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BIBLIOGRAPHY.bib
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@article{Abasi2020a,
title = {Distance Metrics for Very Large Color Differences},
author = {Abasi, Saeedeh and Amani Tehran, Mohammad and Fairchild, Mark D.},
year = {2020},
month = apr,
journal = {Color Research \& Application},
volume = {45},
number = {2},
pages = {208--223},
issn = {0361-2317, 1520-6378},
doi = {10.1002/col.22451},
urldate = {2024-10-23},
abstract = {Abstract Small, supra-threshold color differences are typically described with Euclidean distance metrics, or dimension-weighted Euclidean metrics, in color appearance spaces such as CIELAB. This research examines the perception and modeling of very large color differences in the order of 10 CIELAB units or larger, with an aim of describing the salience of color differences between distinct objects in real-world scenes and images. A psychophysical experiment was completed to compare directly large color-difference pairs designed to probe various Euclidean and non-Euclidean distance metrics. The results indicate that very large color differences are best described by HyAB, a combination of a Euclidean metric in hue and chroma with a city-block metric to incorporate lightness differences.},
langid = {english},
file = {/Users/kelsolaar/Zotero/storage/FLS78JB7/Abasi et al. - 2020 - Distance metrics for very large color differences.pdf;/Users/kelsolaar/Zotero/storage/X345Z8RL/Abasi et al. - 2020 - Distance metrics for very large color differences.pdf}
}
@article{Abebe2017,
title = {Perceptual {{Lightness Modeling}} for {{High-Dynamic-Range Imaging}}},
author = {Abebe, Mekides Assefa and Pouli, Tania and Larabi, Mohamed-Chaker and Reinhard, Erik},
year = {2017},
month = jul,
journal = {ACM Transactions on Applied Perception},
volume = {15},
number = {1},
pages = {1--19},
issn = {15443558},
doi = {10.1145/3086577},
abstract = {{\copyright} 2017 ACM. The human visual system (HVS) non-linearly processes light from the real world, allowing us to perceive detail over a wide range of illumination. Although models that describe this non-linearity are constructed based on psycho-visual experiments, they generally apply to a limited range of illumination and therefore may not fully explain the behavior of theHVS under more extreme illumination conditions. We propose a modified experimental protocol for measuring visual responses to emissive stimuli that do not require participant training, nor requiring the exclusion of non-expert participants. Furthermore, the protocol can be applied to stimuli covering an extended luminance range. Based on the outcome of our experiment, we propose a new model describing lightness response over an extended luminance range. The model can be integrated with existing color appearance models or perceptual color spaces. To demonstrate the effectiveness of our model in high dynamic range applications, we evaluate its suitability for dynamic range expansion relative to existing solutions.},
file = {/Users/kelsolaar/Zotero/storage/PVZGMBRZ/Abebe et al. - 2017 - Perceptual Lightness Modeling for High-Dynamic-Ran.pdf;/Users/kelsolaar/Zotero/storage/V33CXH9X/Abebe et al. - 2017 - Perceptual Lightness Modeling for High-Dynamic-Range Imaging.pdf}
}
@misc{AdobeSystems2005a,
title = {Adobe {{RGB}} (1998) {{Color Image Encoding}}},
author = {{Adobe Systems}},
year = {2005},
file = {/Users/kelsolaar/Zotero/storage/Y9MJZ34N/Adobe Systems - 2005 - Adobe RGB (1998) Color Image Encoding.pdf}
}
@misc{AdobeSystems2013,
title = {Adobe {{DNG Software Development Kit}} ({{SDK}}) - 1.3.0.0 - Dng\_sdk\_1\_3/Dng\_sdk/Source/Dng\_temperature.Cpp::Dng\_temperature::{{Set}}\_xy\_coord},
author = {{Adobe Systems}},
year = {2013}
}
@misc{AdobeSystems2013a,
title = {Adobe {{DNG Software Development Kit}} ({{SDK}}) - 1.3.0.0 - Dng\_sdk\_1\_3/Dng\_sdk/Source/Dng\_temperature.Cpp::Dng\_temperature::Xy\_coord},
author = {{Adobe Systems}},
year = {2013}
}
@misc{AdobeSystems2013b,
title = {Cube {{LUT Specification}}},
author = {{Adobe Systems}},
year = {2013},
keywords = {Iridas,look-up table,specification},
file = {/Users/kelsolaar/Zotero/storage/LLPBPADA/Adobe Systems - 2013 - Cube LUT Specification.pdf}
}
@misc{ANSI2003a,
title = {Specification of {{ROMM RGB}}},
author = {{ANSI}},
year = {2003},
pages = {1--2},
file = {/Users/kelsolaar/Zotero/storage/HKFYZ5YF/ANSI - 2003 - Specification of ROMM RGB.pdf}
}
@book{ANSI2018,
title = {{{ANSI}}/{{IES TM-30-18}} - {{IES Method}} for {{Evaluating Light Source Color Rendition}}},
author = {{ANSI} and {IES Color Committee}},
year = {2018},
publisher = {ANSI/IES},
isbn = {978-0-87995-379-9},
annotation = {[email protected]},
file = {/Users/kelsolaar/Zotero/storage/GIU9NWLP/TM-30-18_tools_etc.zip;/Users/kelsolaar/Zotero/storage/JZHTHWRW/ANSI and IES Color Committee - ANSIIES TM-30-18 - IES Method for Evaluating Ligh.pdf}
}
@misc{AppleInc.2019,
title = {{{displayP3}}},
author = {{Apple Inc.}},
year = {2019},
urldate = {2019-12-18},
howpublished = {https://developer.apple.com/documentation/coregraphics/cgcolorspace/1408916-displayp3}
}
@misc{AppleInc.2023,
title = {Apple {{Log Profile White Paper}}},
author = {{Apple Inc.}},
year = {2023},
langid = {english},
file = {/Users/kelsolaar/Zotero/storage/E3QYPTPS/2023 - Apple Log Profile White Paper.pdf}
}
@misc{ARRI2012a,
title = {{{ALEXA}} - {{Log C Curve}} - {{Usage}} in {{VFX}}},
author = {{ARRI}},
year = {2012},
file = {/Users/kelsolaar/Zotero/storage/JIDE329W/ARRI - 2012 - ALEXA - Log C Curve - Usage in VFX.pdf}
}
@misc{AssociationofRadioIndustriesandBusinesses2015a,
title = {Essential {{Parameter Values}} for the {{Extended Image Dynamic Range Television}} ({{EIDRTV}}) {{System}} for {{Programme Production}}},
author = {{Association of Radio Industries and Businesses}},
year = {2015},
file = {/Users/kelsolaar/Zotero/storage/UK6PZDJ4/Association of Radio Industries and Businesses - 2015 - Essential Parameter Values for the Extended Image Dynamic Range Television (EIDR.pdf}
