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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ESSD</journal-id><journal-title-group>
    <journal-title>Earth System Science Data</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ESSD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Earth Syst. Sci. Data</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1866-3516</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/essd-18-4677-2026</article-id><title-group><article-title>Earthquake catalog and continuous waveforms from a two-week distributed acoustic sensing experiment on Kefalonia Island, Greece</article-title><alt-title>Earthquake catalog and DAS waveforms from Kefalonia Island</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Bocchini</surname><given-names>Gian Maria</given-names></name>
          <email>gian.bocchini@rub.de</email>
        <ext-link>https://orcid.org/0000-0001-9265-7859</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Bozzi</surname><given-names>Emanuele</given-names></name>
          
        <ext-link>https://orcid.org/0009-0002-6570-9013</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Roth</surname><given-names>Marco P.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-7640-3437</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Gaviano</surname><given-names>Sonja</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Pascucci</surname><given-names>Giulio</given-names></name>
          
        <ext-link>https://orcid.org/0009-0008-3723-9003</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Grigoli</surname><given-names>Francesco</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2858-9756</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Biondi</surname><given-names>Ettore</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3305-0982</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Sokos</surname><given-names>Efthimios</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7742-7251</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Harrington</surname><given-names>Rebecca M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3538-8020</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Institute of Geosciences, Ruhr University Bochum, Bochum, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Earth Sciences, University of Pisa, Pisa, Italy</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Seismix srl, Palermo, Italy</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Geophysics Department, Stanford University, 397 Panama Mall, Stanford, CA 94305, USA</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Geology, Seismological Laboratory, University of Patras, Patras, Greece</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Gian Maria Bocchini (gian.bocchini@rub.de)</corresp></author-notes><pub-date><day>6</day><month>July</month><year>2026</year></pub-date>
      
      <volume>18</volume>
      <issue>7</issue>
      <fpage>4677</fpage><lpage>4695</lpage>
      <history>
        <date date-type="received"><day>19</day><month>November</month><year>2025</year></date>
           <date date-type="rev-request"><day>13</day><month>January</month><year>2026</year></date>
           <date date-type="rev-recd"><day>2</day><month>June</month><year>2026</year></date>
           <date date-type="accepted"><day>22</day><month>June</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Gian Maria Bocchini et al.</copyright-statement>
        <copyright-year>2026</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026.html">This article is available from https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026.html</self-uri><self-uri xlink:href="https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026.pdf">The full text article is available as a PDF file from https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e181">In this work, we present a new, high-resolution earthquake catalog for the Kefalonia region, Greece, together with the distributed acoustic sensing (DAS) waveform dataset used for its construction (<ext-link xlink:href="https://doi.org/10.60517/cv43p1601" ext-link-type="DOI">10.60517/cv43p1601</ext-link>, Bocchini et al., 2025; <ext-link xlink:href="https://doi.org/10.5281/zenodo.20558686" ext-link-type="DOI">10.5281/zenodo.20558686</ext-link>, Bocchini, 2026). We build the catalog from DAS data recorded between 1 August 2024, 23:00 UTC and 15 August 2024, 23:00 UTC, combined with open-access seismic-station recordings from the Hellenic Unified Seismic Network (HUSN). The DAS dataset consists of continuous strain measurements acquired along a 15 km long telecommunications fiber-optic cable connecting northern Kefalonia and Ithaki. We use a semblance-based detector on the DAS waveforms to identify 5734 earthquakes within <inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> km of the cable origin. We jointly locate 356 high-SNR (SNR <inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula> dB) events with DAS and seismic stations and calculate their local magnitudes from seismic records. We then apply waveform cross-correlation to match unlocated detections with the most similar template events and estimate relative magnitudes from amplitude ratios to enhance the newly constructed catalog. Enhancement adds 2515 earthquakes, resulting in 2871 events with assigned locations and magnitudes and represents a <inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">32</mml:mn></mml:mrow></mml:math></inline-formula>-fold increase in the number of earthquakes with respect to the official National Observatory of Athens (NOA) catalog. Most events (2790) cluster within a <inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km radius offshore northwest of Kefalonia, where seismicity rates reach <inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> events per hour. We achieve a <inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">38</mml:mn></mml:mrow></mml:math></inline-formula>-fold increase in the number of earthquakes with respect to the official catalog from NOA in the region encompassing the earthquake cluster northwest of Kefalonia. Our dataset provides a detailed spatio-temporal view of seismicity in a region with limited station coverage and demonstrates the value of integrating DAS with conventional seismic networks to monitor intense earthquake sequences. The combination of high seismicity and open-access data from the HUSN makes this DAS dataset particularly valuable for the seismological community. We provide a 2-week-long catalog, the full detection list (local and distant events and false detections), and two weeks of continuous DAS recordings. Possible applications of the datasets include testing and benchmarking DAS processing algorithms for tectonic earthquakes, as well as studies of physical processes associated with complex seismic sequences.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
<sec id="Ch1.S1.SS1">
  <label>1.1</label><title>Why a new open-access dataset of DAS records?</title>
      <p id="d2e267">Distributed acoustic sensing (DAS) has become an increasingly innovative approach in seismology to enable effective continuous spatiotemporal sampling of the recorded seismic wavefield through strain or strain-rate measurements on fiber-optic cables (Zhan, 2020). The dense sampling has proven particularly well suited for applications that include seismic and microseismic monitoring (Glubokovskikh et al., 2023; Lellouch et al., 2021; Lindsey et al., 2017; Lior et al., 2021a; Porras et al., 2024), seismic imaging (Biondi et al., 2023a; Zeng et al., 2017), earthquake source-parameter estimation (Li et al., 2023; Lior et al., 2021b), and monitoring of volcanic activity (Currenti et al., 2023; Jousset et al., 2022; Li et al., 2025), among others. Nevertheless, despite its rapid adoption, several factors still limit the broader exploitation of DAS data. The high sampling rates and density of measurement points generate large data volumes that challenge effective data storage and sharing (Seguí et al., 2025). Moreover, because DAS technology is still relatively new in seismology, many aspects of data processing and interpretation remain under active development, including seismic event detection and location, signal enhancement, strain-to-ground-motion calibration, and earthquake source parameter analysis. A further limitation is that most large publicly available DAS datasets are mainly related to microseismic monitoring of industrial operations (e.g., hydraulic stimulations) rather than natural seismicity, as technology evolved from industry. While several open-access datasets dedicated to the monitoring of natural earthquakes are present, they often lack elevated seismicity rates and/or data from permanent seismic networks to augment the DAS experiment. The capability of using publicly available DAS datasets for the analysis of highly productive seismic sequences remains limited, slowing the validation and generalization of emerging data analysis methods across different tectonic contexts. Among the DAS datasets now publicly available (as of September 2025), PubDAS provides a repository with data from a variety of experiments, including natural and induced seismicity (Spica et al., 2023). The collection spans urban noise monitoring, volcanic environments, underground mines, and teleseismic events (Spica et al., 2023). FORGE (Frontier Observatory for Research in Geothermal Energy) (Pankow, 2022) and PoroTomo (Feigl et al., 2016) offer DAS data closely tied to geothermal research, including microseismicity monitoring related to hydraulic stimulation operations and subsurface characterization. Greenland Calving-Front Dataset offers a demonstration of the DAS and DTS potential in cryospheric research (Gräff et al., 2025). The Global DAS Month of February 2023 dataset (Wuestefeld et al., 2024) comprises globally coordinated DAS recordings acquired to advance efforts toward a Global Fiber Sensing Network and promote standardized, collaborative seismic monitoring.</p>
      <p id="d2e270">Here we present a new dataset of DAS recordings that captured a period of high seismic activity near the Kefalonia Transform Fault (KTF) in Greece (Fig. 1). The main seismic sequence occurred northwest of Kefalonia at an epicentral distance of <inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> km from the interrogated fiber-optic cable. Additional regional earthquakes   were also recorded during the acquistion period. In addition, we complement the data from seven open-access permanent seismic stations of the Hellenic Unified Seismic Network (HUSN) that are located within <inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> km of the cable's starting point to enhance the analysis. The integration of DAS and seismic station data enables the construction of an enhanced seismicity catalog in a natural tectonic setting, where such joint analysis remains relatively unexplored.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e295"><bold>(a)</bold> Map view of the study region, including the location of the fiber-optic cable, seismic events (colored circles) reported by NOA, and the publicly available seismic stations from the HUSN used (colored triangles) to locate seismic events. Grey triangles indicate public seismic stations from the HUSN not used in this study because they are too distant from the most seismically active region (pink box) or provide azimuthal coverage similar to that of closer seismic stations. Thick brown lines indicate major active faults (Basili et al., 2024). <bold>(b)</bold> Inset showing the location of the study region within the Central-Eastern Mediterranean Sea. <bold>(c)</bold> Zoom on the fiber-optic cable. The fiber-optic cable is divided into 12 segments (see methods) that are used for earthquake location. Continuous black lines indicate isobaths. Black circles along the cable indicated the position of channels (ch.) mentioned in the text.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026-f01.jpg"/>

