DISCOVER NEW HORIZONS
Telescope: Takahashi FSQ-106EDX4
Mount: Astro-Physics Mach1 GTO
Frames:
Chroma Blue 50 mm: 21×205″(1h 11′ 45″)
Chroma Green 50 mm: 22×150″(55′)
Chroma Lum 50 mm: 463×45″(5h 47′ 15″)
Chroma Red 50 mm: 24×130″(52′)
Integration: 8h 46′
QHY411 Pro has 150 megapixels, with 54*40mm sensor size, while QHY461 Pro has 100 megapixels and 44*33mm sensor size. The features of their sensors are similar, back-illuminated, native 16bit A/D, medium format. Both QHY411 Pro and QHY461 Pro have 2*10GigaE interfaces and support higher readout speed. Mono and color version are both available. The applications include astronomy imaging, astronomy photography, space object survey, satellite tracking, etc.
*Please contact QHYCCD about the price.
Benefiting from its back-illuminated pixel structure, the QHY411 has a large full well of 80ke-. And when using 2 * 2 binning, the full well can reach 320ke-, corresponding to a merged pixel size of 7.5um * 7.5um. Combined with the low readout noise, the camera has a large dynamic range advantage.
Updated: now QHY411 supports 3*3 onchip binning. Learn more at “QHY411 3*3 Onchip Binning 12bit （high frame rate）Mode Instructions” part.
Native 16 bit A/D: The new Sony sensor has native 16-bit A/D on-chip. The output is real 16-bits with 65536 levels. Compared to 12-bit and 14-bit A/D, a 16-bit A/D yields higher sample resolution and the system gain will be less than 1e-/ADU with no sample error noise and very low read noise.
BSI: One benefit of the back-illuminated CMOS structure is improved full well capacity. In the back- illuminated sensor the light is allowed to enter the photosensitive surface from the reverse side. In this case the sensor’s embedded wiring structure is below the photosensitive layer. As a result, more incoming photons strike the photosensitive layer and more electrons are generated and captured in the pixel well. This ratio of photon to electron production is called quantum efficiency. The higher the quantum efficiency the more efficient the sensor is at converting photons to electrons and hence the more sensitive the sensor is to capturing an image of something dim.
TRUE RAW Data: In the DSLR implementation there is a RAW image output, but typically it is not completely RAW. Some evidence of noise reduction and hot pixel removal is still visible on close inspection. This can have a negative effect on the image for astronomy such as the “star eater” effect. However, QHY Cameras offer TRUE RAW IMAGE OUTPUT and produces an image comprised of the original signal only, thereby maintaining the maximum flexibility for post-acquisition astronomical image processing programs and other scientific imaging applications.
Zero Amplify Glow: This is also a zero amplifer glow camera.
Cooling & Anti-dew Control: In addition to dual stage TE cooling, QHYCCD implements proprietary technology in hardware to control the dark current noise. The optic window has built-in dew heater and the chamber is protected from internal humidity condensation. An electric heating board for the chamber window can prevent the formation of dew.
Sealing Technology: Based on almost 20-year cooled camera design experience, The QHY cooled camera has implemented the sealing control solutions. The sensor itself is kept dry with our silicon gel tube socket design for control of humidity within the sensor chamber. By the way, there’s no oil leaking.
Multiple Readout Modes are special for QHY 16-bit Cameras (QHY600/268/461/411). Different readout modes have different driver timing, etc., and result in different performance. See details at “Multiple Readout Modes and Curves” Part.
You may find some types of thermal noise can change with time in some back-illuminated CMOS cameras. This thermal noises has the characteristic of the fixed position of typical thermal noise, but the value is not related to the exposure time. Instead, each frame appears to have its own characteristics. The QHY600/268/461/411 use an innovative suppression technology that can significantly reduce the apparent level of such noise.
UVLO（Under Voltage Locking) is to protect the electronic device from damage caused by abnormally low voltages.
Our daily life experience tells us that the actual operational voltage of an electrical device must not significantly exceed the rated voltage, otherwise it will be damaged. For such precision equipment as cameras, long-term work at too low input voltage can also be detrimental to the working life of the camera, and may even make some devices, such as power manager, burn up due to long-term overload. In the all-in-one driver and SDK after 2021.10.23 stable version, the camera will give a warning when the input voltage of the camera is below 11V.
