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BIBLIOGRAPHY.bib
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@misc{AdobeSystems2013b,
author = {{Adobe Systems}},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Adobe Systems - 2013 - Cube LUT Specification.pdf:pdf},
keywords = {Iridas,look-up table,specification},
title = {{Cube LUT Specification}},
url = {https://drive.google.com/open?id=143Eh08ZYncCAMwJ1q4gWxVOqR_OSWYvs},
year = {2013}
}
@misc{AdobeSystems2005a,
author = {{Adobe Systems}},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Adobe Systems - 2005 - Adobe RGB (1998) Color Image Encoding.pdf:pdf},
number = {May},
title = {{Adobe RGB (1998) Color Image Encoding}},
url = {http://www.adobe.com/digitalimag/pdfs/AdobeRGB1998.pdf},
volume = {2704},
year = {2005}
}
@misc{AdobeSystems2013,
author = {{Adobe Systems}},
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}},
url = {https://www.adobe.com/support/downloads/dng/dng_sdk.html},
year = {2013}
}
@misc{AdobeSystems2013a,
author = {{Adobe Systems}},
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}},
url = {https://www.adobe.com/support/downloads/dng/dng_sdk.html},
year = {2013}
}
@misc{ANSI2003a,
author = {ANSI},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/ANSI - 2003 - Specification of ROMM RGB.pdf:pdf},
pages = {1--2},
title = {{Specification of ROMM RGB}},
url = {http://www.color.org/ROMMRGB.pdf},
year = {2003}
}
@misc{ARRI2012a,
author = {ARRI},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/ARRI - 2012 - ALEXA - Log C Curve - Usage in VFX.pdf:pdf},
number = {June},
pages = {1--12},
title = {{ALEXA - Log C Curve - Usage in VFX}},
url = {http://www.arri.com/?eID=registration&file_uid=8026},
year = {2012}
}
@misc{AssociationofRadioIndustriesandBusinesses2015a,
author = {{Association of Radio Industries and Businesses}},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Association of Radio Industries and Businesses - 2015 - Essential Parameter Values for the Extended Image Dynamic Range Television (EIDR.pdf:pdf},
title = {{Essential Parameter Values for the Extended Image Dynamic Range Television (EIDRTV) System for Programme Production}},
url = {https://www.arib.or.jp/english/std_tr/broadcasting/desc/std-b67.html},
year = {2015}
}
@misc{ASTMInternational2007,
author = {{ASTM International}},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/ASTM International - 2007 - ASTM D2244-07 - Standard Practice for Calculation of Color Tolerances and Color Differences from Instrumenta.pdf:pdf},
pages = {1--10},
title = {{ASTM D2244-07 - Standard Practice for Calculation of Color Tolerances and Color Differences from Instrumentally Measured Color Coordinates}},
volume = {i},
year = {2007}
}
@misc{ASTMInternational1989a,
annote = {https://law.resource.org/pub/us/cfr/ibr/003/a},
author = {{ASTM International}},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/ASTM International - 1989 - ASTM D1535-89 - Standard Practice for Specifying Color by the Munsell System.pdf:pdf},
keywords = {D1535,Munsell,Munsell color order system,Munsell notation,color},
pages = {1--29},
title = {{ASTM D1535-89 - Standard Practice for Specifying Color by the Munsell System}},
url = {http://www.astm.org/DATABASE.CART/HISTORICAL/D1535-89.htm},
year = {1989}
}
@misc{ASTMInternational2011a,
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.},
author = {{ASTM International}},
doi = {10.1520/E2022-11},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/ASTM International - 2011 - ASTM E2022-11 - Standard Practice for Calculation of Weighting Factors for Tristimulus Integration.pdf:pdf},
pages = {1--10},
title = {{ASTM E2022-11 - Standard Practice for Calculation of Weighting Factors for Tristimulus Integration}},
year = {2011}
}
@misc{ASTMInternational2015b,
author = {{ASTM International}},
doi = {10.1520/E0308-15},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/ASTM International - 2015 - ASTM E308-15 - Standard Practice for Computing the Colors of Objects by Using the CIE System.pdf:pdf},
pages = {1--47},
title = {{ASTM E308-15 - Standard Practice for Computing the Colors of Objects by Using the CIE System}},
year = {2015}
}
@misc{ASTMInternational2008a,
author = {{ASTM International}},
doi = {10.1520/D1535-08E01},
title = {{ASTM D1535-08e1 - Standard Practice for Specifying Color by the Munsell System}},
year = {2008}
}
@misc{BabelColor2012b,
author = {BabelColor},
title = {{The ColorChecker (since 1976!)}},
url = {http://www.babelcolor.com/main_level/ColorChecker.htm},
urldate = {2014-09-26},
year = {2012}
}
@misc{BabelColor2012c,
author = {BabelColor},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/BabelColor - 2012 - ColorChecker RGB and spectra.xls:xls},
title = {{ColorChecker RGB and spectra}},
url = {http://www.babelcolor.com/download/ColorChecker_RGB_and_spectra.xls},
year = {2012}
}
@article{Bianco2010a,
annote = {http://web.stanford.edu/$\sim$sujason/ColorBalancing/Papers/Two New von Kries Based Chromatic Adaptation.pdf},
author = {Bianco, S. and Schettini, R.},
doi = {10.1002/col.20573},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Bianco, Schettini - 2010 - Two new von Kries based chromatic adaptation transforms found by numerical optimization.pdf:pdf},
issn = {03612317},
journal = {Color Research & Application},
month = {jun},
number = {3},
pages = {184--192},
title = {{Two new von Kries based chromatic adaptation transforms found by numerical optimization}},
url = {http://doi.wiley.com/10.1002/col.20573},
volume = {35},
year = {2010}