        </fig>

      <p id="d2e313">This study releases two main products: (i) a high-resolution earthquake catalog covering a two-week period of elevated seismicity within <inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> km of the start of the interrogated fiber-optic cable, and (ii) the continuous DAS waveform dataset from which we derived the catalog. In the following, we describe the methodological workflow we use to integrate DAS and seismic station data for catalog construction. We also provide additional supporting products, including a comprehensive detection list and cable geometry metadata.</p>
      <p id="d2e326">The datasets presented here may support further research in DAS-based earthquake detection and processing, integration of DAS and seismic-station data, as well as studies in earthquake physics and statistical seismology, with potential benefits from the analysis of DAS data.</p>
</sec>
<sec id="Ch1.S1.SS2">
  <label>1.2</label><title>The Kefalonia Transform Fault and the 2024 seismic sequence</title>
      <p id="d2e337">The KTF is a major tectonic structure in the Eastern Mediterranean that marks the transition from oceanic subduction to the south to continental collision to the north (Bocchini et al., 2018; Louvari et al., 1999; Royden and Papanikolaou, 2011; Scordilis et al., 1985). The KTF accommodates 2–2.5 cm yr<sup>−1</sup> of differential convergence between the oceanic subduction and continental collision zones (Pérouse et al., 2012), making it one of the most seismically active faults in Europe, as evidenced by frequent M6–7<inline-formula><mml:math id="M11" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> earthquakes (Papadimitriou, 2002). A period of increased seismic activity started offshore northwest of Kefalonia at the end of February 2024 and lasted until the end of the year. The largest magnitude earthquakes (local magnitude, <inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, 3.6–3.8) occurred in the first weeks of March 2024, and earthquakes with <inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">3.0</mml:mn></mml:mrow></mml:math></inline-formula> were also recorded in April, August, and October  and are listed in the revised catalog of the National Observatory of Athens (NOA) (<uri>https://bbnet.gein.noa.gr/HL/databases/database</uri>, last access: 20 September 2025). Anagnostou et al. (2025) analyzed the seismic activity from February to April 2024, interpreting it as a complex, swarm-like sequence for which fluid dynamics played a primary role in its triggering. Notably, the authors report that the primary structure(s) that were activated include WNW-ESE left-lateral strike-slip fault(s), rather than the main branch of the KTF.</p>
</sec>
<sec id="Ch1.S1.SS3">
  <label>1.3</label><title>Description of the DAS experiment in Kefalonia</title>
      <p id="d2e396">We used DAS to measure strain along a dark telecommunications fiber-optic cable connecting the islands of Kefalonia and Ithaki, in the Ionian Sea (Greece) (Fig. 1). The cable starts in the village of Antipata (Kefalonia), runs inland for slightly more than half of its <inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> km length, crosses the Strait of Ithaki over steep bathymetry, and terminates in the village of Stavros (Ithaki) (Fig. 1). The DAS measurement period ranges from early July to late September 2024, where we recorded continuous data using an OptaSense QuantX interrogator. This study focuses on the analysis of a two-week period that captures the highest activity within the earthquake cluster northwest of Kefalonia and the broader Kefalonia region (Fig. 1). Using the revised seismicity catalog from NOA as a basis for selection, we identify the study period as spanning 2–15 August 2024 (1 August 23:00 UTC–15 August 23:00 UTC) as well-suited to construct an enhanced earthquake catalog. We combine DAS strain recordings with continuous recordings of ground velocity from seven seismic stations of the HUSN to mitigate the azimuthal gap caused by the relatively short cable length, which is comparable to the epicentral distance between the cable and the recorded seismicity, and obtain higher quality earthquake locations than would be possible with DAS or seismic data alone. The complementary seismic data also enables more accurate magnitude estimations, which are hindered by the lack of a calibrated instrument response for converting strain to displacement (Lior et al., 2021b). In other words, complementing DAS with seismic station data enables building a high-quality, earthquake catalog during the two-week study period.</p>
</sec>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data</title>
      <p id="d2e418">We recorded DAS data with a temporal sampling rate (i.e., ping rate) of 5000 Hz, which we decimated by a factor of 20 before storing them, yielding a sampling rate of 250 Hz. The system configuration has a gauge length of 10.2 m and a channel spacing of 2.04 m, resulting in a total of 7750 channels. Data is saved in 30 s segments (<inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">80</mml:mn></mml:mrow></mml:math></inline-formula> MB per file), resulting in a total size of 3.04 TB for the two-week experiment, with a short gap in data archiving occurring between 09:14 and 09:48 on  6 August 2024. The file name is UTC time <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> h (default naming from the system).</p>
      <p id="d2e441">We performed tap tests on both Kefalonia and Ithaki islands to precisely identify the channel locations onshore. The cable onshore was visible along the entire length because it had been covered by asphalt along streets. Offshore, the cable path and channel positions are less certain. To reconstruct the offshore cable geometry and channel locations, we rely on the expected number of offshore channels (after subtracting those onshore) and refine the cable path by aligning the trend of the picked DAS P-wave arrival times with the earthquake-to-channel epicentral distances (using earthquake locations from NOA) (Fig. S1 in the Supplement). Automatic picking of P-wave arrivals along the cable result from applying PhaseNet-DAS (Zhu et al., 2023). We employ EMODnet bathymetry (<uri>https://emodnet.ec.europa.eu/en/</uri>, last access: 15 March 2025) to assign an elevation to the channels offshore, while for the onshore channels, we rely on the elevation from our GPS device. We also check for loops (typical of telecom infrastructure) in the onshore cable sections by analyzing the normalized energy recorded on each channel (Biondi et al., 2023b), and then cross-validate it with vehicle signals generated while driving along the cable (Fig. S2). We show the locations of identified loops in Fig. 2 (gray areas between dashed vertical lines).</p>