It is common behavior for a CMOS sensor to contain some horizontal banding. Normally, random horizontal banding can be removed with multiple frame stacking so it does not affect the final image. However, periodic horizontal banding is not removed with stacking so it may appear in the final image. By adjust the USB traffic in Single Frame mode or Live Frame mode, you can adjust the frequency of the CMOS sensor driver and it can optimize the horizontal banding appeared on the image. This optimized is very effective to remove the periodic banding in some conditions.
A typical Periodic Horizontal Noise under certain USB_TRAFFIC values.
After Adjusting the USB Traffic to avoid the periodic horizontal noise.
The camera is designed to use the +12V to reboot the camera without disconnecting and reconnecting the USB interface. This means that you can reboot the camera simply by shutting down the +12V and then powering it back on. This feature is very handy for remote controlling the camera in an observatory. You can use a remotely controlled power supply to reboot the camera. There is no need to consider how to reconnect the USB in the case of remote control.
Now QHY411 supports onchip 3 * 3 binning. Compared with software binning of most software binning, onchip (hardware) binning can reach higher frame rates.
Since most software that provides continuous mode/video output, like SharpCap, only support 8-bit or 16-bit oupout, so you must select 8-bit output to achieve a frame rate boost.
Data comparison (USB3.0 full resolution)
1*1 bin: 8-bit, 2fps
3*3 Onchip Binning 12bit Mode: max 20fps
To get the update, you need the latest firmware and All-in-one Driver Pack.
Allinone Update: please refer to the description on the “Download” page of the website.
Firmware Update: Requires downloading firmware update kit 20220824 or later. If you have an old firmware upgrade tool locally, please discard it. The compressed package contains firmware upgrade tools, new QHY411 firmware and upgrade operation instructions. Please read the upgrade instructions in the firmware installation package carefully. If you encounter any problems during the upgrade, please contact us.
Firmware upgrade kit 20220824 download address:
Firmware upgrade instructions:
Refer to the compressed document or web version instructions
| Model | QHY411 Pro | QHY461 Pro |
| Image Sensor | Sony IMX411 | Sony IMX461 |
| Sensor Type | Both Available | Both Available |
| FSI/BSI | BSI | BSI |
| Pixel Size | 3.76μm*3.76μm | 3.76μm*3.76μm |
| Effective Pixels | 151 Megapixels | 102 Megapixels |
| Effective Image Area | Typical 4.2inch (54mm*40mm) | Typical 3.4inch (44mm*33mm) |
| Effective Pixel Area | 14208*10656 | 11664*8748 |
| Total Pixel | 14304*10748 (include optical black area and overscan area) | 11760*8842 (include optical black area and overscan area) |
| A/D | Native 16-bit (0-65535 greyscale) A/D | Native 16-bit (0-65535 greyscale) A/D |
| Full Well Capacity (1×1, 2×2, 3×3)
|
Standard Mode
50ke- / 200ke- / 450ke- Extended Fullwell Mode 80ke- / 320ke- / 720ke- |
Standard Mode
50ke- / 200ke- / 450ke- Extended Fullwell Mode 80ke- / 320ke- / 720ke- |
| Read Noise | 1e- to 3e- (HGC Mode) | 1e- to 3e- (HGC Mode) |
| Dark Current | Apporx 0.0011e-/pixel/sec @-20℃ | Approx 0.003e-/pixel/sec @-20℃ |
| Exposure Time Range | 20μs – 3600sec | 50μs – 3600sec |
| Shutter Type | Electronic Rolling Shutter | Electronic Rolling Shutter |
| Computer Interface | USB3.0
2*10Gigabit Fiber |
USB3.0
2*10Gigabit Fiber |
| Filter Wheel Interface
|
4PIN QHYCCD CFW Port | 4PIN QHYCCD CFW Port |
| Trigger Port | Programmable TrigOut, High Speed Sync Port / GPS interface Port | Programmable TrigOut, High Speed Sync Port / GPS interface Port |
