With the advantage of low readout noise and high-speed readout, CMOS technology has revolutionized astronomical imaging. A monochrome, back-illuminated, high-sensitivity, astronomical imaging camera is the ideal choice for astro-imagers. The QHY600 Series uses SONY IMX455, a BSI full frame (35mm format) sensor with 3.76um pixels and native 16-bit A/D.

QHY600PH Series

Model	Retail Price (USD)*	Year-End Sale Price (USD)*
QHY600PH-M	4,599	3,909
QHY600PH-C	4,599	3,909
QHY600PH-M SBFL	4,599	3,909
QHY600PH-C SBFL	4,499	3,909

*Price shall be slightly different among countries and regions; Shipment expenses, customs or other taxes are not included.

Overview

With the advantage of low readout noise and high-speed readout, CMOS technology has revolutionized astronomical imaging. A monochrome, back-illuminated, high-sensitivity, astronomical imaging camera is the ideal choice for astro-imagers. The QHY600 Series uses SONY IMX455, a BSI full frame (35mm format) sensor with 3.76um pixels and native 16-bit A/D. This sensor is available in both monochrome and color versions. The QHY600 Series ends the days of non-16bit cooling CMOS cameras and it ends the days non-full frame (and larger) monochrome cooling CMOS cameras.

Extremely low dark current (0.002e/p/s@-20C) using SONY’s Exmor BSI CMOS technology.
Zero amplifer glow.
Only one electron of read noise at high gain and full resolution and 4FPS readout speed. One electron of read noise means the camera can achieve a SNR>3 at only 4 to 6 photons. This is perfect performance when conditions are photon limited, i.e., short exposures, narrow band imaging, etc., making this large area sensor ideal for sky surveys, time domain astronomy, fluorescence imaging, DNA sequencing and microscopy.

In order to provide smooth uninterrupted data transfer of the entire 60MP sensor at high speed, the QHY600 Series (except QHY600M-PH L) have 2GB DDR3 image buffer. The pixel count of the latest generation of CMOS sensors is very high resulting in greater memory requirements for temporary and permanent storage. When using some computers that do not have fast processors or have poor support for USB 3.0, the computer can’t transfer high-speed data well, and the data is often lost. The DDR can buffer a lot of image data and send it to the computer. Even if the USB 3.0 transmission frequently gets suspended, it will ensure that data is not lost.

For example, the QHY600 sensor produces about 120MB of data per frame. The data band-width is also increased from the original 16-bits to the current 32-bits. Transferring such a large file sizes necessarily requires the camera to have sufficient memory. This large image buffer meets the needs of high-speed image acquisition and transmission of the new generation of CMOS, making shooting of multiple frames smoother and less stuttered, further reducing the pressure on the computer CPU.

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.

QHY600Series Naming Rules and Introduction

QHY600 Naming Rules

PH–Photographic Grade. Mainly for astrographers.

Pro–Scientific Grade. Mainly for scientific instituations. Since 2023, the Pro series have been devided to Pro I and Pro II series, the original “Pro” models will be replaced by “Pro I” models.

Pro I–Upgraded from the previous Pro series, it has 2*10G fiber interface with shorter body length.

Pro II–Based on Pro I models, it provides another two CameraLink interfaces.

M–Monochrome.

C–Colored.

L–Lite version is only available in PH Grade. Its body length becomes shorter and the built-in memory storage is 1GB instead of 2GB. Mono only.

SBFL–has a shorter back focal length.

LQ–supports liquid cooling.

Sensor Grade: All monochrome cameras (except the Lite version) are equipped with Industrial-Grade sensors, while the others are equipped with Consumer-Grade sensors.