}
@misc{ASTMInternational1989a,
title = {{{ASTM D1535-89}} - {{Standard Practice}} for {{Specifying Color}} by the {{Munsell System}}},
author = {{ASTM International}},
year = {1989},
pages = {1--29},
urldate = {2014-09-25},
keywords = {color,D1535,Munsell,Munsell color order system,Munsell notation},
file = {/Users/kelsolaar/Zotero/storage/L25FKG5G/ASTM International - 1989 - ASTM D1535-89 - Standard Practice for Specifying Color by the Munsell System.pdf}
}
@misc{ASTMInternational2007,
title = {{{ASTM D2244-07}} - {{Standard Practice}} for {{Calculation}} of {{Color Tolerances}} and {{Color Differences}} from {{Instrumentally Measured Color Coordinates}}},
author = {{ASTM International}},
year = {2007},
volume = {i},
pages = {1--10},
doi = {10.1520/D2244-16},
file = {/Users/kelsolaar/Zotero/storage/XJCF7QV3/ASTM International - 2007 - ASTM D2244-07 - Standard Practice for Calculation of Color Tolerances and Color Differences from Instrumenta.pdf}
}
@misc{ASTMInternational2008a,
title = {{{ASTM D1535-08e1}} - {{Standard Practice}} for {{Specifying Color}} by the {{Munsell System}}},
author = {{ASTM International}},
year = {2008},
doi = {10.1520/D1535-08E01}
}
@misc{ASTMInternational2011a,
title = {{{ASTM E2022-11}} - {{Standard Practice}} for {{Calculation}} of {{Weighting Factors}} for {{Tristimulus Integration}}},
author = {{ASTM International}},
year = {2011},
pages = {1--10},
doi = {10.1520/E2022-11},
abstract = {This standard is issued under the fixed designation E2022; the number immediately following the designation indicates the year of original adoption or, in the case of revision, the year of last revision. A number in parentheses indicates the year of last reapproval. A superscript epsilon) indicates an editorial change since the last revision or reapproval.},
file = {/Users/kelsolaar/Zotero/storage/YAYJ5HAI/ASTM International - 2011 - ASTM E2022-11 - Standard Practice for Calculation of Weighting Factors for Tristimulus Integration.pdf}
}
@misc{ASTMInternational2015,
title = {{{ASTM E313-15e1}} - {{Standard Practice}} for {{Calculating Yellowness}} and {{Whiteness Indices}} from {{Instrumentally Measured Color Coordinates}}},
author = {{ASTM International}},
year = {2015},
doi = {10.1520/E0313-20},
file = {/Users/kelsolaar/Zotero/storage/WXZIPWTS/ASTM International - ASTM E313-15e1 - Standard Practice for Calculating.pdf}
}
@misc{ASTMInternational2015b,
title = {{{ASTM E308-15}} - {{Standard Practice}} for {{Computing}} the {{Colors}} of {{Objects}} by {{Using}} the {{CIE System}}},
author = {{ASTM International}},
year = {2015},
pages = {1--47},
doi = {10.1520/E0308-15},
file = {/Users/kelsolaar/Zotero/storage/6NCHYYI5/ASTM International - 2015 - ASTM E308-15 - Standard Practice for Computing the Colors of Objects by Using the CIE System.pdf}
}
@misc{ASWFColorInteropForum2024,
title = {Color {{Space Encodings}} for {{Texture Assets}} and {{CG Rendering}}},
author = {{ASWF Color Interop Forum}},
year = {2024},
month = oct
}
@misc{BabelColor2012b,
title = {The {{ColorChecker}} (since 1976!)},
author = {{BabelColor}},
year = {2012},
urldate = {2014-09-26},
howpublished = {http://www.babelcolor.com/main\_level/ColorChecker.htm}
}
@misc{BabelColor2012c,
title = {{{ColorChecker RGB}} and Spectra},
author = {{BabelColor}},
year = {2012},
file = {/Users/kelsolaar/Zotero/storage/BASARME2/BabelColor - 2012 - ColorChecker RGB and spectra.xls}
}
@book{Barten1999,
title = {Contrast {{Sensitivity}} of the {{Human Eye}} and {{Its Effects}} on {{Image Quality}}},
author = {Barten, Peter G.},
year = {1999},
month = dec,
number = {1999},
publisher = {SPIE},
issn = {10924388},
doi = {10.1117/3.353254},
isbn = {978-0-8194-7849-8},
pmid = {18723593},
file = {/Users/kelsolaar/Zotero/storage/A35HIELA/Barten - 1999 - Contrast Sensitivity of the Human Eye and Its Effects on Image Quality.pdf}
}
@inproceedings{Barten2003,
title = {Formula for the Contrast Sensitivity of the Human Eye},
booktitle = {Proceedings of {{SPIE}}},
author = {Barten, Peter G. J.},
editor = {Miyake, Yoichi and Rasmussen, D. Rene},
year = {2003},
month = dec,
volume = {5294},
pages = {231--238},
issn = {0277786X},
doi = {10.1117/12.537476},
abstract = {The contrast sensitivity of the human eye and its dependence on luminance and display size is described on the basis of internal noise in the visual system. With the addition of a global description of the optical MTF of the eye, a complete physical model is presented for the spatial contrast sensitivity function. Calculation results obtained with this model are compared with measurements published in literature.},
isbn = {0-8194-3496-5},
keywords = {contrast sensitivity,csf,human eye,orientation angle,standard observer,surround luminance}
}
@article{Bianco2010a,
title = {Two New von {{Kries}} Based Chromatic Adaptation Transforms Found by Numerical Optimization},
author = {Bianco, S. and Schettini, R.},
year = {2010},
month = jun,
journal = {Color Research \& Application},
volume = {35},
number = {3},
pages = {184--192},
issn = {03612317},
doi = {10.1002/col.20573},
urldate = {2014-09-26},
file = {/Users/kelsolaar/Zotero/storage/9MT6YK3T/Bianco, Schettini - 2010 - Two new von Kries based chromatic adaptation transforms found by numerical optimization.pdf}
}
@misc{BlackmagicDesign2020,
title = {{{DaVinci Wide Gamut}} - {{DaVinci Resolve Studio}} 17 {{Public Beta}} 1},
author = {{Blackmagic Design}},
year = {2020},
month = nov
}
@misc{BlackmagicDesign2020a,
title = {Wide {{Gamut Intermediate DaVinci Resolve}}},
author = {{Blackmagic Design}},
year = {2020},
urldate = {2020-12-12},
file = {/Users/kelsolaar/Zotero/storage/QRUMYRLW/Blackmagic Design - 2020 - Wide Gamut Intermediate DaVinci Resolve.pdf}
}
@misc{BlackmagicDesign2021,
title = {Blackmagic {{Generation}} 5 {{Color Science}}},
author = {{Blackmagic Design}},
year = {2021},
file = {/Users/kelsolaar/Zotero/storage/UHWCNCMJ/Blackmagic Design - 2021 - Blackmagic Generation 5 Color Science.pdf}
}
@article{Bodhaine1999a,
title = {On {{Rayleigh Optical Depth Calculations}}},
