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<article id="srt70374" xml:lang="en" article-type="research-article" dtd-version="1.4"><?da-xref-anchor-style superscripted?><processing-meta base-tagset="archiving" mathml-version="3.0" table-model="xhtml" tagset-family="jats"><restricted-by>pmc</restricted-by></processing-meta><front><journal-meta><journal-id journal-id-type="nlm-ta">Skin Res Technol</journal-id><journal-id journal-id-type="iso-abbrev">Skin Res Technol</journal-id><journal-id journal-id-type="pmc-domain-id">4358</journal-id><journal-id journal-id-type="pmc-domain">skinres</journal-id><journal-id journal-id-type="nlm-id">9504453</journal-id><journal-id journal-id-type="publisher-id">SRT</journal-id><journal-title-group><journal-title>Skin Research and Technology</journal-title></journal-title-group><issn pub-type="ppub">0909-752X</issn><issn pub-type="epub">1600-0846</issn><?publisher_abbrev blackwell?><publisher><publisher-name>Wiley</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="pmcid">PMC13459198</article-id><article-id pub-id-type="pmcid-ver">PMC13459198.1</article-id><article-id pub-id-type="pmcaid">13459198</article-id><article-id pub-id-type="pmcaiid">13459198</article-id><article-id pub-id-type="pmid">42578529</article-id><article-id pub-id-type="doi">10.1111/srt.70374</article-id><article-id pub-id-type="publisher-id">SRT70374</article-id><article-version article-version-type="pmc-version">1</article-version><article-categories><subj-group subj-group-type="overline"><subject>Original Article</subject></subj-group><subj-group subj-group-type="heading"><subject>Original Article</subject></subj-group></article-categories><title-group><article-title>Limitations of ITA for Skin Type Estimation Under Uncontrolled Imaging Conditions</article-title></title-group><contrib-group><contrib id="srt70374-cr-0001" contrib-type="author" corresp="yes"><name name-style="western"><surname>Alipour</surname><given-names initials="N">Neda</given-names></name><xref rid="srt70374-aff-0001" ref-type="aff">
<sup>1</sup>
</xref><address><email>neda.alipourmoradbeglouei@tudublin.ie</email></address></contrib><contrib id="srt70374-cr-0002" contrib-type="author"><name name-style="western"><surname>Burke</surname><given-names initials="T">Ted</given-names></name><xref rid="srt70374-aff-0001" ref-type="aff">
<sup>1</sup>
</xref></contrib><contrib id="srt70374-cr-0003" contrib-type="author"><name name-style="western"><surname>Courtney</surname><given-names initials="J">Jane</given-names></name><xref rid="srt70374-aff-0001" ref-type="aff">
<sup>1</sup>
</xref></contrib></contrib-group><aff id="srt70374-aff-0001">
<label>
<sup>1</sup>
</label>
<named-content content-type="organisation-division">School of Electrical and Electronic Engineering</named-content>
<institution>Technological University Dublin</institution>
<city>Dublin</city>
<country country="IE">Ireland</country>
</aff><pub-date pub-type="epub"><day>11</day><month>8</month><year>2026</year></pub-date><pub-date pub-type="collection"><month>8</month><year>2026</year></pub-date><volume>32</volume><issue seq="20">8</issue><issue-id pub-id-type="pmc-issue-id">519404</issue-id><issue-id pub-id-type="doi">10.1111/srt.v32.8</issue-id><elocation-id>e70374</elocation-id><history>
<date date-type="rev-recd"><day>02</day><month>6</month><year>2026</year></date>
<date date-type="received"><day>02</day><month>4</month><year>2025</year></date>
<date date-type="accepted"><day>18</day><month>7</month><year>2026</year></date>
</history><pub-history><event event-type="pmc-release"><date><day>11</day><month>08</month><year>2026</year></date></event><event event-type="pmc-live"><date><day>12</day><month>08</month><year>2026</year></date></event><event event-type="pmc-last-change"><date iso-8601-date="2026-08-24 20:25:17.903"><day>24</day><month>08</month><year>2026</year></date></event></pub-history><permissions><copyright-statement content-type="article-copyright">© 2026 The Author(s). <italic toggle="yes">Skin Research and Technology</italic> published by John Wiley &amp; Sons Ltd.</copyright-statement><license><ali:license_ref xmlns:ali="http://www.niso.org/schemas/ali/1.0/" specific-use="textmining" content-type="ccbylicense">https://creativecommons.org/licenses/by/4.0/</ali:license_ref><license-p>This is an open access article under the terms of the <ext-link xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">http://creativecommons.org/licenses/by/4.0/</ext-link> License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.</license-p></license></permissions><self-uri xmlns:xlink="http://www.w3.org/1999/xlink" content-type="pmc-pdf" xlink:href="SRT-32-e70374.pdf"><?pdf-name SRT-32-e70374.pdf?><?pdf-size 3269966?><?pdf-md5 c74384d66f02564fd664b56db0ea7ace?><?pdf-image-server-status NEVER_LOAD?><?pdf-cloudpmc-urn urn:app:2871/13459198/c74384d66f02/SRT-32-e70374.pdf?></self-uri><self-uri xmlns:xlink="http://www.w3.org/1999/xlink" content-type="pdf" xlink:href="file:SRT-32-e70374.pdf"/><abstract><title>ABSTRACT</title><sec id="srt70374-sec-0010"><title>Background</title><p>Accurately assessing skin color diversity is essential for evaluating whether image datasets without explicit skin type labels are sufficiently diverse for training deep learning models. Traditional methods, such as the Fitzpatrick scale, categorize skin types into six discrete classes but may not fully capture the complexity of skin color and its interaction with light under varying conditions. Continuous and quantitative approaches have been proposed to better represent skin color variation, but their reliability under uncontrolled imaging conditions remains unclear.</p></sec><sec id="srt70374-sec-0020"><title>Materials and Methods</title><p>This study evaluated individual typology angle (ITA), an image‐derived color or lightness metric commonly mapped to Fitzpatrick skin type (FST) categories. A dermatologist‐labeled dataset (PAD‐UFES‐20) was used to analyze the performance of ITA. A skin patch image dataset was derived from PAD‐UFES‐20, and skin color features were extracted for evaluation.</p></sec><sec id="srt70374-sec-0030"><title>Results</title><p>The results showed substantial overlap between ITA distributions across FST categories and poor agreement with dermatologist‐assigned labels. Fixed‐threshold ITA classification achieved 22.9% accuracy, below the majority‐class baseline accuracy of 51.3%, and failed to correctly classify the darkest skin type (FST VI). Lighting variation, threshold misalignment, overlapping ITA distributions, and dataset imbalance contributed to unstable ITA behavior across skin types.</p></sec><sec id="srt70374-sec-0040"><title>Conclusion</title><p>Under uncontrolled imaging conditions, fixed‐threshold ITA did not provide reliable Fitzpatrick skin type classification and should not be interpreted as a validated skin type measurement method. These findings demonstrate that ITA is highly sensitive to lighting variation and does not reliably correspond to dermatologist‐assigned FST labels. The results highlight the limitations of using ITA as a proxy for skin type assessment in image datasets.</p></sec></abstract><kwd-group kwd-group-type="author-generated"><kwd id="srt70374-kwd-0001">Fitzpatrick skin type</kwd><kwd id="srt70374-kwd-0002">ITA</kwd><kwd id="srt70374-kwd-0003">lighting variation</kwd><kwd id="srt70374-kwd-0004">skin type measurement</kwd></kwd-group><funding-group><award-group id="funding-0001"><funding-source>
<institution-wrap><institution>Science Foundation Ireland</institution><institution-id institution-id-type="doi">10.13039/501100001602</institution-id></institution-wrap>
</funding-source><award-id>18/CRT/6222</award-id></award-group></funding-group><counts><fig-count count="16"/><table-count count="5"/><page-count count="18"/><word-count count="10452"/></counts><custom-meta-group><custom-meta><meta-name>pmc-status-qastatus</meta-name><meta-value>0</meta-value></custom-meta><custom-meta><meta-name>pmc-status-live</meta-name><meta-value>yes</meta-value></custom-meta><custom-meta><meta-name>pmc-status-embargo</meta-name><meta-value>no</meta-value></custom-meta><custom-meta><meta-name>pmc-status-released</meta-name><meta-value>yes</meta-value></custom-meta><custom-meta><meta-name>pmc-prop-open-access</meta-name><meta-value>yes</meta-value></custom-meta><custom-meta><meta-name>pmc-prop-olf</meta-name><meta-value>no</meta-value></custom-meta><custom-meta><meta-name>pmc-prop-manuscript</meta-name><meta-value>no</meta-value></custom-meta><custom-meta><meta-name>pmc-prop-legally-suppressed</meta-name><meta-value>no</meta-value></custom-meta><custom-meta><meta-name>pmc-prop-has-pdf</meta-name><meta-value>yes</meta-value></custom-meta><custom-meta><meta-name>pmc-prop-has-supplement</meta-name><meta-value>no</meta-value></custom-meta><custom-meta><meta-name>pmc-prop-pdf-only</meta-name><meta-value>no</meta-value></custom-meta><custom-meta><meta-name>pmc-prop-suppress-copyright</meta-name><meta-value>no</meta-value></custom-meta><custom-meta><meta-name>pmc-prop-is-real-version</meta-name><meta-value>no</meta-value></custom-meta><custom-meta><meta-name>pmc-prop-is-scanned-article</meta-name><meta-value>no</meta-value></custom-meta><custom-meta><meta-name>pmc-prop-preprint</meta-name><meta-value>no</meta-value></custom-meta><custom-meta><meta-name>pmc-prop-in-epmc</meta-name><meta-value>yes</meta-value></custom-meta><custom-meta><meta-name>pmc-license-ref</meta-name><meta-value>CC BY</meta-value></custom-meta><custom-meta><meta-name>source-schema-version-number</meta-name><meta-value>2.0</meta-value></custom-meta><custom-meta><meta-name>cover-date</meta-name><meta-value>August 2026</meta-value></custom-meta><custom-meta><meta-name>details-of-publishers-convertor</meta-name><meta-value>Converter:WILEY_ML3GV2_TO_JATSPMC version:6.8.5 mode:remove_FC converted:11.08.2026</meta-value></custom-meta></custom-meta-group></article-meta></front><body><sec id="srt70374-sec-0050"><label>1</label><title>Introduction</title><p>Ensuring skin type diversity is essential for AI‐based skin analysis applications, as it affects the accuracy of tasks such as detecting skin conditions and evaluating treatment outcomes [<xref rid="srt70374-bib-0001" ref-type="bibr">1</xref>, <xref rid="srt70374-bib-0002" ref-type="bibr">2</xref>]. Studies like Gender Shades have highlighted how disparities in dataset representation can lead to significant performance gaps in AI systems, particularly for underrepresented groups such as individuals with darker skin types [<xref rid="srt70374-bib-0003" ref-type="bibr">3</xref>]. Reliable measurement of skin type diversity is crucial for creating datasets that allow AI models to generalize across different skin types. In dermatology, the Fitzpatrick skin type (FST) is the most used system to classify skin type, providing a standard for healthcare professionals and aesthetic practitioners [<xref rid="srt70374-bib-0004" ref-type="bibr">4</xref>]. This system involves a face‐to‐face meeting with dermatologists [<xref rid="srt70374-bib-0005" ref-type="bibr">5</xref>, <xref rid="srt70374-bib-0006" ref-type="bibr">6</xref>]. The Fitzpatrick scale, which categorizes skin based on its color and reaction to initial sun exposure resulting in erythema (burning or tanning), was originally developed by Thomas B. Fitzpatrick in 1975 [<xref rid="srt70374-bib-0007" ref-type="bibr">7</xref>]. This classification system is subjective, as it relies on self‐reporting or dermatologist assessment rather than quantitative metrics. These six skin types are shown in Figure <xref rid="srt70374-fig-0001" ref-type="fig">1</xref>.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0001" orientation="portrait"><label>FIGURE 1</label><caption><p>The FST system categorizes various skin colors from type I (very light) to type VI (dark).</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-1" orientation="portrait" xlink:href="SRT-32-e70374-g005.jpg"><?image-name SRT-32-e70374-g005.jpg?><?image-size 10284?><?image-md5 81ff7df3e4cba98c3771a30cd7286036?><?image-image-server-status NEVER_LOAD?><?image-original-height 135?><?image-original-width 700?><?image-scaled-height 135?><?image-scaled-width 700?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/81ff7df3e4cb/SRT-32-e70374-g005.jpg?><?thumb-name SRT-32-e70374-g005.gif?><?thumb-size 4541?><?thumb-md5 e057a651e216ae70bc60033f70580b5f?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 39?><?thumb-scaled-width 200?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/e057a651e216/SRT-32-e70374-g005.gif?></graphic></fig><p>An alternative extension to the Fitzpatrick classification is the Monk Skin Tone (MST) [<xref rid="srt70374-bib-0008" ref-type="bibr">8</xref>] scale, a 10‐point system developed by Ellis Monk to more comprehensively represent the diversity of human skin tones in fairness‐focused AI applications. However, like Fitzpatrick, it discretizes the continuous skin color spectrum into fixed categories and therefore cannot fully capture the nuanced variations observed in real‐world skin colors.