From 4175bdd1f40c421fea2b3156aaf9abe57f1ded73 Mon Sep 17 00:00:00 2001 From: Thomas Mansencal Date: Wed, 1 May 2024 20:05:15 +1200 Subject: [PATCH] Update `BIBLIOGRAPHY.bib` file. --- BIBLIOGRAPHY.bib | 301 ++++++++++++++++++++++++----------------------- 1 file changed, 156 insertions(+), 145 deletions(-) diff --git a/BIBLIOGRAPHY.bib b/BIBLIOGRAPHY.bib index fab24e24b..d39ba3eb3 100644 --- a/BIBLIOGRAPHY.bib +++ b/BIBLIOGRAPHY.bib @@ -9,7 +9,7 @@ @book{ANSI2018 {{Evaluating Light Source Color Rendition}}}, author = {{ANSI} and {IES Color Committee}}, year = 2018, - publisher = {{ANSI/IES}}, + publisher = {ANSI/IES}, isbn = {978-0-87995-379-9}, annotation = {thomas.mansencal@gmail.com}, } @@ -90,10 +90,10 @@ @article{Abebe2017 pages = {1--19}, issn = 15443558, doi = {10.1145/3086577}, - abstract = {{\textcopyright} 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 + 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 @@ -173,7 +173,7 @@ @book{Barten1999 year = 1999, month = dec, number = 1999, - publisher = {{SPIE}}, + publisher = {SPIE}, issn = 10924388, doi = {10.1117/3.353254}, isbn = {978-0-8194-7849-8}, @@ -369,7 +369,7 @@ @misc{Broadbent2009a author = {Broadbent, A. D.}, year = 2009, journal = {Qu{\'e}bec, Canada: D{\'e}partement de g{\'e}nie - chimique, {\ldots}}, + chimique, {\dots}}, pages = {1--17}, urldate = {2014-06-12}, abstract = {This paper describes all the steps in the @@ -391,8 +391,8 @@ @book{Burger2009b title = {Principles of {{Digital Image Processing}}}, author = {Burger, Wilhelm and Burge, Mark James}, year = 2009, - publisher = {{Springer London}}, - address = {{London}}, + publisher = {Springer London}, + address = {London}, doi = {10.1007/978-1-84800-195-4}, isbn = {978-1-84800-194-7}, } @@ -401,7 +401,7 @@ @book{CIEDivision12022 Appearance Model}} for {{Colour Management Systems}}: {{CIECAM16}}}, author = {{CIE Division 1} and {CIE Division 8}}, year = 2022, - publisher = {{Commission Internationale de l'Eclairage}}, + publisher = {Commission Internationale de l'Eclairage}, isbn = {978-3-902842-94-7}, } @book{CIETC1-321994b, @@ -410,7 +410,7 @@ @book{CIETC1-321994b {{Illuminance Adaptations}}}, author = {{CIE TC 1-32}}, year = 1994, - publisher = {{Commission Internationale de l'Eclairage}}, + publisher = {Commission Internationale de l'Eclairage}, isbn = {978-3-900734-51-0}, } @book{CIETC1-362006a, @@ -418,7 +418,7 @@ @book{CIETC1-362006a Diagram}} with {{Physiological Axes}} - {{Part}} 1}, author = {{CIE TC 1-36}}, year = 2006, - publisher = {{Commission Internationale de l'Eclairage}}, + publisher = {Commission Internationale de l'Eclairage}, isbn = {978-3-901906-46-6}, } @incollection{CIETC1-382005e, @@ -476,7 +476,7 @@ @book{CIETC1-482004h author = {{CIE TC 1-48}}, year = 2004, journal = {CIE 015:2004 Colorimetry, 3rd Edition}, - publisher = {{Commission Internationale de l'Eclairage}}, + publisher = {Commission Internationale de l'Eclairage}, isbn = {978-3-901906-33-6}, } @incollection{CIETC1-482004i, @@ -545,8 +545,8 @@ @book{CIETC1-902017 year = 2017, series = {{Technical report / CIE}}, number = 224, - publisher = {{CIE Central Bureau}}, - address = {{Vienna}}, + publisher = {CIE Central Bureau}, + address = {Vienna}, isbn = {978-3-902842-61-9}, langid = {eng fre ger}, annotation = {OCLC: 988568299}, @@ -682,8 +682,8 @@ @techreport{Carter2018 J.H.}, year = 2018, month = oct, - address = {{Vienna}}, - institution = {{International Commission on Illumination}}, + address = {Vienna}, + institution = {International Commission on Illumination}, doi = {10.25039/TR.015.2018}, isbn = 9783902842138, } @@ -900,12 +900,10 @@ @article{Cui2002 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*. {\textcopyright} 2002 Wiley Periodicals, Inc. - Col Res Appl, 27, 282{\textendash}290, 2002; Published online in - Wiley InterScience (www.interscience.wiley.com). DOI - 10.1002/col.10066}, - copyright = {Copyright {\textcopyright} 2002 Wiley Periodicals, - Inc.