}
@article{Bodhaine1999a,
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.},
author = {Bodhaine, Barry A. and Wood, Norman B. and Dutton, Ellsworth G. and Slusser, James R.},
doi = {10.1175/1520-0426(1999)016<1854:ORODC>2.0.CO;2},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Bodhaine et al. - 1999 - On Rayleigh Optical Depth Calculations.pdf:pdf},
issn = {0739-0572},
journal = {Journal of Atmospheric and Oceanic Technology},
month = {nov},
number = {11},
pages = {1854--1861},
title = {{On Rayleigh Optical Depth Calculations}},
url = {http://journals.ametsoc.org/doi/abs/10.1175/1520-0426%281999%29016%3C1854%3AORODC%3E2.0.CO%3B2},
volume = {16},
year = {1999}
}
@misc{Borer2017a,
author = {Borer, Tim},
title = {{Private Discussion with Mansencal, T. and Shaw, N.}},
year = {2017}
}
@misc{Bourkeb,
author = {Bourke, Paul},
title = {{Trilinear Interpolation}},
url = {http://paulbourke.net/miscellaneous/interpolation/},
urldate = {2018-01-13}
}
@misc{Bourkea,
author = {Bourke, Paul},
title = {{Intersection point of two line segments in 2 dimensions}},
url = {http://paulbourke.net/geometry/pointlineplane/},
urldate = {2016-01-15}
}
@article{Breneman1987b,
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.},
author = {Breneman, Edwin J},
doi = {10.1364/JOSAA.4.001115},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Breneman - 1987 - Corresponding chromaticities for different states of adaptation to complex visual fields(2).pdf:pdf},
issn = {1084-7529},
journal = {Journal of the Optical Society of America A},
month = {jun},
number = {6},
pages = {1115},
pmid = {3598755},
title = {{Corresponding chromaticities for different states of adaptation to complex visual fields}},
url = {https://www.osapublishing.org/abstract.cfm?URI=josaa-4-6-1115},
volume = {4},
year = {1987}
}
@article{Brill2008a,
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.},
author = {Brill, Michael H. and Susstrunk, Sabine},
doi = {10.1002/col.20432},
issn = {03612317},
journal = {Color Research & Application},
keywords = {CIECAM02,Chromatic adaptation,Color appearance,Gamut,Model,Primary},
month = {oct},
number = {5},
pages = {424--426},
title = {{Repairing gamut problems in CIECAM02: A progress report}},
url = {http://doi.wiley.com/10.1002/col.20432},
volume = {33},
year = {2008}
}
@misc{Broadbent2009a,
author = {Broadbent, A. D.},
title = {{Calculation from the original experimental data of the CIE 1931 RGB standard observer spectral chromaticity co-ordinates and color matching functions}},
url = {http://www.cis.rit.edu/mcsl/research/1931.php},
urldate = {2014-06-12},
year = {2009}
}
@book{Burger2009b,
address = {London},
author = {Burger, Wilhelm and Burge, Mark James},
doi = {10.1007/978-1-84800-195-4},
isbn = {978-1-84800-194-7},
publisher = {Springer London},
series = {Undergraduate Topics in Computer Science},
title = {{Principles of Digital Image Processing}},
url = {http://link.springer.com/10.1007/978-1-84800-195-4},
year = {2009}
}
@misc{Canona,
author = {Canon},
title = {{EOS C300 Mark II - EOS C300 Mark II Input Transform Version 2.0 (for Cinema Gamut / BT.2020)}},
url = {https://www.usa.canon.com/internet/portal/us/home/support/details/cameras/cinema-eos/eos-c300-mark-ii},
urldate = {2016-08-23}
}
@misc{Canon2014a,
author = {Canon},
title = {{EOS C500 Firmware Update}},
url = {https://www.usa.canon.com/internet/portal/us/home/explore/product-showcases/cameras-and-lenses/cinema-eos-firmware/c500},
urldate = {2016-08-27},
year = {2014}
}
@article{Cao2013,
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.},
author = {Cao, Renbo and Trussell, H Joel and Shamey, Renzo},
doi = {10.1364/JOSAA.30.001508},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Cao, Trussell, Shamey - 2013 - Comparison of the performance of inverse transformation methods from OSA-UCS to CIEXYZ.pdf:pdf},
isbn = {1520-8532 (Electronic)\r1084-7529 (Linking)},
issn = {1084-7529},
journal = {Journal of the Optical Society of America A},
month = {aug},
number = {8},
pages = {1508},
pmid = {24323208},
title = {{Comparison of the performance of inverse transformation methods from OSA-UCS to CIEXYZ}},
url = {https://www.osapublishing.org/abstract.cfm?URI=josaa-30-8-1508},
volume = {30},
year = {2013}
}
@misc{Castro2014a,
author = {Castro, Saullo},
title = {{Numpy: Fastest way of computing diagonal for each row of a 2d array}},
url = {http://stackoverflow.com/questions/26511401/numpy-fastest-way-of-computing-diagonal-for-each-row-of-a-2d-array/26517247#26517247},
urldate = {2014-08-22},
year = {2014}
}
@article{Centore2012a,
author = {Centore, Paul},
doi = {10.1002/col.20715},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Centore - 2012 - An open-source inversion algorithm for the Munsell renotation.pdf:pdf},
issn = {03612317},
journal = {Color Research & Application},
keywords = {algorithm,inverse renotation,munsell,open source,renotation},
month = {dec},
number = {6},
pages = {455--464},
title = {{An open-source inversion algorithm for the Munsell renotation}},
url = {http://doi.wiley.com/10.1002/col.20715},
volume = {37},
year = {2012}
}
@misc{Centore2014u,
annote = {http://www.99main.com/$\sim$centore/MunsellAndKubelkaMunkToolbox/MunsellAndKubelkaMunkToolbox.html},
author = {Centore, Paul},
title = {{MunsellAndKubelkaMunkToolboxApr2014 - GeneralRoutines/CIELABtoApproxMunsellSpec.m}},
url = {https://github.com/colour-science/MunsellAndKubelkaMunkToolbox},
year = {2014}
}
@misc{Centore2014n,
annote = {http://www.99main.com/$\sim$centore/MunsellAndKubelkaMunkToolbox/MunsellAndKubelkaMunkToolbox.html},