	Grade	Body Length	Back Focal Length	Cooling Method	Buffer	2*10g	CameraLink	Note
QHY600PH L	Photographic	123mm	17.5+6mm（CAA）	Air Cooling	1GB DDR3	–	–
QHY600PH	Photographic	142mm	17.5+6mm（CAA）	Air Cooling	2GB DDR3	–	–
QHY600PH SBFL	Photographic	138mm	14.5mm	Air Cooling	2GB DDR3	–	–
QHY600PH EB	Photographic	185mm	17.5+6mm（CAA）	Air Cooling	2GB DDR3	–	–	Discontinued
QHY600Pro	Scientific	185mm	17.5+6mm（CAA）	Air Cooling	2GB DDR3	Yes	–	Replaced by Pro I
QHY600Pro SBFL	Scientific	181mm	14.5mm	Air Cooling	2GB DDR3	Yes	–	Replaced by Pro I
QHY600Pro LQ	Scientific	185mm	17.5+6mm（CAA）	Liquid Cooling	2GB DDR3	Yes	–	Replaced by Pro I
QHY600Pro SBFL LQ	Scientific	181mm	14.5mm	Liquid Cooling	2GB DDR3	Yes	–	Replaced by Pro I
QHY600Pro I	Scientific	142mm	17.5+6mm（CAA）	Air Cooling	2GB DDR3	Yes	–
QHY600Pro I LQ	Scientific	142mm	17.5+6mm（CAA）	Liquid Cooling	2GB DDR3	Yes	–
QHY600Pro I SBFL	Scientific	138mm	14.5mm	Air Cooling	2GB DDR3	Yes	–
QHY600Pro I SBFL LQ	Scientific	138mm	14.5mm	Liquid Cooling	2GB DDR3	Yes	–
QHY600Pro II	Scientific	142mm	17.5+6mm（CAA）	Air Cooling	2GB DDR3	Yes	Yes
QHY600Pro II LQ	Scientific	142mm	17.5+6mm（CAA）	Liquid Cooling	2GB DDR3	Yes	Yes
QHY600Pro II SBFL	Scientific	138mm	14.5mm	Air Cooling	2GB DDR3	Yes	Yes
QHY600Pro II SBFL LQ	Scientific	138mm	14.5mm	Liquid Cooling	2GB DDR3	Yes	Yes

Introduction of "SBFL" Version

SBFL (Short back-focal length version) models are specially designed for DSLR lens users or those who has special requirment of short back focal length. This version has a special front part version which has 14.5mm B.F.L only (The B.F.L consumed equals 12.5mm when connecting QHYCFW. About the defination of “BFL Comsumed” and our adapter system please view: https://www.qhyccd.com/astronomical-camera-adapter-bfl-solution/). A model with “SBFL” suffix can easily match Canon/Nikon lens even with filter wheel. On the side of this adapter there is a 4mm hole to connect air pump through plastic pipe in case of the dewing glass when necessary.

Introduction of "LQ" Version

A model with “LQ” suffix supports Liqiud cooling. Since LQ models need customization, please contact the QHYCCD sales department. Compared to air cooling, liquid cooling offers the following advantages:

More efficient cooling. When using ambient temperature pure water for water cooling, the maximum cooling temperature is about 10 degrees Celsius lower than that of air cooling. QHYCCD is improving its support for ultra-low temperature liquid cooling.

No vibration. No matter how high-quality the fan is, it is inevitable to generate some image jitter. The water-cooling version does not have moving mechanical parts that cause camera vibration, thus avoiding negative effects on the image.

No turbulent hot air. For certain cameras that need to be installed in front of the optical system, such as Schmidt-Cassegrain telescopes, the hot air generated by air cooling systems may cause slight interference with the optical path. Water cooling does not produce this kind of impact.

Advanced Functions

Multiple Readout Modes

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.

Random change thermal noise suppression function

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 Protection

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.

Optimizing USB Traffic to Minimize Horizontal Banding

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.

Reboot the camera by power off and on

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.