</p><p>Prior research has shown that using automated methods, skin type assessment can be done directly from images [<xref rid="srt70374-bib-0009" ref-type="bibr">9</xref>, <xref rid="srt70374-bib-0010" ref-type="bibr">10</xref>]. However, there are some limitations when detecting exact skin types using automatic methods; for instance, the methods face challenges in determining skin type in images taken under different lighting conditions and may not perform well for all skin type groups. Therefore, a comprehensive review of existing skin type measurement methods used in previous studies was conducted to identify which methods were most frequently used and whether the limitations were considered for each method.</p><p>An overview of studies that have used different skin type measurement methods is presented in Table <xref rid="srt70374-tbl-0001" ref-type="table">1</xref>. For example, the importance of accounting for varying lighting conditions in skin type measurements lies in its direct impact on skin color perception, texture representation, and the overall quality of captured images. Fitzpatrick labels can also give insight into the different skin types utilized to develop these methods. Table <xref rid="srt70374-tbl-0001" ref-type="table">1</xref> shows a comparative overview of skin type classification and measurement methods used in peer‐reviewed publications. Papers were selected as follows: A systematic search was performed on the PubMed, IEEE Xplore, and Google Scholar databases using the search terms “Fitzpatrick skin type”, “illumination variation”, and “skin type measurement”. The comparison included only peer‐reviewed journal papers and peer‐reviewed conference papers from those search results. The investigation revealed that various methods are used to measure skin type, ranging from physical devices like spectrophotometers to computational approaches, including AI‐based methods, ITA (individual typology angle), and others.</p><table-wrap position="float" id="srt70374-tbl-0001" content-type="TABLE" orientation="portrait"><label>TABLE 1</label><caption><p>A comparative overview of skin type classification methods includes light variation consideration and FST label inclusion. Among these methods, individual typology angle (ITA) has been the most widely used in previous studies.</p></caption><table frame="hsides" rules="groups"><col align="left" span="1"/><col align="center" span="1"/><col align="center" span="1"/><col align="center" span="1"/><col align="center" span="1"/><col align="center" span="1"/><thead><tr style="border-bottom:solid 1px #000000"><th align="left" rowspan="1" colspan="1">Reference</th><th align="center" rowspan="1" colspan="1">Year</th><th align="center" rowspan="1" colspan="1">Method</th><th align="center" rowspan="1" colspan="1">Light variation</th><th align="center" rowspan="1" colspan="1">Dermatologist‐assigned FST label</th><th align="center" rowspan="1" colspan="1">Image dataset with FST label</th></tr></thead><tbody><tr><td align="left" rowspan="1" colspan="1">Meinhardt et al. [<xref rid="srt70374-bib-0011" ref-type="bibr">11</xref>]</td><td align="center" rowspan="1" colspan="1">2008</td><td align="center" rowspan="1" colspan="1">Minimal Erythema Dose (MED)/ ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Girardeau et al. [<xref rid="srt70374-bib-0012" ref-type="bibr">12</xref>]</td><td align="center" rowspan="1" colspan="1">2009</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Reeder et al. [<xref rid="srt70374-bib-0013" ref-type="bibr">13</xref>]</td><td align="center" rowspan="1" colspan="1">2010</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Huixia et al. [<xref rid="srt70374-bib-0014" ref-type="bibr">14</xref>]</td><td align="center" rowspan="1" colspan="1">2012</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Arce‐Lopera [<xref rid="srt70374-bib-0015" ref-type="bibr">15</xref>]</td><td align="center" rowspan="1" colspan="1">2012</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Bino &amp; Bernerd [<xref rid="srt70374-bib-0016" ref-type="bibr">16</xref>]</td><td align="center" rowspan="1" colspan="1">2013</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Huang et al. [<xref rid="srt70374-bib-0017" ref-type="bibr">17</xref>]</td><td align="center" rowspan="1" colspan="1">2013</td><td align="center" rowspan="1" colspan="1">Haar transform &amp; Fuzzy</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Battie [<xref rid="srt70374-bib-0018" ref-type="bibr">18</xref>]</td><td align="center" rowspan="1" colspan="1">2014</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Reeder [<xref rid="srt70374-bib-0019" ref-type="bibr">19</xref>]</td><td align="center" rowspan="1" colspan="1">2014</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Treesirichod et al. [<xref rid="srt70374-bib-0020" ref-type="bibr">20</xref>]</td><td align="center" rowspan="1" colspan="1">2014</td><td align="center" rowspan="1" colspan="1">Spectrophotometer </td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Ryu et al. [<xref rid="srt70374-bib-0021" ref-type="bibr">21</xref>]</td><td align="center" rowspan="1" colspan="1">2015</td><td align="center" rowspan="1" colspan="1">Spectrophotometer / ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Wilkes et al. [<xref rid="srt70374-bib-0022" ref-type="bibr">22</xref>]</td><td align="center" rowspan="1" colspan="1">2015</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Youn [<xref rid="srt70374-bib-0023" ref-type="bibr">23</xref>]</td><td align="center" rowspan="1" colspan="1">2015</td><td align="center" rowspan="1" colspan="1">Sebumeter</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Ash et al. [<xref rid="srt70374-bib-0024" ref-type="bibr">24</xref>]</td><td align="center" rowspan="1" colspan="1">2015</td><td align="center" rowspan="1" colspan="1">Skin Tone Meter (STM)</td><td align="center" rowspan="1" colspan="1">Yes</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Cinotti et al. [<xref rid="srt70374-bib-0025" ref-type="bibr">25</xref>]</td><td align="center" rowspan="1" colspan="1">2016</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">McCreath et al. [<xref rid="srt70374-bib-0026" ref-type="bibr">26</xref>]</td><td align="center" rowspan="1" colspan="1">2016</td><td align="center" rowspan="1" colspan="1">Munsell color chart</td><td align="center" rowspan="1" colspan="1">Yes</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Piazena et al. [<xref rid="srt70374-bib-0027" ref-type="bibr">27</xref>]</td><td align="center" rowspan="1" colspan="1">2017</td><td align="center" rowspan="1" colspan="1">Spectrophotometer / ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Choi &amp; Suk [<xref rid="srt70374-bib-0028" ref-type="bibr">28</xref>]</td><td align="center" rowspan="1" colspan="1">2017</td><td align="center" rowspan="1" colspan="1">Spectrophotometer / ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Wang et al. [<xref rid="srt70374-bib-0029" ref-type="bibr">29</xref>]</td><td align="center" rowspan="1" colspan="1">2018</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Chang et al. [<xref rid="srt70374-bib-0030" ref-type="bibr">30</xref>]</td><td align="center" rowspan="1" colspan="1">2018</td><td align="center" rowspan="1" colspan="1">AI</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Kinyanjui et al. [<xref rid="srt70374-bib-0031" ref-type="bibr">31</xref>]</td><td align="center" rowspan="1" colspan="1">2019</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Wang et al. [<xref rid="srt70374-bib-0032" ref-type="bibr">32</xref>]</td><td align="center" rowspan="1" colspan="1">2019</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Campiche et al. [<xref rid="srt70374-bib-0033" ref-type="bibr">33</xref>]</td><td align="center" rowspan="1" colspan="1">2019</td><td align="center" rowspan="1" colspan="1">ITA &amp; IWA<sub>Newtone</sub>
</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Humber et al. [<xref rid="srt70374-bib-0034" ref-type="bibr">34</xref>]</td><td align="center" rowspan="1" colspan="1">2019</td><td align="center" rowspan="1" colspan="1">DWT &amp; LBP</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Kinyanjui et al. [<xref rid="srt70374-bib-0035" ref-type="bibr">35</xref>]</td><td align="center" rowspan="1" colspan="1">2020</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Indriyani &amp; Sudarma [<xref rid="srt70374-bib-0036" ref-type="bibr">36</xref>]</td><td align="center" rowspan="1" colspan="1">2020</td><td align="center" rowspan="1" colspan="1">SVM</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Ly et al. [<xref rid="srt70374-bib-0037" ref-type="bibr">37</xref>]</td><td align="center" rowspan="1" colspan="1">2020</td><td align="center" rowspan="1" colspan="1">Spectrophotometer / ITA</td><td align="center" rowspan="1" colspan="1">Yes</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Bahmani et al. [<xref rid="srt70374-bib-0038" ref-type="bibr">38</xref>]</td><td align="center" rowspan="1" colspan="1">2021</td><td align="center" rowspan="1" colspan="1">SREDS</td><td align="center" rowspan="1" colspan="1">Yes</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Krishnapriya et al. [<xref rid="srt70374-bib-0039" ref-type="bibr">39</xref>]</td><td align="center" rowspan="1" colspan="1">2021</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">Yes</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Kothari et al. [<xref rid="srt70374-bib-0040" ref-type="bibr">40</xref>]</td><td align="center" rowspan="1" colspan="1">2021</td><td align="center" rowspan="1" colspan="1">AI</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Flament et al. [<xref rid="srt70374-bib-0041" ref-type="bibr">41</xref>].</td><td align="center" rowspan="1" colspan="1">2021</td><td align="center" rowspan="1" colspan="1">AI</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Tadesse et al. [<xref rid="srt70374-bib-0042" ref-type="bibr">42</xref>]</td><td align="center" rowspan="1" colspan="1">2021</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">John et al. [<xref rid="srt70374-bib-0043" ref-type="bibr">43</xref>]</td><td align="center" rowspan="1" colspan="1">2021</td><td align="center" rowspan="1" colspan="1">FALMS</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Bevan &amp; Abarghouei [<xref rid="srt70374-bib-0044" ref-type="bibr">44</xref>]</td><td align="center" rowspan="1" colspan="1">2022</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Feng et al. [<xref rid="srt70374-bib-0045" ref-type="bibr">45</xref>]</td><td align="center" rowspan="1" colspan="1">2022</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">Yes</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Groh et al. [<xref rid="srt70374-bib-0046" ref-type="bibr">46</xref>]</td><td align="center" rowspan="1" colspan="1">2022</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">Yes</td><td align="center" rowspan="1" colspan="1">Fitzpatrick 17k</td></tr><tr><td align="left" rowspan="1" colspan="1">Li et al. [<xref rid="srt70374-bib-0047" ref-type="bibr">47</xref>]</td><td align="center" rowspan="1" colspan="1">2022</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">W et al. [<xref rid="srt70374-bib-0048" ref-type="bibr">48</xref>]</td><td align="center" rowspan="1" colspan="1">2022</td><td align="center" rowspan="1" colspan="1">AI</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Jung et al. [<xref rid="srt70374-bib-0049" ref-type="bibr">49</xref>]</td><td align="center" rowspan="1" colspan="1">2023</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Kalb et al. [<xref rid="srt70374-bib-0050" ref-type="bibr">50</xref>]</td><td align="center" rowspan="1" colspan="1">2023</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">Yes</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Barrett et al. [<xref rid="srt70374-bib-0051" ref-type="bibr">51</xref>]</td><td align="center" rowspan="1" colspan="1">2023</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Corbin &amp; Marques [<xref rid="srt70374-bib-0052" ref-type="bibr">52</xref>]</td><td align="center" rowspan="1" colspan="1">2023</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Mohamed et al. [<xref rid="srt70374-bib-0053" ref-type="bibr">53</xref>]</td><td align="center" rowspan="1" colspan="1">2023</td><td align="center" rowspan="1" colspan="1">ITA</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Thong et al. [<xref rid="srt70374-bib-0054" ref-type="bibr">54</xref>]</td><td align="center" rowspan="1" colspan="1">2023</td><td align="center" rowspan="1" colspan="1">ITA &amp; Hue angle</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Tadesse et al. [<xref rid="srt70374-bib-0055" ref-type="bibr">55</xref>]</td><td align="center" rowspan="1" colspan="1">2023</td><td align="center" rowspan="1" colspan="1">AI</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">Yes</td><td align="center" rowspan="1" colspan="1">Fitzpatrick 17k</td></tr><tr><td align="left" rowspan="1" colspan="1">Leizaola et al. [<xref rid="srt70374-bib-0056" ref-type="bibr">56</xref>].