      <fig id="F2"><label>Figure 2</label><caption><p id="d2e449">Example of earthquakes recorded along the cable. <bold>(a)</bold> <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 0.6 on 8 August 2024 at 10:35 UTC (NOA event-id: noa2024pmvwc). <bold>(b)</bold> <inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 3.0 Earthquake on 8 August 2024 at 19:18 UTC (NOA event-id: noa2024pnndk). <bold>(c)</bold> Maximum absolute amplitudes of signal and noise shown in panels <bold>(a)</bold>–<bold>(b)</bold>. <bold>(c)</bold> Horizontal dashed black and purple lines indicate average amplitudes for events displayed in panel <bold>(a)</bold> and <bold>(b)</bold>, respectively. The length of the horizontal lines shows the range of channels used for calculating the average amplitudes (4000–5900). Panels <bold>(a)</bold>–<bold>(b)</bold> detail the location of onshore and offshore channels, the location of the channels used for the detection, and the location of the identified loops. Traces are band-pass filtered 3–20 Hz. The light and dark orange, and violet and blue lines in panels <bold>(a)</bold>–<bold>(b)</bold> highlight the noise and signal windows shown in panel <bold>(c)</bold>.</p></caption>
        <graphic xlink:href="https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026-f02.jpg"/>

      </fig>

      <p id="d2e522">We perform an initial assessment of data quality by manually inspecting recordings of earthquakes within a <inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> km radius of the cable starting point using the revised NOA catalog (<inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 0.5–3.4). The catalog lists 91 earthquakes  within the two-week study period, all of which are clearly visible along the cable (Figs. 2, S3). Earthquake recordings show strong amplification (a factor <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula>–20) in the offshore segment, while onshore and offshore maximum noise amplitudes are similar, with slightly higher noise amplitudes offshore (Fig. 2). We observe amplitude scaling with earthquake magnitude that is consistent with theoretical expectations. For example, we obtain an amplitude ratio of <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">148</mml:mn></mml:mrow></mml:math></inline-formula> between an <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 0.6 and <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 3.0 event separated by <inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.7</mml:mn></mml:mrow></mml:math></inline-formula> km (epicentral locations from the NOA catalog), as shown in Fig. 2c. We compute the amplitude for each event as a trimmed mean after excluding the upper and lower 10 % of values to reduce the influence of outliers. We band-pass filter the waveforms between 3–20 Hz and use channels 4000–5900. Assuming a theoretical scaling of <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>M</mml:mi></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>M</mml:mi></mml:mrow></mml:math></inline-formula> is the magnitude difference between the two events, the observed amplitude ratio corresponds to an implied <inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>M</mml:mi><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">2.17</mml:mn></mml:mrow></mml:math></inline-formula>. This value is slightly lower than the idealized expectation for perfectly co-located events and may reflect the minor differences in source location and measurement uncertainties. We note that magnitude estimate of the <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 0.6 event in the NOA catalog is based on two station observations. We also observe consistently elevated amplitudes at both the onshore–offshore transition zones of the cable (Fig. 2). In addition, we successfully record signals from teleseismic earthquakes, predominantly on the offshore portion of the cable (Fig. S4).</p>
      <p id="d2e648">The seven seismic stations of the HUSN that complement the DAS data include: FSK (University of Patras, 2000), ATHR (University of Athens, 2008), VLS (National Observatory of Athens, Institute of Geodynamics, 1975), EVGI, DLMN, ITHC, DRAG (Aristotle University of Thessaloniki, 1981) (Figs. 1, S3).</p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Earthquake detection using DAS data</title>
      <p id="d2e659">We use a semblance-based earthquake detector, HECTOR, to detect earthquakes recorded along the fiber-optic cable (Porras et al., 2024). The detector evaluates the coherence of the waveforms along pre-computed hyperbolic trajectories with varying curvature and vertex along the cable and time axes (<inline-formula><mml:math id="M30" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M31" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>) using a modified semblance function (Fig. 3). The run of the detector requires a set of pre-processing steps that include: (1) removing the mean and linear trend of each trace; (2) normalizing trace amplitudes to reduce the effect of geometrical spreading, cable coupling, and nonlinear effects; (3) applying a band-pass filter of 5–30 Hz as well as a (4) common mode noise removal via a frequency–wavenumber (fk) filter by removing the zero-wavenumber (<inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>) component, which corresponds to coherent signals that arrive simultaneously across all DAS channels without exhibiting any phase delay.</p>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e690"><bold>(a)</bold> Coherence time series in a 45 s window showing six detections. Vertical dashed black lines mark detection times. Violet vertical dashed line (second from the right) indicates a detection identified in the subsequent window (30–75 s) and not in the time window shown here (see text). <bold>(b)</bold> Semblance matrix, where the coherence maxima highlight events detected by HECTOR (Porras et al., 2024). <bold>(c)</bold> DAS recording with <inline-formula><mml:math id="M33" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>-axis channels ranging from 4000 (bottom) to 5900 (top). See text for details of trace processing (Sect. 3). Note that detection times may mark the S-wave arrival, where P-waves are not always clearly visible.</p></caption>
        <graphic xlink:href="https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026-f03.jpg"/>