author = {Centore, Paul},
title = {{MunsellAndKubelkaMunkToolboxApr2014 - MunsellRenotationRoutines/FindHueOnRenotationOvoid.m}},
url = {https://github.com/colour-science/MunsellAndKubelkaMunkToolbox},
year = {2014}
}
@misc{Centore2014p,
annote = {http://www.99main.com/$\sim$centore/MunsellAndKubelkaMunkToolbox/MunsellAndKubelkaMunkToolbox.html},
author = {Centore, Paul},
title = {{MunsellAndKubelkaMunkToolboxApr2014 - MunsellRenotationRoutines/xyYtoMunsell.m}},
url = {https://github.com/colour-science/MunsellAndKubelkaMunkToolbox},
year = {2014}
}
@misc{Centore2014r,
annote = {http://www.99main.com/$\sim$centore/MunsellAndKubelkaMunkToolbox/MunsellAndKubelkaMunkToolbox.html},
author = {Centore, Paul},
title = {{MunsellAndKubelkaMunkToolboxApr2014 - MunsellRenotationRoutines/MaxChromaForExtrapolatedRenotation.m}},
url = {https://github.com/colour-science/MunsellAndKubelkaMunkToolbox},
year = {2014}
}
@misc{Centore2014m,
annote = {http://www.99main.com/$\sim$centore/MunsellAndKubelkaMunkToolbox/MunsellAndKubelkaMunkToolbox.html},
author = {Centore, Paul},
title = {{MunsellAndKubelkaMunkToolboxApr2014 - MunsellRenotationRoutines/MunsellToxyY.m}},
url = {https://github.com/colour-science/MunsellAndKubelkaMunkToolbox},
year = {2014}
}
@misc{Centore2014q,
annote = {http://www.99main.com/$\sim$centore/MunsellAndKubelkaMunkToolbox/MunsellAndKubelkaMunkToolbox.html},
author = {Centore, Paul},
title = {{MunsellAndKubelkaMunkToolboxApr2014 - MunsellRenotationRoutines/MunsellToxyForIntegerMunsellValue.m}},
url = {https://github.com/colour-science/MunsellAndKubelkaMunkToolbox},
year = {2014}
}
@misc{Centorea,
author = {Centore, Paul},
title = {{The Munsell and Kubelka-Munk Toolbox}},
url = {http://www.munsellcolourscienceforpainters.com/MunsellAndKubelkaMunkToolbox/MunsellAndKubelkaMunkToolbox.html},
urldate = {2018-01-23}
}
@misc{Centore2014t,
annote = {http://www.99main.com/$\sim$centore/MunsellAndKubelkaMunkToolbox/MunsellAndKubelkaMunkToolbox.html},
author = {Centore, Paul},
title = {{MunsellAndKubelkaMunkToolboxApr2014 - MunsellRenotationRoutines/ChromDiagHueAngleToMunsellHue.m}},
url = {https://github.com/colour-science/MunsellAndKubelkaMunkToolbox},
year = {2014}
}
@misc{Centore2014s,
annote = {http://www.99main.com/$\sim$centore/MunsellAndKubelkaMunkToolbox/MunsellAndKubelkaMunkToolbox.html},
author = {Centore, Paul},
title = {{MunsellAndKubelkaMunkToolboxApr2014 - MunsellRenotationRoutines/MunsellHueToChromDiagHueAngle.m}},
url = {https://github.com/colour-science/MunsellAndKubelkaMunkToolbox},
year = {2014}
}
@misc{Centore2014o,
annote = {http://www.99main.com/$\sim$centore/MunsellAndKubelkaMunkToolbox/MunsellAndKubelkaMunkToolbox.html},
author = {Centore, Paul},
title = {{MunsellAndKubelkaMunkToolboxApr2014 - MunsellSystemRoutines/BoundingRenotationHues.m}},
url = {https://github.com/colour-science/MunsellAndKubelkaMunkToolbox},
year = {2014}
}
@misc{Centore2014k,
annote = {http://www.99main.com/$\sim$centore/MunsellAndKubelkaMunkToolbox/MunsellAndKubelkaMunkToolbox.html},
author = {Centore, Paul},
title = {{MunsellAndKubelkaMunkToolboxApr2014 - MunsellRenotationRoutines/MunsellHueToASTMHue.m}},
url = {https://github.com/colour-science/MunsellAndKubelkaMunkToolbox},
year = {2014}
}
@misc{Centore2014l,
annote = {http://www.99main.com/$\sim$centore/MunsellAndKubelkaMunkToolbox/MunsellAndKubelkaMunkToolbox.html},
author = {Centore, Paul},
title = {{MunsellAndKubelkaMunkToolboxApr2014 - MunsellSystemRoutines/LinearVsRadialInterpOnRenotationOvoid.m}},
url = {https://github.com/colour-science/MunsellAndKubelkaMunkToolbox},
year = {2014}
}
@article{Cheung2004,
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.},
author = {Cheung, Vien and Westland, Stephen and Connah, David and Ripamonti, Caterina},
doi = {10.1111/j.1478-4408.2004.tb00201.x},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Cheung et al. - 2004 - A comparative study of the characterisation of colour cameras by means of neural networks and polynomial transfor.pdf:pdf},
issn = {14723581},
journal = {Coloration Technology},
number = {1},
pages = {19--25},
title = {{A comparative study of the characterisation of colour cameras by means of neural networks and polynomial transforms}},
volume = {120},
year = {2004}
}
@misc{CIEce,
author = {CIE},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/CIE - 2004 - CIE 152004 Tables Data.xls:xls},
title = {{CIE 15:2004 Tables Data}},
url = {https://law.resource.org/pub/us/cfr/ibr/003/cie.15.2004.tables.xls},
year = {2004}
}
@misc{CIEcf,
author = {CIE},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/CIE - Unknown - CIE Spectral Data.xls:xls},
title = {{CIE Spectral Data}},
url = {http://files.cie.co.at/204.xls}
}
@misc{CIETC1-321994b,
author = {{CIE TC 1-32}},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/CIE TC 1-32 - 1994 - CIE 109-1994 A Method of Predicting Corresponding Colours under Different Chromatic and Illuminance Adaptations.pdf:pdf},
isbn = {978-3-900734-51-0},
pages = {1--18},
title = {{CIE 109-1994 A Method of Predicting Corresponding Colours under Different Chromatic and Illuminance Adaptations}},
url = {http://div1.cie.co.at/?i_ca_id=551&pubid=34},
year = {1994}
}
@misc{CIETC1-362006a,
author = {{CIE TC 1-36}},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/CIE TC 1-36 - 2006 - CIE 170-12006 Fundamental Chromaticity Diagram with Physiological Axes - Part 1.pdf:pdf},
isbn = {978-3-901-90646-6},
pages = {1--56},
title = {{CIE 170-1:2006 Fundamental Chromaticity Diagram with Physiological Axes - Part 1}},