author = {Bodhaine, Barry A. and Wood, Norman B. and Dutton, Ellsworth G. and Slusser, James R.},
year = {1999},
month = nov,
journal = {Journal of Atmospheric and Oceanic Technology},
volume = {16},
number = {11},
pages = {1854--1861},
issn = {0739-0572},
doi = {10.1175/1520-0426(1999)016<1854:ORODC>2.0.CO;2},
urldate = {2014-09-25},
abstract = {Many different techniques are used for the calculation of Rayleigh optical depth in the atmosphere. In some cases differences among these techniques can be important, especially in the UV region of the spectrum and under clean atmospheric conditions. The authors recommend that the calculation of Rayleigh optical depth be approached by going back to the first principles of Rayleigh scattering theory rather than the variety of curve- fitting techniques currently in use. A survey of the literature was conducted in order to determine the latest values of the physical constants necessary and to review the methods available for the calculation of Rayleigh optical depth. The recommended approach requires the accurate calculation of the refractive index of air based on the latest published measurements. Calculations estimating Rayleigh optical depth should be done as accurately as possible because the inaccuracies that arise can equal or even exceed other quantities being estimated, such as aerosol optical depth, particularly in the UV region of the spectrum. All of the calculations are simple enough to be done easily in a spreadsheet.},
file = {/Users/kelsolaar/Zotero/storage/GP3Y5RGW/Bodhaine et al. - 1999 - On Rayleigh Optical Depth Calculations.pdf}
}
@misc{Borer2017a,
title = {Private {{Discussion}} with {{Mansencal}}, {{T}}. and {{Shaw}}, {{N}}.},
author = {Borer, Tim},
year = {2017}
}
@misc{Bourkea,
title = {Intersection Point of Two Line Segments in 2 Dimensions},
author = {Bourke, Paul},
urldate = {2016-01-15},
howpublished = {http://paulbourke.net/geometry/pointlineplane/}
}
@misc{Bourkeb,
title = {Trilinear {{Interpolation}}},
author = {Bourke, Paul},
urldate = {2018-01-13},
howpublished = {http://paulbourke.net/miscellaneous/interpolation/}
}
@article{Breneman1987b,
title = {Corresponding Chromaticities for Different States of Adaptation to Complex Visual Fields},
author = {Breneman, Edwin J.},
year = {1987},
month = jun,
journal = {Journal of the Optical Society of America A},
volume = {4},
number = {6},
pages = {1115},
issn = {1084-7529},
doi = {10.1364/JOSAA.4.001115},
urldate = {2014-09-27},
abstract = {While each of his or her two eyes was independently adapted to a different illuminant in viewing a complex visual field, each of a number of observers matched a series of test colors seen by one eye with a juxtaposed variable stimulus seen by the other eye. The 2 degrees test and matching stimuli were located centrally in the complex adapting field, which subtended an angle of 31 degrees X 24 degrees. In making the matches, the observer viewed the test and matching stimuli for a series of brief intervals (approximately 1 sec) while viewing the complex adapting field with normal eye movements. Nine experiments were performed with different pairs of illuminants and different illuminances ranging from that of an average living room to that of a scene illuminated with hazy sunlight. In three other experiments each of the observer's two eyes was adapted to a different illuminance of D55. The amount of adaptation was more nearly complete at high levels of illuminance than at low levels, and the proportional amount of adaptation was less for the "blue" receptors. When adaptation coefficients were determined from the actual adaptation differences (e.g., from corresponding tristimulus values for matching neutrals) rather than from the adapting illuminants, a linear von Kries transformation based on experimentally determined visual primaries gave corresponding chromaticities that were in good agreement with the results obtained in each of the chromatic-adaptation experiments, except at the lowest illuminances. The results of the experiments in which each eye was adapted to different levels of the same illuminant indicated again that adaptation to the different levels was incomplete, the proportional amount of adaptation being less at low illuminances and for the "blue" receptors. This caused a change in chromatic adaptation with the level of illuminance even when the chromaticities of the adapting lights were equal. The results of these experiments also indicated that higher purities are needed in order to produce the same absolute color appearances at low levels of illuminance.},
pmid = {3598755},
file = {/Users/kelsolaar/Zotero/storage/3PERLZ56/Breneman - 1987 - Corresponding chromaticities for different states of adaptation to complex visual fields(2).pdf;/Users/kelsolaar/Zotero/storage/Y6Z63Q67/Breneman - 1987 - Corresponding chromaticities for different states of adaptation to complex visual fields.pdf}
}
@article{Brill2008a,
title = {Repairing Gamut Problems in {{CIECAM02}}: {{A}} Progress Report},
author = {Brill, Michael H. and Susstrunk, Sabine},
year = {2008},
month = oct,
journal = {Color Research \& Application},
volume = {33},
number = {5},
pages = {424--426},
issn = {03612317},
doi = {10.1002/col.20432},
urldate = {2014-10-02},
abstract = {The color-appearance model CIECAM02 has several problems. which can result in mathematical instabilities, due to the position of the chromatic-adaptation primaries relative to the spectrum locus and to the presumed physiological cone primaries. To keep a corresponding (adapted) color within the positive gamut given by the chromatic adaptation primaries, the gamut must he within the cone primary octant. To contain adapted colors within the positive cone-primary octan, it suffices to truncate the action of adaptation at the boundary of that octant. Such modifications may be needed to avoid the mathematical problems in CIECAM02.},
keywords = {Chromatic adaptation,CIECAM02,Color appearance,Gamut,Model,Primary}
}
@misc{Broadbent2009a,
