BSL Deep-Sky Imaging – Full Well / Dynamic Range / Read Noise

Here are two examples of different camera models below.
oooo

ZWO ASI2600MM/MC Pro

ZWO ASI58MM/MC Pro

(Click each box above to enlarge)

oooo

Full Well Capacity, Read Noise, and Dynamic Range

They are fundamental sensor specifications in digital imaging and astrophotography.
oooo


oooo

oooo
oooo

Full Well Capacity, Read Noise, and Dynamic Range
oooo

They are fundamental sensor specifications in digital imaging and astrophotography.
o

Together, they determine how much signal a camera can capture before saturating, how faint a light signal it can detect, and the overall breadth of light intensity it can record in a single frame.
(DDR = Double Data Rate)


o
o


oooo

1) Full Well Capacity (FWC)
o

Definition:
The maximum charge (measured in electrons, e⁻) that an individual pixel can store before it saturates.

Impact:
A larger full well capacity allows pixels to collect more light without clipping.

When a pixel exceeds its full well capacity, it becomes saturated (reaching pure white, ADU max), causing bright targets (such as star cores or bright nebulae) to lose colour and structural detail.
o
(ADU = Analog-to-Digital Unit)

Typical Range:
~10,000 e⁻ to over 100,000 e⁻ depending on pixel size and sensor architecture.

oooo
oooo
oooo

oooo


oooo
o
2. Read Noise (RN)

oooo
Definition:
The uncertainty or electronic noise introduced by the camera’s readout circuitry and analogue-to-digital converter (ADC) during sensor readout, measured in electrons (e⁻).
o
o

Impact:
Read noise sets the camera’s absolute noise floor – the minimum detectable light signal ~ Signals weaker than or buried beneath the read noise floor cannot be easily separated from background noise.
o
Lower read noise allows shorter exposures to be stacked effectively without degradation from accumulated sensor read errors.
o
o

Typical Range:
~0.5 e⁻ to 7 e⁻ (varies inversely with gain settings).

ooo
oooo
oooo
oooo

oooo

oooo


oooo
o

3) Dynamic Range (DR)
o

Definition:
The ratio of the maximum readable signal (FWC = Full Well Capacity) to the noise floor (Read Noise) within a single exposure.
oooo
o
Mathematical Formula:

Dynamic Range (Linear Ratio) = FWC ÷ Read Noise
o
Dynamic Range (Stops) = log2 (FWC.÷.Read Noise)
o
Dynamic Range (dB) = log10 (FWC.÷.Read Noise)
oooo
oooo

Impact:
High dynamic range enables a camera to simultaneously capture faint details in shadow regions without blowing out highlight areas.

oooo

oooo



oooo

oooo

Interplay & Gain Trade-Offs

ParameterLow GainHigh GainHigh Conversion Gain (HCG) Mode
Full Well Capacity (FWC)MaximumReduced (saturates faster)Slightly lower than base
Read Noise (RN)HigherSubstantially lowerDrops dramatically
Dynamic Range (DR)Maximum headroom for highlightsSlightly lower total rangeOptimizes both low read noise & high DR
Best Target UseBright targets, star clusters, high light levelsNarrowband, faint targets, planetaryDeep-sky imaging with weak signals

oooo


oooo

oooo

Back to

oooo

Back to page 32

Next to page 34

oooo


Page 33 – Full Well / Dynamic Range / Read Noise
Derek Rowley – Derekscope’s BSL Guide to Deep-Sky Imaging
oooo


oooo

Comments are closed.