Direct answer
In brief
For reference SDR evaluation, use BT.1886 as the target EOTF after black level, white luminance, and D65 white balance are established. BT.1886 uses exponent 2.4 plus measured black and white luminance, so it is not always identical to a pure gamma 2.4 curve. Without measurement, use the best documented reference-oriented SDR preset and leave multipoint controls at reset. With measurement, calculate the complete target, compare multiple grayscale levels, correct broad errors first, and verify PQ and HLG separately because they are not SDR gamma modes.
Black level determines where the visible range begins.
White level determines the selected SDR reference-white luminance and clipping behavior.
White balance determines whether the grayscale is neutral.
The SDR EOTF determines how luminance is distributed between black and white.
That last relationship is often called gamma.
For a reference HDTV display, the formal target is Recommendation ITU-R BT.1886. [1][2]
The practical process is:
- Set the room.
- Set black and white.
- Set D65 white balance.
- Select the intended SDR EOTF preset.
- Measure the grayscale luminance.
- Compare the display with the complete target equation.
- Create a separate room-adapted mode only when needed.
Do not select gamma only from a generic bright-room or dark-room table.
Do not assume that a menu label produces the stated curve.
Do not use an SDR gamma chart to calibrate PQ or HLG.
What gamma means
Pure power gamma
A simple power function can be written as:
Lrelative = V^γ
where:
Vis normalized signal levelγis the exponentLrelativeis luminance relative to white
At the same black and white endpoints:
- a lower exponent produces brighter midtones
- a higher exponent produces darker midtones
This is useful for comparison.
It is not the complete BT.1886 equation when display black is above zero.
EOTF
The electro-optical transfer function maps the nonlinear video signal to display light.
For reference HDTV production, BT.1886 specifies that display function. [1]
OETF
The opto-electronic transfer function maps source or scene-light values into a nonlinear signal.
BT.709 defines the source-side function for its production system.
OOTF
The opto-optical transfer function describes the overall relationship between scene light and display light.
Report ITU-R BT.2390-12 explains that the television system includes:
- source OETF
- artistic adjustment
- display EOTF
- display adjustment
The result is not merely one curve undoing another. [3]
System gamma
System gamma can describe the overall contrast rendering of the end-to-end system.
HLG uses this term explicitly.
Do not confuse HLG system gamma with an SDR menu preset labeled 2.2 or 2.4.
BT.1886
Scope
BT.1886 specifies the reference EOTF that flat-panel displays used in HDTV programme production should follow for consistent picture presentation. [1]
BT.2035 says the display’s gamma characteristics should be adjusted to the BT.1886 curve over the full range in its reference environment. [2]
Equation
BT.1886 defines:
L = a(max[V + b, 0])^γ
with:
γ = 2.4aderived fromLWandLBbderived fromLWandLBLWequal to screen luminance for whiteLBequal to screen luminance for black [1]
For narrow-range 10-bit BT.709 content:
V = (D - 64) / 876
where:
- code 64 is reference black
- code 940 is reference white [1]
Why black and white matter
The target cannot be calculated fully until these values are known:
- displayed reference black
- displayed reference white
Changing either can change the BT.1886 equation.
That is why black level and white luminance come before EOTF calibration.
BT.1886 versus pure gamma 2.4
Zero-black case
When LB is effectively zero:
- the offset
bapproaches zero - BT.1886 approaches a pure power curve
- the exponent remains 2.4
This is close to what many menus call gamma 2.4.
With zero black, it is mathematically the same as a pure gamma 2.4 curve.
The practical difference is small compared with many consumer-display errors.
Nonzero-black case
When LB is above zero:
- the offset becomes nonzero
- lower signal values produce more luminance
- the curve is no longer one simple power law from zero
Calling the result “gamma 2.4” hides that behavior.
Calculated illustration
Assume:
- white
LW = 100 cd/m² - black
LB = 0.1 cd/m²
At normalized signal V = 0.5:
- BT.1886 gives approximately 21.60 cd/m²
- pure gamma 2.4 gives approximately 18.95 cd/m²
- pure gamma 2.2 gives approximately 21.76 cd/m²
The example shows why a BT.1886 display with nonzero black can resemble a lower pure exponent through part of the range.
It is not a recommendation to target 0.1 cd/m² black.
OLED and emissive black
An OLED can produce a black measurement close to the meter’s lower limit under suitable conditions.