title = {Calculation from the {{Original Experimental Data}} of the {{Cie}} 1931 {{RGB Standard Observer Spectral Chromaticity Co-Ordinates}} and {{Color Matching Functions}}.},
author = {Broadbent, A. D.},
year = {2009},
journal = {Qu{\'e}bec, Canada: D{\'e}partement de g{\'e}nie chimique, {\dots}},
pages = {1--17},
urldate = {2014-06-12},
abstract = {This paper describes all the steps in the calculations of the CIE 1931 RGB spectral chromaticity co-ordinates and color matching functions starting from the initial experimental data of W. D. Wright and J. Guild. Sufficient information is given to allow the reader to reproduce and verify the results obtained at each stage of the calculations and to critically analyze the procedures used. In some instances, the available literature only provides limited descriptions of the actual steps in the calculations and, in others, important data were not published. Nevertheless, it has been possible to more or less reproduce the entire sequence of calculations. All the tables of numerical data are given in the accompanying computer worksheet file CIE1931\_RGB.xls.},
howpublished = {http://www.cis.rit.edu/mcsl/research/1931.php},
file = {/Users/kelsolaar/Zotero/storage/N5MAJMIE/Broadbent - 2009 - Calculation from the Original Experimental Data of the Cie 1931 RGB Standard Observer Spectral Chromaticity Co-Ordina.pdf}
}
@book{Burger2009b,
title = {Principles of {{Digital Image Processing}}},
author = {Burger, Wilhelm and Burge, Mark James},
year = {2009},
publisher = {Springer London},
address = {London},
doi = {10.1007/978-1-84800-195-4},
isbn = {978-1-84800-194-7}
}
@misc{Cabello2015,
title = {{{PlaneGeometry}}.Js},
author = {Cabello, Ricardo},
urldate = {2015-05-12},
howpublished = {https://github.com/mrdoob/three.js/blob/dev/src/geometries/PlaneGeometry.js}
}
@misc{Canon2014a,
title = {{{EOS C500 Firmware Update}}},
author = {{Canon}},
year = {2014},
urldate = {2016-08-27},
howpublished = {https://www.usa.canon.com/internet/portal/us/home/explore/product-showcases/cameras-and-lenses/cinema-eos-firmware/c500}
}
@misc{Canon2016,
title = {Input {{Transform Version}} 201612 for {{EOS C300 Mark II}}},
author = {{Canon}},
year = {2016},
urldate = {2016-08-23},
howpublished = {https://www.usa.canon.com/internet/portal/us/home/support/details/cameras/cinema-eos/eos-c300-mark-ii}
}
@misc{Canon2020,
title = {Input {{Transform Version}} 202007 for {{EOS C300 Mark II}}},
author = {{Canon}},
year = {2020},
urldate = {2023-07-16},
howpublished = {https://www.usa.canon.com/internet/portal/us/home/support/details/cameras/cinema-eos/eos-c300-mark-ii}
}
@article{Cao2013,
title = {Comparison of the Performance of Inverse Transformation Methods from {{OSA-UCS}} to {{CIEXYZ}}},
author = {Cao, Renbo and Trussell, H Joel and Shamey, Renzo},
year = {2013},
month = aug,
journal = {Journal of the Optical Society of America A},
volume = {30},
number = {8},
pages = {1508},
issn = {1084-7529},
doi = {10.1364/JOSAA.30.001508},
abstract = {The Optical Society of America's Uniform Color Scales (OSA-UCS) is one of the color spaces that most closely approximate a "true" uniform color space. Different techniques have been used to convert OSA-UCS-based color specification parameters, L, j, and g, to the CIE tristimulus values, X, Y, and Z. However, none of these methods provides a direct method of inverting OSA-UCS to CIEXYZ values. Thus, numerical algorithms, such as the Newton-Raphson method, have been employed to obtain the transformations. The relative low accuracy and long computation time of this method makes it undesirable for practical applications. An artificial neural network (ANN) was employed to convert OSA-UCS to CIEXYZ. Its performance was compared with that of numerical methods. After optimization, ANN gave a better performance with a mean error (DeltaEXYZ) of 1.0x10(-4) and a conversion time of less than 1 s for 1891 samples.},
isbn = {1520-8532 (Electronic){\textbackslash}r1084-7529 (Linking)},
pmid = {24323208},
file = {/Users/kelsolaar/Zotero/storage/NIFLE5ID/Cao, Trussell, Shamey - 2013 - Comparison of the performance of inverse transformation methods from OSA-UCS to CIEXYZ.pdf}
}
@techreport{Carter2018,
title = {{{CIE}} 015:2018 {{Colorimetry}}, 4th {{Edition}}},
author = {Carter, E.C. and Schanda, J.D. and Hirschler, R. and Jost, S. and Luo, M.R. and Melgosa, M. and Ohno, Y. and Pointer, M.R. and Rich, D.C. and Vienot, F. and Whitehead, L. and Wold, J.H.},
year = {2018},
month = oct,
address = {Vienna},
institution = {International Commission on Illumination},
doi = {10.25039/TR.015.2018},
isbn = {9783902842138},
file = {/Users/kelsolaar/Zotero/storage/YH47BDDY/Carter et al. - 2018 - CIE 0152018 Colorimetry, 4th Edition.pdf}
}
@misc{Castro2014a,
title = {Numpy: {{Fastest}} Way of Computing Diagonal for Each Row of a 2d Array},
author = {Castro, Saullo},
year = {2014},
urldate = {2014-08-22},
howpublished = {http://stackoverflow.com/questions/26511401/numpy-fastest-way-of-computing-diagonal-for-each-row-of-a-2d-array/26517247\#26517247}
}
@article{Centore2012a,
title = {An Open-Source Inversion Algorithm for the {{Munsell}} Renotation},
author = {Centore, Paul},
year = {2012},
month = dec,
journal = {Color Research \& Application},
volume = {37},
number = {6},
pages = {455--464},
issn = {03612317},
doi = {10.1002/col.20715},
urldate = {2014-09-26},
keywords = {algorithm,inverse renotation,munsell,open source,renotation},
file = {/Users/kelsolaar/Zotero/storage/QB5MY39J/Centore - 2012 - An open-source inversion algorithm for the Munsell renotation.pdf}
}
@misc{Centore2014k,
title = {{{MunsellAndKubelkaMunkToolboxApr2014}} - {{MunsellRenotationRoutines}}/{{MunsellHueToASTMHue}}.m},
author = {Centore, Paul},
year = {2014}
}
@misc{Centore2014l,
title = {{{MunsellAndKubelkaMunkToolboxApr2014}} - {{MunsellSystemRoutines}}/{{LinearVsRadialInterpOnRenotationOvoid}}.m},
author = {Centore, Paul},
year = {2014}
}
@misc{Centore2014m,
title = {{{MunsellAndKubelkaMunkToolboxApr2014}} - {{MunsellRenotationRoutines}}/{{MunsellToxyY}}.m},