User Images

Captured by QHYCCD Astronomy Camera — Contrasted and colorful M78 area Photographer: Patrick Dufour Imaging telescopes or lenses: AG Optical 12.5″ iHW Imaging cameras: QHYCCD QHY600 Mounts: iOptron CEM120 EC2 Integration: 33.3 hours

Specifications

Model	QHY600PH (Photographic Ver.) QHY600PH SBFL (Short Back Focal Length Ver.)
CMOS Sensor	SONY IMX455
Mono/Color	Both Available
FSI/BSI	BSI
Pixel Size	3.76um x 3.76um
Effective Pixel Area	95766388（96006422 with overscan and optically black area)
Effective Pixels	61.17Megapixels
Sensor Size	Full Frame (36mm x 24mm)
A/D Sample Depth	Native 16-bit (0-65535 greyscale) A/D
Full Well Capacity (1×1, 2×2, 3×3)	Standard Mode >51ke- / >204ke- / >408ke- Super Full Well Mode >80ke- / >320ke- / >720ke-
Frame Rate	Full Resolution: 4.0FPS (8-bit output) ; 2.5FPS (16-bit output) ROI: 7.2FPS@9600×3194, 22.5FPS@9600×1080, 28FPS@9600×768, 47FPS@9600×480, 160FPS@9600×100
Readout Noise	1.0e- to 3.7e- (Standard Mode)
Dark Current	0.0022e-/p/s @ -20℃ 0.0046e-/p/s @ -10℃
Exposure Time Range	40us – 3600sec
Unity Gain*	25 (PH Mode, or Extended Full Well Mode) 56 (High Gain Mode) *Learn more at the introduction of “Readout Modes”.
Amp Control	Zero Amplifer Glow
Firmware/FPGA remote Upgrade	Support via Camera USB port
Shutter Type	Electric Rolling Shutter
Computer Interface	USB3.0
Built-in Image Buffer	2GB DDR3 Memory
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℃）
Optic Window Type	AR+AR High Quality Multi-Layer Anti-Reflection Coating
Anti-Dew Heater	Yes
Telescope Interface	Support M54 or M48 (Combined with adapters )
Back Focal Length	QHY600PH: 17.5mm+6mm (CAA) QHY600SBFL: 14.5mm（±0.2） *Learm more: https://www.qhyccd.com/adapters/
Weigth	About 850g

Linearity Test

We did a test for the QHY600 under the ultra high fullwell mode. The results is quite good to show a good linearity response range up to 73ke-. The results can be found here:

https://www.qhyccd.com/qhy600-linearity-test/

QHY600 linear test results show good linearity up to 73000e-. This is in readout modes # 0 and # 2. Gain = 0. In the linear fit graph we deleted the data above 73000e- and got R ^ 2 = 0.9998.

At very short exposure times below 20ms the value is quite small and may be flicker induced by the tablet.

Mechanical Dimensions

QHY600 PH

QHY600PH-SBFL

Image Area Layout

The QHY600 can output the whole active area of the sensor, including the optically black pixels and the overscan area. The total image size including the optically black area area is 9600 x 6422 pixels. The optically black area is on the left of the image and the overscan area is on bottom of the image.

The difference of optically black area and overscan area is that the optically black area includes the dark current during a long exposure while the overscan area does not include the dark current during an exposure. Neither the optically black area nor the overscan area respond to light, so they are regarded as the “non-effective” area of the sensor.

In the bottom of the overscan area you may find some vertical series of dots in single frame that can become vertical lines after stacking. One of the reasons for this is that the FPN calibration results represented in the overscan area can’t be found in the effective image area.

The following picture is the left bottom corner of a 300 second dark image. You can see these dots in the overscan area. The optically black level area and overscan area are usually used for precise calibration of an image and for calibration of an image without using a bias frame or dark frame, or for some scientific applications. Because the optically black and overscan areas are not part of the effective image area, QHYCCD does not guarantee the signal quality in these areas. If you do not use these areas, you can select the option “Ignore overscan area” in the ASCOM driver or select a ROI of effective area in SharpCAP.

Multiple Readout Modes and Curves

Readout Mode #0 (Photographic Mode)

Readout Mode #1 (High Gain Mode)

Readout Mode #2 (Super Fullwell Mode)

Readout Mode #3 (Extend Fullwell Mode-2CMS)

The curve shows absolute QE

Multiple Readout Modes are special for QHY 16-bit Cameras (QHY600/268/461/411). Different readout modes result in different performance. These readout modes are currently supported in the ASCOM, SharpCap and N.I.N.A.