</td><td align="center" rowspan="1" colspan="1">2023</td><td align="center" rowspan="1" colspan="1">AI</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Kara et al. [<xref rid="srt70374-bib-0057" ref-type="bibr">57</xref>]</td><td align="center" rowspan="1" colspan="1">2023</td><td align="center" rowspan="1" colspan="1">AI</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Oliveira et al. [<xref rid="srt70374-bib-0058" ref-type="bibr">58</xref>]</td><td align="center" rowspan="1" colspan="1">2023</td><td align="center" rowspan="1" colspan="1">Human annotator</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Schumann et al. [<xref rid="srt70374-bib-0059" ref-type="bibr">59</xref>]</td><td align="center" rowspan="1" colspan="1">2024</td><td align="center" rowspan="1" colspan="1">Human annotator</td><td align="center" rowspan="1" colspan="1">Yes</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Srimaharaj &amp; Chaising [<xref rid="srt70374-bib-0060" ref-type="bibr">60</xref>]</td><td align="center" rowspan="1" colspan="1">2024</td><td align="center" rowspan="1" colspan="1">Distance‐based</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Mbatha et al. [<xref rid="srt70374-bib-0061" ref-type="bibr">61</xref>].</td><td align="center" rowspan="1" colspan="1">2024</td><td align="center" rowspan="1" colspan="1">AI</td><td align="center" rowspan="1" colspan="1">Yes</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Draelos et al. [<xref rid="srt70374-bib-0062" ref-type="bibr">62</xref>].</td><td align="center" rowspan="1" colspan="1">2025</td><td align="center" rowspan="1" colspan="1">AI</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Dissanayake &amp; Manukalpa [<xref rid="srt70374-bib-0063" ref-type="bibr">63</xref>]</td><td align="center" rowspan="1" colspan="1">2025</td><td align="center" rowspan="1" colspan="1">AI</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr><tr><td align="left" rowspan="1" colspan="1">Paxton et al. [<xref rid="srt70374-bib-0064" ref-type="bibr">64</xref>].</td><td align="center" rowspan="1" colspan="1">2026</td><td align="center" rowspan="1" colspan="1">AI</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">No</td><td align="center" rowspan="1" colspan="1">−</td></tr></tbody></table><permissions><copyright-holder>John Wiley &amp; Sons, Ltd.</copyright-holder></permissions></table-wrap><p>As Table <xref rid="srt70374-tbl-0001" ref-type="table">1</xref> shows, ITA is the dominant skin type measurement method in existing literature. This method measures skin pigmentation in the L<sup>*</sup>a<sup>*</sup>b<sup>*</sup> color space, while the discrete and subjective Fitzpatrick categories are based on the pigmentation and response to UV exposure. Although ITA provides a continuous image‐derived representation of skin color, it can also be mapped onto discrete categories, like Fitzpatrick classification system. Some previous research has treated ITA classifications as synonymous with those of Fitzpatrick [<xref rid="srt70374-bib-0065" ref-type="bibr">65</xref>, <xref rid="srt70374-bib-0066" ref-type="bibr">66</xref>]. ITA is not a classification method itself, but it is a feature used in skin type assessment, representing the angle between the color and luminance vectors of a person's skin color in the L<sup>*</sup>a<sup>*</sup>b<sup>*</sup> color space, to estimate image‐derived skin color characteristics based on the calculated angle.</p><p>However, other existing skin type measurement methods, as outlined in Table <xref rid="srt70374-tbl-0001" ref-type="table">1</xref>, are physically based techniques, which require in‐person assessment and are therefore not suitable for evaluation through digital images. For example, skin reflectance estimation based on dichromatic separation (SREDS) was proposed to measure skin color from a single image by decomposing the light reflected from the skin into two components [<xref rid="srt70374-bib-0038" ref-type="bibr">38</xref>]. Three datasets, the CMU Multi‐PIE face database, MEDS‐II, and Morph‐II—were used to evaluate the superior performance of the new model compared to ITA and Relative Skin Reflectance (RSR). Although this method outperforms other methods in uncontrolled lighting conditions, it still has difficulties with variations in lighting conditions. In [<xref rid="srt70374-bib-0043" ref-type="bibr">43</xref>], face area lightness measures (FALMs) are calculated to estimate skin color from images using color analysis or FSTs. The estimated FALMs from the images are then compared to ground truth skin measurements from a calibrated dermatological device specifically designed to measure skin lightness, showing a large difference between these two measures resulting from camera, background, and environmental conditions.</p><p>In the case of deep learning‐based methods, which typically require large, diverse datasets and often do not use reliable or consistent Fitzpatrick labels. In many prior works, dermatologist‐assigned FST labels were either unavailable or generated using non‐expert annotators, which undermines the reliability of comparisons. Chang et al. [<xref rid="srt70374-bib-0030" ref-type="bibr">30</xref>] introduce a convolutional neural network model to classify their created skin spectra dataset into the six FSTs, assessing sun exposure reactions. Their performance evaluation includes a comparison with an artificial neural network model. Mbatha et al. [<xref rid="srt70374-bib-0061" ref-type="bibr">61</xref>]. developed a neural network model trained on human‐annotated data under 15 different lighting conditions to predict MST values with improved robustness. Their work demonstrates how modern machine learning techniques can produce consistent estimates across variable environments. However, such approaches typically require large, well‐labeled datasets and careful control of image acquisition, which may not always be available in real‐world or legacy image collections. The MST labels used for training and evaluation were manually assigned by the participants themselves. The classification of facial features extracted from images into different skin types of normal, oily, dry, and combination is accomplished using a support vector machine with the use of discrete wavelet transform, contrast, and local binary pattern [<xref rid="srt70374-bib-0034" ref-type="bibr">34</xref>]. A multi‐task cascaded convolutional neural network is used to classify skin images into skin types, oily or dry [<xref rid="srt70374-bib-0040" ref-type="bibr">40</xref>]. In another study, a biological approach is adopted, focusing on the detection of skin type through the assessment of Sebum levels [<xref rid="srt70374-bib-0023" ref-type="bibr">23</xref>].</p><p>Corbin and Marques [<xref rid="srt70374-bib-0052" ref-type="bibr">52</xref>] used ITA with four different approaches to estimate FST in three skin lesion image datasets: ISIC 2018, ISIC 2017, and ISIC 2016 [<xref rid="srt70374-bib-0067" ref-type="bibr">67</xref>], none of which provide information on skin types. Their study compares different methods for ITA‐based estimation and skin type classification, highlighting the impact of skin lesion size on their results. They proposed new methods based on AI models and ITA to address the lack of skin type information in skin image datasets lacking this metadata. Their research aims to address the underrepresentation of darker skin types in public skin lesion image datasets to produce fair models.</p><p>Kinyanjui et al. [<xref rid="srt70374-bib-0031" ref-type="bibr">31</xref>] used ITA to assign FST categories in other dermatology datasets that do not include Fitzpatrick skin type information: SD‐198 [<xref rid="srt70374-bib-0068" ref-type="bibr">68</xref>] and ISIC‐2018 [<xref rid="srt70374-bib-0067" ref-type="bibr">67</xref>]. They highlighted the limitation of the underrepresentation of darker skin populations in publicly available skin disease datasets. The skin type classification results showed that the majority of images belonged to lighter skin types. Campiche et al. [<xref rid="srt70374-bib-0033" ref-type="bibr">33</xref>]. used ITA and IWA<sub>Newtone</sub> [<xref rid="srt70374-bib-0069" ref-type="bibr">69</xref>] to show the significant difference in skin type between these two groups of lighter‐ and darker‐skinned women. These two methods were compared in terms of skin color and signs of aging using the ColorFace imaging system. IWA<sub>Newtone</sub> was developed by Newtone Technologies and incorporates components of luminance and chrominance in its assessment. There was a lack of some skin types, including lighter skin types and darker skin types.</p><p>As it was highlighted in the study by Alipour et al. [<xref rid="srt70374-bib-0070" ref-type="bibr">70</xref>]., the availability of large and diverse datasets is a major challenge in skin type research. There are two publicly available FST‐labeled datasets (e.g., PAD‐UFES‐20 and Fitzpatrick17k) that exhibit significant class imbalance and potential bias; using them to train deep learning models may reproduce and reinforce these biases. As a result, applying such models to these datasets may unintentionally propagate biased labeling and worsen the fairness issues the field aims to address. However, dermatologist‐assigned FST labels derived from the PAD‐UFES‐20 dataset were used in our study, providing a more consistent basis for evaluation.</p><p>According to the explanations above regarding skin type measurement methods, most existing literature either overlooks the influence of varying lighting conditions on their results or fails to assess their methodologies across all six skin types. Therefore, it is necessary to assess the performance of skin type measurement methods in these challenging scenarios to understand how they respond to such conditions and identify their weaknesses. Among these methods, ITA has emerged as a widely used image‐derived color/lightness metric commonly mapped to Fitzpatrick skin type categories, particularly in studies involving image datasets without expert‐assigned skin type labels. However, its reliability under uncontrolled lighting conditions and imbalanced data remains insufficiently understood. Our study does not introduce a new measurement method but rather investigates ITA's limitations in accurately measuring skin type diversity and offers new insights into its practical performance. Unlike previous studies that addressed general biases and proposed broad solutions in skin type measurement methods, our work delves into the limitations of this method itself on an image dataset with Fitzpatrick labels. It is investigated whether ITA can reliably characterize dataset‐level skin color variation under uncontrolled imaging conditions. Due to the limited availability of datasets with expert‐assigned Fitzpatrick skin type labels, our study focused on PAD‐UFES‐20, which also offers clear separation between lesions and surrounding healthy skin, facilitating reliable skin patch extraction. This level of detailed analysis has not been a focus of previous research.</p><p>The major contributions in this work include:
<list list-type="order" id="srt70374-list-0001"><list-item><p>A systematic review of skin type measurement methods, highlighting the widespread use of ITA as a proxy for image‐derived skin color in prior research.</p></list-item><list-item><p>Construction of a skin patch image dataset with dermatologist‐assigned Fitzpatrick skin type (FST) labels, enabling evaluation under real‐world imaging conditions.</p></list-item><list-item><p>Analysis of color and lightness characteristics across all six FST categories, providing insight into skin tone variation in image datasets.</p></list-item><list-item><p>A critical evaluation of ITA under lighting variability and dataset imbalance, to examine its practical behavior in real‐world scenarios.</p></list-item><list-item><p>Empirical comparison between ITA‐derived predictions and dermatologist‐assigned FST labels to assess their level of agreement.</p></list-item><list-item><p>Critical analysis of ITA's limitations for dataset‐level skin color characterization.</p></list-item></list>
