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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Environ. Archaeol.</journal-id>
<journal-title>Frontiers in Environmental Archaeology</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Environ. Archaeol.</abbrev-journal-title>
<issn pub-type="epub">2813-432X</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.3389/fearc.2025.1464315</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Environmental Archaeology</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Investigating historical attribution: luminescence dating of bricks from a submerged structure in southeastern India</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name><surname>Morthekai</surname> <given-names>Paulramasamy</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
<xref ref-type="corresp" rid="c001"><sup>&#x0002A;</sup></xref>
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<contrib contrib-type="author">
<name><surname>Singhal</surname> <given-names>Malika</given-names></name>
<xref ref-type="aff" rid="aff2"><sup>2</sup></xref>
<xref ref-type="aff" rid="aff3"><sup>3</sup></xref>
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<contrib contrib-type="author">
<name><surname>Sharma</surname> <given-names>Suchinder K.</given-names></name>
<xref ref-type="aff" rid="aff4"><sup>4</sup></xref>
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<contrib contrib-type="author">
<name><surname>Sivasubramaniam</surname> <given-names>Sudhakar</given-names></name>
<xref ref-type="aff" rid="aff5"><sup>5</sup></xref>
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<contrib contrib-type="author">
<name><surname>Kamarasu</surname> <given-names>Muthalankurichi</given-names></name>
<xref ref-type="aff" rid="aff6"><sup>6</sup></xref>
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<contrib contrib-type="author">
<name><surname>Singh</surname> <given-names>Priyanka</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
<xref ref-type="aff" rid="aff7"><sup>7</sup></xref>
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<contrib contrib-type="author">
<name><surname>Chauhan</surname> <given-names>Naveen</given-names></name>
<xref ref-type="aff" rid="aff2"><sup>2</sup></xref>
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<contrib contrib-type="author">
<name><surname>Kumar</surname> <given-names>Kamlesh</given-names></name>
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<contrib contrib-type="author">
<name><surname>Nawaz</surname> <given-names>Sheikh Ali</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
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<contrib contrib-type="author">
<name><surname>Khonde</surname> <given-names>Nitesh</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
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<aff id="aff1"><sup>1</sup><institution>Birbal Sahni Institute of Palaeosciences</institution>, <addr-line>Lucknow, UP</addr-line>, <country>India</country></aff>
<aff id="aff2"><sup>2</sup><institution>Physical Research Laboratory, Ahmedabad</institution>, <addr-line>Gujarat</addr-line>, <country>India</country></aff>
<aff id="aff3"><sup>3</sup><institution>Indian Institute of Technology, Gandhinagar</institution>, <addr-line>Gujarat</addr-line>, <country>India</country></aff>
<aff id="aff4"><sup>4</sup><institution>Amity School of Physical Sciences, Amity University Punjab</institution>, <addr-line>Mohali</addr-line>, <country>India</country></aff>
<aff id="aff5"><sup>5</sup><institution>Department of Archaeology, Manonmaniam Sundaranar University</institution>, <addr-line>Tirunelveli, TN</addr-line>, <country>India</country></aff>
<aff id="aff6"><sup>6</sup><institution>Independent Researcher</institution>, <addr-line>Seidhunganallur</addr-line>, <country>India</country></aff>
<aff id="aff7"><sup>7</sup><institution>Indian Institute of Geomagnetism, Navi Mumbai, Mumbai</institution>, <addr-line>Maharashtra</addr-line>, <country>India</country></aff>
<author-notes>
<fn fn-type="edited-by"><p>Edited by: Aditi K. Dave, Universit&#x000E9; de Lausanne, Switzerland</p></fn>
<fn fn-type="edited-by"><p>Reviewed by: Chantal Tribolo, Centre National de la Recherche Scientifique (CNRS), France</p>
<p>Manoj Kumar Jaiswal, Indian Institute of Science Education and Research Kolkata, India</p></fn>
<corresp id="c001">&#x0002A;Correspondence: Paulramasamy Morthekai <email>morthekai&#x00040;gmail.com</email></corresp>
</author-notes>
<pub-date pub-type="epub">
<day>11</day>
<month>03</month>
<year>2025</year>
</pub-date>
<pub-date pub-type="collection">
<year>2025</year>
</pub-date>
<volume>4</volume>
<elocation-id>1464315</elocation-id>
<history>
<date date-type="received">
<day>13</day>
<month>07</month>
<year>2024</year>
</date>
<date date-type="accepted">
<day>18</day>
<month>02</month>
<year>2025</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#x000A9; 2025 Morthekai, Singhal, Sharma, Sivasubramaniam, Kamarasu, Singh, Chauhan, Kumar, Nawaz and Khonde.</copyright-statement>
<copyright-year>2025</copyright-year>
<copyright-holder>Morthekai, Singhal, Sharma, Sivasubramaniam, Kamarasu, Singh, Chauhan, Kumar, Nawaz and Khonde</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/"><p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</p></license>
</permissions>
<abstract>
<p>By 2019, a long brick platform with some structures was exposed when the Thamirabarani River, the southernmost river in the city of Thirunelveli, dried up. The civic society rejoiced at the discovery of the exposed structure as it was thought to be the palace of the first capital city of the Pandya dynasty, an ancient Tamil dynasty of southern India. Two bricks were removed from the structure to determine their ages using the luminescence dating method, and their geochemical composition was analyzed using the X-ray fluorescence method. The bricks were composed of mud that underwent intermediate silicate weathering. High values of anomalous fading rate were observed from both the fine-grain polymineral (9.5&#x02013;10.5%.decade<sup>&#x02212;1</sup>) and coarse-grain K-feldspar (15.5%.decade<sup>&#x02212;1</sup>), and this could be attributed to the significant presence of sanidine phase of K-feldspar. The fading corrected luminescence ages (1430&#x02013;1530 CE) based on the coarse grain K-feldspar of the bricks placed the structure historically in the period of the Vijayanagar Empire, where the Late Pandyas had some autonomy in the south. These age estimates could resolve the hypothesis that the structure was not made by the Early Pandyas (400 BCE&#x02212;300 CE). This study also reports discrepant ages for coarse quartz grains samples (1,689 CE; &#x000B1; 10 years, 1 &#x003C3;) and two fine polymineral grains samples (1634 CE; &#x000B1; 90 years and 1699 CE; &#x000B1; 30 years) compared to the age of the coarse K-feldspar grains samples. This discrepancy requires further investigation.</p></abstract>
<kwd-group>
<kwd>Luminescence dating</kwd>
<kwd>IRSL</kwd>
<kwd>OSL</kwd>
<kwd>brick</kwd>
<kwd>Pandya dynasty</kwd>
<kwd>Vijayanagar Empire</kwd>
<kwd>South India</kwd>
</kwd-group>
<counts>
<fig-count count="8"/>
<table-count count="2"/>
<equation-count count="2"/>
<ref-count count="52"/>
<page-count count="12"/>
<word-count count="7716"/>
</counts>
<custom-meta-wrap>
<custom-meta>
<meta-name>section-at-acceptance</meta-name>
<meta-value>Landscape and Geological Processes</meta-value>
</custom-meta>
</custom-meta-wrap>
</article-meta>
</front>
<body>
<sec id="s1">
<title>1 Introduction</title>
