ATR585C User Manual

Version 1.1
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.

1 Description and Features

The ATR585C (ATR3CMOS08300KPA) camera is designed specifically for astrophotography. It is mainly used for deep sky photo shooting, as the camera has a cooled CMOS sensor, ultra-low readout noise, and zero amp-glow. It can also be used for planetary photo shooting. Its extraordinary performance and extensive usage will provide a great astrophotography experience.

The features of ATR585C are listed below:

  • IMX 585 Color CMOS Sensor
  • Resolution: 3840 x 2160
  • 2.9µm Square Pixel
  • 1/1.2-inch Optical Format
  • 12-bit ADC
  • 512 Mbyte Memory
  • Precise Temperature Regulation
  • G Sensitivity: 5970mv with 1/30s
  • Zero Amp-Glow
  • Low Noise: 0.46 to 5.18e⁻
  • Support High Frame Rate Mode (24 FPS at all Pixel Readout 12 bit)
  • SNR Max: 46 dB
  • Dynamic Range: 85.6 dB (HDR)
  • -35°C below ambient under short exposure / -45°C under long exposure time (> 1s)

Figure 1: IMX585 Image Sensor and its Pixel Structure

Diagram showing the IMX585 image sensor and its pixel structure. It indicates dimensions of 3840x2160 pixels and a pixel size of 2.9 µm. Color channels are labeled R (Red), Gr (Green), Gb (Green-blue), and B (Blue).

2 ATR585C Specifications and Performance

2.1 Camera Specifications

Table 1: ATR585C Technique Specifications

SensorSony IMX585 back illuminated sensor
Diagonal12.85 mm
Image Resolution8.3 mega pixels (3840*2160)
Pixel Size2.9µm × 2.9µm
Image Area11.2mm x 6.3mm
Max FPS at Resolution (USB 3.0)12bit: 24 FPS @ 3840*2160, 70 FPS @ 1920*1080
8bit: 47 FPS @ 3840*2160, 70 FPS @ 1920*1080
Max FPS at Resolution (USB 2.0)14bit: 1.9 FPS @ 3840*2160, 3.9 FPS @ 1920*1080
8bit: 3.8 FPS @ 3840*2160, 7.9 FPS @ 1920*1080
Shutter TypeRolling shutter
Exposure Time0.1ms - 3600s
Gain1x - 100x
SNR46 dB
Dynamic Range86.5 dB (HDR Mode)
Read Noise0.65 - 0.46 e⁻
QE Peak>91%
Full Well40ke⁻
ADC12bit (16bit @ HDR)
DDR3 Buffer512MB (4Gb)
Connection PortUSB3.0/USB2.0
Camera AdaptorM42 x 0.75mm
Protect WindowsIR-cut filter/AR-window
Spectral Range380-690nm (with IR-cut filter)
Capture/Control SDKWindows/Linux/macOS/Android Multiple Platform SDK (Native C/C++, C#/VB.NET, Python, Java, DirectShow, Twain, etc.)
Recording SystemStill picture and movie
Camera DimensionsDiameter 80mm * height 107.1mm
Camera Weight0.577kg
Back Focus Distance17.5mm
Cooling:Two stage TEC
Effective Cooling Temp:-35°C below ambient under short exposure / -45°C under long exposure (> 1s)
Supported OSMicrosoft® Windows® XP / Vista / 7 / 8 / 10 / 11 (32 & 64 bit)
OS x (Mac OS X)
Linux

2.2 Sony IMX585 Sensitivity

The sensor G Sensitivity of ATR585C is 5970mv with 1/30s. Its spectral sensitivity is shown in Figure 2.

Figure 2: IMX585 Spectral Sensitivity Characteristic

Spectral Sensitivity Characteristic graph for the IMX585 sensor, showing relative response [a.u.] on the y-axis against Wavelength [nm] on the x-axis. Three curves represent Red, Green, and Blue spectral sensitivity.

2.3 12bit ADC and ROI

ATR585C has a built-in 12bit ADC. It also supports a 12bit output mode for hardware binning and smaller resolution. The camera also supports hardware ROI (Region of Interest), and the smaller the ROI size, the higher the frame rate.