</p></sec><sec id="srt70374-sec-0060"><label>2</label><title>Method</title><p>The performance of ITA for the skin patch image dataset is evaluated using the method shown in Figure <xref rid="srt70374-fig-0002" ref-type="fig">2</xref>. This evaluation includes analysis of the distribution of ITA values across the dataset and within all six FST categories, as well as a comparison between ITA‐based predictions and dermatologist‐assigned FST labels. Although ITA is not inherently a skin type classifier, it is analyzed in a classification‐like setting to examine its behavior when mapped to Fitzpatrick categories. The dataset's color and lightness distributions were analyzed to gain insights into the variations of color and lightness across different skin types in the images. The approach involves several key steps, including dataset preparation, color space conversion, and ITA‐based FST classifications.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0002" orientation="portrait"><label>FIGURE 2</label><caption><p>Flowchart of skin type measurement assessment. A dataset of 920 images is created, sourced from PAD‐UFES‐20, and labeled with FST. Skin patches are segmented and converted to L<sup>*</sup>a<sup>*</sup>b<sup>*</sup> color space, and mean color values are extracted. ITA is calculated, mapped to thresholds, and classified into FST categories (I‐VI). Performance is evaluated using a confusion matrix based on FST ground truth labels.</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-3" orientation="portrait" xlink:href="SRT-32-e70374-g008.jpg"><?image-name SRT-32-e70374-g008.jpg?><?image-size 76689?><?image-md5 0ba99dc7d70d101690b18d4805dea246?><?image-image-server-status NEVER_LOAD?><?image-original-height 676?><?image-original-width 600?><?image-scaled-height 676?><?image-scaled-width 600?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/0ba99dc7d70d/SRT-32-e70374-g008.jpg?><?thumb-name SRT-32-e70374-g008.gif?><?thumb-size 6855?><?thumb-md5 714f85815c1cf9d40519e3b8a866c922?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 113?><?thumb-scaled-width 100?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/714f85815c1c/SRT-32-e70374-g008.gif?></graphic></fig><sec id="srt70374-sec-0070"><label>2.1</label><title>Image Dataset Creation</title><p>The first step of the evaluation process is the creation of a dataset of healthy skin patch images, labeled with FST. To achieve this, existing skin lesion image datasets were reviewed to identify suitable candidates based on the following criteria: availability of FST labels, representation of all FST categories, and clear differentiation between skin and background. Two publicly available datasets, PAD‐UFES‐20 [<xref rid="srt70374-bib-0071" ref-type="bibr">71</xref>] and Fitzpatrick17k [<xref rid="srt70374-bib-0072" ref-type="bibr">72</xref>], were identified as potential sources and are shown in Figure <xref rid="srt70374-fig-0003" ref-type="fig">3(a)</xref>) and Figure <xref rid="srt70374-fig-0003" ref-type="fig">3(b)</xref>), respectively. PAD‐UFES‐20 was ultimately selected due to its distinct advantage over Fitzpatrick17k, as shown in Figure <xref rid="srt70374-fig-0003" ref-type="fig">3</xref>. Most images in PAD‐UFES‐20 display a clear separation between skin lesions and the background, facilitating reliable segmentation and extraction of healthy skin patches for the experiments. This dataset was used to manually generate skin patch images of different sizes for each FST category.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0003" orientation="portrait"><label>FIGURE 3</label><caption><p>Some samples of images from (a) Fitzpatrick17k [<xref rid="srt70374-bib-0072" ref-type="bibr">72</xref>] and (b) PAD‐UFES‐20 [<xref rid="srt70374-bib-0071" ref-type="bibr">71</xref>].</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-5" orientation="portrait" xlink:href="SRT-32-e70374-g006.jpg"><?image-name SRT-32-e70374-g006.jpg?><?image-size 46330?><?image-md5 f3c683f2df1e872e773b1cc0d8aa1da7?><?image-image-server-status LOAD_COMPLETED?><?image-original-height 293?><?image-original-width 840?><?image-scaled-height 195?><?image-scaled-width 560?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/f3c683f2df1e/SRT-32-e70374-g006.jpg?><?thumb-name SRT-32-e70374-g006.gif?><?thumb-size 13056?><?thumb-md5 4634e6c12ccba4602c45dccb16b15ad1?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 70?><?thumb-scaled-width 200?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/4634e6c12ccb/SRT-32-e70374-g006.gif?></graphic></fig><p>It should be noted that both datasets are imbalanced in favor of lighter skin types and have images of different sizes. In the process of generating skin patch datasets from PAD‐UFES‐20, a systematic approach was followed, as shown in Figure <xref rid="srt70374-fig-0004" ref-type="fig">4</xref>.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0004" orientation="portrait"><label>FIGURE 4</label><caption><p>The process to create the skin patch image dataset for evaluating ITA as an image‐derived color/lightness measurement approach. Starting with 2298 images from the PAD‐UFES‐20 dataset, this process involves filtering images based on FST labels and visual quality, followed by manual extraction of skin patches.</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-7" orientation="portrait" xlink:href="SRT-32-e70374-g016.jpg"><?image-name SRT-32-e70374-g016.jpg?><?image-size 42789?><?image-md5 381fb339bb2a33e06d8cb8eb8ebb2bff?><?image-image-server-status NEVER_LOAD?><?image-original-height 344?><?image-original-width 400?><?image-scaled-height 344?><?image-scaled-width 400?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/381fb339bb2a/SRT-32-e70374-g016.jpg?><?thumb-name SRT-32-e70374-g016.gif?><?thumb-size 6453?><?thumb-md5 ea9f295870271f2a6685370dd3ec088a?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 86?><?thumb-scaled-width 100?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/ea9f29587027/SRT-32-e70374-g016.gif?></graphic></fig><p>The PAD‐UFES‐20 dataset contains 2298 images of skin lesions of varying sizes, originally collected for the diagnosis of six different skin conditions. However, this study focuses only on the healthy skin surrounding the lesions to create a dataset of skin patches labeled with FST. Images containing significant amounts of hair, ink, or wrinkles that obscured the skin region of interest were excluded from consideration. However, images with minimal hair that did not interfere with skin visibility were retained to avoid unnecessary exclusion and potential bias. From each image, multiple skin patches were extracted based on avoiding regions with hair, ink, wrinkles, or other obstructions; ensuring representation of diverse lighting conditions when present; selecting areas with uniform texture to exclude scars or lesions; and maintaining consistent resolution across the dataset. These criteria ensured that the extracted patches represented healthy skin regions suitable for ITA‐based skin type classifier evaluation, as illustrated in Figure <xref rid="srt70374-fig-0003" ref-type="fig">3</xref>. Consequently, the resulting skin patch image dataset encompasses samples of varying sizes. This process aimed at creating six different skin patch image datasets, each corresponding to a specific FST. In the end, 920 images remained for the experiments. The distribution of each skin type for the created skin patch image dataset and the PAD‐UFES‐20 are shown in Table <xref rid="srt70374-tbl-0002" ref-type="table">2</xref>.</p><table-wrap position="float" id="srt70374-tbl-0002" content-type="TABLE" orientation="portrait"><label>TABLE 2</label><caption><p>Number of images in each skin type group (FST) within the PAD‐UFES‐20 and the created skin patch image dataset.</p></caption><table frame="hsides" rules="groups"><col align="left" span="1"/><col align="center" span="1"/><col align="center" span="1"/><col align="center" span="1"/><col align="center" span="1"/><col align="center" span="1"/><col align="center" span="1"/><col align="center" span="1"/><thead><tr style="border-bottom:solid 1px #000000"><th align="left" rowspan="1" colspan="1">Dataset</th><th align="center" rowspan="1" colspan="1">Total number</th><th align="center" rowspan="1" colspan="1">Skin type I</th><th align="center" rowspan="1" colspan="1">Skin type II</th><th align="center" rowspan="1" colspan="1">Skin type III</th><th align="center" rowspan="1" colspan="1">Skin type IV</th><th align="center" rowspan="1" colspan="1">Skin type V</th><th align="center" rowspan="1" colspan="1">Skin type VI</th></tr></thead><tbody><tr><td align="left" rowspan="1" colspan="1">PAD‐UFES‐20</td><td align="center" rowspan="1" colspan="1">2298</td><td align="center" rowspan="1" colspan="1">153</td><td align="center" rowspan="1" colspan="1">876</td><td align="center" rowspan="1" colspan="1">392</td><td align="center" rowspan="1" colspan="1">62</td><td align="center" rowspan="1" colspan="1">10</td><td align="center" rowspan="1" colspan="1">1</td></tr><tr><td align="left" rowspan="1" colspan="1">Skin patch dataset</td><td align="center" rowspan="1" colspan="1">920</td><td align="center" rowspan="1" colspan="1">110</td><td align="center" rowspan="1" colspan="1">472</td><td align="center" rowspan="1" colspan="1">277</td><td align="center" rowspan="1" colspan="1">46</td><td align="center" rowspan="1" colspan="1">12</td><td align="center" rowspan="1" colspan="1">3</td></tr></tbody></table><permissions><copyright-holder>John Wiley &amp; Sons, Ltd.</copyright-holder></permissions></table-wrap><p>Figure <xref rid="srt70374-fig-0005" ref-type="fig">5(a)</xref>) presents sample original images from the PAD‐UFES‐20 dataset, while Figure <xref rid="srt70374-fig-0005" ref-type="fig">5(b)</xref>) displays the corresponding skin patch images extracted from these samples, representing different skin types in the skin patch image dataset. The images in the PAD‐UFES‐20 present a wide range of lighting conditions, including shadowed areas, uneven lighting, and local overexposure.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0005" orientation="portrait"><label>FIGURE 5</label><caption><p>(a) Six samples of skin lesion images from Pad‐UFES‐20, (b) their corresponding skin patch images. (left to right) Skin types (FST) I‐VI, respectively.</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-9" orientation="portrait" xlink:href="SRT-32-e70374-g014.jpg"><?image-name SRT-32-e70374-g014.jpg?><?image-size 44935?><?image-md5 afcacf0bb79d9230eb37e34742ecf629?><?image-image-server-status LOAD_COMPLETED?><?image-original-height 305?><?image-original-width 840?><?image-scaled-height 203?><?image-scaled-width 560?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/afcacf0bb79d/SRT-32-e70374-g014.jpg?><?thumb-name SRT-32-e70374-g014.gif?><?thumb-size 14843?><?thumb-md5 fced5ac5dac154e25c2ab3987a6bc514?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 73?><?thumb-scaled-width 200?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/fced5ac5dac1/SRT-32-e70374-g014.gif?></graphic></fig></sec><sec id="srt70374-sec-0080"><label>2.2</label><title>Skin Color Extraction</title><p>
<italic toggle="yes">Convert to L<sup>*</sup>a<sup>*</sup>b<sup>*</sup> color space</italic>: The skin patch images were converted from RGB into the L<sup>*</sup>a<sup>*</sup>b<sup>*</sup> color space, a color space defined by the International Commission on Illumination (CIE) in 1976 [<xref rid="srt70374-bib-0073" ref-type="bibr">73</xref>]. Luminance (L<sup>*</sup>) represents the lightness of the color, while chrominance components (a<sup>*</sup> and b<sup>*</sup>) capture the color variations along the green‐red (a<sup>*</sup>) and blue‐yellow (b<sup>*</sup>) axes, independent of lightness [<xref rid="srt70374-bib-0073" ref-type="bibr">73</xref>]. This color space is designed to be more consistent with human vision and enhances the precision of measurements by reducing the impact of lighting conditions, a common issue in the RGB color space. The color space conversion is performed on each pixel in each skin patch image. The first step involves converting the RGB values (from 0 to 255) to XYZ using a linear transformation [<xref rid="srt70374-bib-0073" ref-type="bibr">73</xref>, <xref rid="srt70374-bib-0074" ref-type="bibr">74</xref>] as follows:
<disp-formula id="srt70374-disp-0001">
<label>(1)</label>
<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" id="jats-math-1" display="block"><mml:mrow><mml:mrow><mml:mfenced separators="" open="(" close=")"><mml:mtable><mml:mtr><mml:mtd><mml:mi>X</mml:mi></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mi>Y</mml:mi></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mi>Z</mml:mi></mml:mtd></mml:mtr></mml:mtable></mml:mfenced><mml:mo linebreak="badbreak">=</mml:mo><mml:mfenced separators="" open="(" close=")"><mml:mtable><mml:mtr><mml:mtd><mml:mrow><mml:mn>0.4124</mml:mn></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mn>0.3576</mml:mn></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mn>0.1805</mml:mn></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mn>0.2126</mml:mn></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mn>0.7152</mml:mn></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mn>0.0722</mml:mn></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mn>0.0193</mml:mn></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mn>0.1192</mml:mn></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mn>0.9505</mml:mn></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced><mml:mfenced separators="" open="(" close=")"><mml:mtable><mml:mtr><mml:mtd><mml:mi>R</mml:mi></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mi>G</mml:mi></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mi>B</mml:mi></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:mrow></mml:math>
</disp-formula>
</p><p>The L<sup>*</sup>a<sup>*</sup>b<sup>*</sup> color space components are calculated from the XYZ using the following equations:
<disp-formula id="srt70374-disp-0002">
<label>(2)</label>