<p>The Pandyas Dynasty reigned in southeastern Tamil Nadu, the southernmost Indian State, for more than 2,000 years from as early as the 4th century BCE until the 17th century CE. The Tamil literature suggests that they shifted their capital cities to Korkai, Madurai, and Tenkasi at various periods (Foote, <xref ref-type="bibr" rid="B14">1883</xref>; Manoranjithamoni, <xref ref-type="bibr" rid="B32">2012</xref>; Ganapathy, <xref ref-type="bibr" rid="B15">2015</xref>). However, considering that Korkai had indeed been one of the capital cities of Pandyas is debatable (Nilakanta Sastri, <xref ref-type="bibr" rid="B38">1929</xref>). Indeed, Madurai and Tenkasi had palaces, whereas no such buildings were ever discovered in Korkai. Thus, this leads to the question regarding material evidence to support (or reject) the Early Pandyas (400 BCE&#x02212;300 CE) ruling from Korkai.</p>
<p>While usual summer and winter monsoons fill the Thamirabarani River (also known as Tambraparni and Porunai), in 2019, a submerged structure built using bricks was exposed as the river dried, owing to poor monsoon rainfall. The structure was located near Authoor, a small town in Thoothukudi District, Tamil Nadu, India (<xref ref-type="fig" rid="F1">Figure 1</xref>), 1.5 km away from Korkai (to the north side) and 3 km from the Bay of Bengal (to the east), where the river confluences with the sea (<xref ref-type="fig" rid="F2">Figure 2</xref>). The structure was found in the middle (<xref ref-type="fig" rid="F3">Figures 3A</xref>&#x02013;<xref ref-type="fig" rid="F3">E</xref>) and at the right bank (<xref ref-type="fig" rid="F3">Figure 3F</xref>) of the river (flowing toward the Bay of Bengal; <xref ref-type="fig" rid="F2">Figure 2</xref>). There were stone pillars with Hindu deities found near these parts of the structure in the middle of the river (<xref ref-type="fig" rid="F3">Figures 3C</xref>, <xref ref-type="fig" rid="F3">D</xref>), and they could either belong to Nayak period (1529&#x02013;1736 CE) or to the Vijayanagara Empire (1336&#x02013;1565 CE) period (Pathy, <xref ref-type="bibr" rid="B39">2013</xref>; Mahalingam, <xref ref-type="bibr" rid="B31">2015</xref>). Meanwhile, it was believed by the locals to be the long-awaited evidence of the existence of the palace of the Early Pandyas.</p>
<fig id="F1" position="float">
<label>Figure 1</label>
<caption><p>The location of study area <bold>(A)</bold> and the archaeologically important sites around the study area <bold>(B)</bold>. Pazhayakayal and Korkai were ports earlier, and Thoothukudi is the present port. White arrow indicates the study site. In <bold>(B)</bold> was modified after Gupta and Rajani (<xref ref-type="bibr" rid="B17">2023</xref>). Relevant places are indicated.</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fearc-04-1464315-g0001.tif"/>
</fig>
<fig id="F2" position="float">
<label>Figure 2</label>
<caption><p>The schematic diagram that shows the brick structures that appeared in the Thamirabarani River.</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fearc-04-1464315-g0002.tif"/>
</fig>
<fig id="F3" position="float">
<label>Figure 3</label>
<caption><p>Brick structures <bold>(A, B)</bold>, stone sculptures <bold>(C, D)</bold> and the samples used in this study [<bold>(E)</bold> middle of the river and <bold>(F)</bold> the right side of the river]. Except the authors (PM and MK&#x02014;in squad position), others faces are not shown.</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fearc-04-1464315-g0003.tif"/>
</fig>
<p>Therefore, this raised two questions: what was the actual age of the structure, and what was its exact nature and relation to the river? Indeed, the entire stretch of the structure in Thamirabarani River was not exposed except at the sides (<xref ref-type="fig" rid="F3">Figure 3</xref>); therefore, it was unclear whether the structure was part of a ruined palace, temple, bridge, irrigation check dam, or bathing step. Korkai was a port city till at least 302 BCE-130 CE, according to Megasthanese, author of the Periplus of the Erythraean Sea, and Ptolemy (Caldwell, <xref ref-type="bibr" rid="B11">1877</xref>, <xref ref-type="bibr" rid="B12">1881</xref>; Foote, <xref ref-type="bibr" rid="B14">1883</xref>; Arunachalam et al., <xref ref-type="bibr" rid="B4">2006</xref>). At present, Korkai is located 5 km inland from the present-day coast to the east, with the Thamirabarani River to the south. This river had different course in earlier times (4th century BCE&#x02014;red line, 8th century CE&#x02014;dark blue line, 1750 CE&#x02014;purple line, and at present&#x02014;light blue line) and it had shown a southward migration with time based on remote sensing study (Arunachalam et al., <xref ref-type="bibr" rid="B4">2006</xref>).</p>
<p>While the question about the nature of the structure remains open, this paper deals with the determination of the age, which would help to determine whether it was built by the Early Pandyas or not. Therefore, to resolve the debate, we took samples from the exposed structure in order to estimate the age using luminescence dating methods and study the geochemical composition.</p>
</sec>
<sec id="s2">
<title>2 Materials and methods</title>
<p>Two full bricks from the structure (typically of 2&#x02013;3 m<sup>3</sup>; <xref ref-type="fig" rid="F3">Figure 3</xref>) were used in this study. One brick was from the structure in the middle of the river (ABL, <xref ref-type="fig" rid="F2">Figures 2</xref>, <xref ref-type="fig" rid="F3">3E</xref>) and the other was on the right side of the river (ABR, <xref ref-type="fig" rid="F3">Figure 3F</xref>). Both of them were of same dimension (20 cm, 13 cm, 3.5 cm; lbh). From the bricks, we collected samples for luminescence dating and X-ray fluorescence (XRF) measurements. To understand the detailed mineralogical composition and crystallinity of the samples used for luminescence dating, powder X-ray diffraction (pXRD) patterns were measured on the extracted coarser grains of quartz and K-feldspar.</p>
<sec>
<title>2.1 Materials</title>
<p>The light-exposed outer layer (&#x0007E;1 cm) of the bricks was removed in the Luminescence Dating Laboratory (LumDL) of the Birbal Sahni Institute of Paleosciences (BSIP) in a subdued red light environment. The part of the brick that was unexposed to light was used for dose measurement using luminescence, while the exposed part was used for dose rate estimation.</p>
<p>The brick unexposed to light was gently crushed using an agate mortar and pestle without disturbing the original grain size distribution. The crushed samples were treated with 1N hydrochloric acid (HCl) to remove carbonates and 35% hydrogen peroxide to remove organic materials. The finer grains that were stuck to the coarser grains were deflocculated using 0.01N sodium oxalate. The fine-grained fraction (4&#x02013;11 &#x003BC;m) of the polymineral was extracted using the settling method based on Stokes&#x00027; law in an acetone medium (15 cm column) by allowing it to settle for 1.5 min (&#x0003C;11 &#x003BC;m) and 15 min (&#x0003E;4 &#x003BC;m). This fine-grain fraction (1 ml) was deposited on cleaned aluminum discs (9.6 mm) in a flat-bottom vial (6 cm) with acetone (2 ml). Dried aliquots were used to measure the dose using the fine-grained polymineral method. Fine grain polymineral fractions were extracted from both brick samples.</p>