      </fig>

      <p id="d2e714">Owing to the strong signal amplification offshore and the clearer hyperbolic seismic phase arrival moveout, we perform  detection using an offshore segment of the cable (Fig. 2). Testing different configurations led us to use channels 4000–5900 for detection (Figs. 1c, 2), corresponding to a total length of <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3900</mml:mn></mml:mrow></mml:math></inline-formula> m. Since the target seismicity cluster northwest of Kefalonia lies beyond the cable's extent, we fix the hyperbola vertex at channel 4000 (bottom Fig. 3c). We let the curvature of the hyperbola vary between 130–200° with steps of 5° and use temporal windows of 30 samples with steps of 10 samples to calculate the semblance and evaluate the coherence of the signals. We run the detection algorithm on 45 s data windows with a 15 s overlap (Fig. 3). The overlap ensures that potential earthquakes that might occur across two consecutive files are not missed. To eliminate duplicate entries, we de-cluster the initial detection list by removing signals that occur within 3 s of each other, retaining only the earliest detection. We choose this 3 s threshold specifically to account for the detector's inability to distinguish between P- and S-wave arrivals, which would otherwise register as separate events. Because the observed <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>  times, where <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> denote S- and P-wave arrival times, along along the offshore channels do not exceed <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2.5</mml:mn></mml:mrow></mml:math></inline-formula> s for earthquakes within cluster northwest of Kefalonia (Fig. 2a–b), a 3 s window safely merges these phases into a single event identification for most detections. The 15 s overlap between consecutive windows may also cause the same event to be detected twice, which we also mitigate with the de-clustering. We note that detection time (Fig. 3a) may be shifted with respect to the phase arrival observed in Fig. 3c because the vertex and the curvature of the hyperbola provide the highest signal coherence, which may not  perfectly correspond with the earliest time of the phase arrival.</p>
      <p id="d2e783">Running the HECTOR detection algorithm on the 2 weeks of data leads to a total of 6817 detections (Fig. 4). The number of detections increases substantially relative to the revised NOA catalog, with the highest counts occurring after <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M41" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> earthquakes listed in that catalog (Fig. 4). The number of detections within 1 h bins following <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M43" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> events from the NOA catalog exceeds 100 and exhibits an Omori-like decay (Fig. 4). We note that all <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M45" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NOA earthquakes reported in Fig. 4 occurred within the active cluster northwest of Kefalonia (pink box in Fig. 1). Importantly, although we calibrate the detector parameters to maximize sensitivity to the region of elevated seismicity offshore northwest of Kefalonia Island, we successfully detect all 91 earthquakes reported in the NOA catalog that occurred within <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> km of the cable's starting point (Fig. 1). The sensitivity to various azimuthal directions, distances, and magnitudes suggests that the set of parameters, DAS channels, and waveform processing used in the detector (as applied in this study) offer sufficient flexibility.</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e853">Histogram of detections in 1 h bins obtained with HECTOR from 1 August 2024 at 23:00 to 15 August 2024 at 23:00. Detections are classified after manual inspection of the signals. Distant earthquakes represent signals with <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula> s, where all 91 earthquakes from the revised NOA catalog within <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> km of the cable starting point (Fig. 1b) are included in the histogram. Vertical lines indicate <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M51" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> earthquakes from the revised NOA catalog.</p></caption>
        <graphic xlink:href="https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026-f04.png"/>

      </fig>

      <p id="d2e918">We manually inspect all detections and classify them into three groups based on their manually determined <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>S</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values and arrival moveout: (i) local earthquakes (Figs. 4, 5a–b), (ii) distant earthquakes (with <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>S</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula> s) (Figs. 4, 5c), and (iii) false detections (Figs. 4, 5d–e). Local earthquakes (5734) include events within <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> km of the start of the cable and are identified by coherent signals along the nodes that commonly have clearly visible P- and/or S-wave arrivals (Fig. 5a–b). Smaller-amplitude earthquakes are recognizable primarily from characteristic reverberations between channels 5000–5500 in the submarine section of the cable (Fig. 5b). We inspect some of the weaker amplitude earthquakes with a spectral over-subtraction denoiser (Pascucci et al., 2026) to confirm that the signals correspond to real seismic events (Fig. S4). False detections (684) include non-seismic signals (e.g., boat noise; Fig. 5d), triggers within the coda of larger events where P- and S-wave arrivals are absent or unclear (Fig. 5e), and duplicate entries. In the case of duplicate detections, we retain the earliest detection (typically the P-wave arrival) and classify the latter detection as false. For example, we retain the P-wave arrival in Fig. 5c as the detection of the distant event, while the S-wave arrival is rejected as a false detection. We obtain a false detection rate of approximately 6 % (399 out of 6817 detections), which we consider a conservative overestimate. This is because some cases classified as false detections correspond to S-wave arrivals for which the associated P-wave is also detected, but the S-wave was not automatically removed during the 3 s de-clustering process. Manual inspection of signals also reveals  missed events, particularly during the most active periods (i.e., after 8 August, Fig. S6).</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e983">Typical examples of detected signals. <bold>(a)</bold> <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 1.2 earthquake, <bold>(b)</bold> <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 0.3 earthquake, <bold>(c)</bold> distant earthquake, <bold>(d)</bold> false detection, <bold>(e)</bold> false detection. Panel <bold>(d)</bold> likely shows a signal from a boat while <bold>(e)</bold> represents a detection within the coda of an earthquake. We obtain two detections in panel <bold>(c)</bold>, where the earlier detection (P-wave arrival) is retained. We declare the second detection from the S-wave arrival as false. Dashed horizontal lines indicate the detection time obtained from HECTOR while the orange and purple lines in panels <bold>(a)</bold>–<bold>(b)</bold> indicate noise and signal windows (4 s), respectively, that are used to calculate the signal-to-noise ratios (SNR). The detections are obtained from channels 4000–5900, while SNR are calculated from all offshore channels 4000–6800 (channels with the highest SNR, Fig. 2). Figure S5a–b shows the event in panel <bold>(b)</bold> before and after the application of a spectral over-subtraction denoiser.</p></caption>
        <graphic xlink:href="https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026-f05.jpg"/>

      </fig>

</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Earthquake location and local magnitude estimates</title>
      <p id="d2e1057">We initially locate and calculate local magnitudes for high-SNR detected local earthquakes by combining DAS and seismic station data. We calculate SNR on offshore cable channels (4000–6800) considering a noise window from 1–5 s before the detection time and a signal window from 0.5–4.5 s after the detection time (Fig. 5). We compute the average Root-Mean-Square (RMS) values for noise and signal on traces band-pass filtered between 5–20 Hz, using a trimmed mean that removes the highest and lowest 10 % of values (trim fraction 0.1).</p>
      <p id="d2e1060">We then calculate SNR as follows:

          <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M59" display="block"><mml:mrow><mml:mi mathvariant="normal">SNR</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">20</mml:mn><mml:msub><mml:mi mathvariant="normal">log</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">RMS</mml:mi><mml:mi mathvariant="normal">signal</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">RMS</mml:mi><mml:mi mathvariant="normal">noise</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p id="d2e1097">We consider local earthquakes (following the criteria outlined above) with a SNR <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula> dB for hypocentral location and magnitude estimation, resulting in a subset of 456 events out of the 5734 detected local earthquakes. We manually include a <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 3.4 earthquake on 8 August 2024 at 19:18 (event id: kef2196) despite its low SNR of 5.3 dB, as it represents the largest earthquake recorded northwest of Kefalonia during our study period. The low SNR results from the origin time being <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula> s after a nearby <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 3.0 (event id: kef2195) whose coda wave contaminates the window containing the primary phase arrival of the <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 3.4 earthquake. Thus, our initial dataset consists of 457 earthquakes for location. The restrictive SNR threshold reflects the goal of building a high-quality reference catalog of locations and magnitudes. We perform automatic P- and S-wave arrival picking on DAS data using PhaseNet-DAS (Zhu et al., 2023) for each of the 457 earthquakes. We define 20 s windows for PhaseNet-DAS that start 6 s before the detection time and end 14 s after it (same as in Fig. 5). We follow the preprocessing used in the PhaseNet-DAS implementation (<uri>https://ai4eps.github.io/EQNet/phasenet_das/</uri>, last access: 26 May 2026), including conversion of strain to strain rate via temporal differentiation. We apply an additional band-pass filter between 5–40 Hz as part of our preprocessing. We manually inspect all picking results and observe good quality P- and S-phase picks (Fig. S7).</p>
      <p id="d2e1157">To reduce the number of DAS channels for earthquake location and achieve a number comparable to the seismic stations, we subdivide the cable into 12 segments (Fig. 1c) using a custom geometric clustering algorithm. The algorithm uses Density-Based Spatial Clustering of Applications with Noise (DBSCAN, Ester et al., 1996) to group channels exclusively by their spatial coordinates. It automatically instantiates a new segment boundary whenever the azimuthal angle variation exceeds a specified threshold. We allow a maximum azimuthal variation of 60°, applied an azimuth smoothing window of 50 channels, and enforce a minimum constraint of 100 channels per segment. We assign median P- and S-wave arrival times that we estimate in a prior step with PhaseNet-DAS applied to the entire cable to the median channel for each of the 12 segments. Finally, we download waveforms from the seven stations closest to the cable (Figs. 1, S3) and manually pick P- and S-wave arrival for each of the 457 earthquakes in Snuffler (Heimann et al., 2017) when data quality permits.</p>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Earthquake location</title>
      <p id="d2e1168">We consider events with a P- or an S-wave arrival identified by Phasenet-DAS on at least 10 of the 12 cable segments and with a clear P- or S-wave arrival at a minimum of three seismic stations for earthquake location. The minimum required number of segments and stations assures adequate azimuthal coverage for the events in the cluster offshore northwest of Kefalonia. We compute earthquake locations with NLLoc (Lomax et al., 2000) using arrival times from both DAS and seismic station data and a local 1D velocity model (Haslinger et al., 1999). We revised the original velocity model by removing the second layer at 0.5 km depth (Vp <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">5.47</mml:mn></mml:mrow></mml:math></inline-formula> km s<sup>−1</sup>), maintaining lower velocities from 0 to 2 km depth (Table S1) to reflect the presence of unconsolidated sediments beneath the offshore cable segment. The removal of the second layer from the original velocity model reduces the number of very shallow earthquakes (0–1 km) and improves depth resolution slightly. We calculate static phase arrival time residuals at the seismic stations and DAS channels used for location and include them in the final NLLoc run. Incorporating these residuals partially accounts for velocity model heterogeneities and mitigates the limitations of a 1D model. We note, however, that static station corrections are influenced by the spatial distribution of seismicity and are most appropriate for the region with the highest event density for this data set. We successfully locate 356 of the 457 local earthquakes (Fig. 6). The remaining events were either recorded at only two seismic stations or lacked a median phase arrival time on at least 10 cable segments, which inhibited robust hypocentral solutions. We obtain average semi-major and semi-minor horizontal ellipse error axis values of <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.5</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.8</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.4</mml:mn></mml:mrow></mml:math></inline-formula> km, respectively, and vertical errors of <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.9</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.6</mml:mn></mml:mrow></mml:math></inline-formula> km (Fig. S8).</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e1231">EHypocentral locations of earthquakes   with average SNR <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula> dB, estimated along the offshore portion of the cable (channels 4000–6800) by combining P- and S-wave arrival times from DAS and seven nearby seismic station data. Local magnitudes are computed using data from the four seismic stations on Kefalonia and one on Ithaki (shown in Fig. 1). Blue squares indicate the median channel positions for each cable segment, associated with the corresponding median P- and S-wave arrival times (see Fig. 1 and Sect. 4). The black box denotes the area shown by the pink box in Fig. 1 and outlines the most seismically active region during the two-week study period. Seismicity cross-sections include events located within 2 km of either side of each profile trace.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026-f06.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Earthquake magnitude estimate</title>
      <p id="d2e1258">We estimate <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> using seismic station data following the empirical relation of Hutton and Boore (1987) because the relation is also employed by NOA for <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> calculations (Melis and Konstantinou, 2006). We remove instrument response and convert waveforms to Wood-Anderson equivalent amplitudes. We then apply a 1 Hz, high-pass filter before calculating amplitudes at seismic stations. The 1 Hz high-pass filter helps remove longer period microseismic noise and improves magnitude estimates for smaller earthquakes (<inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub><mml:mi mathvariant="italic">&lt;</mml:mi></mml:mrow></mml:math></inline-formula> 0.6–0.8). We restrict the magnitude analysis to the four stations with the largest number of picks (FSK, DMLN, ITHC, VLS), as well as a fifth station, ATHR, because of its proximity to the cluster of seismicity northwest of Kefalonia (Fig. 1). For each station we use the maximum amplitude between the two horizontal components to estimate magnitude. Because some events have low amplitudes and are not always clearly visible at five stations, or because some signal windows may contain overlapping earthquakes, we calculate <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> using only the individual station magnitudes that differ by less than <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>M</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> from the average event magnitude estimate. We require at least three station magnitudes with <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>M</mml:mi><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> to assign a final <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which is then computed as the average of the retained values. <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> estimates are possible for all 356 earthquakes based on the above quality control requirements, and values range from 0.2 to 3.4. A comparison of earthquake magnitudes estimated here and common events in the revised NOA catalog shows a correlation coefficient of <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.95</mml:mn></mml:mrow></mml:math></inline-formula> and a near one-to-one relationship, with most of the absolute residuals <inline-formula><mml:math id="M80" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 0.1–0.2, suggesting a strong correlation (Fig. S9). The observed deviation between <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> estimates from this study and those reported by NOA can be attributed to differences in the seismic stations used and in hypocentral locations.</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Catalog enhancement using waveform cross-correlation of DAS data</title>
      <p id="d2e1398">For clarity in our catalog enhancement workflow, we define template events as earthquakes with absolute hypocentral locations and magnitude estimates derived from the seismic network, and target events denote local earthquakes whose locations and magnitudes are initially unknown. We begin catalog enhancement by using 352 of the 356 located earthquakes as templates. We omit four events from the group of templates that have either a semi-major horizontal error ellipse axis and/or a depth error <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km, or a depth above the sea level. This error threshold is necessary because large location uncertainties propagate into significant errors in <inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which in turn, affect the relative magnitudes that are calculated during enhancement using the amplitude ratios between templates and target events. Prior to calculating these cross-correlations, the continuous waveform records are downsampled to 50 Hz and the analysis is restricted to the same offshore cable section (channels 4000–5900) used for event detection (Fig. 7). We band-pass filter all traces between 5–20 Hz before computing a channel-based cross-correlation coefficient (CCC) using 4 s time windows that begin 0.5 s after the detection time (Figs. 7 and 8). We cross-correlate each of the 5378 target events with the 352 template events. Each target event is subsequently assigned the location of its most highly correlated template event. We retain the initial absolute locations and magnitude estimates in the final catalog for the four events previously excluded from the template database due to large hypocentral errors (<inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km) or because located above sea level.</p>