| Full Frame Rates | USB3.0:
2.1FPS@8bit 1.0FPS@16bit
PCIE Mode: 2.1FPS@8bit 1.0FPS@16bit |
USB3.0:
2.7FPS@8bit 1.7FPS@16bit
PCIE Mode: 3.0FPS@8bit 2.0FPS@16bit |
| ROI Frame Rates
|
USB3.0:
2048lines, 10.2FPS@8bit, 5.1FPS@16bit 1080lines, 18.5FPS@8bit, 9.8FPS@16bit 768lines, 25.3FPS@8bit, 12.9FPS@16bit 480lines, 36.6FPS@8bit, 19.2FPS@16bit
3×3 Onchip Binning 12bit: 3548lines, 20.2FPS@8bit, 10.1FPS@16bit 1080lines, 62.6FPS@8bit, 32.8FPS@16bit 768lines, 84.8FPS@8bit, 43.2FPS@16bit 480lines, 131FPS@8bit, 68.8FPS@16bit
PCIE Mode: 2048lines, 10.2FPS@8bit, 5.1FPS@16bit 1080lines, 18.5FPS@8bit, 9.8FPS@16bit 768lines, 25.3FPS@8bit, 12.9FPS@16bit 480lines, 36.6FPS@8bit, 19.2FPS@16bit
PCIE 3×3 Onchip Binning 12bit: 3548lines, 20.2FPS@8bit, 12.6FPS@16bit 1080lines, 62.6FPS@8bit, 43.6FPS@16bit 768lines, 84.8FPS@8bit, 43.2FPS@16bit 480lines, 131FPS@8bit, 102FPS@16bit |
USB3.0:
2048lines, 10.8FPS@8bit, 6.1FPS@16bit 1080lines, 19.5FPS@8bit, 10.8FPS@16bit 768lines, 26.1FPS@8bit, 14.7FPS@16bit 480lines, 37.1FPS@8bit, 20.5FPS@16bit
PCIE Mode: 2048lines, 10.9FPS@8bit, 9.2FPS@16bit 1080lines, 19.7FPS@8bit, 18.6FPS@16bit 768lines, 25.8FPS@8bit, 24.6FPS@16bit 480lines, 36.6FPS@8bit, 35.5FPS@16bit |
| Built-in Image Buffer | 2GB DDR3 Memory Buffer | 2GB DDR3 Memory Buffer |
| Air Cooling System | Dual Stage TEC cooler:
– Long exposures (> 1 second) Typically -35℃ below ambient – Short exposure (< 1second) high FPS, Typically -30℃ below ambient（Test temperature +20℃） |
Dual Stage TEC cooler:
– Long exposures (> 1 second) Typically -35℃ below ambient – Short exposure (< 1second) high FPS, Typically -30℃ below ambient（Test temperature +20℃） |
| Liquid Cooling | Available.
-45℃ below ambient with water cooling; more deltaT below ambient with cold liquid. |
Available.
-45℃ below ambient with water cooling; more deltaT below ambient with cold liquid. |
| Recommended Flow Rates | 12ml/s | 12ml/s |
| Anti-Dew Heater | Available | Available |
| Humidity Sensor | Available | Available |
| Firmware/FPGA remote Upgrade | Available via Camera USB port | Available via Camera USB port
|
| Optic Window Type | AR+AR High Quality Multi-Layer Anti-Reflection Coating | AR+AR High Quality Multi-Layer Anti-Reflection Coating |
| Back Focal Length | 16mm(without tilt adjust ring)
28.5mm (with tilt adjust ring) |
16mm (without tilt adjust ring）
28.5mm (with tilt adjust ring) |
| Adapters | Customization | Customization |
| Weight | 2.9kg | 2.9kg |
| Power | 49.2W/100%
28.9W/50% 17.3W/0% |
49.2W/100%
28.8W/50% 16.8W/0% |
QHY411 QE. Since SONY has not release the absolutely QE curve of IMX411. There is only the relativity QE Curve. QHYCCD did some test of absolutely QE for the 3.76um BSI sensor in another model. It can be used for just a reference. This article can be found in https://www.qhyccd.com/index.php?m=content&c=index&a=show&catid=23&id=261
Fireworks Galaxy
Image credit and copyright: Denis Salnikov
https://www.astrobin.com/4arko5/
Telescope: AG Optical iDK 14.5 inch F6.7
Camera: QHY461
Mount: Paramount Taurus 400
Filters: Astrodon Gen2 E-Series Tru-Balance Blue 50×50 mm · Astrodon Gen2 E-Series Tru-Balance Green 50×50 mm · Astrodon Gen2 E-Series Tru-Balance Lum 50×50 mm · Astrodon Gen2 E-Series Tru-Balance Red 50×50 mm · Astrodon H-alpha 3nm 50×50 mm
Integration: 118h 53′ 20″
IC 1396 Elephant’s Trunk Nebula in Bi-Color palette
Image credit and copyright: Denis Salnikov
https://www.astrobin.com/x51ogf/0/
Telescope: AG Optical iDK 14.5 inch F6.7
Camera: QHY461
Mount: Paramount Taurus 400
Filters: Astrodon OIII 3nm 50mm · Astrodon Ha 3nm 50mm
Integration: 12h 30′
Some scholars in Italy found secrets hidden in ancient manuscripts with the QHY411 camera.