<p>Polymineral grains larger than 11 &#x003BC;m (settled before 1.5 min in acetone medium) were oven dried and sieved to obtain a 90&#x02013;150 &#x003BC;m portion. The heavy mineral fraction was extracted from this sieved portion using Franz Magnetic Laboratory Separator (LB 1) at 0.5 Ampere current, and subsequently, quartz and bulk feldspar fractions were separated at 1.5 Ampere with a typical flow rate of 2&#x02013;3 g.min<sup>&#x02212;1</sup>, tilt of 17&#x000B0; and slope of 25&#x000B0; (Porat, <xref ref-type="bibr" rid="B41">2006</xref>). Quartz grains were etched using 40% hydrofluoric acid (HF) for 80 min to remove the outer 20&#x02013;25 &#x003BC;m layer, allowing the ambient alpha dose rate to be ignored in further calculations. These etched quartz grains were treated with 40% HCl for 30 min to remove any spurious luminescent fluoride precipitates and then wet sieved to remove any &#x0003C; 90&#x003BC;m quartz. The oven-dried quartz grains were mounted as a monolayer on silicone-oiled stainless steel (SS) discs, which were used as aliquots (medium size; 3 mm) to measure the dose using the coarse quartz grain method. Only coarse quartz grains for the sample from the middle of the river (ABL) were sufficiently available for measurements. The purity of quartz was checked by measuring the IRSL of the quartz samples and calculating the IR percentage depletion ratio (IRpDR; Ali et al., <xref ref-type="bibr" rid="B3">2022</xref>).</p>
<p>K-feldspar grains (floating grains) were separated from the bulk feldspar fraction (separated using a magnetic separator at 1.5 Ampere) using sodium polytungstate of density 2.58 g/cm<sup>&#x02212;3</sup>. The K-feldspar grains were then etched using diluted (10%) HF for 80 min, followed by concentrated HCl for 30 min, for reasons similar to the treatment of quartz. Grains sized &#x0003C;90 &#x003BC;m were wet-sieved, and &#x0003E;90 &#x003BC;m were oven-dried. Medium-sized SS aliquots were prepared with the K-feldspar grains and used for dose measurements, applying the coarse K-feldspar grain method. Coarse K-feldspar grains were sufficiently available in the ABL sample only. Overall, the ABL sample was measured using fine-grained polyminerals (ABL PM), coarse-grained quartz (ABL Qz), and K-feldspar (ABL KF), whereas only fine-grained polyminerals (ABR PM) were measured for the ABR.</p>
<p>The light-exposed parts of the samples were crushed using a Retsch disc mill (RS-200) and used to measure the concentrations of uranium, thorium, potassium, and major oxides in these samples.</p>
</sec>
<sec>
<title>2.2 Dose rate estimation</title>
<p>The dose rate was computed by measuring the concentrations of uranium, thorium, and potassium using a high-purity Ge gamma spectrometer calibrated using the NUSSY standard (Preusser and Kasper, <xref ref-type="bibr" rid="B43">2001</xref>). The crushed samples were stored in airtight plastic boxes for a minimum of 20 days to allow <sup>222</sup>Rn (half-life = 3.82 days), a radioactive daughter in the <sup>238</sup>U decay series, to reach secular equilibrium with its immediate parent, <sup>226</sup>Ra. This equilibrium is necessary because crushing the samples caused radon, a gas, to escape, disrupting the secular equilibrium. The gamma spectra of NUSSY and the background were obtained over a counting time of 4 days. The samples and subsequent background were obtained after counting for 7&#x02013;8 and 12 h, respectively. The concentrations of uranium, thorium, and potassium were determined by comparing the background-subtracted NUSSY and sample spectra. Assuming secular equilibrium between the radioactive daughters and parents in the uranium and thorium series, the concentrations of uranium and thorium were calculated by averaging the concentrations of their respective radioactive daughter elements (<sup>226</sup>Ra, <sup>214</sup>Pb, and <sup>214</sup>Bi for the uranium series and <sup>212</sup>Pb, <sup>228</sup>Ac, and <sup>208</sup>Tl for the thorium series) in the samples (Singh et al., <xref ref-type="bibr" rid="B47">2024</xref>). The alpha efficiency (a-value) for the fine grain polymineral was assumed to be 0.08 &#x000B1; 0.04 (no unit) for dose rate calculation (Kreutzer et al., <xref ref-type="bibr" rid="B24">2014</xref>). The concentration of internal potassium (K<sub>int</sub>) was assumed to be 12.5 &#x000B1; 0.5% (Huntley and Baril, <xref ref-type="bibr" rid="B18">1997</xref>). For quartz, the attenuation factors of Brennan et al. (<xref ref-type="bibr" rid="B10">1991</xref>) and Guerin et al. (<xref ref-type="bibr" rid="B16">2012</xref>) were used for alpha and beta particles, respectively. For K-feldspar, they were from Bell (<xref ref-type="bibr" rid="B7">1980</xref>) and Mejdahl (<xref ref-type="bibr" rid="B33">1979</xref>) for alpha and beta particles, respectively. The conversion factors of Adamiec and Aitken (<xref ref-type="bibr" rid="B2">1998</xref>) were applied. The water content of ABL was measured to be 0.97%. Assuming the bricks, at least ABL, were in the water most of the time, the water content was assumed to be 5 &#x000B1; 2%. Considering the thickness of the structure (<xref ref-type="fig" rid="F3">Figure 3</xref>), the gamma dose rate does not need any geometric correction. As the brick was taken from one layer below the multi-layered brick structure of the size of 2&#x02013;3 m<sup>3</sup> and considering the effective water column variation with time, 30 cm was considered as depth of the sample below the surface for dose rate computation. The cosmic ray dose rate was computed using the latitude, longitude, altitude, and depth of the samples (Prescott and Hutton, <xref ref-type="bibr" rid="B42">1994</xref>). Finally, the dose rate was calculated using DRAC, a freely available online calculator (Durcan et al., <xref ref-type="bibr" rid="B13">2015</xref>).</p>
</sec>
<sec>
<title>2.3 Equivalent dose estimation</title>
<p>All luminescence measurements and beta irradiation were performed using a Risoe TL/OSL Reader TA-20 (Lapp et al., <xref ref-type="bibr" rid="B29">2015</xref>). A calibrated beta source (<sup>90</sup>Sr/<sup>90</sup>Y) was used to irradiate the samples. The dose rates were 0.089 Gy.s<sup>&#x02212;1</sup> and 0.062 Gy.s<sup>&#x02212;1</sup> for the SS and Al discs, respectively at BSIP, and 0.045 Gy.s<sup>&#x02212;1</sup> for the SS discs at the Physical Research Laboratory, Ahmedabad (PRL). Infrared-stimulated luminescence (IRSL) signal was used to estimate the dose of the fine-grained polymineral and coarse K-feldspar grains, whereas blue stimulated luminescence (OSL) signal was used for the coarse quartz grains.</p>
<p>The IRSL<sub>50&#x000B0;C; 200&#x000B0;C</sub> and IRSL<sub>50&#x000B0;C; 250&#x000B0;C</sub> (the first subscripted value indicates the stimulation temperature and the second one indicates the preheat temperature) were measured respectively from a preheated polymineral (to 200&#x000B0;C) or K-feldspar (to 250&#x000B0;C) sample by stimulating with infrared (IR) photons (850 &#x000B1; 40 nm) at 50&#x000B0;C. Thus, IR stimulated signals were detected in the violet-blue range using combined BG-39 and Corning 7&#x02013;59 filters in front of the photo-multiplier tube (PMT; PDM 9107Q-AP-TTL-03). Preheat plateau tests (from 175 to 275&#x000B0;C at 25&#x000B0;C interval) and dose recovery tests were done to check the efficiency of the dose measurement protocol.</p>
<p>The post IR IRSL was also measured from the coarse K-feldspar grains, but the measurement of this signal was not possible for the fine polymineral grains due to our laboratory specific logistic reasons. The pIR IRSL<sub>290&#x000B0;C; 320&#x000B0;C</sub> signal was measured after a IRSL (IRSL<sub>50&#x000B0;C; 320&#x000B0;C</sub>) measurement on a preheated K-feldspar (to 320&#x000B0;C) sample by stimulating with IR photons and detecting photons in the violet-blue range. This was done in PRL. A dose recovery test was carried out on this signal as well.</p>
<p>The OSL signal was measured on the quartz sample by stimulating with blue photons (470 &#x000B1; 20 nm) at 125&#x000B0;C, and detecting UV photons using a Hoya U-340 filter of 7.5 mm size in front of the same PMT. A preheat plateau test (from 180 to 260&#x000B0;C at 20&#x000B0;C interval) was carried out to optimize the preheating temperature and a dose recovery test was done as well. As the sample was a heated material, the preheat plateau tests were carried out on the fresh aliquots with natural dose in them and three aliquots were used per preheat temperature. However, due to the unavailability of samples, 6 of already used aliquots were used for the dose recovery tests by recovering a known dose of 1.2 Gy.</p>