<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" id="jats-math-2" display="block"><mml:mrow><mml:mrow><mml:msup><mml:mi>L</mml:mi><mml:mo>∗</mml:mo></mml:msup><mml:mo linebreak="badbreak">=</mml:mo><mml:mfenced separators="" open="{" close="}"><mml:mtable><mml:mtr><mml:mtd><mml:mrow><mml:mn>116</mml:mn><mml:mo>.</mml:mo><mml:msup><mml:mfenced separators="" open="(" close=")"><mml:mfrac><mml:mi>Y</mml:mi><mml:msub><mml:mi>Y</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mfrac></mml:mfenced><mml:mfrac><mml:mn>1</mml:mn><mml:mn>3</mml:mn></mml:mfrac></mml:msup><mml:mo linebreak="goodbreak">−</mml:mo><mml:mn>16</mml:mn><mml:mo>,</mml:mo><mml:mi>i</mml:mi><mml:mi>f</mml:mi><mml:mspace width="0.28em"/><mml:mfrac><mml:mi>Y</mml:mi><mml:msub><mml:mi>Y</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mfrac><mml:mo>&gt;</mml:mo><mml:mn>0.008856</mml:mn></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mn>903.3</mml:mn><mml:mfenced separators="" open="(" close=")"><mml:mfrac><mml:mi>Y</mml:mi><mml:msub><mml:mi>Y</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mfrac></mml:mfenced><mml:mo>,</mml:mo><mml:mi>i</mml:mi><mml:mi>f</mml:mi><mml:mspace width="0.28em"/><mml:mfrac><mml:mi>Y</mml:mi><mml:msub><mml:mi>Y</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mfrac><mml:mo>≤</mml:mo><mml:mn>0.008856</mml:mn></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:mrow></mml:math>
</disp-formula>
<disp-formula id="srt70374-disp-0003">
<label>(3)</label>
<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" id="jats-math-3" display="block"><mml:mrow><mml:mrow><mml:msup><mml:mi>a</mml:mi><mml:mo>∗</mml:mo></mml:msup><mml:mo linebreak="badbreak">=</mml:mo><mml:mn>500</mml:mn><mml:mfenced separators="" open="[" close="]"><mml:mrow><mml:msup><mml:mfenced separators="" open="(" close=")"><mml:mfrac><mml:mi>X</mml:mi><mml:msub><mml:mi>X</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mfrac></mml:mfenced><mml:mfrac><mml:mn>1</mml:mn><mml:mn>3</mml:mn></mml:mfrac></mml:msup><mml:mo>−</mml:mo><mml:msup><mml:mfenced separators="" open="(" close=")"><mml:mfrac><mml:mi>Y</mml:mi><mml:msub><mml:mi>Y</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mfrac></mml:mfenced><mml:mfrac><mml:mn>1</mml:mn><mml:mn>3</mml:mn></mml:mfrac></mml:msup></mml:mrow></mml:mfenced></mml:mrow></mml:mrow></mml:math>
</disp-formula>
<disp-formula id="srt70374-disp-0004">
<label>(4)</label>
<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" id="jats-math-4" display="block"><mml:mrow><mml:mrow><mml:msup><mml:mi>b</mml:mi><mml:mo>∗</mml:mo></mml:msup><mml:mo linebreak="badbreak">=</mml:mo><mml:mn>200</mml:mn><mml:mfenced separators="" open="[" close="]"><mml:mrow><mml:msup><mml:mfenced separators="" open="(" close=")"><mml:mfrac><mml:mi>Y</mml:mi><mml:msub><mml:mi>Y</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mfrac></mml:mfenced><mml:mfrac><mml:mn>1</mml:mn><mml:mn>3</mml:mn></mml:mfrac></mml:msup><mml:mo>−</mml:mo><mml:msup><mml:mfenced separators="" open="(" close=")"><mml:mfrac><mml:mi>Z</mml:mi><mml:msub><mml:mi>Z</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mfrac></mml:mfenced><mml:mfrac><mml:mn>1</mml:mn><mml:mn>3</mml:mn></mml:mfrac></mml:msup></mml:mrow></mml:mfenced></mml:mrow></mml:mrow></mml:math>
</disp-formula> Where <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" id="jats-math-5" display="inline"><mml:mrow><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>Y</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>Z</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mspace width="0.28em"/></mml:mrow></mml:mrow></mml:math> represent the tristimulus values associated with the illuminant, which the human eye perceives as “white” [<xref rid="srt70374-bib-0075" ref-type="bibr">75</xref>]. The maximum value of L<sup>*</sup> is 100 (white) and the minimum is 0 (black). The b<sup>*</sup> axis indicates yellow to blue, and a<sup>*</sup> axis shows red to green, with values ranging from ‐128 to +127 for each.</p><p>
<italic toggle="yes">Image mean L<sup>*</sup>a<sup>*</sup>b<sup>*</sup> value</italic>: The L<sup>*</sup>a<sup>*</sup>b<sup>*</sup> mean value represents the average values of the L<sup>*</sup>, a<sup>*</sup>, and b<sup>*</sup> channels across all pixels in each image within the skin patch dataset. This provides a consistent color representation for each image by averaging out local variations or anomalies, such as noise, lighting inconsistencies, or minor irregularities in the image. Although the mean values are visualized as solid‐color images, they are fundamentally single‐color values calculated for each image. Figure <xref rid="srt70374-fig-0006" ref-type="fig">6(a)</xref>) shows examples of images from the skin patch dataset alongside their corresponding extracted skin color for six FSTs in Figure <xref rid="srt70374-fig-0006" ref-type="fig">6(b)</xref>).</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0006" orientation="portrait"><label>FIGURE 6</label><caption><p>From left to right: (a) images from skin types (FST) I to VI, respectively. (b) Each image shows the corresponding estimated skin tone.</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-11" orientation="portrait" xlink:href="SRT-32-e70374-g009.jpg"><?image-name SRT-32-e70374-g009.jpg?><?image-size 19744?><?image-md5 5a0165e51fafca8ba47c4ae13a18ff3e?><?image-image-server-status LOAD_COMPLETED?><?image-original-height 189?><?image-original-width 840?><?image-scaled-height 126?><?image-scaled-width 560?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/5a0165e51faf/SRT-32-e70374-g009.jpg?><?thumb-name SRT-32-e70374-g009.gif?><?thumb-size 7333?><?thumb-md5 1e9430a23a36112388d2cf2cbbe5d2c8?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 45?><?thumb-scaled-width 200?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/1e9430a23a36/SRT-32-e70374-g009.gif?></graphic></fig><p>
<italic toggle="yes">ITA calculation</italic>: The ITA method provides a numerical representation of skin color using the key colorimetric parameters L<sup>*</sup> and b<sup>*</sup> in the L<sup>*</sup>a<sup>*</sup>b<sup>*</sup> color space. This method has emerged as a widely used image‐derived color metric commonly mapped to Fitzpatrick categories [<xref rid="srt70374-bib-0010" ref-type="bibr">10</xref>]. To quantify skin color, ITA measure is calculated from the mean Lab images as shown in equation (<xref rid="srt70374-disp-0005" ref-type="disp-formula">5</xref>):
<disp-formula id="srt70374-disp-0005">
<label>(5)</label>
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</p><p>This method was originally proposed by Chardon et al. [<xref rid="srt70374-bib-0076" ref-type="bibr">76</xref>] to categorize different skin types based on ITA values. Higher ITA values indicate lighter skin types. The FST classification is determined by comparing the ITA values with predefined thresholds corresponding to specific skin type categories, as shown in Figure <xref rid="srt70374-fig-0007" ref-type="fig">7</xref>.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0007" orientation="portrait"><label>FIGURE 7</label><caption><p>Partitioning of the ITA spectrum into six discrete categories (FST I‐VI) based on predefined thresholds [<xref rid="srt70374-bib-0076" ref-type="bibr">76</xref>], which reflect variations in lightness (L<sup>*</sup>) and chrominance (b<sup>*</sup>).</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-13" orientation="portrait" xlink:href="SRT-32-e70374-g011.jpg"><?image-name SRT-32-e70374-g011.jpg?><?image-size 26570?><?image-md5 d18eb6c64a7c1c8ef631ba10becc6fde?><?image-image-server-status NEVER_LOAD?><?image-original-height 335?><?image-original-width 400?><?image-scaled-height 335?><?image-scaled-width 400?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/d18eb6c64a7c/SRT-32-e70374-g011.jpg?><?thumb-name SRT-32-e70374-g011.gif?><?thumb-size 5297?><?thumb-md5 0490f0432c7786079e97a516232e8145?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 84?><?thumb-scaled-width 100?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/0490f0432c77/SRT-32-e70374-g011.gif?></graphic></fig></sec><sec id="srt70374-sec-0090"><label>2.3</label><title>Skin Type Classification</title><p>
<italic toggle="yes">Mapping to thresholds</italic>: ITA values were calculated from the previous step and were mapped to the predefined thresholds [<xref rid="srt70374-bib-0076" ref-type="bibr">76</xref>] to classify images into one of six FSTs according to Table <xref rid="srt70374-tbl-0003" ref-type="table">3</xref>. The thresholds were established using measurements from individuals with lighter skin types.</p><table-wrap position="float" id="srt70374-tbl-0003" content-type="TABLE" orientation="portrait"><label>TABLE 3</label><caption><p>Skin type (FST) classification based on ITA threshold values [<xref rid="srt70374-bib-0076" ref-type="bibr">76</xref>].</p></caption><table frame="hsides" rules="groups"><col align="left" span="1"/><col align="center" span="1"/><thead><tr style="border-bottom:solid 1px #000000"><th align="left" rowspan="1" colspan="1">ITA range [°]</th><th align="center" rowspan="1" colspan="1">Predicted skin type</th></tr></thead><tbody><tr><td align="left" rowspan="1" colspan="1">ITA&gt;55°</td><td align="center" rowspan="1" colspan="1">Skin type I</td></tr><tr><td align="left" rowspan="1" colspan="1">41°&lt; ITA ≤55°</td><td align="center" rowspan="1" colspan="1">Skin type II</td></tr><tr><td align="left" rowspan="1" colspan="1">28°&lt; ITA ≤41°</td><td align="center" rowspan="1" colspan="1">Skin type III</td></tr><tr><td align="left" rowspan="1" colspan="1">10°&lt; ITA ≤28°</td><td align="center" rowspan="1" colspan="1">Skin type IV</td></tr><tr><td align="left" rowspan="1" colspan="1">−30°&lt; ITA ≤10°</td><td align="center" rowspan="1" colspan="1">Skin type V</td></tr><tr><td align="left" rowspan="1" colspan="1">ITA←30°</td><td align="center" rowspan="1" colspan="1">Skin type VI</td></tr></tbody></table><permissions><copyright-holder>John Wiley &amp; Sons, Ltd.</copyright-holder></permissions></table-wrap></sec></sec><sec id="srt70374-sec-0100"><label>3</label><title>Results</title><p>The experiments were conducted using Python 3.11.0 and various libraries such as OpenCV and Matplotlib. The skin patch image dataset was outlined in PNG format with image dimensions ranging from 59×67 to 2929×593. In section <xref rid="srt70374-sec-0110" ref-type="sec">3.1</xref>, the analysis of images in terms of color and lightness is assessed. In Section <xref rid="srt70374-sec-0120" ref-type="sec">3.2</xref>, the overall distribution of ITA values is analyzed to highlight skin color imbalances in the dataset. Section <xref rid="srt70374-sec-0130" ref-type="sec">3.3</xref> examines ITA distributions within each Fitzpatrick skin type (FST) category. Section <xref rid="srt70374-sec-0140" ref-type="sec">3.4</xref> explores the influence of ITA parameters (L<sup>*</sup>, b<sup>*</sup>) on their values. Section <xref rid="srt70374-sec-0150" ref-type="sec">3.5</xref> compares ITA predictions with expert‐assigned FST labels using a confusion matrix. Finally, Section <xref rid="srt70374-sec-0160" ref-type="sec">3.6</xref> presents examples of misclassified images and analyzes how lighting variation impacts ITA‐based classification accuracy. The code and dataset can be found here: <ext-link xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="https://github.com/NedaAlip/Assessment-of-skin-type-measurement-method/tree/main" ext-link-type="uri">https://github.com/NedaAlip/Assessment‐of‐skin‐type‐measurement‐method/tree/main</ext-link>
</p><sec id="srt70374-sec-0110"><label>3.1</label><title>Color and Lightness Analysis of Skin Patch Images</title><p>Figures <xref rid="srt70374-fig-0008" ref-type="fig">8</xref> (a)‐(b) compare the lightness and color values in three color spaces across all skin types. The aim is to observe how lightness and color vary across different skin types and whether these parameters accurately suit measuring skin color diversity. Labels of type I to type VI refer to the different FSTs. These figures are shown in three HSV, YCbCr, and L<sup>*</sup>a<sup>*</sup>b<sup>*</sup> color spaces. V, Y, and L<sup>*</sup> parameters correspond to lightness, and H, Cb, Cr, a<sup>*</sup>, and b<sup>*</sup> refer to the chrominance parameters.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0008" orientation="portrait"><label>FIGURE 8</label><caption><p>(a)‐(b). Comparison of mean lightness and color values in three color spaces of HSV, YCbCr, and L<sup>*</sup>a<sup>*</sup>b<sup>*</sup>. Each bar represents the mean value of the corresponding parameters for dermatologist‐assigned Fitzpatrick skin types (FST). Figures show that lightness values (V, Y, L<sup>*</sup>) exhibit some variation across FSTs, and a decrease in skin type VI. The color components (Cb, Cr) remain relatively stable, but H, a<sup>*</sup>, and b<sup>*</sup> show changes over various skin types.</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-15" orientation="portrait" xlink:href="SRT-32-e70374-g003.jpg"><?image-name SRT-32-e70374-g003.jpg?><?image-size 67822?><?image-md5 79742cd08b6a40b7412e9e376ea8b41a?><?image-image-server-status NEVER_LOAD?><?image-original-height 691?><?image-original-width 540?><?image-scaled-height 691?><?image-scaled-width 540?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/79742cd08b6a/SRT-32-e70374-g003.jpg?><?thumb-name SRT-32-e70374-g003.gif?><?thumb-size 6758?><?thumb-md5 27db73e33517f63d2153654d45aa1f35?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 128?><?thumb-scaled-width 100?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/27db73e33517/SRT-32-e70374-g003.gif?