      <fig id="F7" specific-use="star"><label>Figure 7</label><caption><p id="d2e1434">Waveform cross-correlation coefficient (CCC) analysis for event pair kef0367 (<inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 1.6) and kef0395 (<inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 0.9). <bold>(a)</bold> CCC of individual DAS traces from channels 4000–5900. <bold>(a)</bold> Purple and gold symbols are CCC values above and below a SNR threshold calculated from the smaller amplitude event in the pair (see text and description in panel <bold>b</bold> of this figure). <bold>(b)</bold> Signal-to-noise ratio (SNR) of each event in the pair. SNR (in dB) is calculated as the ratio between the root-mean-square of the signal in 4 s windows starting 0.5 s after the detection time and noise windows of the same length starting 5 s before the detection time (refer to Fig. 3a for SNR windows). The thick horizontal black line marks the minimum SNR threshold required for the CCC calculation, which is defined by the lower-amplitude event. The threshold corresponds to the cutoff of the top 33 % of channels with the highest SNR. <bold>(c–d)</bold> CCC versus SNR for events kef0367 and kef0395. The vertical black line indicates the minimum SNR threshold. Average CCC of the event pair is 0.85, estimated as the Fisher mean of the individual CCC values. Traces are band-pass filtered 5–20 Hz. The correlation between SNR and CCC at individual traces is even clearer when showing CCC values over the entire cable (Fig. S10).</p></caption>
        <graphic xlink:href="https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026-f07.png"/>

      </fig>

      <fig id="F8" specific-use="star"><label>Figure 8</label><caption><p id="d2e1483">Event pair (template-target) cross-correlation. Black traces are template events with location, and a <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> estimates, while in magenta it is the target event with no (initial) location or magnitude estimate. <bold>(a)</bold> Event pair kef1934 (<inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 1.3) and kef1398 (<inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 0.3) with average CCC of 0.93. <bold>(b)</bold> Event pair kef1740 (<inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 0.4) and kef4621 (<inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M92" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.2) with an average CCC of 0.58. Traces are band-pass filtered at 5–20 Hz and normalized to make waveforms comparable. CCC is calculated in 4 s windows starting 0.5 s after the detection time. CCC at a given channel and time shift (in samples) are indicated for each subpanel.</p></caption>
        <graphic xlink:href="https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026-f08.png"/>

      </fig>

      <p id="d2e1562">We observe that CCC varies across channels (Figs. 7a, S10a) and that higher CCC values are associated with channels with higher SNR (Figs. 7c–d, S10c–d). To account for varying CCC with SNR, we apply a SNR criterion before averaging the CCC values of individual channels. We then compute the average CCC between event pairs using the Fisher mean (Fisher, 1921; Silver and Dunlap, 1987), after excluding 67 % of the channels (i.e., 1273 channels) with the lowest SNR (Figs. 7e, S10e). The SNR estimation uses the 4 s signal and noise windows noted above (Fig. 5), and the cutoff threshold is determined based on the lowest-amplitude earthquake in each event pair (Fig. 7b).</p>
      <p id="d2e1565">Before selecting the minimum CCC value for associating a target event with a template and proceeding with relative magnitude calculations, we first examine the expected decay of CCC with inter-event distance (Menke et al., 1990). We do so by cross correlating all independent template event pairs (excluding the four events noted above with larger hypocentral uncertainties) following the procedure outlined in the previous paragraph. We restrict the analysis to template earthquakes since we know their locations. Because our analysis relies solely on absolute event locations, the calculated inter-event distances for a given CCC value are likely to overestimate the true physical separation of the event pairs. As expected, we observe a systematic inverse correlation between CCC and inter-event distance (Fig. S11). For instance, we obtain a median inter-event distance of <inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> km and a 95th percentile of <inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km for a pair with a CCC of 0.52 (Fig. S11). At 15 km distance, this corresponds to a magnitude error of 0.06 for a 2 km inter-event separation and 0.15 for a 5 km inter-event separation. At 10 km distance, the corresponding errors are 0.05 and 0.2, respectively. In this study, we use a CCC threshold of 0.52 that is empirically determined from the observed CCC–distance relationship. Specifically, Fig. S11 indicates a notable increase in inter-event distance for CCC values below <inline-formula><mml:math id="M95" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.52–0.53. While median inter-event distances remain below <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> km for CCC values between 0.40 and 0.52, the 95th percentile increases substantially, indicating a higher risk of large spatial mismatches. We therefore exclude lower CCC values to ensure robustness of the event associations. By using a CCC threshold of 0.52, we associate 2515 target events to template events. We test slightly different CCC thresholds, namely 0.50 and 0.54, in addition to the preferred value of 0.52 used to construct the final enhanced catalog. We find that differences in the number of detected events occur primarily for magnitudes <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> (Fig. S12). We provide all event-pair CCC values to enable reproducibility and allow assessment of the sensitivity of event associations to different CCC thresholds (see Data and code availability). Figure 8 shows examples of target-template pairs exceeding the CCC threshold. We observe that nearly all target events (<inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">97</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:math></inline-formula>) are associated with template events from the cluster northwest of Kefalonia (Fig. S13).</p>
      <p id="d2e1631">Before calculating amplitude ratios for the determination of relative magnitudes, we first inspect whether we can correctly retrieve the magnitudes of template events using amplitude ratios, where template <inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> estimates originate from seismic stations (Fig. 9). We associate each template event with its most similar template and recalculate the magnitude from the amplitude ratio of band-passed traces (3–20 Hz) on channels 4000–5900. The lower corner frequency of 3 Hz suppresses long-period noise present in the offshore DAS segment. The upper corner frequency of 20 Hz is sufficiently high to capture the peak amplitudes of smaller earthquakes (<inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>) with expected peak spectral amplitudes below the source corner frequency (e.g., Baltay and Abercrombie, 2025), and is sufficiently low to minimize high-frequency effects related to source complexity (e.g., Trugman et al., 2021). We consider the average of the maximum amplitudes of traces between 4000–5900 after removing the highest and lowest 10 % values (i.e., trimmed mean) for event pairs with CCC values <inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">0.52</mml:mn></mml:mrow></mml:math></inline-formula>. We calculate relative magnitudes as follows:</p>