}, + 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}, @@ -980,15 +978,15 @@ @article{Davis2010a doi = {10.1117/1.3360335}, abstract = {The color rendering index (CRI) has been shown to have deficiencies when applied to white - light-emitting-diode{\textendash}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 + 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, @@ -1215,7 +1213,7 @@ @incollection{Fairchild2004c year = 2004, edition = 2, pages = {289--301}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-470-01216-1}, } @inproceedings{Fairchild2010, @@ -1251,7 +1249,7 @@ @incollection{Fairchild2013ba year = 2013, edition = 3, pages = {4810--5085}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {B00DAYO8E2}, } @incollection{Fairchild2013s, @@ -1261,7 +1259,7 @@ @incollection{Fairchild2013s year = 2013, edition = 3, pages = {4418--4495}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {B00DAYO8E2}, } @incollection{Fairchild2013t, @@ -1271,7 +1269,7 @@ @incollection{Fairchild2013t year = 2013, edition = 3, pages = {4179--4252}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {B00DAYO8E2}, } @incollection{Fairchild2013u, @@ -1281,7 +1279,7 @@ @incollection{Fairchild2013u year = 2013, edition = 3, pages = {5094--5556}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {B00DAYO8E2}, } @incollection{Fairchild2013v, @@ -1291,7 +1289,7 @@ @incollection{Fairchild2013v year = 2013, edition = 3, pages = {5852--5991}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {B00DAYO8E2}, } @incollection{Fairchild2013w, @@ -1301,7 +1299,7 @@ @incollection{Fairchild2013w year = 2013, edition = 3, pages = {5563--5824}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {B00DAYO8E2}, } @incollection{Fairchild2013x, @@ -1311,7 +1309,7 @@ @incollection{Fairchild2013x year = 2013, edition = 3, pages = {6025--6178}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {B00DAYO8E2}, } @incollection{Fairchild2013y, @@ -1321,7 +1319,7 @@ @incollection{Fairchild2013y year = 2013, edition = 3, pages = {6197--6223}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {B00DAYO8E2}, } @article{Fairchild2020, @@ -1399,6 +1397,22 @@ @misc{FiLMiCInc2017 year = 2017, pages = {1--46}, } +@article{Fichet2021, + title = {An {{OpenEXR Layout}} for {{Spectral Images}}}, + author = {Fichet, A and Pacanowski, R and Wilkie, A}, + year = 2021, + volume = 10, + number = 3, + urldate = {2024-04-26}, + abstract = {We propose a standardized layout to organize + spectral data stored in OpenEXR images. We motivate why we chose + the OpenEXR format as the basis for our work, and we explain our + choices with regard to data selection and organization: our goal + is to define a standard for the exchange of measured or simulated + spectral and bi-spectral data. We also provide sample code to + store spectral images in OpenEXR format.}, + langid = {english}, +} @article{Finlayson2015, title = {Color {{Correction Using Root-Polynomial Regression}}}, @@ -1414,18 +1428,18 @@ @article{Finlayson2015 doi = {10.1109/TIP.2015.2405336}, abstract = {Cameras record three color responses (RGB) which are device dependent. Camera coordinates are mapped to a standard - color space, such as XYZ{\textemdash}useful for color - measurement{\textemdash}by amapping function, e.g., the simple - 3{\texttimes}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, + color space, such as XYZ---useful for color measurement---by + amapping function, e.g., the