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SVBONY SV905C 1.23MP Type-C Guide Camera - 1.25"

par SVBONY
UGC SV-F9198N
Prix d'origine CA$154.00 - Prix d'origine CA$154.00
Prix d'origine
CA$154.00
CA$154.00 - CA$154.00
Prix actuel CA$154.00
Égalisation de prix!
  • 1.2MP IMX225 CMOS Sensor
  • 3.75µm Pixel Size
  • Peak Quantum Efficiency: 80%
  • Read Noise: 4.0e
  • Maximum Frame Rate: 39 FPS
  • Back Intercept: 8.5mm / 12.5mm
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  • Description
  • FAQ
  • Specifications
  • In the Box
  • Downloads
  • Warranty
  • Svbony SV905C 1.23MP Type-C 1.25" Guide Camera

    The Svbony SV905C guide camera combines a sensitive 1.2MP IMX225 sensor with 3.75µm pixels for precise autoguiding corrections. Its peak Quantum Efficiency of 80% and low 4.0e read noise allow it to reliably detect faint guide stars, even in sparse fields. A 12-bit ADC and a maximum frame rate of 39 FPS ensure your mount receives corrections quickly and accurately, keeping your long exposures sharp.

    IMX225 Sensor: 80% QE and 4.0e Read Noise for Reliable Guiding

    At the core of the SV905C is the Sony IMX225 sensor, chosen for its high sensitivity and low noise characteristics. A peak QE of 80% means the camera makes efficient use of incoming light, enabling it to lock onto fainter guide stars than less sensitive cameras. This is critical when your target is in a star-poor region of the sky or when using an off-axis guider.

    The camera's low read noise of 4.0e, combined with its HCG (High Conversion Gain) mode, preserves the signal-to-noise ratio even when you increase the gain. This results in cleaner guide star profiles and more stable guiding, as the software isn't chasing atmospheric scintillation or electronic noise.

    Smart Design: 8.5mm/12.5mm Back Intercept and Repeatable Focusing

    The SV905C is built for practical use in the field. It features dual back intercept distances of 8.5mm and 12.5mm, providing the flexibility needed to achieve focus in various setups, from separate guide scopes to off-axis guiders with different prism-to-sensor distances. Its standard 1.25" body fits directly into most guide scopes and focusers.

    For imagers who use portable setups, the camera body includes a scale mark and snap ring. This simple but effective feature allows you to mark your focus position, ensuring you can return to perfect focus quickly night after night without guesswork. The modern Type-C USB 2.0 port provides a reliable connection to your control computer.

    Broad Compatibility: PHD2, ASCOM, and Multi-OS Support

    A guide camera is only as good as its software support, and the SV905C offers wide-ranging compatibility. It works seamlessly with the industry-standard PHD2 guiding software via its ASCOM driver, as well as other popular capture programs like SharpCap and FireCapture on Windows.

    The SV905C isn't limited to a single operating system. With support for Windows, Mac OS, Linux, and even Raspberry Pi through AstroDMX Capture, it integrates into virtually any imaging setup, from a laptop in the field to a remote observatory running on a mini-PC.

    Svbony SV905C vs. ZWO ASI120MM Mini: A Guiding Comparison

    The SV905C is a direct competitor to the popular ZWO ASI120MM Mini, with both cameras targeting the entry-level autoguiding market. While they share the same 1.2MP resolution and 3.75µm pixel size, the SV905C holds a few key advantages.

    • Higher Sensitivity: The ZWO ASI120MM Mini's AR0130CS sensor has a peak QE of around 75%. The Svbony SV905C's IMX225 sensor achieves a higher peak QE of 80%, giving it a measurable edge in detecting faint stars.
    • Modern Sensor and Connector: The IMX225 is a more modern sensor known for its excellent sensitivity and low-noise performance. The SV905C also uses a more robust and reversible Type-C USB 2.0 connector.
    • Focusing Aids: The SV905C's built-in scale mark is a practical feature for achieving repeatable focus that the ASI120MM Mini lacks.

    While the USB 2.0 interface limits the SV905C for serious high-speed planetary imaging, its sensor and thoughtful design make it a highly capable and cost-effective autoguider.

  • What makes the Svbony SV905C a good guide camera?

    The Svbony SV905C is an excellent guide camera due to its combination of high sensitivity and low noise. Its IMX225 sensor has a peak QE of 80% and read noise of 4.0e, allowing it to detect faint guide stars easily. Combined with broad software compatibility (including PHD2) and a practical 1.25" design, it provides reliable and precise autoguiding.

    What software do I need to use the Svbony SV905C for guiding?

    For autoguiding, you will primarily use PHD2 Guiding, which is the standard for amateur astronomers. You will also need to install the Svbony ASCOM driver to allow PHD2 to communicate with the camera. The SV905C is also compatible with capture software like SharpCap and FireCapture for other uses.

    Can I use the Svbony SV905C with an Off-Axis Guider (OAG) on my 8" SCT?

    Yes, the SV905C is well-suited for use with an OAG on a Schmidt-Cassegrain telescope. Its high sensitivity (80% QE) is crucial for finding a suitable guide star in the small field of view provided by an OAG's pick-off prism. The camera's dual back intercept options of 8.5mm and 12.5mm provide the flexibility needed to reach focus alongside your main imaging camera.

    How will the SV905C perform with a 50mm f/4 guide scope on a target like the Andromeda Galaxy (M31)?

    The SV905C is an excellent match for a 50mm guide scope. The camera's 3.75µm pixels create a good image scale with the short 200mm focal length, allowing for very precise guiding corrections. When imaging a large target like the Andromeda Galaxy (M31), the camera's high sensitivity will ensure you can find a suitable guide star in the surrounding field to keep your main image sharp.

    Does the SV905C work with a Mac or Raspberry Pi?

    Yes, the Svbony SV905C supports multiple operating systems beyond Windows. It is compatible with Mac OS and Linux / Raspberry Pi using the AstroDMX Capture software, making it a flexible choice for various remote or portable imaging setups.

    What is HCG mode on the SV905C and when should I use it?

    HCG (High Conversion Gain) mode is a feature of the IMX225 sensor that automatically reduces read noise at higher gain settings. This allows you to increase the camera's sensitivity to see fainter stars without suffering the penalty of excessive electronic noise. You don't need to manually turn it on; the camera engages it when the gain is raised above a certain level, ensuring you get the cleanest signal possible.

  • Sensor Sony IMX225 CMOS
    Resolution 1280 × 960 (1.2 MP)
    Pixel Size 3.75µm x 3.75µm
    Image Area 4.8mm x 3.6mm
    Sensor Diagonal 6mm
    Peak QE 80%
    Read Noise 4.0e
    Full Well Capacity 13ke
    ADC 12-bit
    Max Frame Rate 39 FPS
    Shutter Type Electronic Rolling Shutter
    Exposure Time 64µs to 20s
    Gain 0-100
    HCG Mode Yes
    ROI Support Yes
    Binning 1x1, 2x2
    Back Intercept 8.5mm / 12.5mm
    Protective Glass AR Coated
    Data Interface Type-C USB 2.0
    Software Compatibility Sharpcap, Firecapture, PHD2, AstroDMX Capture
    Platform Support ASCOM, DirectShow
    Supported OS Windows, Mac OS, Linux, Raspberry Pi
    Power Consumption <0.5W
    Working Temperature -5℃ to 45℃
    Storage Temperature -20℃ to 60℃
    Weight 230g (with parcel)
  • SVBONY 1-Year Warranty