2 arcsec seeing, 3.76 µm pixels, 480 mm
2 / 1.6157 = approximately 1.2378 pixels per entered seeing FWHM. The output is a numerical ratio, not a well-sampled purchasing certification.
Load this example in the calculatorExpress an entered seeing FWHM in pixels using your camera pitch and effective focal length, without an automatic good/bad verdict.
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Sampling combines two different quantities: angular image scale and an estimate of seeing width. Keep them separate. Changing a camera pixel size changes the sampling ratio; it does not improve atmospheric seeing.
Pixels per FWHM = entered seeing FWHM (arcsec) / image scale (arcsec/pixel). Image scale = 206.264806 × pitch (µm) / focal length (mm).
2 / 1.6157 = approximately 1.2378 pixels per entered seeing FWHM. The output is a numerical ratio, not a well-sampled purchasing certification.
Load this example in the calculator4 / 1.6157 = approximately 2.4756 pixels per FWHM. The larger ratio describes a broader seeing width, not sharper stars.
Load this example in the calculatorA seeing-only estimate omits diffraction, focus, guiding and sensor response. Measured stellar FWHM can contain several of those effects and is not interchangeable with atmospheric seeing alone.
No universal under/over/well-sampled label is assigned. Camera purchasing also depends on field size, optical correction and the intended imaging workflow.
Source for the pixel-size/focal-length conversion. Its ideal-scale purchasing thresholds are not adopted here.
Calculation notes maintained by AstroGearFit. Updated September 7, 2026. Examples are numerical demonstrations, not hands-on equipment tests. The method notes are currently in English; the existing interface language selector remains available.
Five focused checks with reproducible examples and explicit limits. These tools do not certify a complete equipment combination.
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Convert camera pixel pitch and telescope effective focal length to angular image scale in arcseconds per pixel.
Express an entered seeing FWHM in pixels using your camera pitch and effective focal length, without an automatic good/bad verdict.
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Filter sizing is paused. Whole-system compatibility needs verified interfaces, optical specifications and configuration-specific evidence.