      <fig id="F9" specific-use="star"><label>Figure 9</label><caption><p id="d2e1672"><bold>(a)</bold> <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from seismic stations versus relative <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> derived from DAS data. <bold>(b)</bold> Histogram of differences between <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from seismic stations and relative <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> derived from DAS data. The analysis includes all located earthquakes (i.e. templates) with semi-major horizontal error ellipse axes and vertical error <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km (352 events). Relative <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for each template event is obtained from the mean amplitude ratio with respect to the most similar event using band-pass filtered waveforms (5–20 Hz). Average amplitude ratios are calculated using event pairs with a cross-correlation coefficient <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">0.52</mml:mn></mml:mrow></mml:math></inline-formula> (333 of the 352 template events) on channels 4000–5900 using a trimmed mean that exclude the highest and lowest 10 % of values.</p></caption>
        <graphic xlink:href="https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026-f09.png"/>

      </fig>

      <p id="d2e1762"><disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M109" display="block"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">target</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">template</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">log</mml:mi><mml:mn mathvariant="normal">10</mml:mn><mml:mo>(</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">target</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">template</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></disp-formula>
        where <inline-formula><mml:math id="M110" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> is the magnitude and <inline-formula><mml:math id="M111" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> is the average of the maximum amplitude.</p>
      <p id="d2e1819">We observe good agreement between initial <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and relative <inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> estimates over the full magnitude range, as indicated by a coefficient of determination <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.92</mml:mn></mml:mrow></mml:math></inline-formula>, mean absolute deviations of <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.1</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.1</mml:mn></mml:mrow></mml:math></inline-formula>, and a best-fitting line with an approximately unit slope (Fig. 9). Remaining deviations between seismic-station <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and DAS-derived relative <inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> estimates may be attributed to imperfectly collocated event pairs and/or uncertainties in the initial magnitudes estimated from the seismic stations. Accordingly, we compute relative magnitudes for all target events with a minimum CCC <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">0.52</mml:mn></mml:mrow></mml:math></inline-formula> (2515 events) with respect to their template events.</p>
      <p id="d2e1904">Adding relative magnitude estimates to the 356 events with <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> calculated from seismic stations leads to 2871 magnitude estimates (50 % of the local earthquakes). We observe that 2790 earthquakes with a magnitude estimate (97 %) are located offshore northwest of Kefalonia and are mostly clustered in space (Figs. 1, 5, S13). The remaining events are scattered within the study region (Fig. S13), with a few clusters located along the Strait of Ithaki. Figure S13 shows the distribution of all events detected and located in this study with a magnitude estimate. There are 10 events in common with the revised NOA catalog (the NOA catalog reports 91 earthquakes within a radius of 50 km from the start of the cable) that are not included in our catalog of 356 events, despite being successfully detected. Eight of the ten events common to the NOA catalog are omitted because of their average SNR at offshore DAS channels being <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula> dB, and they were therefore not considered for initial location (Sect. 4.1). The last two of the ten events are omitted because we observe <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula> s at offshore DAS channels. The fact that we detect but do not locate a few earthquakes included in the revised NOA catalog reflects our focus on detecting and locating seismicity in the highly active region offshore northwest of Kefalonia. By considering events within the active region northwest of Kefalonia (Figs. 1, 5, S13), we observe a <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">38</mml:mn></mml:mrow></mml:math></inline-formula>-fold increase in the number of events with a magnitude estimate relative to the revised NOA catalog (Fig. 10). All events in our catalog down to <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 2.4 are common to the NOA catalog (Fig. 10a), while the number of events from this study significantly increases at lower magnitudes (Fig. 10). Specifically, we estimate a magnitude of completeness of <inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.4</mml:mn></mml:mrow></mml:math></inline-formula> using both a maximum curvature and Goodness-of-Fit Test (Wiemer and Wyss, 2000) and a <inline-formula><mml:math id="M126" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula>-value <inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.95</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.03</mml:mn></mml:mrow></mml:math></inline-formula> based on the maximum likelihood estimate (Aki, 1965) (Fig. 10a). The enhanced earthquake catalog shows inter-event times as short as 3 s (the minimum allowed inter-event time from de-clustering) and average inter-event times for 100-event windows down to 30 s.</p>

      <fig id="F10" specific-use="star"><label>Figure 10</label><caption><p id="d2e2016">Time–space–magnitude distribution of seismicity in the region 38.35–38.46° N, 20.41–20.525° E (black box in Figs. 1 and 6). <bold>(a)</bold> Frequency–magnitude distribution of events from this study compared with events from NOA for the same period and region. The <inline-formula><mml:math id="M128" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula>-value is estimated using Maximum Likelihood (Aki, 1965), and the magnitude of completeness (<inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) using the Goodness-of-Fit Test and Maximum Curvature method (Wiemer and Wyss, 2000). <bold>(b)</bold> Number of events over time (3 h bins). Red stars indicate <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">2.5</mml:mn></mml:mrow></mml:math></inline-formula> earthquakes. <bold>(c)</bold> Event magnitudes versus time for individual events. <bold>(d)</bold> Inter-event times (100-event sliding windows with 90 % overlap) between successive events with <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub><mml:mi mathvariant="italic">&gt;</mml:mi><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> plotted against time.</p></caption>
        <graphic xlink:href="https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026-f10.jpg"/>