Table 2 shows the frame rate of ATR585C in 12/8bit mode, using USB3.0 / USB2.0 data transfer interface at different resolutions. When HDR mode is enabled, the frame rate is reduced by half.

Table 2: ATR585C Frame Rate at Different Resolution/Data Bit/Data Transfer (USB3.0/ USB2.0)

Resolution12bit ADC8bit ADC
USB3.0USB2.0USB 3.0USB 2.0
3840 * 2160241.9473.8
1920*1080703.9707.9

2.4 DDR3 Buffer

The ATR585C camera features a 512MB (4Gb) DDR3 buffer, which 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

ATR585C supports digital binning from 1×1 to 8×8 (stacking or averaging method) and hardware binning from 1×1 to 2×2 (averaging method). Hardware pixel binning is significantly faster than software binning.

2.6 Conversion Gain Switch

ATR585C supports HCG, LCG, and HDR mode switching.

2.7 Power and Cooling System for Precise Temperature Regulation

The camera must be powered by a DC12V 3A power source. The cooling system of ATR585C is a two-stage Thermoelectric Cooling (TEC) with a controllable electric fan for heat dissipation. The TEC system is controlled by a PID algorithm, allowing precise regulation to the target temperature with a 0.1°C deviation. The working temperature can be set to a specific number, with an effective temperature drop of -45°C from ambient temperature. This efficient cooling system guarantees high-quality camera images.

2.8 Zero Amp-Glow

ATR585C has been carefully designed to achieve zero amp-glow photo shooting. Figures 3 and 4 show images from different cameras at 20°C with a 5-minute exposure time, with and without amp-glow. The image captured by ATR585C shows zero amp-glow.

Figure 3: Amp-glow

Image showing amp-glow, likely from a different camera, with bright artifacts.

Figure 4: Zero amp-glow

Image showing zero amp-glow, captured by the ATR585C, appearing clean.

2.9 Camera Performance Analysis

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

  • e-/ADU: Pixels in vision application sensors convert photons into electrons. Gain represents the conversion factor from electrons (e⁻) into digital counts (ADUs), expressed as electrons per ADU.
  • Read Noise: Generated within the camera electronics during readout, it's a key performance indicator. Lower read noise generally means better SNR and image quality.
  • Full Well: The maximum electrical charge a pixel can hold, indicating the amount of light it can capture. A larger full well capacity generally leads to a wider dynamic range.
  • Dynamic Range: The ratio between the maximum output signal level and the noise floor. It represents the camera's ability to display both the brightest and darkest portions of an image simultaneously.

For the ATR series camera, the Gain Value is in xxx% mode, where xxx represents the x-axis (Gain Value) for performance descriptions.

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

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

All following data were acquired in SharpCap with ASCOM driver. Camera settings for HCG performance analysis: Full resolution, RAW 12-bit mode, Temperature: -10°C.

Figure 5: e/ADU, Read Noise, Full Well and Dynamic Range for ATR585C (HCG Mode)

Graphs showing e/ADU, Read Noise, Full Well, and Dynamic Range for ATR585C in HCG Mode against Gain / Gain(dB). The x-axis shows Gain Value and Gain(dB), with the formula Gain / Gain(dB)=20*log(GainValue/100).

Table 3: Camera Analysis Data (HCG Mode)

Gain Value10017731656210001778316256231000015000
Rel Gain (dB)05.1210.231520.0925.2229.9134.9639.9543.07
e⁻/ADU1.010.560.310.180.10.060.030.020.010.01
Read Noise (e⁻)0.550.650.60.530.510.460.470.490.480.5
Full Well (ke⁻)4.12.31.30.70.40.230.130.070.040.03
Dynamic Range (stop)1211.9711.2710.479.698.868.057.266.375.79

Camera settings for LCG performance analysis: Full resolution, RAW 12-bit mode, Temperature: -10°C.