<p>A single-aliquot regenerative (SAR) dose protocol was used to estimate the equivalent dose (D<sub>e</sub>; Gy) for all three types of samples (Murray and Roberts, <xref ref-type="bibr" rid="B36">1998</xref>; Murray and Wintle, <xref ref-type="bibr" rid="B37">2000</xref>). The dose response curve (DRC) was constructed using sensitivity-corrected IRSL (PM and KF) or OSL (Quartz) for five laboratory doses, including three increasing doses with one repetition and one zero dose. Aliquots were accepted for D<sub>e</sub> estimation if they had a recycling ratio within 10% of unity, a relative test dose error within 10%, and recuperation within 5%. The fading-uncorrected D<sub>e</sub> was estimated by interpolating the natural IRSL (L<sub>n</sub>/T<sub>n</sub>) onto the DRC.</p>
</sec>
<sec>
<title>2.4 Fading correction</title>
<p>The IRSL signal fades over time (Wintle, <xref ref-type="bibr" rid="B51">1973</xref>; Visocekas et al., <xref ref-type="bibr" rid="B50">1994</xref>) and occasionally does the quartz OSL as well (Tsukamoto et al., <xref ref-type="bibr" rid="B49">2007</xref>), so this fading needs to be corrected. The fading rate of the IRSL (from fine-grained polymineral), IRSL<sub>50&#x000B0;C; 320&#x000B0;C</sub> and pIR IRSL<sub>290&#x000B0;C; 320&#x000B0;C</sub> (from coarse-grained K-feldspar) and OSL (from coarse-grained quartz) were measured using the single-aliquot regenerative-dose protocol (Auclair et al., <xref ref-type="bibr" rid="B5">2003</xref>) and the fading rate parameter, &#x003C1;&#x02032;&#x02013;a dimensionless number&#x02014;was obtained by fitting the data using the fading equation of Huntley (<xref ref-type="bibr" rid="B19">2006</xref>). Fading was corrected using the Huntley and Kars Method (Huntley, <xref ref-type="bibr" rid="B19">2006</xref>; Kars et al., <xref ref-type="bibr" rid="B21">2008</xref>). In this method, each point (L<sub>x</sub>/T<sub>x</sub>) in the DRC used for D<sub>e</sub> estimation was corrected for fading that occurred during the respective irradiation times (in minutes at 0.062&#x02013;0.089 Gy.s<sup>&#x02212;1</sup> in BSIP, and at 0.045 Gy.s<sup>&#x02212;1</sup> in PRL) of the laboratory dose using &#x003C1;&#x02032;. This corrected DRC is called the unfaded DRC. Each data point of the unfaded DRC was further adjusted to account for fading that would have occurred if the laboratory dose had been administered at a natural dose rate (in thousands of years at 4&#x02013;6 Gy.ka<sup>&#x02212;1</sup>), resulting in what was called the natural DRC. The fading-corrected D<sub>e</sub> was calculated by interpolating L<sub>n</sub>/T<sub>n</sub> onto the natural DRC (Morthekai et al., <xref ref-type="bibr" rid="B34">2011</xref>; Biswas et al., <xref ref-type="bibr" rid="B9">2013</xref>; Singh et al., <xref ref-type="bibr" rid="B46">2023</xref>). The representative D<sub>e</sub> for age calculation was optimized using the central age model (CAM; Singh et al., <xref ref-type="bibr" rid="B46">2023</xref>). Error in the fading corrected age was calculated by error propagation (quadrature addition of fractional errors of D<sub>e</sub> and dose rate) and an added component. The added component was the increase in the error between the fading corrected and un-corrected age as obtained from the <italic>Luminescence</italic> package of R using <italic>calc_Huntley2006()</italic> and <italic>calc_CentralDose()</italic> methods sequentially (Kreutzer et al., <xref ref-type="bibr" rid="B23">2018</xref>; R Core Team, <xref ref-type="bibr" rid="B44">2020</xref>).</p>
</sec>
<sec>
<title>2.5 Synthesis of age estimates</title>
<p>The ages were synthesized using two methods. The first method was based on conventional statistical methods. The equations provided below were used to calculate the mean and standard deviation of the synthesized age, and from these values, the age range was established.</p>
<disp-formula id="E1"><label>(1)</label><mml:math id="M13"><mml:mtable class="eqnarray" columnalign="left"><mml:mtr><mml:mtd><mml:msub><mml:mrow><mml:mi>&#x003BC;</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi><mml:mi>b</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mtext>&#x000A0;</mml:mtext><mml:mfrac><mml:mrow><mml:msub><mml:mrow><mml:mi>&#x003BC;</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msub><mml:msubsup><mml:mrow><mml:mi>&#x003C3;</mml:mi></mml:mrow><mml:mrow><mml:mi>b</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:mo>&#x0002B;</mml:mo><mml:msub><mml:mrow><mml:mi>&#x003BC;</mml:mi></mml:mrow><mml:mrow><mml:mi>b</mml:mi></mml:mrow></mml:msub><mml:msubsup><mml:mrow><mml:mi>&#x003C3;</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:mtext>&#x000A0;</mml:mtext></mml:mrow><mml:mrow><mml:msubsup><mml:mrow><mml:mi>&#x003C3;</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:mo>&#x0002B;</mml:mo><mml:mtext>&#x000A0;</mml:mtext><mml:msubsup><mml:mrow><mml:mi>&#x003C3;</mml:mi></mml:mrow><mml:mrow><mml:mi>b</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:mfrac></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
<p>and</p>
<disp-formula id="E2"><label>(2)</label><mml:math id="M14"><mml:mtable class="eqnarray" columnalign="left"><mml:mtr><mml:mtd><mml:msub><mml:mrow><mml:mi>&#x003C3;</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi><mml:mi>b</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mtext>&#x000A0;</mml:mtext><mml:msqrt><mml:mrow><mml:mfrac><mml:mrow><mml:msubsup><mml:mrow><mml:mi>&#x003C3;</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:msubsup><mml:mrow><mml:mi>&#x003C3;</mml:mi></mml:mrow><mml:mrow><mml:mi>b</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup></mml:mrow><mml:mrow><mml:msubsup><mml:mrow><mml:mi>&#x003C3;</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:mo>&#x0002B;</mml:mo><mml:mtext>&#x000A0;</mml:mtext><mml:msubsup><mml:mrow><mml:mi>&#x003C3;</mml:mi></mml:mrow><mml:mrow><mml:mi>b</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:mfrac></mml:mrow></mml:msqrt></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
<p>where &#x003BC; and &#x003C3; are the mean and standard deviation of two given ages of a and b, respectively. Likewise any number of ages can be subsequently added, and the order of the ages to be combined does not matter. The second method involves modeling within a Bayesian framework. ChronoModel v2.0 18, a free software for hierarchical Bayesian modeling, was used to synthesize the ages (Banks, <xref ref-type="bibr" rid="B6">2015</xref>; Binder et al., <xref ref-type="bibr" rid="B8">2017</xref>; Lanos and Philippe, <xref ref-type="bibr" rid="B28">2017</xref>; Lanos and Dufresne, <xref ref-type="bibr" rid="B27">2019</xref>). The requirement for synthesis is that the ages must be independent to some extent. The structure was created within the age uncertainties at a particular time, representing the Event (only one) here. The posterior age estimates and variances were verified by checking the convergence of Markov chains to equilibrium (History plots) and the correlation between successive values in the Markov chain (Autocorrelation). All calculations were conducted in calendar years, with the reference year being 2019 CE.</p>
</sec>
<sec>
<title>2.6 Mineralogical composition of bricks</title>