url = {http://div1.cie.co.at/?i_ca_id=551&pubid=48},
year = {2006}
}
@incollection{CIETC1-382005f,
author = {{CIE TC 1-38}},
booktitle = {CIE 167:2005 Recommended Practice for Tabulating Spectral Data for Use in Colour Computations},
chapter = {9.2.4},
isbn = {978-3-901-90641-1},
pages = {1--27},
title = {{9.2.4 Method of interpolation for uniformly spaced independent variable}},
url = {http://div1.cie.co.at/?i_ca_id=551&pubid=47},
year = {2005}
}
@incollection{CIETC1-382005e,
author = {{CIE TC 1-38}},
booktitle = {CIE 167:2005 Recommended Practice for Tabulating Spectral Data for Use in Colour Computations},
chapter = {9},
isbn = {978-3-901-90641-1},
pages = {14--19},
title = {{9. INTERPOLATION}},
url = {http://div1.cie.co.at/?i_ca_id=551&pubid=47},
year = {2005}
}
@incollection{CIETC1-382005h,
author = {{CIE TC 1-38}},
booktitle = {CIE 167:2005 Recommended Practice for Tabulating Spectral Data for Use in Colour Computations},
chapter = {Table V},
isbn = {978-3-901-90641-1},
pages = {19},
title = {{Table V. Values of the c-coefficients of Equ.s 6 and 7.}},
url = {http://div1.cie.co.at/?i_ca_id=551&pubid=47},
year = {2005}
}
@incollection{CIETC1-382005g,
author = {{CIE TC 1-38}},
booktitle = {CIE 167:2005 Recommended Practice for Tabulating Spectral Data for Use in Colour Computations},
chapter = {10},
isbn = {978-3-901-90641-1},
pages = {19--20},
title = {{EXTRAPOLATION}},
url = {http://div1.cie.co.at/?i_ca_id=551&pubid=47},
year = {2005}
}
@incollection{CIETC1-482004,
author = {{CIE TC 1-48}},
booktitle = {CIE 015:2004 Colorimetry, 3rd Edition},
isbn = {978-3-901-90633-6},
pages = {68--68},
title = {{EXPLANATORY COMMENTS - 5}},
url = {http://www.cie.co.at/publications/colorimetry-3rd-edition},
year = {2004}
}
@incollection{CIETC1-482004k,
author = {{CIE TC 1-48}},
booktitle = {CIE 015:2004 Colorimetry, 3rd Edition},
chapter = {9.4},
isbn = {978-3-901-90633-6},
pages = {24},
title = {{The evaluation of whiteness}},
url = {http://www.cie.co.at/publications/colorimetry-3rd-edition},
year = {2004}
}
@incollection{CIETC1-482004i,
author = {{CIE TC 1-48}},
booktitle = {CIE 015:2004 Colorimetry, 3rd Edition},
chapter = {APPENDIX E},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/CIE TC 1-48 - 2004 - APPENDIX E. INFORMATION ON THE USE OF PLANCK'S EQUATION FOR STANDARD AIR.pdf:pdf},
isbn = {978-3-901-90633-6},
pages = {77--82},
title = {{APPENDIX E. INFORMATION ON THE USE OF PLANCK'S EQUATION FOR STANDARD AIR}},
url = {http://www.cie.co.at/publications/colorimetry-3rd-edition},
year = {2004}
}
@incollection{CIETC1-482004o,
author = {{CIE TC 1-48}},
booktitle = {CIE 015:2004 Colorimetry, 3rd Edition},
chapter = {9.1},
isbn = {978-3-901-90633-6},
pages = {32--33},
title = {{9.1 Dominant wavelength and purity}},
url = {http://www.cie.co.at/publications/colorimetry-3rd-edition},
year = {2004}
}
@incollection{CIETC1-482004m,
author = {{CIE TC 1-48}},
booktitle = {CIE 015:2004 Colorimetry, 3rd Edition},
chapter = {8.2},
isbn = {978-3-901-90633-6},
pages = {24},
title = {{CIE 1976 uniform colour spaces}},
url = {http://www.cie.co.at/publications/colorimetry-3rd-edition},
year = {2004}
}
@incollection{CIETC1-482004j,
author = {{CIE TC 1-48}},
booktitle = {CIE 015:2004 Colorimetry, 3rd Edition},
chapter = {8.1},
isbn = {978-3-901-90633-6},
pages = {24},
title = {{CIE 1976 uniform chromaticity scale diagram (UCS diagram)}},
url = {http://www.cie.co.at/publications/colorimetry-3rd-edition},
year = {2004}
}
@book{CIETC1-482004h,
author = {{CIE TC 1-48}},
booktitle = {CIE 015:2004 Colorimetry, 3rd Edition},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/CIE TC 1-48 - 2004 - CIE 0152004 Colorimetry, 3rd Edition.pdf:pdf},
isbn = {978-3-901-90633-6},
pages = {1--82},
publisher = {Commission internationale de l'{\'{e}}clairage},
title = {{CIE 015:2004 Colorimetry, 3rd Edition}},
url = {http://www.cie.co.at/publications/colorimetry-3rd-edition},
year = {2004}
}
@incollection{CIETC1-482004n,
author = {{CIE TC 1-48}},
booktitle = {CIE 015:2004 Colorimetry, 3rd Edition},
chapter = {3.1},
isbn = {978-3-901-90633-6},
pages = {12--13},
title = {{3.1 Recommendations concerning standard physical data of illuminants}},
url = {http://www.cie.co.at/publications/colorimetry-3rd-edition},
year = {2004}
}
@incollection{CIETC1-482004l,
author = {{CIE TC 1-48}},
booktitle = {CIE 015:2004 Colorimetry, 3rd Edition},
chapter = {7.2.2.1},
isbn = {978-3-901-90633-6},
pages = {24},
title = {{Extrapolation}},
url = {http://www.cie.co.at/publications/colorimetry-3rd-edition},
year = {2004}
}
@misc{Colblindora,
author = {Colblindor},
title = {{Deuteranopia - Red-Green Color Blindness}},
url = {http://www.color-blindness.com/deuteranopia-red-green-color-blindness/},
urldate = {2015-07-04}
}
@misc{Colblindorc,
author = {Colblindor},
title = {{Tritanopia - Blue-Yellow Color Blindness}},
url = {http://www.color-blindness.com/tritanopia-blue-yellow-color-blindness/},
urldate = {2015-07-04}
}
@misc{Colblindorb,
author = {Colblindor},
title = {{Protanopia - Red-Green Color Blindness}},
url = {http://www.color-blindness.com/protanopia-red-green-color-blindness/},
urldate = {2015-07-04}
}
@misc{Cottrella,
annote = {http://www.russellcottrell.com/photo/RussellRGB.htm},
author = {Cottrell, Russell},
title = {{The Russell RGB working color space}},
url = {http://www.russellcottrell.com/photo/downloads/RussellRGB.icc}
}
@misc{CVRLt,
author = {CVRL},
title = {{Stiles & Burch individual 10-deg colour matching data}},
url = {http://www.cvrl.org/stilesburch10_ind.htm},