Photographic DSO Mode (Mode #0)

This mode is suitable for most DSO imaging situations. Since there is a drop in the noise between Gain 25 and Gain 26 (unity gain), we recommend it as default gain setting; however, gain0 is also good enough for a 16-bit sensor.

High Gain Mode (Mode #1)

This mode is something like double native iso of some new digital cameras, whose danamic range can greatly incerase at the vary high iso value, like iso800, iso3200, etc. The high gain mode provide such improvement for QHYCCD 16bit cameras. We recommend you choose this mode when you have to capture at high gain, for example, a vary dark object. Please note the switch point of HGC/LGC of QHY600/268/461 is 56. That means you must set Gain 56 to make the best of it.

Extended Fullwell Mode (Mode#2)

With a pixel size of 3.76um, these sensors already have an impressive full well capacity of 51ke. Nevertheless, QHYCCD has implemented a unique approach to achieve a full well capacity higher than 51ke- through innovative user controllable read mode settings. In Extended Fullwell Mode, the QHY600 can achieve an extremely large full-well charge value of nearly 80ke- and the QHY268 can achieve nearly 75ke-. Greater full-well capacity provides greater dynamic range and large variations in magnitude of brightness are less likely to saturate.

2CMS Modes

Extended Fullwell Mode-2CMS (Mode#3)

Photographic DSO Mode-2CMS (Mode#4)

High Gain Mode-2CMS (Mode#5)

Based on the three basic modes above, 2CMS mode can greatly reduce readout noise by secondary sampling while keeping the same full well value and system gain. We prefer 2CMS modes than basic modes in astrophotography. By the way, the recommend gain values are the same as their basic modes.

Accessories (What's in the box)

Name	Amount
Camera	1
Locking Power Cable	1
USB3.0 Cable	1
12V Power Adapter	1
AV Power Cable	1
Desiccaant Tube	1
M54 to 2” Nosepiece	1
Adapter Kit Instrustion	1
Drive Download Instruction	1
Adapter Kit	C1 (QHY600M-PH) D1 (QHY600C-PH) B1 (QHY600M-PH SBFL)

Combos & Adapters

QHY600M-PH+CFW3L+(OAGM)

Since June 2023, we are adding a 5mm spacer with M54 threads into Adapter kit C1. This addition gives the user a choice of terminating the output in either M48 or M54 threads. Since C1 are standard accessories included with the camera, this addition has no affect on the price list.

Note:

Combo C1 is the solution without OAG. The QHY600M-PH or QHY600M-L with CFW3L and OAG result in a backfocus greater than 55mm. Therefore, if you must limit this BF distance to 55mm due to a corrector lens or DSLR lens, we recommend the QHY600M-PH SBFL.

If you need more than 7 x 50mm filter positions for the QHY600, you can use the CFW3XL filter wheel with 9 x 50mm filter carousel.

QHY600M-PH SBFL+CFW3L+(OAGM）

The New Combo B1 is designed to be more flexible to achieve multiple output specifications. Since June 2023, we are adding a 5mm spacer with M54 threads into Adapter kit B1. This addition gives the user a choice of terminating the output in either M48 or M54 threads. You can get 55/56mm BFL with M48/M54 threads according to your needs. Since are standard accessories included with the camera, this addition has no affect on the price. 55mm M48/M54 are suitable for standard flatteners and multiple purpose coma correctors (MPCC), while 56mm M54 threads are common for Takahashi reflectors.

Note: Please position the OAG as far forward as possible (for example, placing it under the M48 thread), and extend the OAG prism slightly outward to ensure simultaneous focus for both the main camera and the guiding camera.

In 2023, we launched the new version of the QHYOAGM-Pro with a larger prism. Its thickness is 12mm, so it is necessary to reduce the spacer thickness by 2mm in the COMBO above while keeping the rest part unchanged.

The QHY600M-PH SBFL and QHY268M with CFW3L filter wheel can fit an optional Canon EF or Nikon F Lens Adapter without additional spacers. Smaller filter wheels may require additional spacers.

