Astrophotoguru · Compare

cameracomparison · 2-way

QHYCCD QHY9 vs QHYCCD QHY461M

QHYCCD QHY9
QHYCCD

QHY9

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

QHYCCD QHY461M
QHYCCD

QHY461M

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

Key differences

-59% larger sensor
Larger pixels (5.4µm vs 3.76µm)
-92% more resolution

Specifications

SpecificationQHYCCD QHY9QHYCCD QHY461M
Sensor
Typededicateddedicated
SensorKodak KAF-8300Sony IMX461
Sensor techCCDCMOS
Format4/3"Medium format
Sensor size18.0×13.5mm44.0×33.0mm
Diagonal22.5mm55.0mm
Pixel size5.40µm3.76µm
Resolution3358×253611760×8896
Megapixels8.5MP102.0MP
ColorNoNo
Cooling
CooledYesYes
Performance
Full well25500e⁻51000e⁻
Peak QE56%90%
Advantages of QHYCCD QHY9
  • Larger pixels — better low-light per-pixel sensitivity
Advantages of QHYCCD QHY461M
  • Larger sensor (55mm vs 22.5mm diagonal) — wider field
  • Finer sampling at 3.76µm pixels
  • Higher resolution (102MP vs 8.5MP)
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 QHY461M
  • Wide-field mosaics and full-frame telescopes
  • Well-sampled deep-sky at medium focal lengths
  • Long-exposure deep-sky under any sky
  • Narrowband and LRGB workflows
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 QHY461M — typical FOV & scale
  • On 250mm refractor (wide)
    FOV: 10.08° × 7.56°Scale: 3.10"/px
  • On 800mm SCT reducer
    FOV: 3.15° × 2.36°Scale: 0.97"/px
  • On 2000mm SCT native
    FOV: 1.26° × 0.95°Scale: 0.39"/px
QHYCCD QHY9 — recommended user

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

QHYCCD QHY461M — recommended user

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

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