urldate = {2014-02-24}
}
@misc{CVRLp,
author = {CVRL},
title = {{CIE (2012) 10-deg XYZ "physiologically-relevant" colour matching functions}},
url = {http://www.cvrl.org/database/text/cienewxyz/cie2012xyz10.htm},
urldate = {2014-06-25}
}
@misc{CVRLq,
author = {CVRL},
title = {{Luminous efficiency}},
url = {http://www.cvrl.org/lumindex.htm},
urldate = {2014-04-19}
}
@misc{CVRLv,
author = {CVRL},
title = {{CIE (2012) 2-deg XYZ "physiologically-relevant" colour matching functions}},
url = {http://www.cvrl.org/database/text/cienewxyz/cie2012xyz2.htm},
urldate = {2014-06-25}
}
@misc{CVRLs,
author = {CVRL},
title = {{Older CIE Standards}},
url = {http://cvrl.ioo.ucl.ac.uk/cie.htm},
urldate = {2014-02-24}
}
@misc{CVRLw,
author = {CVRL},
title = {{Stiles & Burch individual 2-deg colour matching data}},
url = {http://www.cvrl.org/stilesburch2_ind.htm},
urldate = {2014-02-24}
}
@misc{CVRLu,
author = {CVRL},
title = {{Cone Fundamentals}},
url = {http://www.cvrl.org/cones.htm},
urldate = {2014-06-23}
}
@misc{CVRLr,
author = {CVRL},
title = {{New CIE XYZ functions transformed from the CIE (2006) LMS functions}},
url = {http://cvrl.ioo.ucl.ac.uk/ciexyzpr.htm},
urldate = {2014-02-24}
}
@article{Darrodi2015a,
author = {Darrodi, Maryam Mohammadzadeh and Finlayson, Graham and Goodman, Teresa and Mackiewicz, Michal},
doi = {10.1364/JOSAA.32.000381},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Darrodi et al. - 2015 - Reference data set for camera spectral sensitivity estimation.pdf:pdf},
issn = {1084-7529},
journal = {Journal of the Optical Society of America A},
month = {mar},
number = {3},
pages = {381},
title = {{Reference data set for camera spectral sensitivity estimation}},
url = {https://www.osapublishing.org/abstract.cfm?URI=josaa-32-3-381},
volume = {32},
year = {2015}
}
@article{Davis2010a,
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.},
annote = {https://doi.org/10.1117/1.3360335},
author = {Davis, Wendy and Ohno, Yoshiro},
doi = {10.1117/1.3360335},
isbn = {0091-3286},
issn = {0091-3286},
journal = {Optical Engineering},
month = {mar},
number = {3},
pages = {033602},
title = {{Color quality scale}},
url = {http://opticalengineering.spiedigitallibrary.org/article.aspx?doi=10.1117/1.3360335},
volume = {49},
year = {2010}
}
@misc{DigitalCinemaInitiatives2007b,
author = {{Digital Cinema Initiatives}},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Digital Cinema Initiatives - 2007 - Digital Cinema System Specification - Version 1.1.pdf:pdf},
title = {{Digital Cinema System Specification - Version 1.1}},
url = {http://www.dcimovies.com/archives/spec_v1_1/DCI_DCinema_System_Spec_v1_1.pdf},
year = {2007}
}
@misc{Dolby2016a,
author = {Dolby},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Dolby - 2016 - WHAT IS ICTCP - INTRODUCTION.pdf:pdf},
title = {{WHAT IS ICTCP? - INTRODUCTION}},
url = {https://www.dolby.com/us/en/technologies/dolby-vision/ICtCp-white-paper.pdf},
year = {2016}
}
@misc{EasyRGBk,
author = {EasyRGB},
title = {{HSL —> RGB}},
url = {http://www.easyrgb.com/index.php?X=MATH&H=19#text19},
urldate = {2014-05-18}
}
@misc{EasyRGBo,
author = {EasyRGB},
title = {{CMY —> CMYK}},
url = {http://www.easyrgb.com/index.php?X=MATH&H=13#text13},
urldate = {2014-05-18}
}
@misc{EasyRGBj,
author = {EasyRGB},
title = {{RGB —> HSV}},
url = {http://www.easyrgb.com/index.php?X=MATH&H=20#text20},
urldate = {2014-05-18}
}
@misc{EasyRGBl,
author = {EasyRGB},
title = {{RGB —> HSL}},
url = {http://www.easyrgb.com/index.php?X=MATH&H=18#text18},
urldate = {2014-05-18}
}
@misc{EasyRGBh,
author = {EasyRGB},
title = {{RGB —> CMY}},
url = {http://www.easyrgb.com/index.php?X=MATH&H=11#text11},
urldate = {2014-05-18}
}
@misc{EasyRGBi,
author = {EasyRGB},
title = {{CMY —> RGB}},
url = {http://www.easyrgb.com/index.php?X=MATH&H=12#text12},
urldate = {2014-05-18}
}
@misc{EasyRGBn,
author = {EasyRGB},
title = {{HSV —> RGB}},
url = {http://www.easyrgb.com/index.php?X=MATH&H=21#text21},
urldate = {2014-05-18}
}
@misc{EasyRGBm,
author = {EasyRGB},
title = {{CMYK —> CMY}},
url = {http://www.easyrgb.com/index.php?X=MATH&H=14#text14},
urldate = {2014-05-18}
}
@misc{Erdema,
author = {Erdem, U. Murat},
title = {{Fast Line Segment Intersection}},
url = {http://www.mathworks.com/matlabcentral/fileexchange/27205-fast-line-segment-intersection},
urldate = {2016-01-15}
}
@misc{Erdogana,
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.},
author = {Erdogan, Turan},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Erdogan - Unknown - How to Calculate Luminosity, Dominant Wavelength, and Excitation Purity.pdf:pdf},
pages = {7},
title = {{How to Calculate Luminosity, Dominant Wavelength, and Excitation Purity}},
url = {http://www.semrock.com/Data/Sites/1/semrockpdfs/whitepaper_howtocalculateluminositywavelengthandpurity.pdf}
}
@misc{EuropeanColorInitiative2002a,
annote = {http://www.eci.org/en/colourstandards/workingcolorspaces},
author = {{European Color Initiative}},
title = {{ECI RGB v2}},
url = {http://www.eci.org/_media/downloads/icc_profiles_from_eci/ecirgbv20.zip},
year = {2002}
}
@misc{Fairchild1998b,
abstract = {The colorimetric characterization of a flat-panel LCD monitor, the Apple Studio Display, using traditional CRT characterization techniques was evaluated. The results showed that the display performed up to the manufacturer's specifications in terms of luminance and contrast. However, the traditional CRT gain-offset-gamma (GOG) model for characterization was inadequate and a model with one-dimensional lookup tables followed by a 3x3 matrix was developed. The LUT model performed excellently with average CIE94 color differences between measured and predicted colors of approximately 1.0.},