simple 3{\texttimes}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 @@ -1450,7 +1464,7 @@ @misc{Frohlich2017 Imagery}, author = {Fr{\"o}hlich, Jan}, year = 2017, - publisher = {{Universit{\"a}t Stuttgart}}, + publisher = {Universit{\"a}t Stuttgart}, urldate = {2021-08-07}, abstract = {In dieser Dissertation wird ein szenischer Bewegtbilddatensatz mit erweitertem Dynamikumfang (High Dynamic @@ -1552,7 +1566,7 @@ @article{Glasser1958a volume = 48, number = 10, pages = 736, - publisher = {{OSA}}, + publisher = {OSA}, issn = {0030-3941}, doi = {10.1364/JOSA.48.000736}, abstract = {A visually uniform color coordinate system, based @@ -1620,8 +1634,8 @@ @inproceedings{Hanbury2003 editor = {Bigun, Josef and Gustavsson, Tomas}, year = 2003, pages = {804--811}, - publisher = {{Springer Berlin Heidelberg}}, - address = {{Berlin, Heidelberg}}, + publisher = {Springer Berlin Heidelberg}, + address = {Berlin, Heidelberg}, abstract = {Representations of the RGB space in terms of 3D-polar coordinates (hue, saturation and brightness) are often used in image analysis. The literature describes a large number of @@ -1686,7 +1700,7 @@ @article{Hellwig2022 } @article{Hellwig2022a, title = {Extending {{CIECAM02}} and {{CAM16}} for the - {{Helmholtz}}{\textendash}{{Kohlrausch}} Effect}, + {{Helmholtz}}--{{Kohlrausch}} Effect}, shorttitle = {Extending}, author = {Hellwig, Luke and Stolitzka, Dale and Fairchild, Mark D.}, @@ -1710,8 +1724,8 @@ @article{Hernandez-Andres1999a volume = 38, number = 27, pages = 5703, - publisher = {{Departamento de Optica, Facultad de Ciencias, - Universidad de Granada, Granada 18071, Spain.}}, + publisher = {Departamento de Optica, Facultad de Ciencias, + Universidad de Granada, Granada 18071, Spain.}, issn = {0003-6935}, doi = {10.1364/AO.38.005703}, abstract = {Natural outdoor illumination daily undergoes large @@ -1779,8 +1793,8 @@ @book{Hunt2004b year = 2004, month = sep, edition = 6, - publisher = {{John Wiley \& Sons, Ltd}}, - address = {{Chichester, UK}}, + publisher = {John Wiley \& Sons, Ltd}, + address = {Chichester, UK}, doi = {10.1002/0470024275}, isbn = {978-0-470-02427-0}, keywords = {calanus finmarchicus,egg production,gonad @@ -1828,7 +1842,7 @@ @book{IESComputerCommittee2014a author = {{IES Computer Committee} and {TM-27-14 Working Group}}, year = 2014, - publisher = {{Illuminating Engineering Society}}, + publisher = {Illuminating Engineering Society}, isbn = {978-0-87995-295-2}, } @misc{ImageEngineering2017, @@ -2012,7 +2026,7 @@ @inproceedings{Jiang2013 year = 2013, month = jan, pages = {168--179}, - publisher = {{IEEE}}, + publisher = {IEEE}, issn = 21583978, doi = {10.1109/WACV.2013.6475015}, abstract = {Camera spectral sensitivity functions relate scene @@ -2131,8 +2145,8 @@ @article{Konovalenko2021 to perform linear colour analysis.}, archiveprefix = {arxiv}, langid = {english}, - keywords = {⛔ No DOI found,Computer Science - Computer Vision - and Pattern Recognition}, + keywords = {Computer Science - Computer Vision and Pattern + Recognition,No DOI found}, } @misc{Konovalenko2021a, title = {{{proLab}}\_param.m}, @@ -2148,7 +2162,7 @@ @article{Krystek1985b volume = 10, number = 1, pages = {38--40}, - publisher = {{Wiley Subscription Services, Inc., A Wiley Company}}, + publisher = {Wiley Subscription Services, Inc., A Wiley Company}, issn = 03612317, doi = {10.1002/col.5080100109}, } @@ -2300,23 +2314,23 @@ @article{Lu2016c pages = {32--38}, abstract = {High Dynamic Range (HDR) and Wider Colour Gamut (WCG) content represents a greater range of luminance levels and a - more complete reproduction of colours found in - real{$\hyphenbullet$}world scenes. The current video distribution - environments