Astrophotoguru · Compare

cameracomparison · 2-way

QHYCCD QHY9 vs QHYCCD QHY410C

QHYCCD QHY9
QHYCCD

QHY9

A strong fit for dedicated deep-sky imagers pairing with a broad range of focal lengths.

QHYCCD QHY410C
QHYCCD

QHY410C

A strong fit for dedicated deep-sky imagers pairing with wide-field refractors.

Key differences

-48% larger sensor
Finer pixels (5.4µm vs 5.94µm)
-65% more resolution
Mono vs color

Specifications

SpecificationQHYCCD QHY9QHYCCD QHY410C
Sensor
Typededicateddedicated
SensorKodak KAF-8300Sony IMX410
Sensor techCCDCMOS
Format4/3"Full frame
Sensor size18.0×13.5mm36.0×24.0mm
Diagonal22.5mm43.3mm
Pixel size5.40µm5.94µm
Resolution3358×25366072×4042
Megapixels8.5MP24.5MP
ColorNoYes
Cooling
CooledYesYes
Performance
Full well25500e⁻73000e⁻
Peak QE56%88%
Advantages of QHYCCD QHY9
  • Mono sensor — ideal for narrowband and LRGB
Advantages of QHYCCD QHY410C
  • Larger sensor (43.3mm vs 22.5mm diagonal) — wider field
  • Higher resolution (24.5MP vs 8.5MP)
  • One-shot color — simpler workflow
Best for — QHYCCD QHY9
  • Balanced field for most refractors
  • Fast, low-noise deep-sky at short focal lengths
  • Long-exposure deep-sky under any sky
  • Narrowband and LRGB workflows
Best for — QHYCCD QHY410C
  • Wide-field mosaics and full-frame telescopes
  • Fast, low-noise deep-sky at short focal lengths
  • Long-exposure deep-sky under any sky
  • One-shot color — quick results, less processing
QHYCCD QHY9 — typical FOV & scale
  • On 250mm refractor (wide)
    FOV: 4.13° × 3.09°Scale: 4.46"/px
  • On 800mm SCT reducer
    FOV: 1.29° × 0.97°Scale: 1.39"/px
  • On 2000mm SCT native
    FOV: 0.52° × 0.39°Scale: 0.56"/px
QHYCCD QHY410C — typical FOV & scale
  • On 250mm refractor (wide)
    FOV: 8.25° × 5.50°Scale: 4.90"/px
  • On 800mm SCT reducer
    FOV: 2.58° × 1.72°Scale: 1.53"/px
  • On 2000mm SCT native
    FOV: 1.03° × 0.69°Scale: 0.61"/px
QHYCCD QHY9 — recommended user

A strong fit for dedicated deep-sky imagers pairing with a broad range of focal lengths.

QHYCCD QHY410C — recommended user

A strong fit for dedicated deep-sky imagers pairing with wide-field refractors.

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