author = {Fairchild, M. and Wyble, D.},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Fairchild, Wyble - 1998 - Colorimetric Characterization of The Apple Studio Display (flat panel LCD).pdf:pdf},
pages = {22},
title = {{Colorimetric Characterization of The Apple Studio Display (flat panel LCD)}},
url = {http://scholarworks.rit.edu/cgi/viewcontent.cgi?article=1922&context=article},
year = {1998}
}
@inproceedings{Fairchild2011,
author = {Fairchild, Mark D and Chen, Ping-hsu},
booktitle = {Proc. SPIE 7867, Image Quality and System Performance VIII},
doi = {10.1117/12.872075},
editor = {Farnand, Susan P. and Gaykema, Frans},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Fairchild, Chen - 2011 - Brightness, lightness, and specifying color in high-dynamic-range scenes and images.pdf:pdf},
keywords = {color appearance,color differences,color spaces,hdr,image quality,lightness},
month = {jan},
pages = {78670O},
title = {{Brightness, lightness, and specifying color in high-dynamic-range scenes and images}},
url = {http://proceedings.spiedigitallibrary.org/proceeding.aspx?doi=10.1117/12.872075},
year = {2011}
}
@misc{Fairchildb,
author = {Fairchild, Mark D.},
title = {{Fairchild YSh}},
url = {http://rit-mcsl.org/fairchild//files/FairchildYSh.zip}
}
@incollection{Fairchild2013ba,
author = {Fairchild, Mark D.},
booktitle = {Color Appearance Models},
chapter = {11},
edition = {3},
isbn = {B00DAYO8E2},
pages = {4810--5085},
publisher = {Wiley},
series = {The Wiley-IS&T Series in Imaging Science and Technology},
title = {{The Nayatani et al. Model}},
year = {2013}
}
@incollection{Fairchild2013y,
author = {Fairchild, Mark D.},
booktitle = {Color Appearance Models},
chapter = {20.3},
edition = {3},
isbn = {B00DAYO8E2},
pages = {6197--6223},
publisher = {Wiley},
series = {The Wiley-IS&T Series in Imaging Science and Technology},
title = {{IPT Colourspace}},
year = {2013}
}
@incollection{Fairchild2004c,
author = {Fairchild, Mark D.},
booktitle = {Color Appearance Models},
chapter = {CIECAM02},
edition = {2},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Fairchild - 2004 - CIECAM02.pdf:pdf},
isbn = {978-0470012161},
pages = {289--301},
publisher = {Wiley},
series = {The Wiley-IS&T Series in Imaging Science and Technology},
title = {{CIECAM02}},
year = {2004}
}
@incollection{Fairchild2013x,
author = {Fairchild, Mark D.},
booktitle = {Color Appearance Models},
chapter = {14.3},
edition = {3},
isbn = {B00DAYO8E2},
pages = {6025--6178},
publisher = {Wiley},
series = {The Wiley-IS&T Series in Imaging Science and Technology},
title = {{LLAB Model}},
year = {2013}
}
@incollection{Fairchild2013s,
author = {Fairchild, Mark D.},
booktitle = {Color Appearance Models},
chapter = {11},
edition = {3},
isbn = {B00DAYO8E2},
pages = {4418--4495},
publisher = {Wiley},
series = {The Wiley-IS&T Series in Imaging Science and Technology},
title = {{FAIRCHILD'S 1990 MODEL}},
year = {2013}
}
@incollection{Fairchild2013v,
author = {Fairchild, Mark D.},
booktitle = {Color Appearance Models},
chapter = {14.2},
edition = {3},
isbn = {B00DAYO8E2},
pages = {5852--5991},
publisher = {Wiley},
series = {The Wiley-IS&T Series in Imaging Science and Technology},
title = {{ATD Model}},
year = {2013}
}
@incollection{Fairchild2013w,
author = {Fairchild, Mark D.},
booktitle = {Color Appearance Models},
chapter = {13},
edition = {3},
isbn = {B00DAYO8E2},
pages = {5563--5824},
publisher = {Wiley},
series = {The Wiley-IS&T Series in Imaging Science and Technology},
title = {{The RLAB Model}},
year = {2013}
}
@incollection{Fairchild2013u,
author = {Fairchild, Mark D.},
booktitle = {Color Appearance Models},
chapter = {12},
edition = {3},
isbn = {B00DAYO8E2},
pages = {5094--5556},
publisher = {Wiley},
series = {The Wiley-IS&T Series in Imaging Science and Technology},
title = {{The Hunt Model}},
year = {2013}
}
@incollection{Fairchild2013t,
author = {Fairchild, Mark D.},
booktitle = {Color Appearance Models},
chapter = {11},
edition = {3},
isbn = {B00DAYO8E2},
pages = {4179--4252},
publisher = {Wiley},
series = {The Wiley-IS&T Series in Imaging Science and Technology},
title = {{Chromatic Adaptation Models}},
year = {2013}
}
@article{Fairchild1991a,
abstract = {A mathematical model of chromatic adaptation for calculating corresponding colors across changes of illumination based on the Hunt color appearance model is formulated and tested. This model consists of a modified von Kries transform that accounts for incomplete levels of adaptation. The model predicts that adaptation will be less complete as the saturation of the adapting stimulus increases and more complete as the luminance of the adapting stimulus increases. An experiment is described in which achromatic appearance is measured for various adapting conditions. The model is tested with these experimental results as well as results from another study and found to be significantly better at predicting corresponding colors than other proposed models.},
author = {Fairchild, Mark D.},
doi = {10.1002/col.5080160406},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Fairchild - 1991 - Formulation and testing of an incomplete-chromatic-adaptation model.pdf:pdf},
issn = {03612317},
journal = {Color Research & Application},
month = {aug},
number = {4},
pages = {243--250},
title = {{Formulation and testing of an incomplete-chromatic-adaptation model}},
url = {http://doi.wiley.com/10.1002/col.5080160406},