<p>The X-ray diffraction spectra were measured on the extracted quartz and K-feldspar grains to study the phase of quartz (whether it is &#x003B1;- or &#x003B2;-quartz) and K-feldspar. The powder X-ray diffraction patterns were measured on a Rigaku instrument (MiniFlex 600) having Cu-target that emits wavelength of 1.54060 &#x000C5; (Sharma et al., <xref ref-type="bibr" rid="B45">2024</xref>). The scan speed was 0.01&#x000B0;/s over a 2&#x003B8; range of 10 to 80&#x000B0;. The pXRD patterns were analyzed using Crystal Impact Match software (<ext-link ext-link-type="uri" xlink:href="https://www.crystalimpact.de/match/">https://www.crystalimpact.de/match/</ext-link>), and the mineralogical compositions were quantified.</p>
</sec>
<sec>
<title>2.7 Geochemical composition of bricks</title>
<p>The major oxides were measured using XRF to determine the geochemical compositions of the samples. The samples were initially ground to &#x0007E;200 &#x003BC;m mesh using a Retsch Disc mill (RS-200). The powdered samples were oven-dried (&#x0007E;100&#x000B0;C for 12 h) and pressed into pellets (Stork et al., <xref ref-type="bibr" rid="B48">1987</xref>; Khanna et al., <xref ref-type="bibr" rid="B22">2009</xref>). The analysis was performed using the Wavelength Dispersive X-Ray Fluorescence (WD-XRF) model: Axios max, 4 KW, PANalytical made at BSIP, Lucknow. The precision and accuracy of sample preparation and instrumental performance were checked using international reference standards for sediments (e.g., COQ-1, BCR-2, SGR-1b, Sco-1, JSP-2, RGM-2, and DGH). The accuracy of measurement was better than 2&#x02013;5%, and the precision was &#x0003C;2%.</p>
</sec>
</sec>
<sec id="s3">
<title>3 Results</title>
<p>Three types of results were obtained in this study: the age of the brick-made structure, the phase nature of quartz and K-feldspar grains extracted from the bricks, and the geochemical composition of the bricks from the structure.</p>
<sec>
<title>3.1 Luminescence ages</title>
<p>The measured concentrations of uranium, thorium, and potassium, computed dose rates, and D<sub>e</sub> are listed in <xref ref-type="table" rid="T1">Table 1</xref>. Coarse grains received 56% dose rate from beta particles and 39% from gamma rays whereas fine grains, in addition to these, also received around 20% of the dose rate from alpha particles (<xref ref-type="supplementary-material" rid="SM6">Supplementary Table S1</xref>). The high thorium concentration in the sample might be due to the presence of monazite and sillimanite in the nearby beach sands of this region (Lakshmi et al., <xref ref-type="bibr" rid="B26">2019</xref>; Abishek et al., <xref ref-type="bibr" rid="B1">2022</xref>).</p>
<table-wrap position="float" id="T1">
<label>Table 1</label>
<caption><p>Required parameters that were measured and calculated for final age estimation after fading correction.</p></caption>
<table frame="box" rules="all">
<thead>
<tr style="background-color:#919498;color:#ffffff">
<th valign="top" align="left"><bold>Sample</bold></th>
<th valign="top" align="left"><bold>Material</bold></th>
<th valign="top" align="center"><bold>Signal</bold></th>
<th valign="top" align="center"><bold>U (ppm)</bold></th>
<th valign="top" align="center"><bold>Th</bold><break/> <bold>(ppm)</bold></th>
<th valign="top" align="center"><bold>K (%)</bold></th>
<th valign="top" align="center"><bold>Dose rate</bold><break/> <bold>(Gy.ka<sup>&#x02212;1</sup>)</bold></th>
<th valign="top" align="center"><bold>D<sub>e</sub> (Gy)</bold></th>
<th valign="top" align="center"><bold>N/OD (%)</bold></th>
<th valign="top" align="center"><bold>Age (year)</bold></th>
<th valign="top" align="center"><bold>&#x003C1;&#x02032;</bold><break/> <bold>(x 10<sup>&#x02212;6</sup>)</bold></th>
<th valign="top" align="center"><bold>Age<sub>fc</sub> (year)</bold></th>
<th valign="top" align="center"><bold>Synthesized age (CE)</bold></th>
</tr>
</thead>
<tbody>
<tr>
<td valign="top" align="left">ABR</td>
<td valign="top" align="left">PM</td>
<td valign="top" align="left">IRSL<sub>50&#x000B0;C; 200&#x000B0;C</sub></td>
<td valign="top" align="center">3.1 &#x000B1; 0.7</td>
<td valign="top" align="center">21.9 &#x000B1; 4.3</td>
<td valign="top" align="center">2.0 &#x000B1; 0.1</td>
<td valign="top" align="center">6.2 &#x000B1; 0.5</td>
<td valign="top" align="center">0.87 &#x000B1; 0.18</td>
<td valign="top" align="center">12/13</td>
<td valign="top" align="center">140 &#x000B1; 30</td>
<td valign="top" align="center">6.6 &#x000B1; 0.2</td>
<td valign="top" align="center">385 &#x000B1; 90</td>
<td valign="top" align="center">Not used</td>
</tr>
<tr>
<td valign="top" align="left" rowspan="5">ABL</td>
<td valign="top" align="left">PM</td>
<td valign="top" align="left">IRSL<sub>50&#x000B0;C; 200&#x000B0;C</sub></td>
<td valign="top" align="center" rowspan="5">3.0 &#x000B1; 0.5</td>
<td valign="top" align="center" rowspan="5">17.8 &#x000B1; 1.3</td>
<td valign="top" align="center" rowspan="5">2.4 &#x000B1; 0.1</td>
<td valign="top" align="center">6.0 &#x000B1; 0.3</td>
<td valign="top" align="center">0.76 &#x000B1; 0.07</td>
<td valign="top" align="center">12/8</td>
<td valign="top" align="center">126 &#x000B1; 10</td>
<td valign="top" align="center">6.0 &#x000B1; 0.2</td>
<td valign="top" align="center">320 &#x000B1; 30</td>
<td valign="top" align="center">Not used</td>
</tr>
<tr>
<td valign="top" align="left" rowspan="3">KF</td>
<td valign="top" align="left">IRSL<sub>50&#x000B0;C; 250&#x000B0;C</sub></td>
<td valign="top" align="center" rowspan="3">4.7 &#x000B1; 0.2</td>
<td valign="top" align="center">0.53 &#x000B1; 0.03</td>
<td valign="top" align="center">10/12</td>
<td valign="top" align="center">114 &#x000B1; 10</td>
<td valign="top" align="center">8.9 &#x000B1; 0.2</td>
<td valign="top" align="center">520 &#x000B1; 40</td>
<td valign="top" align="center">1,456&#x02013;1,522<xref ref-type="table-fn" rid="TN1"><sup>a</sup></xref></td>
</tr>
<tr>
<td valign="top" align="left">IRSL<sub>50&#x000B0;C; 320&#x000B0;C</sub></td>
<td valign="top" align="center">0.96 &#x000B1; 0.03</td>
<td valign="top" align="center">15/8</td>
<td valign="top" align="center">205 &#x000B1; 10</td>
<td valign="top" align="center">6.6 &#x000B1; 0.2</td>
<td valign="top" align="center">590 &#x000B1; 40</td>
<td valign="top" align="center" rowspan="2">1,427&#x02013;1,534<xref ref-type="table-fn" rid="TN2"><sup>b</sup></xref></td>
</tr>
<tr>
<td valign="top" align="left">pIRIRSL<sub>290&#x000B0;C; 320&#x000B0;C</sub></td>
<td valign="top" align="center">1.71 &#x000B1; 0.01</td>
<td valign="top" align="center">15/1</td>
<td valign="top" align="center">360 &#x000B1; 20</td>
<td valign="top" align="center">2.4 &#x000B1; 0.1</td>
<td valign="top" align="center">520 &#x000B1; 20</td>
</tr>
<tr>
<td valign="top" align="left">Qz</td>
<td valign="top" align="left">OSL</td>
<td valign="top" align="center">4.3 &#x000B1; 0.1</td>
<td valign="top" align="center">0.73 &#x000B1; 0.03</td>
<td valign="top" align="center">9/9</td>
<td valign="top" align="center">206 &#x000B1; 10</td>
<td valign="top" align="center">2.2 &#x000B1; 0.3</td>
<td valign="top" align="center">330 &#x000B1; 10</td>
<td valign="top" align="center">Not used</td>
</tr></tbody>
</table>
<table-wrap-foot>
<p>The ages of the coarse quartz and polymineral fine grains were not included in the analysis.</p>
<p>N and OD are the number of aliquots measured and over-dispersion observed in the data.</p>
<p><italic>a</italic>-value = 0.08 &#x000B1; 0.04 (dimensionless); Water content = 5 &#x000B1; 2%; Internal potassium (K<sub>int.</sub>) = 12.5 &#x000B1; 0.5%.</p>
<fn id="TN1"><label>a</label><p>Conventional statistical method (Equations 1, 2).</p></fn>
<fn id="TN2"><label>b</label><p>ChronoModel 2.0 18.</p></fn>
</table-wrap-foot>
</table-wrap>