When LB approaches zero, BT.1886 approaches the 2.4 power curve.
BT.1886 does not automatically add a special OLED shadow lift.
If an OLED mode shows lifted near-black detail, that lift comes from the implementation or an additional adjustment.
Reference SDR viewing
BT.2035 environment
BT.2035 specifies an HDTV evaluation environment including:
- 10 lux room illumination
- D65 background
- background luminance around 10 percent of reference white
- reference white 100 cd/m²
- reference black below 0.01 cd/m²
- BT.1886 EOTF [2]
This is a professional repeatable reference condition.
A living room does not have to reproduce it exactly.
Departures should be described as home adaptations.
Dim does not mean total darkness
The formal environment includes a controlled surround.
It is not simply a television in a completely black room.
The surround affects:
- adaptation
- perceived contrast
- comfort
- shadow visibility
Use the room workflow in Article 14.
Bright-room viewing
What room light does
Room light can reach the viewer in two important ways.
Screen reflection
Reflected light raises the viewed black and reduces the effective contrast of the image.
Peripheral adaptation
Light in the room changes the state of visual adaptation.
Both can make dark and midtone content less visible.
Display adjustment
Report BT.2390-12 says that receiver-side display adjustment may compensate for:
- non-reference viewing environment
- display limitation
- viewer preference
It may:
- lift black level
- change system gamma
- add a highlight knee [3]
That is a broader concept than choosing a gamma preset.
Gamma 2.2 as an adaptation
A pure 2.2 curve places midtones above pure 2.4 at the same endpoints.
For example at V = 0.5:
- gamma 2.2: about 21.76 percent of white
- gamma 2.4: about 18.95 percent of white
The difference can improve visibility in some brighter rooms.
It also changes the reference rendering.
Use it as a labeled adaptation, not as a universal standards requirement.
Why one bright-room number is insufficient
The required adaptation depends on:
- reflected screen light
- display black
- SDR white luminance
- room surround
- viewing distance
- user vision
- content
- television processing
One room may need:
- more panel luminance
Another may benefit from:
- lower reflection
- a lower exponent
- black lift
- ambient adaptation
- curtain control
Measure and evaluate the complete mode.
Mixed viewing
There is no universal best compromise.
Useful approaches include:
- BT.1886 night mode
- brighter day mode with measured EOTF
- one stable intermediate mode
- controlled ambient-adaptive mode
- one reference mode and one preference mode
Do not erase the reference baseline.
A mixed-room compromise is a user decision.
Selecting a preset
Start from the reset reference-oriented SDR mode
Use the mode chosen in Article 15.
Verify:
- SDR signal
- black level
- white luminance
- D65
- processing state
Plausible preset names
The menu may contain:
- BT.1886
- 2.2
- 2.4
- Gamma
- Film Gamma
- minus and plus offsets
- Dark
- Medium
- Bright
The name does not establish the result.
Measure candidate presets
Compare each candidate across the grayscale.
Record:
- black
- white
- luminance at each point
- target luminance
- RGB balance
- clipping
- local dimming state
- room
Select the preset that gives the best broad behavior before fine correction.
Offset scales
A scale such as minus 3 to plus 3 can mean:
- higher number brightens the curve
- higher number darkens the curve
- offset from a hidden base
- different behavior in each picture mode
Do not infer the direction.
Measure or consult the exact manual.
Auto and adaptive gamma
Identify the function
An Auto control can respond to:
- signal type
- content
- room light
- picture mode
- internal metadata
- manufacturer logic
Its name is not enough.
Calibration baseline
For measured calibration:
- disable changing room adaptation
- disable dynamic contrast
- keep local dimming in the intended fixed state
- keep power settings stable
- verify repeat readings
An adaptive mode can be evaluated afterward.
Practical adaptive mode
A well-behaved ambient mode can be useful in a changing room.
Test:
- dark room
- moderate room
- bright room
- transition time
- color shift
- black level
- EOTF
- white luminance
Label the result as adaptive.
Do not call it a fixed BT.1886 mode while it is changing.
Visual gamma patterns
Basic concept
A visual gamma pattern can compare:
- a fine spatial mixture
- a solid patch
When the eye integrates the fine mixture, both areas can appear equally bright if the display follows the target behavior at that test point.