StarDICE I: sensor calibration bench and absolute photometric calibration of a Sony IMX411 sensor, a paper about QHY411 camera was published in the Astronomy & Astrophysics.
https://arxiv.org/pdf/2211.04913.pdf
A new paper named Scientific CMOS Sensors in Astronomy: QHY600 and QHY411 has been published! It was finished by researchers from the Institute of Astrophysics of Canarias (IAC), Spain.
https://arxiv.org/abs/2302.03700
A new paper A Shock Flash Breaking out of a Dusty Red Supergiant by researchers from Tsinghua University, PMO, Tel Aviv University, NAOC, and UC Berkeley has been published in Nature. An Antarctic Survey Telescope (AST3)-3 equipped with a QHY411 camera at the Yaoan station of Purple Mountain Observatory, China was involved in this observation and provided important data.
https://www.nature.com/articles/s41586-023-06843-6
https://arxiv.org/abs/2311.14409
The camera requires an input voltage between 11V and 13.8V. If the input voltage is too low the camera will stop functioning or it may reboot when the TEC power percent is high, causing a drain on the power. Therefore, please make sure the input voltage arrived to the camera is adequate. 12V is the best but please note that a 12V cable that is very long or a cable with small conductor wire may exhibit enough resistance to cause a voltage drop between the power supply and the camera. The formular is: V(drop) = I * R (cable). It is advised that a very long 12V power cable not be used. It is better to place the 12V AC adapter closer to the camera.
First connect the 12V power supply, then connect the camera to your computer via the USB3.0 cable. Make sure the camera is plugged in before connecting the camera to the computer, otherwise the camera will not be recognized. When you connect the camera for the first time, the system discovers the new device and looks for drivers for it. You can skip the online search step by clicking “Skip obtaining the driver software from Windows Update” and the computer will automatically find the driver locally and install it. If we take the 5IIISeries driver as an example (shown below), after the driver software is successfully installed, you will see QHY5IIISeries_IO in the device manager.
Please note that the input voltage cannot be lower than 11.5v, otherwise the device will be unable to work normally.
All-in-one Pack supports most QHYCCD models only except PoleMaster and several discontinued CCD cameras.
Download Page: https://www.qhyccd.com/download/
Video Tutorial: https://www.youtube.com/embed/mZDxIK0GZRc?start=1
Before using software, make sure you have connected the cooling camera to the 12V power supply and connected it to the computer with a USB3.0 data cable. If it’s an uncooled camera, 12V power is not needed. We recommend 64-bit Software, like SharpCAP x64 , N.I.N.A x64. etc., especially when you’re using 16bit cameras.
In NINA, you can select the device to connect to QHY Camera directly without ASCOM driver.
If connecting to the camera via ASCOM is desired, first make sure you have installed both the QHYCCD ASCOM Drivers and ASCOM Platform. Then you would select the appropriate camera driver under the ASCOM section. Then click the Connect icon. Here we take NINA as an example, but it’s similar to other software packages supporting ASCOM, like MaxDL, The SkyX, etc.
Launch SharpCap. If the software and drivers mentioned above are installed successfully, the video image will appear automatically about 3 seconds after the software loads. You will also see the frame rate in the lower left corner of the software window as shown below.
If you have already started the SharpCap software before connecting the camera, in order to open the camera, click on the “camera” in the menu bar and then select the device.
Offset adjustment. When you completely block the camera (i.e., like taking a dark frame) you may find that the image is not really zero. Sometimes this will reduce the quality of the image contrast. You can get a better dark field by adjusting the offset. You can confirm this by opening the histogram as indicated in the figure below.
