process,
image browse, and analysis functions. ToupSky was born with the following
features:
Windows:
- x86: XP SP3 or above; CPU supports SSE2 instruction set or above
- x64: Win7 or above
Features
- Fully control of the camera
- Trigger mode and video mode support (raw format or RGB format)
- Automatic capture and quick record function
- Multi-language support
- Hardware ROI and digital binning function
- Extensive image processing functions, like image stitching, live stacking, flat field correction, dark field correction, etc.
Supported Camera:
- All ToupTek astronomy cameras
User-friendly UI Design
- Well-arranged menus and toolbars ensure quick operating;
- The unique design of 3 sidebars — Camera, Folders, Undo/Redo are orderly classified
- Convenient operating method (Double click or right-click context menu) as much as possible;
- Detailed help manual;
Professional Camera Control Panel
Capture & Resolution| Set the live and snap resolution and snap the image or
record video;
---|---
Exposure & Gain| Auto exposure (exposure target preset) and manual exposure
(exposure time can be inputted manually); Up to 5 times gain;
Color Balance| Advanced single-click intelligent white balance setting,
temperature and tint can be manually adjusted;
Color Adjustment| Hue, saturation, brightness, contrast, gamma initialization
adjustment;
Frame Rate| Adjustment of frame rate available for different computer
configurations;
Flip| Check the “horizontal” or “vertical” option to correct the sample
direction;
Sampling| Bin mode can obtain low noise video stream; Skip mode obtains
sharper and smoother video stream. Support video stream
histogram extension, Negative and positive switching, Gray calibration, Clarity factor for focusing etc.
Bit Depth| Switch between 8 bits and 12 bits. 8 bits is the basic Windows
image format. 12bits will have higher image quality but moderate FPS.
ROI| ROI, Region of interest. This function can set the ROI on the video
window. When the ROI group was expanded, a dotted rectangle with “Handles”
will appear around the video window that will let you alter the ROI. Use mouse
button to adjust
the ROI size. If ROI is ok, click Apply will set the video to ROI size, Defaults will return to the original size.
Dark Field Correction| To Enable the Dark Field Correction, one should capture
the dark field image first. After the images are captured, the Enable button
will be clickable. Checking the Enable button will enable the Dark Field
correction. Unchecking it will disable the Dark Field Correction.
Cooling| Set the TE-Cooling target temperature and set the fan On/Off;
Parameters| Load, save, overwrite, import, export self-defined parameters of
camera control panel (including calibration information,
exposure and color setting information);
Practical Functions with Good Results
Video functions| Various professional functions: Video broadcast; Time lapse
capture; Video record; Video stream grid; Image stitch; Video scale bar, date
etc.
---|---
Image Processing and
Enhancement
| Control and adjust image by denoise, sharpen, color toning deinterlace, all kinds of filtering algorithm and mathematical
morphology algorithm, range, binary, pseudo color, surface plot and line profile ital..
Image Stacking| Image stacking adopts advanced image matching technology. With the recorded video, regardless of shifting, rotation, scaling, the high- fidelity image can be stacked to decrease the image noise.
Powerful Compatibility
Video Interface | Support Twain, DirectShow, SDK Package(Native C++、C#/VB.NET) |
---|---|
Operating System | Compatible with Microsoft® Windows® XP / Vista / 7 / 8 /10 |
(32 & 64 bit), Mac OSX, Linux
Language Support| Unlimited language support, currently available in
Simplified Chinese, Traditional Chinese, English, Russian, German, French,
Polish and Turkish
Hardware Requirement
PC Requirements | CPU: Intel Core 2 2.8GHz or higher |
---|
Memory:2GB or more
USB port: USB3.0/USB2.0 port
Display:17” or larger
CD-ROM
SkyEye24AC and Dshow
ToupTekDshowAstroSetup (Click the left blue link to download)
DshowAstro is an interface driver providing Dshow standard support for ToupTek
USB astronomy camera Supported
OS: Windows:
- x86: XP SP3 or above; CPU supports SSE2 instruction set or above
- x64: Win7 or above Supported Camera:
- All ToupTek astronomy cameras
SkyEye24AC and the 3rd Party Software
Support Software
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) | √ | × | / |
-
ASCOM Platform
All AstroCam telescope camera drivers request to install ASCOM p atform, free. http://www.ascomstandards.org/index.htm
You can download the ASCOM package from : http://ascomstandards.org/Downloads/Index.htm -
PHD Guiding
A popular free guide software: http://openphdguiding.org/
ToupTek’s telescope camera support Native/ASCOM/WDM driver to run the video. -
Nebulosity
A popular cooled camera control/image process software directly supported via ASCOM. -
MetaGuide
Autoguiding software with novel method to avoid the atmospheric agitation. The latest version support GCMOS01200KPB and the guide port: http://www.astrogeeks.com/Bliss/MetaGuide/ -
MAXIMDL
Famous full functional CCD Control/Image Process software.
Popular used in US. -
AstroArt
Famous full functional CCD Control/Image Process software. Popular used in Europe. -
FireCapture Great free planetary capture software. Support
part of AstroCam series telescope camera. -
SharpCAP
A nice free planetary capture software support WDM cameras includes AstroCam series telescope camera. -
Registax
A popular free planetary stacking and processing software. -
AstroStack
Aplanetary stacking and process software. -
DeepSky Stacker
A free deep sky image stack and process software.
FAQ
IMX410 sensor might display image with uneven shading, which is decreasing
horizontally. According to Sony, IMX410 sensor allows Horizontal Dark Shading
smaller than 4.5 LSB. There are 3 possible reasons behind this characteristic.
First, due to the full frame size of the sensor, the internal circuit logic is
more complicated, which makes much more difficult to supply identical power.
In this case, due to the large size of full frame, Sony, after evaluation,
determined this specification within the range of 4.5 LSB, which does not
affect the image quality, so that the yield rate of this sensor and mass
production on the assembly line could be guaranteed.
Second, due to the limitation of semiconductor manufacturing equipment, sensor
with frame size larger than APS will be divided in to 2 or more parts in order
to receive exposure process. This will inevitably cause a segment gap at the
stitch position of 2 different exposure parts, and it is the main reason that
large frame sensor’s horizontal dark shading is more obvious.
Third, due to the different batches of mass production, although the sensors’
specifications are all within the predetermined range, products of different
batches will have different deviation.
Seivice
For software upgrades, please refer to “Download” on our official website:
https://ToupTek-astro.com/
For customers who purchase the cameras from local dealer, please contact your
dealer for more inquiry. For technical support, please contact e-mail address:
astro@ToupTek.com
References
- Download Center
- ToupTek | Astronomical camera | Astronomy camera
- VB Shop
- ASCOM - Standards for Astronomy
- astrogeeks.com/Bliss/MetaGuide/
- ToupTek | Astronomical camera | Astronomy camera
- ToupTek | Astronomical camera | Astronomy camera
- ToupTek Astro: Electric filter wheel & Astronomical Cameras | Pro Astrophotography Equipment
Read User Manual Online (PDF format)
Read User Manual Online (PDF format) >>