author = {Centore, Paul},
year = {2014}
}
@misc{Centore2014n,
title = {{{MunsellAndKubelkaMunkToolboxApr2014}} - {{MunsellRenotationRoutines}}/{{FindHueOnRenotationOvoid}}.m},
author = {Centore, Paul},
year = {2014}
}
@misc{Centore2014o,
title = {{{MunsellAndKubelkaMunkToolboxApr2014}} - {{MunsellSystemRoutines}}/{{BoundingRenotationHues}}.m},
author = {Centore, Paul},
year = {2014}
}
@misc{Centore2014p,
title = {{{MunsellAndKubelkaMunkToolboxApr2014}} - {{MunsellRenotationRoutines}}/{{xyYtoMunsell}}.m},
author = {Centore, Paul},
year = {2014}
}
@misc{Centore2014q,
title = {{{MunsellAndKubelkaMunkToolboxApr2014}} - {{MunsellRenotationRoutines}}/{{MunsellToxyForIntegerMunsellValue}}.m},
author = {Centore, Paul},
year = {2014}
}
@misc{Centore2014r,
title = {{{MunsellAndKubelkaMunkToolboxApr2014}} - {{MunsellRenotationRoutines}}/{{MaxChromaForExtrapolatedRenotation}}.m},
author = {Centore, Paul},
year = {2014}
}
@misc{Centore2014s,
title = {{{MunsellAndKubelkaMunkToolboxApr2014}} - {{MunsellRenotationRoutines}}/{{MunsellHueToChromDiagHueAngle}}.m},
author = {Centore, Paul},
year = {2014}
}
@misc{Centore2014t,
title = {{{MunsellAndKubelkaMunkToolboxApr2014}} - {{MunsellRenotationRoutines}}/{{ChromDiagHueAngleToMunsellHue}}.m},
author = {Centore, Paul},
year = {2014}
}
@misc{Centore2014u,
title = {{{MunsellAndKubelkaMunkToolboxApr2014}} - {{GeneralRoutines}}/{{CIELABtoApproxMunsellSpec}}.m},
author = {Centore, Paul},
year = {2014}
}
@misc{Centorea,
title = {The {{Munsell}} and {{Kubelka-Munk Toolbox}}},
author = {Centore, Paul},
urldate = {2018-01-23},
howpublished = {http://www.munsellcolourscienceforpainters.com/MunsellAndKubelkaMunkToolbox/MunsellAndKubelkaMunkToolbox.html}
}
@misc{Chamberlain2015,
title = {{{LUT}} Documentation (to Create from Another Program)},
author = {Chamberlain, Peter},
year = {2015},
urldate = {2018-08-23},
howpublished = {https://forum.blackmagicdesign.com/viewtopic.php?f=21\&t=40284\#p232952}
}
@article{Cheung2004,
title = {A Comparative Study of the Characterisation of Colour Cameras by Means of Neural Networks and Polynomial Transforms},
author = {Cheung, Vien and Westland, Stephen and Connah, David and Ripamonti, Caterina},
year = {2004},
journal = {Coloration Technology},
volume = {120},
number = {1},
pages = {19--25},
issn = {14723581},
doi = {10.1111/j.1478-4408.2004.tb00201.x},
abstract = {The proliferation of low-cost colour imaging devices in the consumer market has led to a greater need to transfer images from one medium or device to another without loss of colour fidelity. A common solution is to characterise each device in terms of its CIE tristimulus values. In this paper two general techniques, artificial neural networks and polynomial transforms, are compared for their usefulness in characterising colour cameras. The neural and polynomial techniques are shown to give approximately similar performance once the parameters of the models are optimised. Since neural networks can be difficult and time-consuming to train, it is concluded that polynomial transforms offer the better alternative for camera characterisation.},
file = {/Users/kelsolaar/Zotero/storage/D4IVRZWP/Cheung et al. - 2004 - A comparative study of the characterisation of colour cameras by means of neural networks and polynomial transfor.pdf}
}
@misc{CIE2024,
title = {Spectral Radiance Factors of Test-Colour Sample \#15 of the {{Japanese}} Skin Complexion, 5nm Wavelength Steps},
author = {{CIE}},
year = {2024},
publisher = {International Commission on Illumination (CIE)},
doi = {10.25039/CIE.DS.7chm7z5h},
urldate = {2025-03-17},
abstract = {Spectral radiance factors of test-colour sample \#15 of the Japanese skin complexion, {$\beta$}15({$\lambda$}), 5nm wavelength steps, original source: CIE 253:2024 Table B.1}
}
@misc{CIEce,
title = {{{CIE}} 15:2004 {{Tables Data}}},
author = {{CIE}},
year = {2004},
file = {/Users/kelsolaar/Zotero/storage/R95FLNMC/CIE - 2004 - CIE 152004 Tables Data.xls}
}
@misc{CIEcf,
title = {{{CIE Spectral Data}}},
author = {{CIE}},
file = {/Users/kelsolaar/Zotero/storage/SH9FS2YZ/CIE - Unknown - CIE Spectral Data.xls}
}
@book{CIEDivision12022,
title = {{{CIE}} 248:2022 {{The CIE}} 2016 {{Colour Appearance Model}} for {{Colour Management Systems}}: {{CIECAM16}}},
author = {{CIE Division 1} and {CIE Division 8}},
year = {2022},
publisher = {Commission Internationale de l'Eclairage},
isbn = {978-3-902842-94-7},
file = {/Users/kelsolaar/Zotero/storage/5LMUJ936/CIE Division 1Division 8 - 2022 - CIE 2482022 The CIE 2016 Colour Appearance Model .pdf}
}
@book{CIETC1-321994b,
title = {{{CIE}} 109-1994 {{A Method}} of {{Predicting Corresponding Colours}} under {{Different Chromatic}} and {{Illuminance Adaptations}}},
author = {{CIE TC 1-32}},
year = {1994},
publisher = {Commission Internationale de l'Eclairage},
isbn = {978-3-900734-51-0},
file = {/Users/kelsolaar/Zotero/storage/MFXWLR4T/CIE TC 1-32 - 1994 - CIE 109-1994 A Method of Predicting Corresponding Colours under Different Chromatic and Illuminance Adaptations.pdf}
}
@book{CIETC1-362006a,
title = {{{CIE}} 170-1:2006 {{Fundamental Chromaticity Diagram}} with {{Physiological Axes}} - {{Part}} 1},
author = {{CIE TC 1-36}},
year = {2006},
publisher = {Commission Internationale de l'Eclairage},
isbn = {978-3-901906-46-6},
file = {/Users/kelsolaar/Zotero/storage/8KV64XHT/CIE TC 1-36 - 2006 - CIE 170-12006 Fundamental Chromaticity Diagram with Physiological Axes - Part 1.pdf}
}
@incollection{CIETC1-382005e,
title = {9. {{INTERPOLATION}}},
booktitle = {{{CIE}} 167:2005 {{Recommended Practice}} for {{Tabulating Spectral Data}} for {{Use}} in {{Colour Computations}}},
author = {{CIE TC 1-38}},
year = {2005},
pages = {14--19},
isbn = {978-3-901906-41-1}
}
@incollection{CIETC1-382005f,
title = {9.2.4 {{Method}} of Interpolation for Uniformly Spaced Independent Variable},
booktitle = {{{CIE}} 167:2005 {{Recommended Practice}} for {{Tabulating Spectral Data}} for {{Use}} in {{Colour Computations}}},
author = {{CIE TC 1-38}},
year = {2005},
pages = {1--27},