Checkerboard average
An equal-area full-black and full-white checkerboard has an average near 50 percent of white luminance when:
- black luminance is negligible
- the white pixels are correct
- the pixels are reproduced without scaling
- no processing changes the pattern
- the observer integrates the pattern
The average is a luminance average.
It is not a 50 percent signal value.
Required solid-patch signal
For a pure power target:
Vmatch = 0.5^(1/γ)
Approximate values are:
| Target | Solid-patch signal matching 50% luminance |
|---|---|
| Gamma 2.2 | 72.97% |
| Gamma 2.4 | 74.92% |
| Gamma 2.5 | 75.79% |
The pattern designer encodes the target-specific solid patch.
The reader should not substitute a generic 50 percent gray image.
BT.1886 pattern
A true BT.1886 match can depend on:
LBLW- exact checkerboard luminance
- display behavior
A fixed visual pattern can only approximate the target under assumed conditions.
Meter measurement is more reliable.
Scaling limits
Native resolution
Spears & Munsil states that its 1080p checkerboard gamma patterns only work when:
A modern 4K television must scale a 1080p pattern to fill its panel.
That invalidates the one-pixel checkerboard relationship unless the pattern and workflow are specifically designed for the target resolution.
Moiré and bands
If the checkerboard shows:
- moiré
- streaks
- bands
- altered pixel structure
Do not adjust the television from that result.
Pixel amplitude
Some displays cannot reproduce the fine black-white checkerboard at full amplitude.
The checkerboard can measure too dark.
Spears & Munsil identifies D-ILA and LCoS projectors as known examples for its pattern. [7]
The solid patch can then look too bright even when the EOTF is not the cause.
Processing risks
The pattern can also be altered by:
- chroma conversion
- sharpening
- noise reduction
- scaling
- pixel shifting
- local dimming
- browser zoom
- image compression
- streaming transcoding
Use a documented pattern path.
What a visual pattern can tell you
A valid pattern can give a rough answer at one point:
- patch appears brighter
- patch appears darker
- patch approximately blends
It can help compare presets.
It cannot establish:
- full BT.1886 tracking
- exact luminance
- black-luminance compensation
- EOTF near black
- EOTF near white
- channel neutrality
- uncertainty
Single-point limitation
Spears & Munsil explicitly describes its equal-energy gamma pattern as a single data point.
The full curve requires meter measurement with suitable grayscale patterns. [7]
Multiple visual points
A set of properly designed target-specific patterns can sample more than one level.
Every pattern must be:
- valid
- native
- unscaled
- documented
The result remains visual and approximate.
Measuring the EOTF
Define the target first
State:
- BT.1886
- pure gamma 2.2
- pure gamma 2.4
- custom room-adapted curve
- another documented target
Do not compare to an unnamed gamma.
Record black and white
For BT.1886 record:
LBLW
The target calculation uses them.
Measure multiple levels
A practical SDR series can include:
- near black
- low gray
- midtones
- upper midtones
- near white
- reference white
Use enough points to show shape.
Avoid points that the meter cannot repeat reliably.
Calculate target luminance
For BT.1886:
- normalize the signal
- calculate
a - calculate
b - calculate target
L - compare measured and target luminance
For a pure power target:
Ltarget = LB + (LW - LB)V^γ
when that simplified adapted form is the declared target.
Do not silently compare a nonzero-black display with a zero-black power curve.
Report error
Useful reports include:
- measured cd/m²
- target cd/m²
- percent luminance error
- logarithmic error
- effective local gamma where appropriate
- RGB balance
- repeat readings
One average gamma value is not enough.
Effective gamma
An effective exponent can be useful away from the endpoints.
It becomes unstable near:
- black
- zero signal
- zero luminance
- clipped white
It can also misrepresent BT.1886 when black is nonzero.
Use it as a diagnostic, not the formal target.
Patterns for meter measurement
Equal-energy windows
Spears & Munsil provides equal-energy windows intended for grayscale and gamma measurement.
The surrounding pattern changes as the center changes so total pattern energy remains more consistent. [7]
This can reduce some display power and iris interactions.
Standard windows
A calibration workflow can use:
- fixed-area windows
- full fields
- constant-average-picture-level patterns
- insertion patterns
The choice affects some displays.
Record it.
Pattern size
A small window can interact with:
- local dimming
- peak algorithms
- pixel response
A large window can interact with:
- ABL
- full-screen power
- heating
- room adaptation
Use a repeatable method.