<p>Quartz was not contaminated by IRSL signals, as inferred from IRpDR values of &#x0003C;2% (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S1</xref>). A D<sub>e</sub>-plateau was observed between the preheating temperatures of 220&#x02013;260&#x000B0;C for coarse quartz grains (<xref ref-type="fig" rid="F4">Figure 4A</xref>), and hence 240&#x000B0;C was selected for further D<sub>e</sub> analyses and age calculation. For the IRSL<sub>50&#x000B0;C</sub> signal of the coarse grain K-feldspar, no D<sub>e</sub>-plateau was observed for the preheat temperature range of 175&#x02013;275&#x000B0;C (<xref ref-type="fig" rid="F4">Figure 4B</xref>). This is contrary to what has been observed by Murray et al. (<xref ref-type="bibr" rid="B35">2009</xref>). However, such an increase with the preheat temperature was observed on polymineral fine grains by Zhang et al. (<xref ref-type="bibr" rid="B52">2015</xref>). For their sample, Zhang et al. also observed a decreasing fading rate with increasing preheat temperature, and consequently, a fading-corrected age plateau was observed in the range of 180&#x02013;320&#x000B0;C. The dose recovery tests using coarse quartz and K-feldspar grains (using IRSL<sub>50&#x000B0;C; 200&#x000B0;C</sub>, pIR IRSL<sub>50&#x000B0;C; 320&#x000B0;C</sub> and pIR IRSL<sub>290&#x000B0;C; 320&#x000B0;C</sub>) recovered the laboratory administered dose (1.2 Gy) within 10% (<xref ref-type="fig" rid="F4">Figure 4C</xref>).</p>
<fig id="F4" position="float">
<label>Figure 4</label>
<caption><p>Preheat plateau test results using coarse grain quartz OSL <bold>(A)</bold> and IRSL of coarse grain K-feldspar <bold>(B)</bold>. The aliquots were not bleached and hence the dose was natural. Each point is the average of three aliquots. <bold>(C)</bold> Dose recovery test results with preheat temperature of 240&#x000B0;C for quartz OSL, 250&#x000B0;C for K-feldspar IRSL<sub>50&#x000B0;C and 320&#x000B0;C</sub> for IRSL<sub>50&#x000B0;C</sub> and pIR IRSL<sub>290&#x000B0;C</sub>.</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fearc-04-1464315-g0004.tif"/>
</fig>
<p>Both the measured ages (Age) and fading corrected ages (Age<sub>fc</sub>) are provided along with the respective fading parameter, &#x003C1;&#x02032; (<xref ref-type="table" rid="T1">Table 1</xref>). The measured dose response curves (DRC) were standardized and given in <xref ref-type="fig" rid="F5">Figure 5A</xref>. The DRC of ABR PM was not shown in this figure, but it was indistinguishable from that of ABL PM. Till around 1.5 Gy, all the signals grow indistinguishably with dose, and both IRSL<sub>50&#x000B0;C; 320&#x000B0;C</sub> and pIR IRSL<sub>290&#x000B0;C; 320&#x000B0;C</sub> from K-feldspar slightly deviates after that dose (<xref ref-type="fig" rid="F5">Figure 5A</xref>). The observed fading rate in both samples was high, particularly for the K-feldspar samples (<xref ref-type="fig" rid="F5">Figure 5B</xref>, <xref ref-type="table" rid="T1">Table 1</xref>). The commonly known fading rate parameter, g-value (directly proportional to &#x003C1;&#x02032;) for t<sub>c</sub> = 1 h (Huntley and Lamothe, <xref ref-type="bibr" rid="B20">2001</xref>) varied from 9.6 &#x000B1; 0.2%&#x000B7;decade<sup>&#x02212;1</sup> (APL PM, IRSL<sub>50&#x000B0;C; 200&#x000B0;C</sub>) to 15.5 &#x000B1; 0.2%&#x000B7;decade<sup>&#x02212;1</sup> (ABL KF, IRSL<sub>50&#x000B0;C; 250&#x000B0;C</sub>) with an intermediate value of 10.4 &#x000B1; 0.2%&#x000B7;decade<sup>&#x02212;1</sup> for ABR PM using IRSL<sub>50&#x000B0;C; 200&#x000B0;C</sub>. Interestingly, the supposedly stable signals such as pIR IRSL<sub>290&#x000B0;C; 320&#x000B0;C</sub> of K-feldspar and OSL of quartz exhibited fading at a rate of 3.4 &#x000B1; 0.2%.decade<sup>&#x02212;1</sup> and 3.1 &#x000B1; 1.3%.decade<sup>&#x02212;1</sup>, respectively. Such high fading rates resulted in fading corrected ages that were more than 2.5 times the measured fine grain polymineral ages (<xref ref-type="supplementary-material" rid="SM2">Supplementary Figures S2A</xref>, <xref ref-type="supplementary-material" rid="SM2">B</xref>, <xref ref-type="supplementary-material" rid="SM3">S3A</xref>, <xref ref-type="supplementary-material" rid="SM3">B</xref>) and &#x0007E;4.5 times the measured age for the coarse grain K-feldspar (<xref ref-type="fig" rid="F6">Figure 6A</xref>, <xref ref-type="table" rid="T1">Table 1</xref>, <xref ref-type="supplementary-material" rid="SM3">Supplementary Figure S3D</xref>). High values of fading rate of IRSL signals both from polymineral and K-feldspar, and fading of otherwise stable quartz OSL signal as if it were a volcanic quartz (Tsukamoto et al., <xref ref-type="bibr" rid="B49">2007</xref>), demand explanation. The pXRD pattern of coarse grain K-feldspar revealed the presence of &#x0007E;46% sanidine in it (<xref ref-type="fig" rid="F7">Figure 7</xref>, <xref ref-type="supplementary-material" rid="SM4">Supplementary Figure S4A</xref>), which is a high temperature and hence disordered K-feldspar phase whose luminescence fades rapidly (Li et al., <xref ref-type="bibr" rid="B30">2016</xref>). However, the pXRD pattern of quartz grains revealed that no presence of &#x003B2;-quartz (phase transition after heating beyond 574.3&#x000B0;C) was observed (<xref ref-type="fig" rid="F7">Figure 7</xref>, <xref ref-type="supplementary-material" rid="SM4">Supplementary Figure S4B</xref>).</p>
<fig id="F5" position="float">
<label>Figure 5</label>
<caption><p><bold>(A)</bold> Dose response curves (standardized) of ABL samples using five signals as indicated. <bold>(B)</bold> Fading rate measurements, and their fitting to the logarithmic function (Huntley and Lamothe, <xref ref-type="bibr" rid="B20">2001</xref>) to calculate the g-value (%&#x000B7;decade<sup>&#x02212;1</sup>), and Huntley function (Huntley, <xref ref-type="bibr" rid="B19">2006</xref>) to calculate &#x003C1;&#x02032;. ABL PM, ABL, KF, and ABL Qz&#x02014;samples from the middle of the river measured using fine-grained polymineral, K-feldspar, and quartz, respectively; ABR PM, samples from the right side of the river measured using fine-grained polymineral.</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fearc-04-1464315-g0005.tif"/>
</fig>
<fig id="F6" position="float">
<label>Figure 6</label>
<caption><p>Fading correction by Huntley (<xref ref-type="bibr" rid="B19">2006</xref>); Kars et al. (<xref ref-type="bibr" rid="B21">2008</xref>) method for coarse K-feldspar grains using <bold>(A)</bold> IRSL<sub>50&#x000B0;C; 250&#x000B0;C</sub>, <bold>(B)</bold> IRSL<sub>50&#x000B0;C; 320&#x000B0;C</sub>, <bold>(C)</bold> pIR IRSL<sub>290&#x000B0;C; 320&#x000B0;C</sub>, and <bold>(D)</bold> coarse quartz grains OSL of ABL. These are the outputs after the method/command of <italic>calc_Huntley2006()</italic> as implemented in <italic>Luminescence</italic> package of R.</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fearc-04-1464315-g0006.tif"/>
</fig>
<fig id="F7" position="float">
<label>Figure 7</label>
<caption><p>XRD spectra measured from quartz and K-feldspar in the ABL sample. The <italic>hkl</italic> planes indicated in black and red numerals indicate the presence of &#x003B1;-quartz and sanidine, respectively. The proportion of &#x003B1;-quartz and sanidine are given in <xref ref-type="supplementary-material" rid="SM4">Supplementary Figures S4A</xref>, <xref ref-type="supplementary-material" rid="SM4">B</xref>.</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fearc-04-1464315-g0007.tif"/>
</fig>