isbn = {978-3-901906-41-1}
}
@incollection{CIETC1-382005g,
title = {{{EXTRAPOLATION}}},
booktitle = {{{CIE}} 167:2005 {{Recommended Practice}} for {{Tabulating Spectral Data}} for {{Use}} in {{Colour Computations}}},
author = {{CIE TC 1-38}},
year = {2005},
pages = {19--20},
isbn = {978-3-901906-41-1}
}
@incollection{CIETC1-382005h,
title = {Table {{V}}. {{Values}} of the c-Coefficients of {{Equ}}.s 6 and 7.},
booktitle = {{{CIE}} 167:2005 {{Recommended Practice}} for {{Tabulating Spectral Data}} for {{Use}} in {{Colour Computations}}},
author = {{CIE TC 1-38}},
year = {2005},
pages = {19},
isbn = {978-3-901906-41-1}
}
@incollection{CIETC1-482004,
title = {{{EXPLANATORY COMMENTS}} - 5},
booktitle = {{{CIE}} 015:2004 {{Colorimetry}}, 3rd {{Edition}}},
author = {{CIE TC 1-48}},
year = {2004},
pages = {68--68},
isbn = {978-3-901906-33-6}
}
@book{CIETC1-482004h,
title = {{{CIE}} 015:2004 {{Colorimetry}}, 3rd {{Edition}}},
author = {{CIE TC 1-48}},
year = {2004},
journal = {CIE 015:2004 Colorimetry, 3rd Edition},
publisher = {Commission Internationale de l'Eclairage},
isbn = {978-3-901906-33-6},
file = {/Users/kelsolaar/Zotero/storage/2RNVBZQX/CIE TC 1-48 - 2004 - CIE 0152004 Colorimetry, 3rd Edition.pdf}
}
@incollection{CIETC1-482004i,
title = {{{APPENDIX E}}. {{INFORMATION ON THE USE OF PLANCK}}'{{S EQUATION FOR STANDARD AIR}}},
booktitle = {{{CIE}} 015:2004 {{Colorimetry}}, 3rd {{Edition}}},
author = {{CIE TC 1-48}},
year = {2004},
pages = {77--82},
isbn = {978-3-901906-33-6},
file = {/Users/kelsolaar/Zotero/storage/6J5GE7WN/CIE TC 1-48 - 2004 - APPENDIX E. INFORMATION ON THE USE OF PLANCK'S EQUATION FOR STANDARD AIR.pdf}
}
@incollection{CIETC1-482004j,
title = {{{CIE}} 1976 Uniform Chromaticity Scale Diagram ({{UCS}} Diagram)},
booktitle = {{{CIE}} 015:2004 {{Colorimetry}}, 3rd {{Edition}}},
author = {{CIE TC 1-48}},
year = {2004},
pages = {24},
isbn = {978-3-901906-33-6}
}
@incollection{CIETC1-482004k,
title = {The Evaluation of Whiteness},
booktitle = {{{CIE}} 015:2004 {{Colorimetry}}, 3rd {{Edition}}},
author = {{CIE TC 1-48}},
year = {2004},
pages = {24},
isbn = {978-3-901906-33-6}
}
@incollection{CIETC1-482004l,
title = {Extrapolation},
booktitle = {{{CIE}} 015:2004 {{Colorimetry}}, 3rd {{Edition}}},
author = {{CIE TC 1-48}},
year = {2004},
pages = {24},
isbn = {978-3-901906-33-6}
}
@incollection{CIETC1-482004m,
title = {{{CIE}} 1976 Uniform Colour Spaces},
booktitle = {{{CIE}} 015:2004 {{Colorimetry}}, 3rd {{Edition}}},
author = {{CIE TC 1-48}},
year = {2004},
pages = {24},
isbn = {978-3-901906-33-6}
}
@incollection{CIETC1-482004n,
title = {3.1 {{Recommendations}} Concerning Standard Physical Data of Illuminants},
booktitle = {{{CIE}} 015:2004 {{Colorimetry}}, 3rd {{Edition}}},
author = {{CIE TC 1-48}},
year = {2004},
pages = {12--13},
isbn = {978-3-901906-33-6}
}
@incollection{CIETC1-482004o,
title = {9.1 {{Dominant}} Wavelength and Purity},
booktitle = {{{CIE}} 015:2004 {{Colorimetry}}, 3rd {{Edition}}},
author = {{CIE TC 1-48}},
year = {2004},
pages = {32--33},
isbn = {978-3-901906-33-6}
}
@book{CIETC1-902017,
title = {{CIE 2017 colour fidelity index for accurate scientific use}},
author = {{CIE TC 1-90}},
year = {2017},
series = {{Technical report / CIE}},
number = {224},
publisher = {CIE Central Bureau},
address = {Vienna},
isbn = {978-3-902842-61-9},
langid = {eng fre ger},
annotation = {OCLC: 988568299},
file = {/Users/kelsolaar/Zotero/storage/HSG7SBTW/CIE TC 1-90 - 2017 - CIE 2017 colour fidelity index for accurate scient.pdf;/Users/kelsolaar/Zotero/storage/JQGCSM8S/933_TC1-90.zip}
}
@misc{Colblindora,
title = {Deuteranopia - {{Red-Green Color Blindness}}},
author = {{Colblindor}},
urldate = {2015-07-04},
howpublished = {http://www.color-blindness.com/deuteranopia-red-green-color-blindness/}
}
@misc{Colblindorb,
title = {Protanopia - {{Red-Green Color Blindness}}},
author = {{Colblindor}},
urldate = {2015-07-04},
howpublished = {http://www.color-blindness.com/protanopia-red-green-color-blindness/}
}
@misc{Colblindorc,
title = {Tritanopia - {{Blue-Yellow Color Blindness}}},
author = {{Colblindor}},
urldate = {2015-07-04},
howpublished = {http://www.color-blindness.com/tritanopia-blue-yellow-color-blindness/}
}
@misc{Cooper2022,
title = {{{ARRI LogC4 Logarithmic Color Space SPECIFICATION}}},
author = {Cooper, Sean and Brendel, Harald},
year = {2022},
urldate = {2022-10-24},
file = {/Users/kelsolaar/Zotero/storage/GKDQLNEX/Cooper and Brendel - 2022 - ARRI LogC4 Logarithmic Color Space SPECIFICATION.pdf}
}
@misc{Cottrella,
title = {The {{Russell RGB}} Working Color Space},
author = {Cottrell, Russell}
}
@article{Cowan2004,
title = {Contrast {{Sensitivity Experiment}} to {{Determine}} the {{Bit Depth}} for {{Digital Cinema}}},
author = {Cowan, Matthew and Kennel, Glenn and Maier, Thomas and Walker, Brad},
year = {2004},
month = sep,
journal = {SMPTE Motion Imaging Journal},
volume = {113},
number = {9},
pages = {281--292},
issn = {2160-2492},
doi = {10.5594/j11549},
abstract = {The SMPTE Color ad hoc group was formed in 2001 (under DC28.2) to investigate the colorimetric requirements for the Digital Cinema Distribution Master (DCDM). A draft specification on color image encoding was published in September 2002 that recommended the use of XYZ color space, a gamma 1/2.6 transfer function, and 12 bits per color. With the support of Digital Cinema Initiatives (DCI), a test was designed to verify these color image encoding parameters. This paper reports the results of the contrast sensitivity experiment, which showed that many of our observers could see a modulation corresponding to a one code value change with 10-bit encoding, but few observers would see a one-code value change with 12-bit encoding. This result matches the results of published contrast sensitivity experiments.},
file = {/Users/kelsolaar/Zotero/storage/72ZNEKRS/Cowan et al. - 2004 - Contrast Sensitivity Experiment to Determine the B.pdf;/Users/kelsolaar/Zotero/storage/QPYY7VA7/Cowan et al. - 2004 - Constant Sensitivity Experiment to Determine the Bit Depth for Digital Cinema.pdf;/Users/kelsolaar/Zotero/storage/5UAUS78N/7262492.html}