Sequence and duration
Record:
- order
- delay
- insertion
- stabilization
- read time
- repeatability
An OLED, LCD, projector, or mini-LED can respond differently.
White balance and EOTF
White balance first
The EOTF is measured from luminance.
Changing red, green, or blue balance changes luminance.
Complete broad grayscale correction before final EOTF correction.
Recheck after gamma adjustment
A Gamma or multipoint luminance control can change RGB balance.
After adjustment recheck:
- x and y
- RGB balance
- D65
- clipping
- color
The calibration is iterative.
Multipoint controls
Broad controls first
Start with:
- correct preset
- black
- white
- white balance
- broad gamma or EOTF control
Use multipoint correction only for repeatable localized errors.
Map the controls
A point labeled 10 percent may affect:
- 5 percent
- 10 percent
- 15 percent
- another region after Contrast changes
Measure neighboring levels.
Use small corrections
Large adjustments can create:
- banding
- contouring
- grayscale tint
- clipping
- non-monotonic luminance
- unstable near black
The numerical chart can improve while the image develops artifacts.
Check monotonicity
Each higher signal level should normally produce higher luminance until intentional clipping or mapping.
A bad correction can make one step equal to or darker than the previous step.
Check the full sweep.
Check ramps
Use:
- smooth grayscale ramp
- skies
- walls
- fog
- faces
- dark gradients
Patterns reveal structure.
Real scenes reveal visibility.
Near-black EOTF
Measurement difficulty
Near black can be affected by:
- meter noise
- panel dithering
- local dimming
- compression
- black-level control
- RGB offset
- temporal behavior
- room reflection
Do not make large multipoint corrections from one unstable read.
OLED and QD-OLED
Possible issues include:
- flashing
- chromatic tint
- near-black overshoot
- crushed first steps
- raised first steps
- temporal dithering
These are model- and sample-specific.
They are not proof that the selected exponent is universally wrong.
LCD and mini-LED
Possible issues include:
- elevated black
- zone thresholds
- local-dimming crush
- blooming
- subtitle interaction
- viewing-angle change
The measured BT.1886 target depends on displayed black.
Projectors
Projection black depends strongly on:
- room
- screen
- iris
- light engine
- reflections
A room-adapted target may be necessary.
State it.
Day and night SDR modes
Night reference mode
A controlled-room mode can target:
- BT.1886
- D65
- selected SDR white luminance
- stable processing
Day mode
A day mode can use:
- higher white luminance
- lower-exponent EOTF
- controlled black lift
- ambient adaptation
- another documented adjustment
Measure it separately.
Naming
Label the modes honestly:
- SDR Reference Night
- SDR Day Adapted
- SDR Energy Saving
- SDR Preference
Do not label all of them BT.1886 if they do not follow it.
HDR
PQ
PQ uses the BT.2100 or ST 2084 EOTF.
It is an absolute display-light relationship before display mapping.
Do not apply:
- gamma 2.2
- gamma 2.4
- BT.1886
as the PQ target.
A user slider can alter PQ tracking.
That does not turn PQ into SDR gamma.
HLG
HLG includes a display and system relationship with system gamma.
BT.2100 specifies:
- system gamma 1.2 for a 1,000 cd/m² nominal-peak reference display
- an equation for other nominal peaks [4]
BT.814 describes a further reduction in HLG display gamma for brighter non-reference environments. [5]
That is a defined HLG adaptation.
Separate verification
For HDR measure:
- PQ EOTF or HLG system behavior
- black
- HDR Reference White [6]
- target peak
- tone mapping
- color volume
- area and duration behavior
The SDR Gamma menu may be unavailable or repurposed.
Use the correct article workflow for Articles 13, 18, and 22.
A no-meter SDR workflow
A reader without a meter can create a safe baseline.
Step 1: Prepare the room
Use the room condition for which the mode will be saved.
Step 2: Select and reset the reference-oriented SDR mode
Confirm SDR.
Step 3: Set earlier controls
Confirm:
- range
- black level
- white luminance
- D65-oriented preset
- optional processing off
Step 4: Choose the intended reference preset
Use BT.1886 when:
- the television offers it
- model-specific evidence supports it
- the room is close to the reference use
Otherwise use the best documented reference-oriented preset.
Step 5: Use real content
Inspect:
- dark faces
- shadowed rooms
- midtone skin
- daylight exteriors
- grayscale ramps
Look for obvious tonal imbalance.