<p>The IRSL signals measured after preheating to 320&#x000B0;C i.e., pIR IRSL<sub>290&#x000B0;C; 320&#x000B0;C</sub> and IRSL<sub>50&#x000B0;C; 320&#x000B0;C</sub> from the K-feldspar grains of ABL yielded fading corrected ages of 520 &#x000B1; 20 years and 590 &#x000B1; 40 years, respectively (<xref ref-type="fig" rid="F6">Figures 6C</xref>, <xref ref-type="fig" rid="F6">B</xref>, <xref ref-type="table" rid="T1">Table 1</xref>). Both these ages are not significantly different from the fading corrected age of IRSL<sub>50&#x000B0;C; 250&#x000B0;C</sub> of ABL KF i.e., 520 &#x000B1; 40 years, and thus validates the fading correction procedure despite large values of fading rate (<xref ref-type="table" rid="T1">Table 1</xref>). As the bricks had been heated with a variable temperature range of 500 to 1,000&#x000B0;C while baking in the kiln (Krishnan and Hegde, <xref ref-type="bibr" rid="B25">1988</xref>), the unbleachable luminescence signal would be near to nil and hence the age using pIR IRSL<sub>290&#x000B0;C; 320&#x000B0;C</sub> might be correct. Thus, the consistency of three corrected ages obtained by different signals (fading corrected ages being 1.4 times, 2.9 times, and 4.5 times the measured age for pIR IRSL<sub>290&#x000B0;C; 320&#x000B0;C</sub>, IRSL<sub>50&#x000B0;C; 320&#x000B0;C</sub> and IRSL<sub>50&#x000B0;C; 250&#x000B0;C</sub>, respectively; <xref ref-type="supplementary-material" rid="SM3">Supplementary Figures S3D</xref>&#x02013;<xref ref-type="supplementary-material" rid="SM3">F</xref>) increases the reliability of the age of ABL.</p>
<p>The ages of both fine grain polymineral (320 &#x000B1; 30 years) and coarse grain quartz (330 &#x000B1; 10 years; <xref ref-type="fig" rid="F6">Figure 6D</xref>, <xref ref-type="table" rid="T1">Table 1</xref>) were significantly younger compared to the coarse grain K-feldspar ages (<xref ref-type="table" rid="T1">Table 1</xref>). A similar age (385 &#x000B1; 90 years) of ABR (using IRSL<sub>50&#x000B0;C; 200&#x000B0;C</sub>) as to that of ABL using both quartz OSL and polymineral fine grain (IRSL<sub>50&#x000B0;C; 200&#x000B0;C</sub>) warrants our attention. There must be a systematic offset that caused underestimation, and that needs to be addressed. Probably the pIR IRSL<sub>290&#x000B0;C; 320&#x000B0;C</sub> measurement on fine grain polymineral samples will help, and it is a future endeavor as there is no sample now left. Regarding quartz age, there is one report where almost 50% underestimation of quartz ages (fine grain) was observed, compared to the polymineral ages, and there is no conclusive reason for this unusual behavior (Peri&#x00107; et al., <xref ref-type="bibr" rid="B40">2021</xref>). In that study, the possible reasons were the thermal and a-thermal (anomalous fading) instability, difference in the natural and laboratory growth curves (Peri&#x00107; et al., <xref ref-type="bibr" rid="B40">2021</xref>). If these ages (of quartz and fine grain polymineral; around 340 years) were correct, then adequate reasons are to be sought to discard the ages of coarse grain K-feldspar of around 540 years, which would be even more difficult. Until further investigation shows the ages of fine grain polymineral and coarse grain quartz are correct, these ages are not included in the final calculation.</p>
<p>So, excluding coarse-grain quartz ages of ABL and both the fine grain polymineral ages of ABL and ABR, all the ages of coarse grain K-feldspar of ABL were synthesized to one age using: a) conventional statistical method (1456&#x02013;1522 CE); and b) ChronoModel (1427&#x02013;1534 CE). These age ranges are within 95% confidence (<xref ref-type="supplementary-material" rid="SM5">Supplementary Figure S5</xref>, <xref ref-type="table" rid="T1">Table 1</xref>). It should be noticed that the assumption of independent ages necessary to apply ChronoModel is not strictly true here since the three ages were calculated with the same dose rate.</p>
<p>Similar ages, however lower due to a systematic error in the D<sub>e</sub> measurement protocol, for the bricks collected from the structures found both at the right side (ABR; 385 &#x000B1; 90 years) and the middle of the river (ABL; 320 &#x000B1; 30 years) using fine grain polymineral (fading corrected), suggest that both the structures were most probably contemporaneous. This, in turn, implies that these two structures were constructed at the same time, thereby excluding the possibility of reworking by rivers from elsewhere. The similar geochemical composition (<xref ref-type="table" rid="T2">Table 2</xref>, <xref ref-type="fig" rid="F8">Figure 8</xref>) of the bricks from both locations further supports the inference that these structures were not reworked from elsewhere but were likely parts of a single structure. Had both the bricks (ABL and ABR) been made from different places and came to the present location by reworking, the geochemical compositions of the mud most probably would be different unless they were brought from shorter distance. Thus, the contemporaneity of the studied two bricks and their similar geochemical composition and moderately weathered nature of the constituting mud suggest these bricks are part of a single structure.</p>
<table-wrap position="float" id="T2">
<label>Table 2</label>
<caption><p>Weight percentage of major oxides measured from XRF are tabulated.</p></caption>
<table frame="box" rules="all">
<thead>
<tr style="background-color:#919498;color:#ffffff">
<th valign="top" align="left"><bold>Sample</bold></th>
<th valign="top" align="center"><bold>SiO<sub>2</sub></bold></th>
<th valign="top" align="center"><bold>Al<sub>2</sub>O<sub>3</sub></bold></th>
<th valign="top" align="center"><bold>Fe<sub>2</sub>O<sub>3</sub></bold></th>
<th valign="top" align="center"><bold>TiO<sub>2</sub></bold></th>
<th valign="top" align="center"><bold>Na<sub>2</sub>O</bold></th>
<th valign="top" align="center"><bold>K<sub>2</sub>O</bold></th>
<th valign="top" align="center"><bold>CaO</bold></th>
<th valign="top" align="center"><bold>MgO</bold></th>
<th valign="top" align="center"><bold>MnO</bold></th>
<th valign="top" align="center"><bold>P<sub>2</sub>O<sub>5</sub></bold></th>
</tr>
</thead>
<tbody>
<tr>
<td valign="top" align="left">ABL</td>
<td valign="top" align="center">64.5</td>
<td valign="top" align="center">21.6</td>
<td valign="top" align="center">3.5</td>
<td valign="top" align="center">0.78</td>
<td valign="top" align="center">2.4</td>
<td valign="top" align="center">2.5</td>
<td valign="top" align="center">2.4</td>
<td valign="top" align="center">1.5</td>
<td valign="top" align="center">0.043</td>
<td valign="top" align="center">0.16</td>
</tr>
<tr>
<td valign="top" align="left">ABR</td>
<td valign="top" align="center">62.9</td>
<td valign="top" align="center">21.0</td>
<td valign="top" align="center">4.6</td>
<td valign="top" align="center">0.96</td>
<td valign="top" align="center">2.0</td>
<td valign="top" align="center">2.7</td>
<td valign="top" align="center">3.4</td>
<td valign="top" align="center">1.5</td>
<td valign="top" align="center">0.096</td>
<td valign="top" align="center">0.17</td>
</tr></tbody>
</table>
</table-wrap>
<fig id="F8" position="float">
<label>Figure 8</label>
<caption><p>Concentration of major oxides (in wt%) from samples from both the middle of the river and the right side of the river.</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fearc-04-1464315-g0008.tif"/>
</fig>
</sec>
</sec>
<sec id="s4">
<title>4 Discussion</title>