volume = {16},
year = {1991}
}
@article{Fairchild1996a,
abstract = {The prediction of color appearance using the RLAB color space has been tested for a variety of viewing conditions and stimulus types. These tests have shown that RLAB performs well for complex stimuli and not-so-well for simple stimuli. This article reviews the various psychophysical results, interprets their differences, and describes evolutionary enhancements to the RLAB model that simplify it and improve its performance. (C) 1996 John Wiley & Sons, Inc.},
annote = {https://ritdml.rit.edu/bitstream/handle/1850/7857/MFairchildArticle12-06-1998.pdf},
author = {Fairchild, Mark D.},
doi = {10.1002/(SICI)1520-6378(199610)21:5<338::AID-COL3>3.0.CO;2-Z},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Fairchild - 1996 - Refinement of the RLAB color space.pdf:pdf},
issn = {0361-2317},
journal = {Color Research & Application},
keywords = {color appearance,color spaces,color-appearance models},
month = {oct},
number = {5},
pages = {338--346},
title = {{Refinement of the RLAB color space}},
url = {http://doi.wiley.com/10.1002/%28SICI%291520-6378%28199610%2921%3A5%3C338%3A%3AAID-COL3%3E3.0.CO%3B2-Z},
volume = {21},
year = {1996}
}
@inproceedings{Fairchild2010,
author = {Fairchild, Mark D. and Wyble, David R.},
booktitle = {Proc. of Color and Imaging Conference},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Fairchild, Wyble - 2010 - hdr-CIELAB and hdr-IPT Simple Models for Describing the Color of High-Dynamic-Range and Wide-Color-Gamut Image.pdf:pdf},
isbn = {9781629932156},
issn = {21669635},
keywords = {Copyright 2010 Society for Imaging Science and Tec},
pages = {322--326},
title = {{hdr-CIELAB and hdr-IPT: Simple Models for Describing the Color of High-Dynamic-Range and Wide-Color-Gamut Images}},
url = {http://www.ingentaconnect.com/content/ist/cic/2010/00002010/00000001/art00057},
year = {2010}
}
@article{Fairman1985b,
author = {Fairman, Hugh S.},
doi = {10.1002/col.5080100407},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Fairman - 1985 - The calculation of weight factors for tristimulus integration.pdf:pdf},
issn = {03612317},
journal = {Color Research & Application},
number = {4},
pages = {199--203},
title = {{The calculation of weight factors for tristimulus integration}},
url = {http://doi.wiley.com/10.1002/col.5080100407},
volume = {10},
year = {1985}
}
@article{Fairman1997,
abstract = {Page 1. How the CIE 1931 Color-Matching Functions Were Derived from Wright-Guild Data Hugh S. Fairman, 1 Michael H. Brill, 2 Henry Hemmendinger 3},
annote = {http://infocom.ing.uniroma1.it/gscarano/texware/Full-How the CIE 1931 Color-Matching Functions Were Derived from Wright-Guild Data.pdf},
author = {Fairman, Hugh S. and Brill, Michael H. and Hemmendinger, Henry},
doi = {10.1002/(SICI)1520-6378(199702)22:1<11::AID-COL4>3.0.CO;2-7},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Fairman, Brill, Hemmendinger - 1997 - How the CIE 1931 color-matching functions were derived from Wright-Guild data.pdf:pdf},
issn = {0361-2317},
journal = {Color Research & Application},
keywords = {alychne,chromaticity diagram,cie,cie 1931 system,color-matching,colorimetry,cus,guild data,mation,primary colors,spectrum lo-,transfor-,wright},
month = {feb},
number = {1},
pages = {11--23},
title = {{How the CIE 1931 color-matching functions were derived from Wright-Guild data}},
url = {http://doi.wiley.com/10.1002/%28SICI%291520-6378%28199702%2922%3A1%3C11%3A%3AAID-COL4%3E3.0.CO%3B2-7},
volume = {22},
year = {1997}
}
@article{Finlayson2015,
abstract = {Cameras record three color responses (RGB) which are device dependent. Camera coordinates are mapped to a standard color space, such as XYZ—useful for color measurement—by amapping function, e.g., the simple 3×3 linear transform (usually derived through regression). This mapping, which we will refer to as linear color correction (LCC), has been demonstrated to work well in the number of studies. However, it can map RGBs to XYZs with high error. The advantage of the LCC is that it is independent of camera exposure. An alternative and potentially more powerful method for color correction is polynomial color correction (PCC). Here, the R, G,and B values at a pixel are extended by the polynomial terms. For a given calibration training set PCC can significantly reduce the colorimetric error. However, the PCC fit depends on exposure, i.e., as exposure changes the vector of polynomial components is altered in a nonlinear way which results in hue and saturation shifts. This paper proposes a new polynomial-type regression loosely related to the idea of fractional polynomials which we call root-PCC (RPCC). Our idea is to take each term in a polynomial expansion and take its kth root of each k-degree term. It is easy to show terms defined in this way scale with exposure. RPCC is a simple (low complexity) extension of LCC. The experiments presented in this paper demonstrate that RPCC enhances color correction performance on real and synthetic data.},
author = {Finlayson, Graham D. and MacKiewicz, Michal and Hurlbert, Anya},
doi = {10.1109/TIP.2015.2405336},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Finlayson, MacKiewicz, Hurlbert - 2015 - Color Correction Using Root-Polynomial Regression.pdf:pdf},
isbn = {1057-7149 VO - 24},
issn = {10577149},
journal = {IEEE Transactions on Image Processing},
keywords = {Color correction,camera characterization,polynomial regression},
month = {may},
number = {5},
pages = {1460--1470},
title = {{Color Correction Using Root-Polynomial Regression}},