Figure 6: e/ADU, Read Noise, Full Well and Dynamic Range for ATR585C (LCG Mode)

Graphs showing e/ADU, Read Noise, Full Well, and Dynamic Range for ATR585C in LCG Mode against Gain / Gain(dB). The x-axis shows Gain Value and Gain(dB), with the formula Gain / Gain(dB)=20*log(GainValue/100).

Table 4: Camera Analysis Data (LCG Mode)

Gain Value10017731656210001778316256231000015000
Rel Gain (dB)0.004.829.9514.7819.8724.9629.8134.8739.9643.53
e⁻/ADU9.645.543.061.760.980.540.310.170.10.06
Read Noise (e⁻)5.183.012.782.782.512.22.142.172.182.22
Full Well (ke⁻)4023137.24.02.21.30.70.40.3
Dynamic Range (stop)12121211.2810.7910.029.338.57.797.01

Camera settings for HDR performance analysis: Full resolution, RAW 16-bit mode, Temperature: -10°C.

Figure 7: e/ADU, Read Noise, Full Well and Dynamic Range for ATR585C (HDR Mode)

Graphs showing e/ADU, Read Noise, Full Well, and Dynamic Range for ATR585C in HDR Mode against Gain / Gain(dB). The x-axis shows Gain Value and Gain(dB), with the formula Gain / Gain(dB)=20*log(GainValue/100).

Table 5: Camera Analysis Data (HDR Mode)

Gain Value10017731656210001778316256231000015000
Rel Gain (dB)04.749.8714.6319.6924.7929.5834.6739.7143.15
e⁻/ADU0.20.120.060.040.020.010.010.010.010.01
Read Noise (e⁻)0.690.630.630.610.570.660.780.770.820.92
Full Well (ke⁻)137.54.12.41.30.70.40.20.130.09
Dynamic Range (stop)14.5213.8213.1112.3211.4510.389.528.437.276.67

3 Product Package and Connections

3.1 Packing List

Figure 8: Packing Information of ATR585C

Shows the camera body (C), cover (K), M42 adapter (J), extenders (H, G), power adapter (D), power cable (E), and USB3.0 cable (F).

Table 6: ATR585C Packing List

ItemSpecification
ACarton L:50cm W:30cm H:30cm (20pcs, 12~17Kg/ carton, 0.045m³), not shown in the photo
B3-A safety equipment case: L:28cm W:23cm H:15cm (1pcs, 3.9Kg/ box); carton size: L:28.2cm W:16.7cm H:25.5cm (TBD), not shown in the photo
CATR series camera (M42x0.75 Mount+2" adapter)
DPower adapter: input: AC 100~240V 50Hz/60Hz, output: DC 12V 3.3A
EPower cable
FHigh-Speed USB3.0 A male to B male gold-plated connectors cable /1.5m
GM48-M42 extender 0mm
HM42M-M42F extender 21mm (TBD)
IM48F - M42M extender 16.5mm (TBD)
JM42M adapter 12.5mm
KCover

3.2 Camera Dimension and Its Mount

Figure 9: Dimension and Mount of ATR585C

Shows front and side views with dimensions: Diameter 80mm, Height 107.1mm, and M42Fx0.75 mount. Includes labels for Cover Glass, CMOS, and Rear Focus (17.5mm / 18.1mm Optical Path).

Table 6: Dimension and Mount of ATR585C

ItemSpecification
DiameterØ80mm
Height107.1mm
MountM42Fx0.75mm

3.3 Camera Outline and Interface

Figure 10: Camera Outline and Interface.

Shows the back of the camera with labeled ports: 1. Protective window (AR window for mono camera, IR-cut filter for color camera), 2. M42x0.75 thread, 3. Thermal outlet or radiator, 4. LED indicators (Power LED, System LED, TEC LED, Fan LED), 5. DC 12V 3A power port (5.5 x 2.1mm), 6. Air inlet, 7. USB 3.0/ USB 2.0 port, 8. USB 2.0 HUB.