If you want to enter the 16-bit image mode, select the “RAW16” mode.
By selecting the “LX” mode you can expand the exposure setting range and take long exposures.
After cooling devices connected to the 12V power supply, the temperature control circuit will be activated. You can control the CMOS temperature by adjusting the settings in the figure below. Basically, you can control the temperature of CMOS by either adjusting “Cooler Power” or clicking “Auto” and setting “Target Temperature”. You can also see the CMOS temperature at the lower-left corner of the software window.
| mode 0 | mode 1 | mode 2 | mode 3 | mode 4 | mode5 | mode6 |
| GPIO1 | GPSBOX_Control | ShutterMessure+ | ShutterMessure+ | n.a | n.a | ShutterMessure+ |
| GPIO2 | GPSBOX_Data (IN） | TrigIn2 | ShutterMessure- | n.a | n.a | TrigIn2 |
| GPIO3 | GPSBOX_ShutterMessure | LinePeriod | n.a | HSYNC(OUT） | HSYNC（IN) | LinePeriod |
| GPIO4 | GPSBOX_CLK | TrigOut | n.a | VSYNC(OUT） | VSYNC(IN) | LED(OUTPUT) |
| GND | GND | GND | GND | GND | GND | GND |
UVLO（Under Voltage Locking), is primarily intended to protect the electronic device from damage caused by abnormally low voltages. Now only QHY600, QHY268, QHY410, QHY411, QHY461, QHY533 cameras have UVLO Protection.
UVLO warning execution
After a warning is given, the camera firmware will automatically turn off the cooler and will turn on the camera’s TEC protection mode. After the camera is reconnected, it will always work in TEC protection mode (maximum power cooler power will be limited to 70%). Since many times the voltage shortage is caused by the high resistance of the power supply cable itself, resulting in a large voltage drop at high currents, the voltage will usually rise after the power is limited. But limiting the power will affect the cooling temperature difference. Therefore, it is recommended that users first check the power supply cable to solve the problem of excessive resistance of the power supply cable.
If the user has solved the problem of insufficient supply voltage, the TEC protection mode can be removed through the menu of EZCAP_QT.
How to improve the power supply?
How to clear the TEC protection status triggered by UVLO?
Once a UVLO event occurs, the camera will automatically memorize it and will work in a protected mode at a maximum of 70% power after reconnection. This memory can be erased as follows:
After you find the system error, you need to turn off the device and check the power supply. After inspecting the problem, open the ezcap software and select “Camera Settings” – “Preferences” – “Reset Flash Code” to reset the error status.
Why does the warning appear even though the power supply voltage is 12 V?
Added functions related to BURST mode in SDK. Currently, cameras that support Burst function include QHY600, QHY411, QHY461, QHY268, QHY6060, QHY4040, QHY4040PRO, QHY2020, QHY42PRO, QHY183A
This mode is a sub-mode of continuous mode. This function can only be used in continuous mode. When this function is enabled, the camera will stop outputting image data, and the software frame rate will be reduced to 0. At this time, send relevant commands to the camera, and the camera will Output the image data with the specified frame number according to the settings, for example, set Start End to 1 6, the camera will output the image data with the frame number 2 3 4 5 when receiving the command.
Note:
1. When using Burst mode in fiber mode, the first Burst shot will be one less. For example, if the start end is set to 1 6, the output of 2 3 4 5 is normal, but in fact, only 3 4 will be output during the first burst shot. 5, 2 will not be received, the second and subsequent shots can normally obtain Burst images 2 3 4 5. This problem will be fixed later.
2. QHY2020, QHY4040 found that the frame number that came out when the exposure time was short is [start+1,end-1] but the one that came out under long exposure was [start+2,end]
3. When the camera is just connected, if the set end value is relatively large, the camera will directly output the picture after entering the burst mode. Therefore, it is necessary to set the camera to enter the IDLE state and then set the start end and related burst operations.
The following is the usage of Burst mode related functions:
The abnormally large thermal noise in the picture above is caused by the failure of the internal voltage to start after the camera is powered on. You can power on the camera again and take an image to see if it can be recovered.
If you encounter this problem during use, you can contact QHYCCD for hardware upgrade. This type of camera purchased before 2022.8.25 may have this problem.