></graphic></fig><p>Figures <xref rid="srt70374-fig-0008" ref-type="fig">8(a)</xref>) and 8(b) show that lightness decreases in all color spaces in type VI, reflecting the darker nature of these skin colors. The Hue values gradually decrease as the skin becomes darker. The Cb and Cr values show fewer variations across different skin types, whereas H, a<sup>*</sup>, and b<sup>*</sup> values show more noticeable changes. In particular, H tends to decrease from type I to type VI, and b<sup>*</sup> reaches its minimum value at type III.</p><p>Figure <xref rid="srt70374-fig-0009" ref-type="fig">9(a)</xref>) shows the lightness distribution across all skin types in the dataset, based on pixel counts. The lightness distribution in the range 60 ≤ L<sup>*</sup> ≤ 80 appears symmetrical, suggesting that most pixels represent moderate L<sup>*</sup> values.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0009" orientation="portrait"><label>FIGURE 9</label><caption><p>Pixel‐level‐based histogram showing the distribution of (a) lightness (L<sup>*</sup>) and (b) chrominance (a<sup>*</sup> and b<sup>*</sup>) across all skin types in the created dataset.</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-17" orientation="portrait" xlink:href="SRT-32-e70374-g001.jpg"><?image-name SRT-32-e70374-g001.jpg?><?image-size 21454?><?image-md5 4ec2bbd20fc02304b01bdd9e2535b789?><?image-image-server-status LOAD_COMPLETED?><?image-original-height 274?><?image-original-width 840?><?image-scaled-height 183?><?image-scaled-width 560?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/4ec2bbd20fc0/SRT-32-e70374-g001.jpg?><?thumb-name SRT-32-e70374-g001.gif?><?thumb-size 6132?><?thumb-md5 7bff993287aeddcdea307473e7a1ab89?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 65?><?thumb-scaled-width 200?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/7bff993287ae/SRT-32-e70374-g001.gif?></graphic></fig><p>The distribution suggests that most of the images in the dataset have relatively balanced lightness, neither too dark nor too light. In ranges L<sup>*</sup>&lt;40 and L<sup>*</sup>&gt;80, there are fewer pixels in very low lightness (very dark), and similarly, the number of pixels with very high lightness (very light) is also low. In Figure <xref rid="srt70374-fig-0009" ref-type="fig">9(b)</xref>), the 2D histogram illustrates the chrominance distribution of the dataset. Most pixels are concentrated near the center, indicating that most skin tones in the dataset have similar chromatic components, with chrominance values clustering closely together. The majority of them fall within the range of 0 to 50.</p></sec><sec id="srt70374-sec-0120"><label>3.2</label><title>ITA Values Distribution across an Imbalanced Dataset</title><p>The effectiveness of ITA as a means of classifying skin patch images into FSTs was evaluated. The experiment assessed how ITA performs when faced with an imbalanced dataset with unequal representation of different FSTs. As the PAD‐UFES‐20 dataset is imbalanced, the skin patch dataset created from it was also imbalanced. Figure <xref rid="srt70374-fig-0010" ref-type="fig">10(a)</xref>) shows the skin patch image distribution in the dataset, and Figure <xref rid="srt70374-fig-0010" ref-type="fig">10(b)</xref>) shows the histogram of ITA values within that dataset. Figure <xref rid="srt70374-fig-0010" ref-type="fig">10(a)</xref>) is a visual representation that depicts an alarming under‐representation of darker skin types, and Figure <xref rid="srt70374-fig-0010" ref-type="fig">10(b)</xref>) reflects this deficiency with the near absence of data points in the negative ITA range values.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0010" orientation="portrait"><label>FIGURE 10</label><caption><p>(a) Distribution of dermatologist‐labeled FSTs that show an imbalance in the skin patch dataset. (b) Histogram of ITA values of the skin patch image dataset indicating disparity in the estimated skin types across the dataset.</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-19" orientation="portrait" xlink:href="SRT-32-e70374-g013.jpg"><?image-name SRT-32-e70374-g013.jpg?><?image-size 23848?><?image-md5 e9967028c96584b4ecf7b0eb8dd57984?><?image-image-server-status LOAD_COMPLETED?><?image-original-height 269?><?image-original-width 840?><?image-scaled-height 179?><?image-scaled-width 560?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/e9967028c965/SRT-32-e70374-g013.jpg?><?thumb-name SRT-32-e70374-g013.gif?><?thumb-size 6402?><?thumb-md5 dadf8632539d722ae519aa344c8dce40?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 64?><?thumb-scaled-width 200?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/dadf8632539d/SRT-32-e70374-g013.gif?></graphic></fig><p>The histogram is left‐skewed, and the increasing density towards the peak of the histogram indicates that these ITA values are much more common in the dataset. The prominent peak occurs in the range of values between 35 and 65, corresponding to lighter skin types. This indicates that the dataset contains mostly ITA values associated with these two skin types. There is an initial decrease in frequency as ITA values move from the positive range towards the center. This decrease suggests that there are fewer images with darker skin types compared to lighter skin types. The bins corresponding to lower ITA values, representing darker skin types, are notably emptier than lighter skin types. Figure <xref rid="srt70374-fig-0010" ref-type="fig">10(b)</xref>) reveals an overlap between the ITA distributions of different Fitzpatrick skin types, suggesting that ITA may struggle to reliably separate Fitzpatrick skin types.</p></sec><sec id="srt70374-sec-0130"><label>3.3</label><title>Distribution of ITA Values across each FST Category</title><p>Concerning ITA's performance across different skin types, Figure <xref rid="srt70374-fig-0011" ref-type="fig">11(a)</xref>) to Figure <xref rid="srt70374-fig-0011" ref-type="fig">11(f)</xref>) present a series of histograms, each corresponding to a different skin type dataset, illustrating the distribution of ITA values. The red lines represent the Fitzpatrick skin type thresholds as defined by ITA values, based on [<xref rid="srt70374-bib-0065" ref-type="bibr">65</xref>] and presented in Table <xref rid="srt70374-tbl-0003" ref-type="table">3</xref>. The arrows indicate the range of ITA values corresponding to each skin type within these threshold domains.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0011" orientation="portrait"><label>FIGURE 11</label><caption><p>ITA histograms across each dermatologist‐based labeled skin type—(a)–(f): skin types I to VI, respectively, with predefined thresholds indicated by red lines. The blue arrows illustrate the range of expected ITA values for each skin type. The histograms reveal variations in ITA values and their deviations from the thresholds.</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-21" orientation="portrait" xlink:href="SRT-32-e70374-g015.jpg"><?image-name SRT-32-e70374-g015.jpg?><?image-size 63704?><?image-md5 745ecb5c5c32ea0d0d5a18335459aad2?><?image-image-server-status LOAD_COMPLETED?><?image-original-height 934?><?image-original-width 840?><?image-scaled-height 623?><?image-scaled-width 560?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/745ecb5c5c32/SRT-32-e70374-g015.jpg?><?thumb-name SRT-32-e70374-g015.gif?><?thumb-size 6265?><?thumb-md5 2aa7dc19f7de91f67d0af124a99416b2?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 111?><?thumb-scaled-width 100?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/2aa7dc19f7de/SRT-32-e70374-g015.gif?></graphic></fig><p>Figure <xref rid="srt70374-fig-0011" ref-type="fig">11</xref> shows that as the skin types darken, the distance between thresholds becomes greater, and also shows a decrease in the number of bins within threshold space, particularly in skin type VI, where there are no bins at the corresponding threshold domain. Therefore, ITA values related to each skin type do not fall exactly within the range related to that type of skin, indicating ITA values cannot follow the fixed thresholds.</p></sec><sec id="srt70374-sec-0140"><label>3.4</label><title>Distribution of ITA Values vs L<sup>*</sup> and b<sup>*</sup> Parameters</title><p>Figure <xref rid="srt70374-fig-0012" ref-type="fig">12</xref> shows the assessment of ITA values' dependence on luminance and chrominance parameters over different skin types, each distinguished by a unique shape.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0012" orientation="portrait"><label>FIGURE 12</label><caption><p>Scatter plot of ITA values according to the dermatologist‐based labels (DBL) versus the mean of L<sup>*</sup> and b<sup>*</sup> parameters. The background shows six different divided sectors, each corresponding to a range of ITA values. It shows how the ITA‐based classifier assigns images to skin type classes based on the ITA value ranges (rays). Points within the same ray are classified into the same skin type category.</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-23" orientation="portrait" xlink:href="SRT-32-e70374-g012.jpg"><?image-name SRT-32-e70374-g012.jpg?><?image-size 49295?><?image-md5 6935fb0b7d0a0ff6e6156427b9955056?><?image-image-server-status NEVER_LOAD?><?image-original-height 254?><?image-original-width 400?><?image-scaled-height 254?><?image-scaled-width 400?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/6935fb0b7d0a/SRT-32-e70374-g012.jpg?><?thumb-name SRT-32-e70374-g012.gif?><?thumb-size 7824?><?thumb-md5 97ebd5bbda221d0b7afd371f9afcba1e?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 79?><?thumb-scaled-width 125?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/97ebd5bbda22/SRT-32-e70374-g012.gif?></graphic></fig><p>In Figure <xref rid="srt70374-fig-0012" ref-type="fig">12</xref>, the densest concentration of data points appears to be in the upper areas of the figure with higher luminance range and moderate chrominance values, which could indicate that most of the measured skin types belong to lighter skin types. At the same time, the distribution of points shows the overlap between different skin types, particularly lighter skin types, showing a challenge for the method to effectively distinguish between them and increasing the rate of misclassification for lighter skin types. For skin type VI, it shows no correct classification. The results indicate that ITA‐based classification in this way is not suitable for reliably assigning images to different FSTs. The classifier assigns images based on predefined thresholds (rays), but these assignments do not correspond accurately to the actual skin types as determined by dermatologist‐assigned ground truth labels.</p></sec><sec id="srt70374-sec-0150"><label>3.5</label><title>ITA Prediction vs Dermatologist‐assigned Labels</title><p>Another method for evaluating the performance of an ITA‐based classifier is by using a confusion matrix, which compares its predictions against dermatologist‐assigned FST labels (ground truth), which is shown in Figure <xref rid="srt70374-fig-0013" ref-type="fig">13</xref>. This matrix compares the results of the ITA‐based skin type classification versus a dermatologist‐based one across six FSTs. Each column shows results for ITA, while rows show results for dermatologist‐based classification, and the diagonal elements from the top left to bottom right indicate the number of occurrences where both systems have the same results for classification.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0013" orientation="portrait"><label>FIGURE 13</label><caption><p>Confusion matrix using the skin patch image dataset. Each cell represents the number of samples from the predicted skin type using ITA method (columns) against the Fitzpatrick dermatologist‐based skin type (rows). The matrix illustrates the method's performance, highlighting the accuracy and misclassification rates for different skin types.</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-25" orientation="portrait" xlink:href="SRT-32-e70374-g010.jpg"><?image-name SRT-32-e70374-g010.jpg?><?image-size 29145?><?image-md5 e9c4fa7b7ba192c7ebd6c9bf75e22a88?><?image-image-server-status NEVER_LOAD?><?image-original-height 272?><?image-original-width 400?><?image-scaled-height 272?><?image-scaled-width 400?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/e9c4fa7b7ba1/SRT-32-e70374-g010.jpg?><?thumb-name SRT-32-e70374-g010.gif?><?thumb-size 6770?><?thumb-md5 7944a7fcfb8aea829b8dbdc2fbfdc1e1?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 80?><?thumb-scaled-width 117?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/7944a7fcfb8a/SRT-32-e70374-g010.gif?></graphic></fig><p>The confusion matrix highlights substantial misclassification across all Fitzpatrick skin types, with fixed‐threshold ITA showing very limited capability to distinguish between dermatologist‐assigned FST categories. Lighter skin types, particularly type II, were frequently misclassified as neighboring categories such as type I, while the darkest skin type (FST VI) received no correct classifications. Overall, fixed‐threshold ITA achieved 22.9% classification accuracy, which is below the majority‐class baseline accuracy of 51.3%. These findings demonstrate that fixed‐threshold ITA does not provide meaningful discriminatory performance for Fitzpatrick skin type classification under uncontrolled imaging conditions.