User Guide: How to Start the Camera

Install “All-In-One” Driver&SDK Pack

Before Start: Input Voltage Requirements

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.

Install "All-In-One" System Pack

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

Since most of the contents of All-in-one package are plug-ins that support third-party software, the third-party capturing software that you want to use must be installed before the All-in-one package. Otherwise the program will report an error.
ALL-IN-ONE Pack contains:
- System Driver, which is necessary for the camera operation and must be installed.
- WDM Broadcast Driver, which can provide a live signal to Obs and other live software, you can install it if you have such needs like opeing a live show.
- EZCAP_QT , which is developed by QHYCCD and can be used in QHY devices tests, and management of updates. So even if you won’t use EZCAP_QT for capturing, we suggest you install it.
- Ascom driver, which is necessary for the camera used in Ascom (the latest version of Ascom is 6.6).
- The two sorts of Ascom CFW Drivers correspond to two methods of controling the filter wheel: USB control and camera serial control. It is recommended that both drivers should be installed if you have a filter wheel.
- CP210X_VCP is a serial driver. Some computers come with the driver, but the computer without the driver may be failed of controling the filter wheel.
- SDKs for Third-party Software: Just pick and install the corresponding SDK according to the software you want to use. Don’t forget to check whether the software you are using is 32-bit or 64-bit and select the right SDKs.
- SHARPCAP is also included in the pack, you can choose 32-bit or 64-bit to install. This is authorized by SHARPCAP.
- QT LIB is a plug-in to ensure that 64-bit software can exeuate normally on some computers with poor compatibility.
Difference between Stable version and Beta Version: Beta version is the latest version, which gives priority to support for the latest products (the stable version may not be compatible with those yet), and has some of the latest optimized ,but experimental features. The stable version is older than the beta version but more stable, so it is recommended for beginners who are not using the latest products.
Don’t let the camera connect to the computer during the All-in-one pack installation process; connect it to the computer after all the installation is complete.

Connect DSO Imaging Software (e.g. NINA)

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.

Connect Planetary Imaging Software (e.g. SharpCap)

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.

User Guide: How to Set Gain and Offset

Unity Gain of Some 16bit Models

Model	Unity Gain
QHY600M/C	25
QHY268M/C	30
QHY461PH	26

Now with the improvement of the CMOS technology, the 16bit CMOS cameras like QHY600/268/411/461, can be directly set gain 0 under default Photographic DSO mode. Even in lowest gain（zero） they’re beyond the requirement (less than 1e/ADU due to sufficient samples).

However, when you use QHY600/268/411/461 under Extended Fullwell Mode, we recommend their unit gain as default.

OFFSET Setting

There is no fixed “best value” for OFFSET. To set OFFSET, you should take the bias frame and dark frame at a certain GAIN value, then check the histogram of the frames.

The histogram distribution is a peak-like curve. While changing the OFFSET value, the histogram will move left or right. We need to guarantee the range of the whole curve won’t be chopped off at the end. At the same time, we need to keep a little residue on the left side, just over 0 a bit.

Pay attention that under different GAIN values, the width of this peak varies. The higher the GAIN is, the wider the distribution will be. So OFFSET value at low GAIN is not suitable for high GAIN because the curve is easily to be chopped off.

Camera Maintenance

Drying the camera CMOS chamber

There are holes in the two sides of the camera near the front plate that is normally plugged by a screw with an o-ring. If there’s moisture in the CMOS chamber that causes fog, you can connect the desiccant tube to this hole for drying. There would better be some cotton inside to prevent the desiccants from entering the CMOS chamber.Please note that you may need to prepare desiccants yourself, because for most countries and regions desiccants are prohibited by air transport. Since QHY always deliver your goods by air, sorry that we can’t provide desiccants for you directly.
Cyclic Drying: The front end of the camera body is equipped with two drying interfaces with M5 threads, which are used in conjunction with drying tubes and circulation pumps for drying treatment inside the sensor chamber. The position of the drying interface is indicated by the red circle in the figure below (take the QHY600 as an example):Under the vacuum pump, the gas inside the sensor chamber is drawn out through one drying interface, enters the drying tube, and then undergoes filtration. It is then reintroduced into the camera through the other drying interface, circulating back and forth for drying.
Note:1.Do not reverse the order of the intake and exhaust ports

2.Before circulating drying, it is necessary to turn off the refrigerator, and then turn on circulating drying after the temperature returns to normal temperature. Only by following this step can the water vapor in the sealed chamber be effectively removed. If the cooler is turned on, the cooler inside the camera will absorb water vapor, causing more water vapor to condense inside the camera instead of being absorbed by the desiccant.