}
@article{Cui2002,
ids = {Cui2002a},
title = {Uniform Colour Spaces Based on the {{DIN99}} Colour-Difference Formula},
author = {Cui, G. and Luo, M. R. and Rigg, B. and Roesler, G. and Witt, K.},
year = {2002},
journal = {Color Research \& Application},
volume = {27},
number = {4},
pages = {282--290},
issn = {1520-6378},
doi = {10.1002/col.10066},
urldate = {2021-01-21},
abstract = {Several colour-difference formulas such as CMC, CIE94, and CIEDE2000 have been developed by modifying CIELAB. These formulas give much better fits for experimental data based on small colour differences than does CIELAB. None of these has an associated uniform colour space (UCS). The need for a UCS is demonstrated by the widespread use of the a*b* diagram despite the lack of uniformity. This article describes the development of formulas, with the same basic structure as the DIN99 formula, that predict the experimental data sets better than do the CMC and CIE94 colour-difference formulas and only slightly worse than CIEDE2000 (which was optimized on the experimental data). However, these formulas all have an associated UCS. The spaces are similar in form to L*a*b*. {\copyright} 2002 Wiley Periodicals, Inc. Col Res Appl, 27, 282--290, 2002; Published online in Wiley InterScience (www.interscience.wiley.com). DOI 10.1002/col.10066},
copyright = {Copyright {\copyright} 2002 Wiley Periodicals, Inc.},
langid = {english},
keywords = {colour discrimination ellipses,colour-difference metrics,uniform colour space},
file = {/Users/kelsolaar/Zotero/storage/VET934GU/Cui et al. - 2002 - Uniform colour spaces based on the DIN99 colour-di.pdf;/Users/kelsolaar/Zotero/storage/TKDLWCHN/col.html}
}
@misc{CVRLp,
title = {{{CIE}} (2012) 10-Deg {{XYZ}} "Physiologically-Relevant" Colour Matching Functions},
author = {{CVRL}},
urldate = {2014-06-25},
howpublished = {http://www.cvrl.org/database/text/cienewxyz/cie2012xyz10.htm}
}
@misc{CVRLq,
title = {Luminous Efficiency},
author = {{CVRL}},
urldate = {2014-04-19},
howpublished = {http://www.cvrl.org/lumindex.htm}
}
@misc{CVRLr,
title = {New {{CIE XYZ}} Functions Transformed from the {{CIE}} (2006) {{LMS}} Functions},
author = {{CVRL}},
urldate = {2014-02-24},
howpublished = {http://cvrl.ioo.ucl.ac.uk/ciexyzpr.htm}
}
@misc{CVRLs,
title = {Older {{CIE Standards}}},
author = {{CVRL}},
urldate = {2014-02-24},
howpublished = {http://cvrl.ioo.ucl.ac.uk/cie.htm}
}
@misc{CVRLt,
title = {Stiles \& {{Burch}} Individual 10-Deg Colour Matching Data},
author = {{CVRL}},
urldate = {2014-02-24},
howpublished = {http://www.cvrl.org/stilesburch10\_ind.htm}
}
@misc{CVRLu,
title = {Cone {{Fundamentals}}},
author = {Stockman, Andrew and Sharpe, Lindsay T.},
year = {2000},
urldate = {2014-06-23},
howpublished = {http://www.cvrl.org/cones.htm}
}
@misc{CVRLv,
title = {{{CIE}} (2012) 2-Deg {{XYZ}} "Physiologically-Relevant" Colour Matching Functions},
author = {{CVRL}},
urldate = {2014-06-25},
howpublished = {http://www.cvrl.org/database/text/cienewxyz/cie2012xyz2.htm}
}
@misc{CVRLw,
title = {Stiles \& {{Burch}} Individual 2-Deg Colour Matching Data},
author = {{CVRL}},
urldate = {2014-02-24},
howpublished = {http://www.cvrl.org/stilesburch2\_ind.htm}
}
@article{Darrodi2015a,
title = {Reference Data Set for Camera Spectral Sensitivity Estimation},
author = {Darrodi, Maryam Mohammadzadeh and Finlayson, Graham and Goodman, Teresa and Mackiewicz, Michal},
year = {2015},
month = mar,
journal = {Journal of the Optical Society of America A},
volume = {32},
number = {3},
pages = {381},
issn = {1084-7529},
doi = {10.1364/JOSAA.32.000381},
file = {/Users/kelsolaar/Zotero/storage/5YWZ3D5W/Darrodi et al. - 2015 - Reference data set for camera spectral sensitivity estimation.pdf}
}
@article{David2015,
title = {Development of the {{IES}} Method for Evaluating the Color Rendition of Light Sources},
author = {David, Aurelien and Fini, Paul T. and Houser, Kevin W. and Ohno, Yoshi and Royer, Michael P. and Smet, Kevin A. G. and Wei, Minchen and Whitehead, Lorne},
year = {2015},
month = jun,
journal = {Optics Express},
volume = {23},
number = {12},
pages = {15888},
issn = {1094-4087},
doi = {10.1364/OE.23.015888},
urldate = {2021-05-22},
abstract = {We have developed a two-measure system for evaluating light sources' color rendition that builds upon conceptual progress of numerous researchers over the last two decades. The system quantifies the color fidelity and color gamut (change in object chroma) of a light source in comparison to a reference illuminant. The calculations are based on a newly developed set of reflectance data from real samples uniformly distributed in color space (thereby fairly representing all colors) and in wavelength space (thereby precluding artificial optimization of the color rendition scores by spectral engineering). The color fidelity score Rf is an improved version of the CIE color rendering index. The color gamut score Rg is an improved version of the Gamut Area Index. In combination, they provide two complementary assessments to guide the optimization of future light sources. This method summarizes the findings of the Color Metric Task Group of the Illuminating Engineering Society of North America (IES). It is adopted in the upcoming IES TM-30-2015, and is proposed for consideration with the International Commission on Illumination (CIE).},
langid = {english},
file = {/Users/kelsolaar/Zotero/storage/68IR97V4/David et al. - 2015 - Development of the IES method for evaluating the c.pdf;/Users/kelsolaar/Zotero/storage/VK4HT79Q/David et al. - 2015 - Development of the IES method for evaluating the color rendition of light sources.pdf}
}
@article{Davis2010a,
title = {Color Quality Scale},
author = {Davis, Wendy and Ohno, Yoshiro},
year = {2010},
month = mar,
journal = {Optical Engineering},
volume = {49},
number = {3},
pages = {033602},
issn = {0091-3286},
doi = {10.1117/1.3360335},