Do not recalibrate from one title.
Step 6: Use a visual gamma pattern only when valid
Confirm:
- native pattern resolution
- no scaling
- no moiré
- documented target
- compatible display
Treat the result as a rough single-point check. [9]
Step 7: Stop
Leave multipoint controls at reset.
Create a separate brighter-room preference mode if necessary.
Do not call the unmeasured result a verified BT.1886 calibration.
A measured SDR workflow
Step 1: Document the system
Record:
- television
- size
- firmware
- input or app
- SDR range
- bit depth
- picture mode
- local dimming
- processing
- room
- meter
- profile
- generator
- pattern
- date
Step 2: Establish endpoints
Measure:
- black
LB - white
LW
Step 3: Stabilize grayscale
Verify D65 and broad RGB balance.
Step 4: Calculate the target
Use the complete BT.1886 equation or the declared alternative target.
Step 5: Measure candidate presets
Choose the closest broad response.
Step 6: Adjust broad controls
Use the least invasive control.
Step 7: Remeasure
Check the entire grayscale.
Step 8: Use multipoint only when required
Use small corrections.
Measure neighbors.
Step 9: Verify image quality
Check:
- black
- white
- RGB clipping
- grayscale
- EOTF
- ramps
- color
- real content
- repeatability
Step 10: Save and report
Preserve a reset-state record and the final report.
Troubleshooting
The image looks too dark in a bright room
Check:
- reflected room light
- SDR white luminance
- curtains or glare
- selected EOTF
- ambient adaptation
- dynamic contrast
- black level
- source grade
A lower exponent can help.
It is not the only solution.
The image looks flat in a dim room
Check:
- lower-exponent preset
- raised black
- room light
- dynamic black lift
- local dimming
- white luminance
- source grade
Do not select a higher exponent until black is correct.
Shadows are crushed with BT.1886
Check:
- signal range
- black level
- near-black measurement
- local dimming
- RGB offset
- noise reduction
- pattern stability
- source compression
- panel limitation
BT.1886 itself is not proof that the display tracks it.
Shadows are raised with BT.1886
Check:
- black level
- display black measurement
- reflected room light
- local dimming
- manufacturer black compensation
- adaptive gamma
- source master
The 2.4 preset measures closer to 2.2
Possible causes include:
- manufacturer labeling
- nonzero black
- hidden processing
- room adaptation
- measurement target
- control interaction
- local dimming
- pattern type
Compare with the full equation.
The checkerboard will not blend
Check:
- resolution
- overscan
- scaling
- moiré
- display pixel structure
- viewing distance
- pattern compression
- source device
- browser or player
Do not adjust gamma until the pattern is valid.
The checkerboard blends but the patch never matches
Possible causes include:
- invalid target patch
- display not reproducing pixel amplitude
- scaling
- local dimming
- EOTF error
- black not negligible
- room reflection
- observer limitation
Use a meter.
Midtones measure correctly but shadows do not
Check:
- black-level target
- near-black processing
- multipoint controls
- meter noise
- local dimming
- panel precision
- RGB offset
Do not change the broad preset only from one unstable low point.
Shadows measure correctly but highlights do not
Check:
- Contrast
- white balance gain
- clipping
- panel-light control
- dynamic contrast
- multipoint overlap
Measurements change between runs
Check:
- pattern duration
- sequence
- panel temperature
- ABL
- local dimming
- adaptive controls
- meter integration
- source conversion
- firmware
- static dimming
Calibrate only stable data.
SDR is correct but HDR is wrong
That is expected when separate paths exist.
Use:
- PQ workflow
- HLG workflow
- HDR mode memory
- correct patterns
Do not copy SDR gamma controls.
What correct SDR EOTF looks like
By measurement
A verified mode should show:
- declared target
- correct
LB - correct
LW - luminance close to target across the range
- neutral grayscale
- monotonic steps
- no avoidable clipping
- smooth ramps
- stable repeat readings
By eye
A practical mode should show:
- dark scenes that remain dark
- available shadow detail without a gray veil
- natural midtone brightness
- highlights that fit the SDR target
- no visible luminance steps or pumping
- consistent appearance across scenes
Visual quality does not prove numerical compliance.
What calibration can fix
Calibration can reduce:
- broad SDR luminance-tracking error
- localized EOTF error
- incorrect preset behavior
- some near-black or midtone imbalance
- mode-to-mode inconsistency
within the control resolution and display capability.