<p>The round off synthesized age estimate (1430&#x02013;1530 CE) situates the structure historically within the Vijayanagar Empire in Tamil Nadu. Although Harihara and Bukka established Vijayanagar Empire in Madurai with the help of their General Kampanna by defeating Madurai Sultanate by the year 1378 CE, the Late Pandyas had some hold in the Tirunelveli region (the study region). They (Late Pandyas) were not fighting with the Vijayanagar Empire but having peace treaties during this time. One of the Late Pandya kings, named Parakrama, renovated the central shrine and the mandapas of a temple in Kutralam of Tirunelveli region by 1387 CE (Nilakanta Sastri, <xref ref-type="bibr" rid="B38">1929</xref>). In another instance, another king named Jatavarman Kulasekhara claimed to have rebuilt a temple at Ilanji of Tirunelveli region and founded a new Brahmin village during 1395&#x02013;1396 CE (Nilakanta Sastri, <xref ref-type="bibr" rid="B38">1929</xref>). Although not many records are available for other Late Pandyan kings, there are copper plates showing that they ruled this region till before 1675 CE (Nilakanta Sastri, <xref ref-type="bibr" rid="B38">1929</xref>). Based on our results and the above records, we can be sure that the brick structure of this study might have been made by the Late Pandyas. Despite discrepancies between the quartz, polymineral, and K-feldspar ages, the chronological constraints provided by this study are sufficient to reject the hypothesis that this structure dates back to the Early Pandyas (400 BCE&#x02212;300 CE).</p>
</sec>
<sec id="s5">
<title>5 Summary</title>
<p>Although the exposed brick structure in the middle of Thamirabarani River turned out not to be of Early Pandyas based on multiple luminescence ages of coarse K-feldspar grain from the bricks, the ages using quartz and fine grain polymineral are poorly understood, and it calls for further investigation. However, a consistent and precise set of ages (1430&#x02013;1530 CE) from coarse grain K-feldspar from the bricks attribute the structure to Late Pandyas who were involved in constructions during Vijayanagar Empire in southern India, even after the decline of the Pandyas since 1335 CE. With the evidence we have, it is difficult to discern whether the structure is a ruined palace, temple, bridge, irrigation check dam, or bathing steps. Further, the actual dimension, lateral connectivity, and extension of these structures need to be investigated through the subsurface geophysical surveys, which will help us to know whether it was built across the river or outside of the course of river in the past.</p>
</sec>
</body>
<back>
<sec sec-type="data-availability" id="s6">
<title>Data availability statement</title>
<p>The original contributions presented in the study are included in the article/<xref ref-type="sec" rid="s11">Supplementary material</xref>, further inquiries can be directed to the corresponding author.</p>
</sec>
<sec sec-type="ethics-statement" id="s7">
<title>Ethics statement</title>
<p>Written informed consent was obtained from the individual(s) for the publication of any potentially identifiable images or data included in this article.</p>
</sec>
<sec sec-type="author-contributions" id="s8">
<title>Author contributions</title>
<p>PM: Conceptualization, Data curation, Formal analysis, Methodology, Project administration, Resources, Supervision, Writing &#x02013; original draft. MS: Data curation, Formal analysis, Writing &#x02013; review &#x00026; editing. SKS: Data curation, Formal analysis, Visualization, Writing &#x02013; review &#x00026; editing. SS: Resources, Writing &#x02013; review &#x00026; editing. MK: Resources, Writing &#x02013; review &#x00026; editing. PS: Data curation, Formal analysis, Writing &#x02013; review &#x00026; editing. NC: Data curation, Supervision, Writing &#x02013; review &#x00026; editing. KK: Data curation, Methodology, Writing &#x02013; review &#x00026; editing. SN: Visualization, Writing &#x02013; review &#x00026; editing. NK: Methodology, Writing &#x02013; review &#x00026; editing.</p>
</sec>
<sec sec-type="funding-information" id="s9">
<title>Funding</title>
<p>The author(s) declare that no financial support was received for the research, authorship, and/or publication of this article.</p>
</sec>
<ack><p>We thank the Director of Birbal Sahni Institute of Palaeosciences for approving this project (BSIP/PROJECTS/2019/L-2478 dated 29.03.2019), its execution and publication (BSIP/RDCC/Publication no. 29/2024-25). We thank Mr. Ishwar Shukla and Dr. Amrit Pal Chadda for their assistance with luminescence sample preparation, measurements, and X-ray fluorescence measurements. We thank Mr. Shubhajit Ghosh and Ms. Prachita Arora for their help in making better visualization. We sincerely thank the reviewers for their comments and suggestions that improved the content and readability of this manuscript.</p>
</ack>
<sec sec-type="COI-statement" id="conf1">
<title>Conflict of interest</title>
<p>The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
<sec sec-type="disclaimer" id="s10">
<title>Publisher&#x00027;s note</title>
<p>All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.</p>
</sec>
<sec sec-type="supplementary-material" id="s11">
<title>Supplementary material</title>
<p>The Supplementary Material for this article can be found online at: <ext-link ext-link-type="uri" xlink:href="https://www.frontiersin.org/articles/10.3389/fearc.2025.1464315/full#supplementary-material">https://www.frontiersin.org/articles/10.3389/fearc.2025.1464315/full#supplementary-material</ext-link></p>
<supplementary-material xlink:href="Image_1.jpeg" id="SM1" mimetype="image/jpeg" xmlns:xlink="http://www.w3.org/1999/xlink">
<label>SUPPLEMENTARY FIGURE S1</label>
<caption><p>OSL with IRSL and OSL without IRSL, and the IRSL itself are plotted for one aliquot of ABL coarse quartz grain for a dose of 0.9 Gy.</p></caption> </supplementary-material>
<supplementary-material xlink:href="Image_2.jpg" id="SM2" mimetype="image/jpeg" xmlns:xlink="http://www.w3.org/1999/xlink">
<label>SUPPLEMENTARY FIGURE S2</label>
<caption><p>Fading correction by Huntley (<xref ref-type="bibr" rid="B19">2006</xref>) and Kars et al. (<xref ref-type="bibr" rid="B21">2008</xref>) method for the fine grain polymineral of both ABL <bold>(A)</bold> and ABR <bold>(B)</bold>.</p></caption> </supplementary-material>
<supplementary-material xlink:href="Image_3.jpeg" id="SM3" mimetype="image/jpeg" xmlns:xlink="http://www.w3.org/1999/xlink">
<label>SUPPLEMENTARY FIGURE S3</label>
<caption><p>Radial plots showing the measured (black points) and fading corrected (red points) ages of <bold>(A)</bold> ABR PM, <bold>(B)</bold> ABL PM, <bold>(C)</bold> ABL Quartz and, IRSL<sub>50&#x000B0;C; 250&#x000B0;C</sub> <bold>(D)</bold>, IRSL<sub>50&#x000B0;C; 320&#x000B0;C</sub> <bold>(E)</bold> and pIR IRSL<sub>290&#x000B0;C; 320&#x000B0;C</sub> <bold>(F)</bold> signals measured from K-feldspar of ABL .</p></caption> </supplementary-material>
<supplementary-material xlink:href="Image_4.jpg" id="SM4" mimetype="image/jpeg" xmlns:xlink="http://www.w3.org/1999/xlink">
<label>SUPPLEMENTARY FIGURE S4</label>
<caption><p>Quantification of the mineralogical composition as measured from the XRD spectra of <bold>(A)</bold> K-feldspar and <bold>(B)</bold> quartz. Quantification was done by Match software (Match! - Phase Analysis using Powder Diffraction, Crystal Impact - Dr. H. Putz &#x00026; Dr. K. Brandenburg GbR, Kreuzherrenstr. 102, 53227 Bonn, Germany, <ext-link ext-link-type="uri" xlink:href="https://www.crystalimpact.de/match">https://www.crystalimpact.de/match</ext-link>.).</p></caption> </supplementary-material>
<supplementary-material xlink:href="Image_5.jpeg" id="SM5" mimetype="image/jpeg" xmlns:xlink="http://www.w3.org/1999/xlink">
<label>SUPPLEMENTARY FIGURE S5</label>
<caption><p>Synthesis of three age estimates of coarse grain K-feldspar of ABL using three distinctive IRSL signals. The synthesized age estimate is shown at the top, and the bottom three ages were the inputs.</p></caption> </supplementary-material>
<supplementary-material xlink:href="Table_1.docx" id="SM6" mimetype="application/vnd.openxmlformats-officedocument.wordprocessingml.document" xmlns:xlink="http://www.w3.org/1999/xlink">
<label>SUPPLEMENTARY Table S1</label>
<caption><p>Alpha, beta, gamma, and internal dose rates are given. The cosmic ray dose rate was 0.21 &#x000B1; 0.02 Gy/ka.</p></caption> </supplementary-material>
</sec>
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