Cleaning the CMOS sensor and optical window

If you find dust on the CMOS sensor, you can first unscrew the front plate of the cam and then clean the CMOS sensor with a cleaning kit for SLR camera sensors. Because the CMOS sensor has an AR (or AR/IR) coating, you need to be careful when cleaning. This coating can scratch easily so you should not use excessive force when cleaning dust from its surface.

Preventing fogging of the CMOS chamber

All QHY cooling cameras have built-in heating plates to prevent fogging. However, If the ambient humidity is very high, the optical window of the CMOS chamber may have condensation issues. Then try the following:

1. Avoid directing the camera towards the ground. The density of cold air is greater than of hot air. If the camera is facing down, cold air will be more accessible to the glass, causing it to cool down and fog.

2. Slightly increase the temperature of the CMOS sensor .

3. Check if the heating plate is normally working. If the heating plate is not working, the glass will be very easy to fog, the temperature of the heating plate can reach 65-70 °C in the environment of 25 °C. If it does not reach this, the heating plate may be damaged. Please contact us for maintenance.

TE Cooler Maintenance

Please avoid thermal shock during use. Thermal shock refers to the internal stress that the TE cooler has to withstand due to the thermal expansion and contraction when the temperature of the TEC suddenly rises or falls. Thermal shock may shorten the life of the TEC or even damage it.

Therefore, when you start using the TEC to adjust the CMOS temperature, you should gradually increase the TEC power rather than turning the TEC to maximum power. If the power of the TEC is high before disconnecting the power supply, you should also gradually reduce the power of the TEC and then disconnect the power supply.

Others

Technical Support

You can login QHYCCD Help Center for any technical support.

Submit a Ticket: Describe the issue you met while you’re using them. Our technicans will reply you in 48 hours during working days. You don’t have to check the Ticket update everyday—they can receive email notifications and know if there’s any update.

Knowledge Base: Here lists some tips for using your gears, or solutions to issues that you may met. Help your self!

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Warranty

Warranty Policy Updated in 2023 (pdf)

Return & Pepair Policy Updated in 2023 (pdf)

Cooled CMOS Camera	Bayer
QHY600C/QHY268C/QHY410C/ QHY367Pro/QHY128Pro/QHY294C/ QHY247C/QHY168C/QHY165C/QHY183C/QHY174C	RGGB
QHY533C/QHY178C/QHY290C/QHY224C	GBRG
QHY163C	GRBG
QHY1920C	BGGR

Cooled CCD Camera
QHY8L-C	GBRG
QHY10-C	RGGB
QHY12-C	BGGR

Planetary and Guiding
QHY5III174C	RGGB
QHY5III178C	GBRG
QHY5III224C	GBRG
QHY5III290C	GBRG
QHY5III462C	GBRG
QHY5III485C	RGGB
QHY5L-II-C	GRBG
QHY5P-II-C	GBRG
QHY5III585C	RGGB
QHY5III678C	RGGB
QHY5III715C	GBRG
QHY5III568C	RGGB

C/2023 A3 (Tsuchinshan–ATLAS)

Astrophotographer
Daniel Nimmervoll (Austria)

QHY600PH Series

Topic DOWNLOAD PDF

QHYCCD

C/2023 A3 (Tsuchinshan–ATLAS)

Astrophotographer Daniel Nimmervoll (Austria)

QHY600PH Series

Related Products

Topic DOWNLOAD PDF

QHYCCD

Astrophotographer
Daniel Nimmervoll (Austria)