abstract = {The color rendering index (CRI) has been shown to have deficiencies when applied to white light-emitting-diode--based sources. Furthermore, evidence suggests that the restricted scope of the CRI unnecessarily penalizes some light sources with desirable color qualities. To solve the problems of the CRI and include other dimensions of color quality, the color quality scale (CQS) has been developed. Although the CQS uses many of elements of the CRI, there are a number of fundamental differences. Like the CRI, the CQS is a test-samples method that compares the appearance of a set of reflective samples when illuminated by the test lamp to their appearance under a reference illuminant. The CQS uses a larger set of reflective samples, all of high chroma, and combines the color differences of the samples with a root mean square. Additionally, the CQS does not penalize light sources for causing increases in the chroma of object colors but does penalize sources with smaller rendered color gamut areas. The scale of the CQS is converted to span 0-100, and the uniform object color space and chromatic adaptation transform used in the calculations are updated. Supplementary scales have also been developed for expert users.},
isbn = {0091-3286},
file = {/Users/kelsolaar/Zotero/storage/W3SHRJ84/Davis and Ohno - 2010 - Color quality scale.pdf}
}
@misc{DigitalCinemaInitiatives2007b,
title = {Digital {{Cinema System Specification}} - {{Version}} 1.1},
author = {{Digital Cinema Initiatives}},
year = {2007},
file = {/Users/kelsolaar/Zotero/storage/WSI7QRSL/Digital Cinema Initiatives - 2007 - Digital Cinema System Specification - Version 1.1.pdf}
}
@misc{DjangoSoftwareFoundation2022,
title = {Slugify},
author = {{Django Software Foundation}},
year = {2022},
urldate = {2022-06-01}
}
@misc{DJI2017,
title = {White {{Paper}} on {{D-Log}} and {{D-Gamut}} of {{DJI Cinema Color System}}},
author = {{Dji}},
year = {2017},
pages = {1--5},
file = {/Users/kelsolaar/Zotero/storage/KHLE47UN/Dji - 2017 - White Paper on D-Log and D-Gamut of DJI Cinema Color System.pdf}
}
@misc{Dolby2016a,
title = {{{WHAT IS ICTCP}}? - {{INTRODUCTION}}},
author = {{Dolby}},
year = {2016},
file = {/Users/kelsolaar/Zotero/storage/TNDLN3NF/Dolby - 2016 - WHAT IS ICTCP - INTRODUCTION.pdf}
}
@misc{Dyer2017,
title = {{{RAW}} to {{ACES}}},
author = {Dyer, Scott and Forsythe, Alexander and Irons, Jonathon and Mansencal, Thomas and Zhu, Miaoqi},
year = {2017}
}
@misc{EasyRGBh,
title = {{{RGB}} --{$>$} {{CMY}}},
author = {{EasyRGB}},
urldate = {2014-05-18},
howpublished = {http://www.easyrgb.com/index.php?X=MATH\&H=11\#text11}
}
@misc{EasyRGBi,
title = {{{CMY}} --{$>$} {{RGB}}},
author = {{EasyRGB}},
urldate = {2014-05-18},
howpublished = {http://www.easyrgb.com/index.php?X=MATH\&H=12\#text12}
}
@misc{EasyRGBj,
title = {{{RGB}} --{$>$} {{HSV}}},
author = {{EasyRGB}},
urldate = {2014-05-18},
howpublished = {http://www.easyrgb.com/index.php?X=MATH\&H=20\#text20}
}
@misc{EasyRGBk,
title = {{{HSL}} --{$>$} {{RGB}}},
author = {{EasyRGB}},
urldate = {2014-05-18},
howpublished = {http://www.easyrgb.com/index.php?X=MATH\&H=19\#text19}
}
@misc{EasyRGBl,
title = {{{RGB}} --{$>$} {{HSL}}},
author = {{EasyRGB}},
urldate = {2014-05-18},
howpublished = {http://www.easyrgb.com/index.php?X=MATH\&H=18\#text18}
}
@misc{EasyRGBm,
title = {{{CMYK}} --{$>$} {{CMY}}},
author = {{EasyRGB}},
urldate = {2014-05-18},
howpublished = {http://www.easyrgb.com/index.php?X=MATH\&H=14\#text14}
}
@misc{EasyRGBn,
title = {{{HSV}} --{$>$} {{RGB}}},
author = {{EasyRGB}},
urldate = {2014-05-18},
howpublished = {http://www.easyrgb.com/index.php?X=MATH\&H=21\#text21}
}
@misc{EasyRGBo,
title = {{{CMY}} --{$>$} {{CMYK}}},
author = {{EasyRGB}},
urldate = {2014-05-18},
howpublished = {http://www.easyrgb.com/index.php?X=MATH\&H=13\#text13}
}
@inproceedings{Ebner1998,
title = {Finding Constant Hue Surfaces in Color Space},
booktitle = {Proc. {{SPIE}} 3300, {{Color Imaging}}: {{Device-Independent Color}}, {{Color Hardcopy}}, and {{Graphic Arts III}}, (2 {{January}} 1998)},
author = {Ebner, Fritz and Fairchild, Mark D.},
editor = {Beretta, Giordano B. and Eschbach, Reiner},
year = {1998},
month = jan,
pages = {107--117},
doi = {10.1117/12.298269},
file = {/Users/kelsolaar/Zotero/storage/BGF9VVJF/Ebner, Fairchild - 1998 - Finding constant hue surfaces in color space.pdf}
}
@misc{Erdema,
title = {Fast {{Line Segment Intersection}}},
author = {Erdem, U. Murat},
urldate = {2016-01-15},
howpublished = {http://www.mathworks.com/matlabcentral/fileexchange/27205-fast-line-segment-intersection}
}
@misc{Erdogana,
title = {How to {{Calculate Luminosity}}, {{Dominant Wavelength}}, and {{Excitation Purity}}},
author = {Erdogan, Turan},
pages = {7},
abstract = {There are many different systems for analyzing and representing the color of an object perceived by a human observer. For the purposes of unambiguously specifying the color an observer sees when looking through an optical filter at a well-defined light source, we have found the CIE Color Specification System to be the most accurate (for a simple and clear description, see [1]). In this article we briefly describe the method to calculate the three main parameters that fully specify color in this system: luminosity, dominant wavelength, and excitation purity. These terms specifically refer to the definitions in the CIE system given below, but they have analogies in many other systems. A set of more general terms often used to qualitatively describe color are: brightness, hue, and saturation (analogous to luminosity, dominant wavelength, and excitation purity, respectively). These terms (and others) are often used interchangeably. Here we will adhere to the official terms assigned to the CIE system to avoid any ambiguity.},
file = {/Users/kelsolaar/Zotero/storage/SMPXUKKN/Erdogan - Unknown - How to Calculate Luminosity, Dominant Wavelength, and Excitation Purity.pdf}
}
@misc{EuropeanBroadcastingUnion1975,
title = {{{EBU Tech}} 3213 - {{EBU Standard}} for {{Chromaticity Tolerances}} for {{Studio Monitors}}},
author = {{European Broadcasting Union}},
year = {1975},
month = aug
}