Table 7: Camera Outline and Interface List

ItemSpecification
1Protective window, AR window for mono camera, IR-cut filter for color camera
2M42F × 0.75 thread
3Thermal outlet or radiator
4LED indicators: 1) Power LED. 2) System LED. 3) TEC LED. 4) Fan LED
5DC 12V 3A power port, 5.5 × 2.1mm
6Air inlet
7USB 3.0/ USB 2.0 port
8USB 2.0 HUB

3.4 Camera Mechanical Connection with Adapter

The ATR585C can be connected to a telescope using a suitable adapter or a camera lens. Common adapters are included, with options for specific requirements. The female flange to the sensor is 17.5mm. The ATR585C features an M42x0.75 mount for direct telescope connection. It can also connect to telescopes using 1.25" or 2" eyepieces via M42M-1.25" or M42M-2" adapters.

Figure 2: The Connection of the ATR Camera and Adapter

Illustrates connecting the camera's M42Fx0.75 mount to telescope adapters like M42M-1.25" and M42M-2", showing telescope side M42 threads.

Table 8: Camera and Its Adapter Connections

ItemSpecification
Back Focal Distance17.50mm
M42M-1.25" AdapterM48M-1.25" adapter for 1.25" telescope
M42M-2" AdapterM42M-2" adapter for 2" telescope

3.5 Camera Mechanical Connection with Lens

Figure 3: Nikon F/Canon EF Lens with ATR Camera

Shows diagrams for connecting Nikon F-mount and Canon EF-mount lenses to the ATR camera via M42 adapters.

Table 9: Camera and Lens Connection

ItemSpecification
1Nikon F-M42 adapter (TBD)
2EOS EF-M42 adapter
3Nikon F-mount lens
4Canon EF-mount lens
5ATR camera with M42Fx0.75 mount

3.6 Camera Electric Connection with Accessories

The back of the ATR585C has three connection ports: DC 12V/3A power port, USB3.0/ USB2.0 port, and USB-HUB. Due to the higher power consumption of the IMX585 sensor and cooling system, the ATR585C requires a 12V/3A power supply. USB3.0 functions solely as a data communication method, not for power. The USB-HUB allows connection to other devices, simplifying cable management. Devices connected via USB-HUB communicate with the PC through the USB3.0/USB2.0 port.

Figure 4: Camera Electric Connection

Illustrates the camera's connections to a computer via USB3.0/USB2.0, USB HUB for accessories, and the DC 12V power adapter. Shows connection to a computer, filter wheel, and guiding camera.

Table 10: Camera Electric Connection Details

ItemSpecification
USB3.0/USB2.0 PortTo computer with USB3.0/USB2.0 cable
USB HUB for AccessoriesTo filter wheel with USB2.0 cable
To guiding camera with USB 2.0 cable
Power PortDC12V/3A

4 ATR585C and Its Software

4.1 Application Installation

For software, customers can download the latest ToupSky from the official website: https://touptek-astro.com/downloads/. The ATR 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 Compatibility: x86: XP SP3 or above; CPU supports SSE2 instruction set or above. x64: Win7 or above.
  • Features: Full camera control, Trigger mode and video mode support (raw or RGB format), Automatic capture and quick record, Multi-language support, Hardware ROI and digital binning, Extensive image processing (stitching, live stacking, flat field correction, dark field correction, etc.).
  • Supported Camera: All ToupTek astronomy cameras.

4.1.1 User-friendly UI Design

  • Well-arranged menus and toolbars for quick operation.
  • Unique design with three sidebars: Camera, Folders, Undo/Redo, for organized classification.
  • Convenient operating methods (double-click or right-click context menu).
  • Detailed help manual available.

Figure 5: ToupSky and Its Video Window

A screenshot of the ToupSky software interface showing the video capture window with camera controls and image preview.

Figure 6: ToupSky and Its Browse Window

A screenshot of the ToupSky software interface showing the image browsing window with file thumbnails.