url = {http://ieeexplore.ieee.org/document/7047834/},
volume = {24},
year = {2015}
}
@misc{Forsythe2018,
author = {Forsythe, Alex},
title = {{Private Discussion with Mansencal, T}},
year = {2018}
}
@misc{Gaggioni,
author = {Gaggioni, Hugo and Dhanendra, Patel and Yamashita, Jin and Kawada, N. and Endo, K. and Clark, Curtis},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Gaggioni et al. - Unknown - S-Log A new LUT for digital production mastering and interchange applications.pdf:pdf},
pages = {1--13},
title = {{S-Log: A new LUT for digital production mastering and interchange applications}},
url = {http://pro.sony.com/bbsccms/assets/files/mkt/cinema/solutions/slog_manual.pdf},
volume = {709}
}
@article{Glasser1958a,
abstract = {A visually uniform color coordinate system, based upon simple mathematical formulas, is described. This system resembles the Adams chromatic-value system but replaces the quintic-parabola function with a cube-root function. For colors having reflectances greater than 0.5% the color spacing obtained agrees with Munsell spacing as closely as the modified Adams system. At lower reflectances an expanded color spacing over that of the Munsell system is provided. The cube-root equations can be solved directly for color coordinate differences in terms of simple functions of the difference in colorimeter readings or tristimulus values. The computation of color coordinates in this system is simpler and requires less computational precision than other visually uniform color coordinate systems. A simple slide rule for computing color differences in cube-root color coordinates is described. A modification of the cube-root color coordinate system which provides nearly perfect representation of the spacing of Munsell colors is described, and the appropriateness of the assumptions required to obtain this behavior is discussed.},
author = {Glasser, L. G. and McKinney, A. H. and Reilly, C. D. and Schnelle, P. D.},
doi = {10.1364/JOSA.48.000736},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Glasser et al. - 1958 - Cube-Root Color Coordinate System.pdf:pdf},
issn = {0030-3941},
journal = {Journal of the Optical Society of America},
month = {oct},
number = {10},
pages = {736},
publisher = {OSA},
title = {{Cube-Root Color Coordinate System}},
url = {https://www.osapublishing.org/abstract.cfm?URI=josa-48-10-736},
volume = {48},
year = {1958}
}
@misc{GoPro2016a,
author = {GoPro and Duiker, Haarm-Pieter and Mansencal, Thomas},
title = {gopro.py},
url = {https://github.com/hpd/OpenColorIO-Configs/blob/master/aces_1.0.3/python/aces_ocio/colorspaces/gopro.py},
urldate = {2017-04-12},
year = {2016}
}
@inproceedings{Guth1995a,
abstract = {Previous and recent revisions of the ATD model for color perception\nand visual adaption are incorporated into the version that is fully\ndescribed in this paper.},
author = {Guth, S. Lee},
booktitle = {Proc. SPIE 2414, Device-Independent Color Imaging II},
doi = {10.1117/12.206546},
editor = {Walowit, Eric},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Guth - 1995 - Further applications of the ATD model for color vision.pdf:pdf},
keywords = {chromatic adaptation,color appearances,color discriminations,color models},
month = {apr},
pages = {12--26},
title = {{Further applications of the ATD model for color vision}},
url = {http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=991324},
volume = {2414},
year = {1995}
}
@article{Hernandez-Andres1999a,
abstract = {Natural outdoor illumination daily undergoes large changes in its correlated color temperature (CCT), yet existing equations for calculating CCT from chromaticity coordinates span only part of this range. To improve both the gamut and accuracy of these CCT calculations, we use chromaticities calculated from our measurements of nearly 7000 daylight and skylight spectra to test an equation that accurately maps CIE 1931 chromaticities x and y into CCT. We extend the work of McCamy [Color Res. Appl. 12, 285-287 (1992)] by using a chromaticity epicenter for CCT and the inverse slope of the line that connects it to x and y. With two epicenters for different CCT ranges, our simple equation is accurate across wide chromaticity and CCT ranges (3000-10(6) K) spanned by daylight and skylight.},
author = {Hern{\'{a}}ndez-Andr{\'{e}}s, Javier and Lee, Raymond L. and Romero, Javier},
doi = {10.1364/AO.38.005703},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Hern{\'{a}}ndez-Andr{\'{e}}s, Lee, Romero - 1999 - Calculating correlated color temperatures across the entire gamut of daylight and skylight chro.pdf:pdf},
institution = {Departamento de Optica, Facultad de Ciencias, Universidad de Granada, Granada 18071, Spain.},
issn = {0003-6935},
journal = {Applied Optics},
month = {sep},
number = {27},
pages = {5703},
title = {{Calculating correlated color temperatures across the entire gamut of daylight and skylight chromaticities}},
url = {https://www.osapublishing.org/abstract.cfm?URI=ao-38-27-5703},
volume = {38},
year = {1999}
}
@misc{Hewlett-PackardDevelopmentCompany2009a,
author = {{Hewlett-Packard Development Company}},
file = {:Users/kelsolaar/Google Drive/Documents/Mendeley Desktop/Hewlett-Packard Development Company - 2009 - Understanding the HP DreamColor LP2480zx DCI-P3 Emulation Color Space.pdf:pdf},
pages = {1--3},
title = {{Understanding the HP DreamColor LP2480zx DCI-P3 Emulation Color Space}},
url = {http://www.hp.com/united-states/campaigns/workstations/pdfs/lp2480zx-dci--p3-emulation.pdf},
year = {2009}