deliver Standard Dynamic Range (SDR) signal - Y{${'}$}CbCr. For HDR and WCG content, it is desirable to examine - if such signal format still works well for compression, and to - know if the overall system performance can be further improved by - exploring different signal formats. In this paper, ITP (ICTCP) - colour space is presented. The paper concentrates on examining the - two aspects of ITP colour space: 1) ITP characteristics in terms - of signal quantization at a given bit depth; 2) ITP compression - performance. The analysis and simulation results show that ITP 10 - bit has better properties than Y{${'}$}CbCr{$\hyphenbullet$}PQ - 10bit in colour quantization, constant luminance, hue property and - chroma subsampling, and it also has good compression efficiency. - Therefore it is desirable to adopt ITP colour space as a new - signal format for HDR/WCG video compression.}, - keywords = {HDR,ICT CP,ITP,WCG,Y{${'}$}CbCr}, + more complete reproduction of colours found in real⁃world scenes. + The current video distribution environments deliver Standard + Dynamic Range (SDR) signal Y{$\prime$}CbCr. For HDR and WCG + content, it is desirable to examine if such signal format still + works well for compression, and to know if the overall system + performance can be further improved by exploring different signal + formats. In this paper, ITP (ICTCP) colour space is presented. The + paper concentrates on examining the two aspects of ITP colour + space: 1) ITP characteristics in terms of signal quantization at a + given bit depth; 2) ITP compression performance. The analysis and + simulation results show that ITP 10 bit has better properties than + Y{$\prime$}CbCr⁃PQ 10bit in colour quantization, constant + luminance, hue property and chroma subsampling, and it also has + good compression efficiency. Therefore it is desirable to adopt + ITP colour space as a new signal format for HDR/WCG video + compression.}, + keywords = {HDR,ICT CP,ITP,WCG,Y'CbCr}, } @article{Luo1996b, title = {The {{LLAB}} (l:C) Colour Model}, @@ -2327,7 +2341,7 @@ @article{Luo1996b volume = 21, number = 6, pages = {412--429}, - publisher = {{Wiley Subscription Services, Inc., A Wiley Company}}, + publisher = {Wiley Subscription Services, Inc., A Wiley Company}, issn = {0361-2317}, doi = {10.1002/(SICI)1520-6378(199612)21:6<412::AID-COL4>3.0.CO;2-Z}, abstract = {A new colour model, named LLAB(l:c) is derived. It @@ -2350,7 +2364,7 @@ @article{Luo1996b constancy, and quantification of colour-rendering properties. The model does not give predictions for chroma (as distinct from colourfulness), or for brightness, and it does not include any rod - response. {\textcopyright} 1996 John Wiley \& Sons, Inc.}, + response. {\copyright} 1996 John Wiley \& Sons, Inc.}, keywords = {chromatic adaptation transform,colour appearance,colour appearance model,colour difference,colour difference formula,corresponding colours,uniform colour space}, @@ -2359,8 +2373,8 @@ @inproceedings{Luo1996c title = {Two {{Unsolved Issues}} in {{Colour Management}} - {{Colour Appearance}} and {{Gamut Mapping}}}, booktitle = {Conference: 5th {{International Conference}} on - {{High Technology}}: {{Imaging Science}} and {{Technology}} - {\textendash} {{Evolution}} \& {{Promise}}}, + {{High Technology}}: {{Imaging Science}} and {{Technology}} -- + {{Evolution}} \& {{Promise}}}, author = {Luo, Ming Ronnier and Morovic, J{\'a}n}, year = 1996, pages = {136--147}, @@ -2444,8 +2458,8 @@ @incollection{Luo2013 editor = {{Fernandez-Maloigne}, Christine}, year = 2013, pages = {19--58}, - publisher = {{Springer New York}}, - address = {{New York, NY}}, + publisher = {Springer New York}, + address = {New York, NY}, doi = {10.1007/978-1-4419-6190-7}, urldate = {2014-09-27}, isbn = {978-1-4419-6189-1}, @@ -2463,7 +2477,7 @@ @article{MacAdam1935a volume = 25, number = 11, pages = {361--367}, - publisher = {{OSA}}, + publisher = {OSA}, doi = {10.1364/JOSA.25.000361}, abstract = {Tristimulus values have been computed for hypothetical spectrophotometric curves of the type found to give @@ -2580,7 +2594,7 @@ @article{Mallett2019 journal = {Eurographics Symposium on Rendering - DL-only and Industry Track}, pages = {7 pages}, - publisher = {{The Eurographics Association}}, + publisher = {The Eurographics Association}, issn = {1727-3463}, doi = {10.2312/SR.20191216}, urldate = {2020-08-08}, @@ -2705,7 +2719,7 @@ @article{Mokrzycki2011 popular colors spaces, as both linear and nonlinear due to perceptual abilities, and are briefly discussed and compared to the sample values.}, - keywords = {⛔ No DOI found}, + keywords = {No DOI found}, } @article{Moroney2003, title = {A {{Radial Sampling}} of the {{OSA Uniform Color @@ -2735,7 +2749,7 @@ @article{Moroney2003 parent_itemid = {infobike://ist/cic}, publication_date = {2003-01-01T00:00:00}, publishercode = {ist}, - keywords = {⛔ No DOI found}, + keywords = {No DOI found}, } @article{Moroneya, title = {The {{CIECAM02}} Color Appearance Model}, @@ -2777,7 +2791,7 @@ @article{Morovic2000 Descriptor obtained using the Segment Maxima Method. Throughout the article, the focus is both on colour reproduction media and colour images as well as on the suitability of the methods for use - in gamut mapping. {\textcopyright} 2000 John Wiley \& Sons. Inc.}, + in gamut mapping. {\copyright} 2000 John Wiley \& Sons. Inc.}, keywords = {Cross-media reproduction,Gamut boundary calculation,Gamut mapping}, } @@ -2814,7 +2828,7 @@ @article{Nayatani1995a volume = 20, number = 3, pages = {156--167}, - publisher = {{Wiley Subscription Services, Inc., A Wiley Company}}, + publisher = {Wiley Subscription Services, Inc., A Wiley Company}, issn = 03612317, doi = {10.1002/col.5080200305}, keywords = {color-vision model,lightness dependency of @@ -2822,7 +2836,7 @@ @article{Nayatani1995a } @article{Nayatani1997, title = {Simple Estimation Methods for the - {{Helmholtz}}{\textemdash}{{Kohlrausch}} Effect}, + {{Helmholtz}}---{{Kohlrausch}} Effect}, author = {Nayatani, Yoshinobu}, year = 1997, journal = {Color Research \& Application}, @@ -2833,32 +2847,29 @@ @article{Nayatani1997 doi = {10.1002/(SICI)1520-6378(199712)22:6<385::AID-COL6>3.0.CO;2-R}, urldate = {2021-06-22}, abstract = {Four kinds of simple estimation equations are - proposed for the Helmholtz{\textemdash}Kohlrausch effect. Two of - them can be used for luminous colors, and the other two for object - colors. In each of luminous and object colors, the two estimation - equations are given to each of the Variable-Achromatic-Color (VAC) - and the Variable-Chromatic-Color (VCC) methods. All the equations - are similar in type to the Ware{\textemdash}Cowan equation. They - give the ratio between luminance (or metric lightness) of test - color stimulus and its equivalent luminance (or equivalent - lightness) directly. Though their computations are simple, they - can apply to various H{\textemdash}K effects including their - adapting luminance dependency. The applicable fields of the - proposed equations are wider than those of the - Ware{\textemdash}Cowan equation. The proposed equations can be - applied to predict the H{\textemdash}K effect within the whole - chromaticity gamut including spectral colors, spectral luminosity - functions based on direct color matching from 0.01 Td to 100 000 - Td using the photopic and the scotopic spectral luminosity - functions specified by CIE, equivalent lightness values of NCS - colors, and others. {\textcopyright} 1997 John Wiley \& Sons, Inc. - Col Res Appl. 22, 385{\textendash}401, 1997}, - copyright = {Copyright {\textcopyright} 1997 John Wiley \& Sons, - Inc.