4.1.2 Professional Camera Control Panel

FunctionDescription
Capture & ResolutionSet live and snap resolution, capture images, or record video.
Exposure & GainAuto exposure (with preset target) and manual exposure (inputtable time). Gain up to 5 times.
Color BalanceAdvanced intelligent white balance, with manual adjustment for temperature and tint.
Color AdjustmentHue, saturation, brightness, contrast, gamma initialization adjustment.
Frame RateAdjustment of frame rate based on computer configuration.
FlipHorizontal or vertical flip option to correct sample orientation.
SamplingBin mode for low noise video stream; Skip mode for sharper stream. Supports histogram extension, Negative/positive switching, Gray calibration, Clarity factor for focusing.
Bit DepthSwitch between 8 bits and 12 bits. 8 bits is standard Windows format; 12 bits offers higher quality but moderate FPS.
ROIRegion of Interest function to set ROI on the video window. Dotted rectangles with handles allow ROI size adjustment. Apply sets video to ROI size; Defaults returns to original size.
Dark Field CorrectionCapture dark field image first. Enable button becomes clickable after capture. Checking enables correction; unchecking disables it.
CoolingSet TE-Cooling target temperature and fan On/Off.
ParametersLoad, save, overwrite, import, export camera control panel parameters (including calibration, exposure, and color settings).

4.1.3 Practical Functions with Good Results

  • Video functions: Video broadcast, time lapse capture, video record, video stream grid, image stitch, video scale bar, date, etc.
  • Image Processing and Enhancement: Denoise, sharpen, color toning, deinterlace, filtering algorithms, mathematical morphology, range, binary, pseudo color, surface plot, line profile.

Figure 7: Image Stacking

A diagram illustrating the process of image stacking, showing multiple images being combined into a final high-fidelity image to decrease noise.

4.1.4 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 / 11 (32 & 64 bit), Mac OSX, Linux.
  • Language Support: Unlimited language support, including Simplified Chinese, Traditional Chinese, English, Russian, German, French, Polish, and Turkish.

4.1.5 Hardware Requirement

  • 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: Required

4.2 ATR585C and Dshow

Download ToupTekDshowAstroSetup from the provided link. DshowAstro is an interface driver providing Dshow standard support for ToupTek USB astronomy cameras.

  • 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.

4.3 ATR585C and the 3rd Party Software

4.3.1 Support Software

The following table lists supported third-party software:

No.SoftwareVersionWDMASCOMNative
1PHD Guiding2.3.0(2014)/
2Nebulosity3.2.2(2014)×/
3MaxIm DL5.23(2013)×/
4SharpCap2.1(2014)×/
5MetaGuide5.2.0(2014)//
6FireCapture2.4.05(2014)//
7Astroart5.0(2014)×/
4.3.2 N.I.N.A

Powerful open-source astronomy equipment management system for deep sky photo shooting, free.

4.3.3 INDI

A popular third-party driver software for astronomy devices, often used on Linux and MacOS.

4.3.4 ASCOM Platform

All AstroCam telescope camera drivers require the ASCOM platform, which is free. Download from http://www.ascom-standards.org/index.htm. The ASCOM package can be downloaded from: http://ascom-standards.org/Downloads/Index.htm.

4.3.5 PHD Guiding

A popular free guide software: http://openphdguiding.org/. ToupTek's telescope cameras support Native/ASCOM/WDM drivers for video operation.

4.3.6 Nebulosity

A popular cooled camera control/image process software directly supported via ASCOM.

4.3.7 MetaGuide

Autoguiding software with a novel method to avoid atmospheric agitation. The latest version supports GCMOS01200KPB. Guide port: http://www.astrogeeks.com/Bliss/MetaGuide/.

4.3.8 MAXIMDL

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

4.3.9 AstroArt

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

4.3.10 FireCapture

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

4.3.11 SharpCAP

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

4.3.12 Registax

A popular free planetary stacking and processing software.

4.3.13 AstroStack

A planetary stacking and process software.

4.3.14 DeepSky Stacker

A free deep sky image stack and process software.

5 Service

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

For customers purchasing cameras from local dealers, please contact your dealer for more information.

For technical support, please contact the e-mail address: astro@touptek.com.

Models: TR585C DSO Cooled Cameras, TR585C, DSO Cooled Cameras, Cooled Cameras, Cameras

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