</p></sec><sec id="srt70374-sec-0160"><label>3.6</label><title>Statistical Analysis of ITA Values across Skin Types</title><p>To support the statistical analysis of ITA performance across skin types, the mean ITA and the corresponding 95% confidence interval (CI) for each dermatologist‐assigned Fitzpatrick group were calculated as shown in Table <xref rid="srt70374-tbl-0004" ref-type="table">4</xref>. The CI provides an estimate of the uncertainty around the mean ITA: the lower bound (CI Low) and upper bound (CI High) delimit the range in which the true mean ITA value is expected to lie with 95% confidence.</p><table-wrap position="float" id="srt70374-tbl-0004" content-type="TABLE" orientation="portrait"><label>TABLE 4</label><caption><p>Mean ITA values and 95% confidence intervals across dermatologist‐assigned FST labels.</p></caption><table frame="hsides" rules="groups"><col align="left" span="1"/><col align="center" span="1"/><col align="center" span="1"/><col align="center" span="1"/><col align="center" span="1"/><thead><tr style="border-bottom:solid 1px #000000"><th align="left" rowspan="1" colspan="1">Skin type (FST)</th><th align="center" rowspan="1" colspan="1">Mean ITA</th><th align="center" rowspan="1" colspan="1">Number of images</th><th align="center" rowspan="1" colspan="1">95% CI (Low)</th><th align="center" rowspan="1" colspan="1">95% CI (High)</th></tr></thead><tbody><tr><td align="left" rowspan="1" colspan="1">I</td><td align="center" rowspan="1" colspan="1">49.04</td><td align="center" rowspan="1" colspan="1">110</td><td align="center" rowspan="1" colspan="1">44.43</td><td align="center" rowspan="1" colspan="1">53.66</td></tr><tr><td align="left" rowspan="1" colspan="1">II</td><td align="center" rowspan="1" colspan="1">44.90</td><td align="center" rowspan="1" colspan="1">472</td><td align="center" rowspan="1" colspan="1">42.58</td><td align="center" rowspan="1" colspan="1">47.22</td></tr><tr><td align="left" rowspan="1" colspan="1">III</td><td align="center" rowspan="1" colspan="1">42.85</td><td align="center" rowspan="1" colspan="1">277</td><td align="center" rowspan="1" colspan="1">39.42</td><td align="center" rowspan="1" colspan="1">46.27</td></tr><tr><td align="left" rowspan="1" colspan="1">IV</td><td align="center" rowspan="1" colspan="1">43.87</td><td align="center" rowspan="1" colspan="1">46</td><td align="center" rowspan="1" colspan="1">35.60</td><td align="center" rowspan="1" colspan="1">52.15</td></tr><tr><td align="left" rowspan="1" colspan="1">V</td><td align="center" rowspan="1" colspan="1">30.89</td><td align="center" rowspan="1" colspan="1">12</td><td align="center" rowspan="1" colspan="1">15.01</td><td align="center" rowspan="1" colspan="1">46.77</td></tr><tr><td align="left" rowspan="1" colspan="1">VI</td><td align="center" rowspan="1" colspan="1">−19.24</td><td align="center" rowspan="1" colspan="1">3</td><td align="center" rowspan="1" colspan="1">−34.36</td><td align="center" rowspan="1" colspan="1">−4.12</td></tr></tbody></table><permissions><copyright-holder>John Wiley &amp; Sons, Ltd.</copyright-holder></permissions></table-wrap><p>As shown in Table <xref rid="srt70374-tbl-0004" ref-type="table">4</xref>, types V and VI exhibit considerably wider intervals due to the small number of available samples, indicating reduced reliability of ITA estimates for darker skin types.</p></sec><sec id="srt70374-sec-0170"><label>3.7</label><title>Examples of Misclassified Images</title><p>Figure <xref rid="srt70374-fig-0014" ref-type="fig">14</xref> and Table <xref rid="srt70374-tbl-0005" ref-type="table">5</xref> illustrate sample images that were misclassified by the ITA method. These examples show how lighting variations, such as uneven lighting, reflections, or shadows, can alter perceived skin color and lead to incorrect ITA calculations.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0014" orientation="portrait"><label>FIGURE 14</label><caption><p>Examples of misclassified images due to varying lighting conditions. They are listed along with their corresponding numbers within the skin patch dataset.</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-27" orientation="portrait" xlink:href="SRT-32-e70374-g004.jpg"><?image-name SRT-32-e70374-g004.jpg?><?image-size 20186?><?image-md5 2f15e5815638cf74539172ab872d1ba7?><?image-image-server-status LOAD_COMPLETED?><?image-original-height 173?><?image-original-width 840?><?image-scaled-height 115?><?image-scaled-width 560?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/2f15e5815638/SRT-32-e70374-g004.jpg?><?thumb-name SRT-32-e70374-g004.gif?><?thumb-size 8843?><?thumb-md5 7847e80ca2394309ddeec9f005e97368?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 41?><?thumb-scaled-width 200?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/7847e80ca239/SRT-32-e70374-g004.gif?></graphic></fig><table-wrap position="float" id="srt70374-tbl-0005" content-type="TABLE" orientation="portrait"><label>TABLE 5</label><caption><p>Summary of misclassification causes, ITA values, and discrepancies between ITA‐based predictions and dermatologist‐assigned skin type labels.</p></caption><table frame="hsides" rules="groups"><col align="left" span="1"/><col align="center" span="1"/><col align="center" span="1"/><col align="center" span="1"/><col align="center" span="1"/><thead><tr style="border-bottom:solid 1px #000000"><th align="left" rowspan="1" colspan="1">Cause of misclassification</th><th align="center" rowspan="1" colspan="1">ITA value</th><th align="center" rowspan="1" colspan="1">Prediction by ITA</th><th align="center" rowspan="1" colspan="1">Dermatologist‐based label</th><th align="center" rowspan="1" colspan="1">Image number</th></tr></thead><tbody><tr><td align="left" rowspan="1" colspan="1">Low light/shadow</td><td align="center" rowspan="1" colspan="1">−6.561</td><td align="center" rowspan="1" colspan="1">5</td><td align="center" rowspan="1" colspan="1">1</td><td align="center" rowspan="1" colspan="1">1–7</td></tr><tr><td align="left" rowspan="1" colspan="1">Uneven lighting, reddish tint</td><td align="center" rowspan="1" colspan="1">−44.238</td><td align="center" rowspan="1" colspan="1">6</td><td align="center" rowspan="1" colspan="1">2</td><td align="center" rowspan="1" colspan="1">2–391</td></tr><tr><td align="left" rowspan="1" colspan="1">Side lighting/reflection loss</td><td align="center" rowspan="1" colspan="1">−34.352</td><td align="center" rowspan="1" colspan="1">6</td><td align="center" rowspan="1" colspan="1">3</td><td align="center" rowspan="1" colspan="1">3–106</td></tr><tr><td align="left" rowspan="1" colspan="1">Overexposure/strong light</td><td align="center" rowspan="1" colspan="1">78.586</td><td align="center" rowspan="1" colspan="1">1</td><td align="center" rowspan="1" colspan="1">4</td><td align="center" rowspan="1" colspan="1">4–10</td></tr><tr><td align="left" rowspan="1" colspan="1">Bright ambient light/flash</td><td align="center" rowspan="1" colspan="1">59.302</td><td align="center" rowspan="1" colspan="1">1</td><td align="center" rowspan="1" colspan="1">5</td><td align="center" rowspan="1" colspan="1">5–5</td></tr><tr><td align="left" rowspan="1" colspan="1">Slight overexposure or reflection effect</td><td align="center" rowspan="1" colspan="1">−27.107</td><td align="center" rowspan="1" colspan="1">5</td><td align="center" rowspan="1" colspan="1">6</td><td align="center" rowspan="1" colspan="1">6–3</td></tr></tbody></table><permissions><copyright-holder>John Wiley &amp; Sons, Ltd.</copyright-holder></permissions></table-wrap><p>This table presents examples of misclassified images to analyze the reasons behind ITA errors. The results indicate that lighting conditions such as low light, reflection, uneven lighting, and direct exposure altered ITA values, leading to incorrect skin type classification.</p></sec></sec><sec id="srt70374-sec-0180"><label>4</label><title>Discussion</title><p>Our study focused on evaluating ITA's robustness and reliability as a continuous quantitative metric of skin color analysis in image datasets. Given the limited access to datasets with expert‐labeled Fitzpatrick types, PAD‐UFES‐20 was chosen for its well‐separated lesion and healthy skin areas, allowing for better skin patch segmentation. The number of images labeled as skin types V or VI in the PAD‐UFES‐20 dataset (and hence in our skin patch image dataset) is very low. The distribution of ITA values across lighter skin types (higher ITA values) and darker skin types (lower ITA values) reflects the over‐representation of light skin types and under‐representation of dark skin types. Also, the skin images in PAD‐UFES‐20 present a wide range of lighting conditions, including shadowed areas, uneven lighting, and local overexposure. The results indicated that while the ITA method provides measurable differences in lightness across the dataset, its ability to assign FST categories accurately based on FST was limited not only by dataset imbalance, but also by substantial overlap between ITA distributions, predictions misalignment, lighting sensitivity, and failure to correctly classify the darkest skin type (FST VI).</p><p>The histogram distribution of ITA values for each FST showed that ITA does not conform well to the predefined FST ranges, particularly for darker types. The broader range of ITA values compared to the FST thresholds suggests that ITA produces broader continuous variation than discrete FST thresholds. Lighting variations further exacerbate ITA‐based classifier's limitations, as shown in Figure <xref rid="srt70374-fig-0015" ref-type="fig">15</xref> and Figure <xref rid="srt70374-fig-0016" ref-type="fig">16</xref>, where the same skin type appears differently under different lighting conditions.</p><fig position="float" fig-type="FIGURE" id="srt70374-fig-0015" orientation="portrait"><label>FIGURE 15</label><caption><p>Four image samples from PAD‐UFES‐20 show a misperception of skin color due to lighting variations. (a) Two images from different skin types (IV and III) show a perceived similarity in skin color due to lighting conditions. (b) Two images of the same patch of skin (I), taken under different lighting conditions, demonstrate significant variability in perceived skin color.</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-29" orientation="portrait" xlink:href="SRT-32-e70374-g002.jpg"><?image-name SRT-32-e70374-g002.jpg?><?image-size 40066?><?image-md5 ee49bcf40c25af0140b4b0fcb15bb4ce?><?image-image-server-status NEVER_LOAD?><?image-original-height 163?><?image-original-width 600?><?image-scaled-height 163?><?image-scaled-width 600?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/ee49bcf40c25/SRT-32-e70374-g002.jpg?><?thumb-name SRT-32-e70374-g002.gif?><?thumb-size 12080?><?thumb-md5 bdbbd19c414356a39580fd16351ed74b?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 54?><?thumb-scaled-width 200?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/bdbbd19c4143/SRT-32-e70374-g002.gif?></graphic></fig><fig position="float" fig-type="FIGURE" id="srt70374-fig-0016" orientation="portrait"><label>FIGURE 16</label><caption><p>Two samples from the skin patch image dataset show how lighting conditions affect how skin colors appear. (a) The image of skin type I looks like dark skin type. (b) The image is from skin type V, which looks like a lighter skin type.</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" position="anchor" id="jats-graphic-31" orientation="portrait" xlink:href="SRT-32-e70374-g007.jpg"><?image-name SRT-32-e70374-g007.jpg?><?image-size 16444?><?image-md5 21b5fb721e8681b216bfb478bc8a027e?><?image-image-server-status NEVER_LOAD?><?image-original-height 162?><?image-original-width 320?><?image-scaled-height 162?><?image-scaled-width 320?><?image-cloudpmc-urn urn:cdn:blobs/2871/13459198/21b5fb721e86/SRT-32-e70374-g007.jpg?><?thumb-name SRT-32-e70374-g007.gif?><?thumb-size 10710?><?thumb-md5 e99ba17545abc7d926814f78d4e744b5?><?thumb-image-server-status NEVER_LOAD?><?thumb-scaled-height 80?><?thumb-scaled-width 158?><?thumb-cloudpmc-urn urn:cdn:blobs/2871/13459198/e99ba17545ab/SRT-32-e70374-g007.gif?></graphic></fig><p>Figure <xref rid="srt70374-fig-0015" ref-type="fig">15(a)</xref>) illustrates that under varying lighting conditions; different lighter skin types may exhibit similar reflection and absorption properties. This results in more overlapping values within ITA method's parameter space, leading to misperceptions of true skin color and confusion with other light skin types. The higher rate of misclassifications between adjacent lighter skin types I and II in the confusion matrix highlights this issue. Figure <xref rid="srt70374-fig-0015" ref-type="fig">15(b)</xref>) illustrates why ITA‐based method classifies the same skin types across different thresholds, instead of classifying them within the same threshold range. It suggests that ITA‐based classifier is primarily influenced by changes in lightness (L<sup>*</sup>), although it is also affected by variations in chrominance (b<sup>*</sup>), depending on the extent of those variations. Figure <xref rid="srt70374-fig-0016" ref-type="fig">16(a)</xref>) and Figure <xref rid="srt70374-fig-0016" ref-type="fig">16(b)</xref>) illustrate how lighting variations can alter the perceived skin color, leading to misclassification of skin types. Accurate lighting calibration and standardized imaging conditions are essential to minimize such inconsistencies and improve the reliability of skin type measurement methods.