What calibration cannot fix
Calibration cannot:
- recover source detail removed upstream
- remove screen reflection electronically
- eliminate panel black limits
- repair every local-dimming artifact
- create missing panel precision
- prevent all ABL or thermal behavior
- make a scaled checkerboard valid
- make copied settings correct for another unit
- make a consumer television identical to a mastering monitor
- force PQ or HLG to behave like SDR gamma
Recommended report
An SDR EOTF report should include:
- target name
- target equation
LBLW- signal levels
- measured luminance
- target luminance
- error metric
- RGB balance
- D65 coordinates
- pattern size and type
- sequence
- meter
- meter profile
- generator
- mode
- controls
- room
- firmware
- date
Where this leaves us
The reference SDR target is BT.1886.
That does not mean:
- every menu should be set to 2.4
- every display uses a pure power curve
- every bright room should use 2.2
- every OLED needs BT.1886 to lift shadows
- every checkerboard pattern is valid
BT.1886 uses:
- exponent 2.4
- measured white luminance
- measured black luminance
A room-adapted mode can depart from the reference.
That departure should be:
- intentional
- measured where possible
- labeled
- reversible
For visual setup:
- use the best reference-oriented preset
- use valid patterns only
- leave multipoint controls alone
For measured setup:
- calculate the target
- measure the full grayscale
- correct broad errors first
- recheck white balance, clipping, ramps, and color
The next article covers color decoding.
The EOTF determines how bright the grayscale is.
Color decoding determines how the color components are interpreted within that luminance structure.
Sources and standards
Primary ITU SDR and HDR transfer-function recommendations and Spears & Munsil calibration-pattern guidance used in this article. Last verified August 6, 2026.
International Telecommunication Union Radiocommunication Sector. Reference Electro-Optical Transfer Function for Flat Panel Displays Used in HDTV Studio Production. Recommendation ITU-R BT.1886-0, March 2011.
↩↩↩↩↩
https://www.itu.int/dms_pubrec/itu-r/rec/bt/R-REC-BT.1886-0-201103-I%21%21PDF-E.pdfInternational Telecommunication Union Radiocommunication Sector. A Reference Viewing Environment for Evaluation of HDTV Program Material or Completed Programmes. Recommendation ITU-R BT.2035-0, July 2013.
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https://www.itu.int/dms_pubrec/itu-r/rec/bt/R-REC-BT.2035-0-201307-I%21%21PDF-E.pdfInternational Telecommunication Union Radiocommunication Sector. High Dynamic Range Television for Production and International Programme Exchange. Report ITU-R BT.2390-12, March 2025.
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https://www.itu.int/dms_pub/itu-r/opb/rep/R-REP-BT.2390-12-2025-PDF-E.pdfInternational Telecommunication Union Radiocommunication Sector. Image Parameter Values for High Dynamic Range Television for Use in Production and International Programme Exchange. Recommendation ITU-R BT.2100-3, February 2025.
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https://www.itu.int/dms_pubrec/itu-r/rec/bt/R-REC-BT.2100-3-202502-I%21%21PDF-E.pdfInternational Telecommunication Union Radiocommunication Sector. Specifications of PLUGE Test Signals and Alignment Procedures for Setting of Brightness and Contrast of Displays. Recommendation ITU-R BT.814-4, July 2018.
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https://www.itu.int/dms_pubrec/itu-r/rec/bt/R-REC-BT.814-4-201807-I%21%21PDF-E.pdfInternational Telecommunication Union Radiocommunication Sector. Guidelines for operational practices in high dynamic range television production. Report ITU-R BT.2408-9, March 2026.
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https://www.itu.int/pub/R-REP-BT.2408-9-2026Spears & Munsil. Pattern Help Text, 2nd Edition. Official calibration documentation, reviewed July 31, 2026.
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https://spearsandmunsil.com/portfolio-item/pattern-help-text/Spears & Munsil. Technical Notes on the Patterns. Official calibration documentation, reviewed July 31, 2026.
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https://spearsandmunsil.com/portfolio-item/technical-notes-on-the-patterns/Spears & Munsil. Getting Started with the Ultra HD Benchmark, 3rd Edition. Official calibration documentation, reviewed July 31, 2026.
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https://spearsandmunsil.com/portfolio-item/getting-started-with-the-ultrahd-benchmark-3rd-edition/