Astrophotoguru · Compare

cameracomparison · 2-way

QHYCCD QHY600C vs QHYCCD QHY411M

QHYCCD QHY600C
QHYCCD

QHY600C

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

QHYCCD QHY411M
QHYCCD

QHY411M

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

Key differences

-36% larger sensor
-60% more resolution
Color vs mono

Specifications

SpecificationQHYCCD QHY600CQHYCCD QHY411M
Sensor
TypeDedicated Cooleddedicated
SensorSony IMX455Sony IMX411
Sensor techCMOSCMOS
FormatFull FrameMedium format
Sensor size36.0×24.0mm54.0×40.0mm
Diagonal43.3mm67.4mm
Pixel size3.76µm3.76µm
Resolution9576×638814304×10748
Megapixels61.0MP151.0MP
ColorYesNo
Cooling
CooledYesYes
Performance
Full well51000e⁻80000e⁻
Peak QE80%90%
Advantages of QHYCCD QHY600C
  • One-shot color — simpler workflow
Advantages of QHYCCD QHY411M
  • Larger sensor (67.4mm vs 43.3mm diagonal) — wider field
  • Higher resolution (151MP vs 61MP)
  • Mono sensor — ideal for narrowband and LRGB
Best for — QHYCCD QHY600C
  • Wide-field mosaics and full-frame telescopes
  • Well-sampled deep-sky at medium focal lengths
  • Long-exposure deep-sky under any sky
  • One-shot color — quick results, less processing
Best for — QHYCCD QHY411M
  • 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 QHY600C — typical FOV & scale
  • On 250mm refractor (wide)
    FOV: 8.25° × 5.50°Scale: 3.10"/px
  • On 800mm SCT reducer
    FOV: 2.58° × 1.72°Scale: 0.97"/px
  • On 2000mm SCT native
    FOV: 1.03° × 0.69°Scale: 0.39"/px
QHYCCD QHY411M — typical FOV & scale
  • On 250mm refractor (wide)
    FOV: 12.38° × 9.17°Scale: 3.10"/px
  • On 800mm SCT reducer
    FOV: 3.87° × 2.87°Scale: 0.97"/px
  • On 2000mm SCT native
    FOV: 1.55° × 1.15°Scale: 0.39"/px
QHYCCD QHY600C — recommended user

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

QHYCCD QHY411M — recommended user

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

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