</p><p>Figures <xref rid="srt70374-fig-0015" ref-type="fig">15</xref> and <xref rid="srt70374-fig-0016" ref-type="fig">16</xref> demonstrated how lighting conditions, such as overexposure, shadowing, and uneven lighting conditions, alter the perceived color and lightness of skin, leading to misclassification. Lighter skin types (I and II), which reflect more diffuse light, exhibited relatively stable ITA values under variable lighting. In contrast, darker skin types, which absorb more light due to higher melanin concentration, showed greater variability in ITA measurements, particularly in the L<sup>*</sup> channel of the L<sup>*</sup>a<sup>*</sup>b<sup>*</sup> color space [<xref rid="srt70374-bib-0077" ref-type="bibr">77</xref>]. This confirms that ITA is disproportionately affected by lighting when evaluating darker skin types.</p><p>The results also indicate that lighting variations disproportionately affect ITA measurements for darker skin types (V‐VI). Because ITA is driven by the L<sup>*</sup> component of the L<sup>*</sup>a<sup>*</sup>b<sup>*</sup> color space, any reduction in lightness caused by shadows, uneven lighting, or optical absorption is amplified in darker skin, where L<sup>*</sup> values are already low. As a result, small lighting changes can cause large shifts in ITA values, making the method less stable for highly pigmented skin. This instability is clearly visible in Figure <xref rid="srt70374-fig-0011" ref-type="fig">11 (e–f)</xref>, where the ITA histograms for types V‐VI show wide dispersion and poor alignment with the expected threshold ranges. These findings highlight that ITA mapping is inherently less robust for darker skin because reduced reflectance and higher melanin absorption magnify lighting‐dependent fluctuations in L<sup>*</sup>. Results show that ITA is more sensitive to lighting variability in darker skin types, which limits its reliability when used in uncontrolled imaging environments.</p><p>The lightness histogram exhibits a broader distribution, reflecting variability in lighting conditions and highlighting ITA's greater sensitivity to lightness over chrominance. The low number of data points in the bins for very dark and very light values suggests the need for more samples to improve the analysis of these skin types. Table <xref rid="srt70374-tbl-0002" ref-type="table">2</xref> indicates a clear dataset imbalance, with very few samples for skin types V and VI. This limits the strength of the conclusions that can be drawn for darker skin types and reduces the reliability of distributional estimates for these groups. However, the unstable ITA distributions observed for darker skin types should be interpreted as the combined result of small sample size, lighting sensitivity, overlapping ITA distributions, and mismatch between fixed ITA thresholds and dermatologist‐assigned FST labels, rather than as a consequence of dataset imbalance alone. As shown in Table <xref rid="srt70374-tbl-0004" ref-type="table">4</xref>, skin types V and VI exhibit wider 95% confidence intervals compared to lighter skin types. This reflects the combined effect of small sample sizes and greater lighting sensitivity in darker skin types. The broad intervals indicate that ITA‐based predictions for darker skins are less stable and less reliable. Also, overlapping ITA values across different FSTs in the histogram showed that FST skin type classification based only on ITA is not reliable.</p><p>Lightness also decreases in the darkest skin type of VI, while chrominance values show little variation, indicating limited color diversity and nuanced differences in representation between different skin types in the dataset. This lack of color diversity reflects the inherent similarity in chrominance values across all skin types, rather than the dominance of any specific skin type in the dataset.</p><p>ITA values were compared against Fitzpatrick labels assigned by dermatologists, which are discrete categories based on in‐person assessment. ITA showed very low classification accuracy when evaluated against subjective and discrete dermatologist‐assigned FST labels, which were used as the ground truth for the analysis. It does not accurately classify images into actual skin types as determined by dermatologist‐assigned labels. The inherent difference between these two continuous and discrete methods limits the direct alignment between ITA and FST. ITA's limitations in aligning with predefined FST thresholds highlight the need for alternative or enhanced metrics that are both robust to lighting changes and sensitive to subtle color variations, especially in darker skin colors. It shows that relying on fixed, discrete thresholds (such as those used in the Fitzpatrick system) may not be sufficient for identifying nuanced skin color variation. This limitation is particularly relevant for dataset fairness assessment, as underestimation or misclassification of darker skin types can cause bias in AI models. This highlights the need for alternative or complementary approaches capable of capturing the complexity of skin color diversity in image datasets.</p><p>Beyond ITA, other approaches have been proposed for skin type assessment. Physical and colorimetric methods, such as spectrophotometer‐based melanin or erythema indices, can provide accurate and lighting‐independent measurements; however, they are impractical for large‐scale image datasets due to their cost, acquisition time, and the need for controlled measurement conditions. More recent AI‐based methods may provide flexible and data‐driven approaches for skin color estimation; however, their performance also depends on the availability of sufficiently diverse and reliably labeled datasets, particularly for underrepresented darker skin types. These limitations help explain why ITA has been commonly used in prior work; however, its application should be treated with caution, particularly under varying lighting conditions, and only with explicit awareness of its inherent limitations, rather than as a standalone solution.</p><p>Threshold recalibration, lighting normalization, incorporating greater diversity, particularly within underrepresented skin colors, and preprocessing approaches may be explored in future work; however, the current results do not demonstrate that such modifications would be sufficient to achieve reliable Fitzpatrick skin type classification. PAD‐UFES‐20 was the only publicly available dataset that provided both dermatologist‐assigned Fitzpatrick labels and high‐resolution skin lesion images suitable for isolating skin regions. This issue restricted our ability to evaluate ITA across multiple datasets. It is considered a limitation, and it should be addressed in future work through collecting additional samples from darker skin types to ensure more balanced representation. Controlled lighting conditions and lighting normalization techniques would be valuable in future evaluations to minimize lighting‐related variability. Several preprocessing techniques have been proposed to address lighting variability in skin image analysis, including color constancy algorithms [<xref rid="srt70374-bib-0078" ref-type="bibr">78</xref>, <xref rid="srt70374-bib-0079" ref-type="bibr">79</xref>], histogram equalization [<xref rid="srt70374-bib-0080" ref-type="bibr">80</xref>], and GAN‐based illumination normalization [<xref rid="srt70374-bib-0081" ref-type="bibr">81</xref>]. These methods may help reduce lighting artifacts and may improve the consistency of color‐based metrics such as ITA. In future work, integrating such preprocessing steps before ITA computation may allow for more robust and fair assessments.</p><p>Our comparison between ITA‐based predictions and dermatologist‐assigned FST labels revealed inconsistencies, largely due to dataset limitations such as class imbalance, rigid Fitzpatrick thresholds, and the sensitivity of ITA to lighting conditions. Although ITA provides a continuous representation of skin color, this is insufficient for reliable alignment with discrete dermatologist‐assigned FST labels. These results indicate that ITA is not suitable for reliable FST classification under real‐world imaging conditions. While ITA provides continuous image‐derived color representation, it cannot reliably characterize dataset‐level skin color diversity or fairness under uncontrolled imaging conditions. To fairly evaluate the performance of that, future work will focus on collecting a diverse dataset with controlled lighting conditions to support accurate evaluation. Such a dataset may support future investigation of threshold recalibration and evaluation of alternative continuous skin color metrics. Also, new ITA thresholds designed specifically for darker skin types should be explored, and ITA should be compared against emerging metrics and spectrophotometric ground‐truth measurements. Finally, using a calibrated imaging system would enable more reliable cross‐dataset comparisons and support the development of lighting‐aware skin tone assessment models. As part of future work, a new dataset has been designed as part of this work, with continuous skin color labels obtained using a colorimeter as a reference, along with controlled and well‐documented lighting conditions.</p><p>ITA has been used in dermatology and AI‐based skin analysis studies as an image‐derived skin color or lightness metric commonly mapped to Fitzpatrick categories [<xref rid="srt70374-bib-0035" ref-type="bibr">35</xref>, <xref rid="srt70374-bib-0050" ref-type="bibr">50</xref>]. Recent studies also highlight the persistent under‐representation of darker skin in dermatology datasets and AI‐generated images [<xref rid="srt70374-bib-0001" ref-type="bibr">1</xref>, <xref rid="srt70374-bib-0082" ref-type="bibr">82</xref>]. Our findings support these concerns, showing that reliance on ITA alone may introduce systematic bias, particularly when datasets lack adequate dark skin representation. The results further demonstrate that ITA is unreliable for FST classification under uncontrolled imaging conditions and should not be interpreted as evidence of reliable skin type assessment performance.</p><p>To assess skin type diversity in datasets used to train AI models and for capturing the detailed color gradations of different skin types, the Fitzpatrick labeling system, based on fixed and rigid thresholds, may not be sufficiently informative. Instead, there is a need to investigate more robust and validated approaches capable of capturing subtle variations in skin color and provide a more nuanced understanding of dataset diversity. The findings suggest that rigid categorical classifications alone may be insufficient for representing the full variability of skin color in image datasets. Given the importance of image‐derived skin color assessment methods in detecting any under‐representation within datasets, it is essential to ensure their performance under varying lighting conditions. This may help identify under‐representation before datasets are used to train AI models to ensure fair and unbiased performance of these models across all skin colors. The results indicate that fixed‐threshold ITA does not provide sufficiently reliable performance for FST classification under uncontrolled imaging conditions. It emphasizes the importance of developing and validating more robust approaches for image‐based skin color assessment, particularly under variable lighting conditions and across diverse skin colors.</p></sec><sec id="srt70374-sec-0190"><title>Funding</title><p>This publication has emanated from research supported by a grant from Science Foundation Ireland under Grant number 18/CRT/6222.</p></sec><sec id="srt70374-sec-0200"><title>Ethics Statement</title><p>This study did not involve any new data collection involving human participants. All datasets used (PAD‐UFES‐20 and Fitzpatrick17k) are publicly available. <ext-link xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="https://doi.org/10.13039/501100001602" ext-link-type="uri">https://doi.org/10.13039/501100001602</ext-link>
</p></sec><sec sec-type="COI-statement" id="srt70374-sec-0210"><title>Conflicts of Interest</title><p>The authors declare no conflicts of interest.</p></sec></body><back><sec sec-type="data-availability" id="srt70374-sec-0230"><title>Data Availability Statement</title><p>The data that support the findings of this study are openly available in Github at <ext-link xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="https://github.com/NedaAlip/Assessment-of-skin-type-measurement-method/tree/main" ext-link-type="uri" specific-use="software is-supplemented-by">https://github.com/NedaAlip/Assessment‐of‐skin‐type‐measurement‐method/tree/main</ext-link>.</p></sec><ref-list id="srt70374-bibl-0001"><title>References</title><ref id="srt70374-bib-0001"><label>1</label><mixed-citation publication-type="journal" id="srt70374-cite-0001">
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