}, + proposed for the Helmholtz---Kohlrausch effect. Two of them can be + used for luminous colors, and the other two for object colors. In + each of luminous and object colors, the two estimation equations + are given to each of the Variable-Achromatic-Color (VAC) and the + Variable-Chromatic-Color (VCC) methods. All the equations are + similar in type to the Ware---Cowan equation. They give the ratio + between luminance (or metric lightness) of test color stimulus and + its equivalent luminance (or equivalent lightness) directly. + Though their computations are simple, they can apply to various + H---K effects including their adapting luminance dependency. The + applicable fields of the proposed equations are wider than those + of the Ware---Cowan equation. The proposed equations can be + applied to predict the H---K effect within the whole chromaticity + gamut including spectral colors, spectral luminosity functions + based on direct color matching from 0.01 Td to 100 000 Td using + the photopic and the scotopic spectral luminosity functions + specified by CIE, equivalent lightness values of NCS colors, and + others. {\copyright} 1997 John Wiley \& Sons, Inc. Col Res Appl. + 22, 385--401, 1997}, + copyright = {Copyright {\copyright} 1997 John Wiley \& Sons, Inc.}, langid = {english}, keywords = {CIELUV formula,color appearance,equivalent - lightness,equivalent luminance,Helmholtz{\textemdash}Kohlrausch - effect}, + lightness,equivalent luminance,Helmholtz-Kohlrausch effect}, } @article{Newhall1943a, title = {Final {{Report}} of the {{OSA Subcommittee}} on the @@ -3219,8 +3230,8 @@ @inproceedings{Smith1978b author = {Smith, Alvy Ray}, year = 1978, pages = {12--19}, - publisher = {{ACM Press}}, - address = {{New York, New York, USA}}, + publisher = {ACM Press}, + address = {New York, New York, USA}, doi = {10.1145/800248.807361}, keywords = {Brightness,Color,Color transform,color transforms,Gamut,HSL,HSV,Hue,Luminance,NTSC,RGB,Saturation,Value}, @@ -3235,7 +3246,7 @@ @article{Smits1999a volume = 4, number = 4, pages = {11--22}, - publisher = {{AK Peters, Ltd.}}, + publisher = {AK Peters, Ltd.}, issn = {1086-7651}, doi = {10.1080/10867651.1999.10487511}, urldate = {2014-09-19}, @@ -3308,7 +3319,7 @@ @misc{SocietyofMotionPictureandTelevisionEngineers2014a } @misc{SocietyofMotionPictureandTelevisionEngineers2019, title = {{{ST}} 428-1:2019 - {{D-Cinema Distribution Master}} - {\textemdash} {{Image Characteristic}}}, + --- {{Image Characteristic}}}, author = {{Society of Motion Picture and Television Engineers}}, year = 2019, doi = {10.5594/SMPTE.ST428-1.2019}, @@ -3388,7 +3399,7 @@ @article{Stearns1988a volume = 13, number = 4, pages = {257--259}, - publisher = {{Wiley Subscription Services, Inc., A Wiley Company}}, + publisher = {Wiley Subscription Services, Inc., A Wiley Company}, issn = 03612317, doi = {10.1002/col.5080130410}, } @@ -3623,7 +3634,7 @@ @article{Ward2002 year = 2002, journal = {Eurographics workshop on Rendering}, pages = {117--124}, - publisher = {{Eurographics Association}}, + publisher = {Eurographics Association}, doi = {10.2312/EGWR/EGWR02/117-124}, urldate = {2014-09-27}, abstract = {Abstract Accurate color requires the consideration @@ -3658,8 +3669,8 @@ @incollection{Westland2004 month = mar, edition = 1, pages = 137, - publisher = {{John Wiley \& Sons, Ltd}}, - address = {{Chichester, UK}}, + publisher = {John Wiley \& Sons, Ltd}, + address = {Chichester, UK}, doi = {10.1002/0470020326}, isbn = {978-0-470-84562-2}, } @@ -3790,11 +3801,11 @@ @misc{Wikipedia2003e howpublished = {https://en.wikipedia.org/wiki/Vandermonde\_matrix}, } @misc{Wikipedia2003f, - title = {Rayleigh{\textendash}{{Jeans}} Law}, + title = {Rayleigh--{{Jeans}} Law}, author = {{Wikipedia}}, year = 2003, urldate = {2022-02-12}, - howpublished = {https://en.wikipedia.org/wiki/Rayleigh{\textendash}Jeans\_law}, + howpublished = {https://en.wikipedia.org/wiki/Rayleigh--Jeans\_law}, } @misc{Wikipedia2004, title = {Peak Signal-to-Noise Ratio}, @@ -3966,7 +3977,7 @@ @article{Wyszecki1963b volume = 53, number = 11, pages = 1318, - publisher = {{OSA}}, + publisher = {OSA}, issn = {0030-3941}, doi = {10.1364/JOSA.53.001318}, urldate = {2014-09-26}, @@ -3981,7 +3992,7 @@ @incollection{Wyszecki2000 author = {Wyszecki, G{\"u}nther and Stiles, W S}, year = 2000, pages = 309, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-471-39918-6}, } @incollection{Wyszecki2000a, @@ -3991,7 +4002,7 @@ @incollection{Wyszecki2000a author = {Wyszecki, G{\"u}nther and Stiles, W S}, year = 2000, pages = 8, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-471-39918-6}, } @incollection{Wyszecki2000ba, @@ -4002,7 +4013,7 @@ @incollection{Wyszecki2000ba author = {Wyszecki, G{\"u}nther and Stiles, W. S.}, year = 2000, pages = {837--839}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-471-39918-6}, } @incollection{Wyszecki2000bb, @@ -4012,7 +4023,7 @@ @incollection{Wyszecki2000bb author = {Wyszecki, G{\"u}nther and Stiles, W. S.}, year = 2000, pages = {776--777}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-471-39918-6}, } @incollection{Wyszecki2000bd, @@ -4023,7 +4034,7 @@ @incollection{Wyszecki2000bd author = {Wyszecki, G{\"u}nther and Stiles, W. S.}, year = 2000, pages = 167, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-471-39918-6}, } @incollection{Wyszecki2000be, @@ -4033,7 +4044,7 @@ @incollection{Wyszecki2000be author = {Wyszecki, G{\"u}nther and Stiles, W. S.}, year = 2000, pages = 141, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-471-39918-6}, } @incollection{Wyszecki2000bf, @@ -4043,7 +4054,7 @@ @incollection{Wyszecki2000bf author = {Wyszecki, G{\"u}nther and Stiles, W. S.}, year = 2000, pages = {158--163}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-471-39918-6}, } @incollection{Wyszecki2000bg, @@ -4053,7 +4064,7 @@ @incollection{Wyszecki2000bg author = {Wyszecki, G{\"u}nther and Stiles, W. S.}, year = 2000, pages = {138--139}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-471-39918-6}, } @incollection{Wyszecki2000bh, @@ -4063,7 +4074,7 @@ @incollection{Wyszecki2000bh author = {Wyszecki, G{\"u}nther and Stiles, W. S.}, year = 2000, pages = {778--779}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-471-39918-6}, } @incollection{Wyszecki2000s, @@ -4073,7 +4084,7 @@ @incollection{Wyszecki2000s author = {Wyszecki, G{\"u}nther and Stiles, W. S.}, year = 2000, pages = {256--259,395}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-471-39918-6}, } @incollection{Wyszecki2000x, @@ -4083,7 +4094,7 @@ @incollection{Wyszecki2000x author = {Wyszecki, G{\"u}nther and Stiles, W. S.}, year = 2000, pages = 228, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-471-39918-6}, } @incollection{Wyszecki2000y, @@ -4094,7 +4105,7 @@ @incollection{Wyszecki2000y author = {Wyszecki, G{\"u}nther and Stiles, W. S.}, year = 2000, pages = {224--229}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-471-39918-6}, } @incollection{Wyszecki2000z, @@ -4104,7 +4115,7 @@ @incollection{Wyszecki2000z author = {Wyszecki, G{\"u}nther and Stiles, W. S.}, year = 2000, pages = {145--146}, - publisher = {{Wiley}}, + publisher = {Wiley}, isbn = {978-0-471-39918-6}, } @misc{X-Rite2012a,