      </fig>

</sec>
<sec id="Ch1.S6">
  <label>6</label><title>Discussion</title>
      <p id="d2e2097">This study releases two-week DAS waveforms and a high-resolution earthquake catalog derived from the integration of DAS recordings and publicly available data from conventional seismic stations. The dataset captures a period of exceptionally high seismicity within 10–15 km of the fiber-optic cable at rates exceeding 100 events per hour (Figs. 1, 6). Although other open-access DAS datasets also contain high event rates, most of them were acquired in boreholes and target induced seismicity (the FORGE dataset, Porras et al., 2024), rather than natural earthquake sequences.</p>
      <p id="d2e2100">The highest seismicity rates occur offshore in a cluster northwest of Kefalonia with a <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km radius where azimuthal coverage from land stations is limited (Figs. 1, 6). The intense seismic activity combined with sparse station geometry are challenging for the monitoring of active seismic sequences (Grigoli et al., 2021; Karastathis et al., 2015). This work shows that combining DAS and seismic station data can make it possible to overcome some of the challenges associated with observing offshore earthquakes: using DAS channels for dense wavefield sampling and earthquake detection, combining DAS and seismic station data for determining hypocenter locations, and using seismic stations for amplitude calibration and magnitude estimation.</p>
      <p id="d2e2113">The enhanced catalog presented here exhibits high temporal resolution, with inter-event times as short as 3 s and a completeness magnitude of <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.4</mml:mn></mml:mrow></mml:math></inline-formula>. It captures evolving statistical features of the seismic sequence, including a transition from more Poisson-like inter-event time distribution to densely clustered activity associated with mainshock–aftershock activity (Fig. 10c). The catalog also reveals notable changes in aftershock productivity. For instance, two <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> earthquakes before 8 August 2024 were not followed by clear aftershock activity, whereas similar-sized and smaller events after that date produced pronounced aftershock sequences (Fig. 10b–c). After 8 August, we observe a systematic relation between mainshock magnitude and aftershock inter-event times, with larger mainshocks followed by shorter aftershock inter-event times (Fig. 10d). The distribution of the seismicity highlights a nearly vertical WNW-ESE striking fault (Fig. 6), which is consistent with the geometry observed by Anagnostou et al. (2025), who used 3-month data between the end of February and the end of April 2025. These observations underscore the high spatial and temporal resolution of the catalog that we will discuss in a detailed analysis of the space–time–magnitude patterns that will be addressed in a separate study.</p>
      <p id="d2e2145">The amphibious nature of the telecommunication cable introduces additional features of shallow crustal structure that warrant further investigation, including the strong signal amplification observed along the marine segment and its potential influence on magnitude determination when using DAS data alone. This offshore amplification may reflect not only variations in shallow crustal structure, but also differences in DAS sensitivity to body and surface waves, mechanical coupling, cable construction, and installation conditions across the onshore–offshore transition.</p>
<sec id="Ch1.S6.SS1">
  <label>6.1</label><title>Distorted waveforms</title>
      <p id="d2e2156">The close proximity of the cable and the large magnitudes of the sequence also led to distorted waveforms on many channels after the S-wave arrival for earthquakes with <inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>. The distortion is mostly limited to offshore channels but can also appear on onshore channels for events with <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2.8</mml:mn></mml:mrow></mml:math></inline-formula>. This distortion is likely related to cycle-skipping issues in DAS caused by dynamic range limitations (Katakami et al., 2024). In fact, for a sample of earthquakes exhibiting distorted waveforms, we observe a phase shift corresponding to an integer multiple of 2<inline-formula><mml:math id="M137" display="inline"><mml:mi mathvariant="italic">π</mml:mi></mml:math></inline-formula> that is consistent with cycle-skipping. However, determining the exact cause is challenging because the data were decimated by a factor of 20 before storage (from 5000 to 250 Hz), eliminating higher-frequency energy above 125 Hz. With our settings, the maximum change measurable between consecutive samples is <inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">0.033</mml:mn><mml:mi mathvariant="italic">μ</mml:mi><mml:mi mathvariant="italic">ε</mml:mi></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mi mathvariant="italic">π</mml:mi></mml:mrow></mml:math></inline-formula>). While the QuantX instrument can measure larger signal amplitudes, it cannot track phase changes exceeding <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mi mathvariant="italic">π</mml:mi></mml:mrow></mml:math></inline-formula> between consecutive samples. Nevertheless, the observed distortion of the signals, likely due to cycle-skipping, did not affect our analysis: maximum earthquake amplitudes are correctly measured (Fig. 9), and waveform shapes remain undistorted after band-passing earthquakes in our frequency range of interest (Fig. 11).</p>

      <fig id="F11" specific-use="star"><label>Figure 11</label><caption><p id="d2e2237">Waveforms of similar events (average CCC <inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula> from DAS), one of which is affected by cycle skipping. The <inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 2.7 event kef1828 (black) shows waveform distortion at the S-wave arrival, while the <inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 1.4 event kef1780 (violet) does not. <bold>(a)</bold> Raw waveforms. <bold>(b)</bold> Band-pass filtered waveforms (5–20 Hz). Hypocentral locations: kef1780 – 38.4018° N, 20.4502° E, depth 3.41 km; kef1828 – 38.4018° N, 20.4547° E, depth 3.76 km. Note the high waveform similarity after filtering the traces. The events show an average CCC of 0.7 at seismic stations (Fig. S14).</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/4677/2026/essd-18-4677-2026-f11.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S7">
  <label>7</label><title>Potential applications of the datasets</title>
      <p id="d2e2293">The datasets released in this work may offer a range of potential applications. The exceptionally high seismicity rate with inter-event times as short as 3 s provides an ideal testbed for developing and evaluating advanced detection and location methods tailored to DAS data. To support such efforts, we provide a manually verified event catalog that can serve as a reference dataset. In addition, the inclusion of very small-amplitude signals, some with magnitude estimates and others without, may be useful for developing and testing denoising approaches (e.g., Fig. S5).</p>
      <p id="d2e2296">The integration of the DAS array within an open-access seismic network offers an opportunity to evaluate DAS-enhanced event location methods and explore hybrid location strategies. This setting also allows testing of various strategies to mitigate biases that could arise from the large differences in the number of sensors between the DAS cable and the traditional network, such as automatic DAS channel selection. Furthermore, DAS recordings acquired on seafloor cables may exhibit higher amplitudes compared to onshore cables, as observed in this study. Such differences could reflect a combination of site, coupling, and propagation effects that may in turn introduce biases in magnitude estimation. Finally, the dataset may offer valuable opportunities for machine learning applications. With nearly 6000 recorded events, it can be used to train new models or to investigate transfer learning of existing ones.</p>
</sec>
<sec id="Ch1.S8">
  <label>8</label><title>Data and code availability</title>
      <p id="d2e2307">Continuous DAS data waveforms are available from Bocchini et al. (2025), <ext-link xlink:href="https://doi.org/10.60517/cv43p1601" ext-link-type="DOI">10.60517/cv43p1601</ext-link>.</p>
      <p id="d2e2313">Codes to read and plot the events (or detections) recorded along the fiber-optic cable, earthquake catalogs, event pairs cross-correlation coefficients, cable geometry, and PhaseNet-DAS picks are available from Bocchini (2026), <ext-link xlink:href="https://doi.org/10.5281/zenodo.20558686" ext-link-type="DOI">10.5281/zenodo.20558686</ext-link>.</p>
      <p id="d2e2319">We use _PhaseNet-DAS (Zhu et al., 2023) for phase picking on DAS data, which is available from <uri>https://ai4eps.github.io/EQNet/phasenet_das/</uri> (last access: 26 May 2026).</p>
      <p id="d2e2325">We use HECTOR (Porras et al., 2024) for event detection on DAS data, which is available from <uri>https://github.com/juanucr/HECTOR/tree/main</uri> (Porras, 2024).</p>
      <p id="d2e2332">We use Snuffler, available through Pyrocko, for manual picking of seismic waveforms (<ext-link xlink:href="https://doi.org/10.5880/GFZ.2.1.2017.001" ext-link-type="DOI">10.5880/GFZ.2.1.2017.001</ext-link>, Heimann et al., 2017).</p>
      <p id="d2e2338">We use Obspy for processing of seismic station waveforms (Beyreuther et al., 2010).</p>
      <p id="d2e2341">We create figures using Matplotlib (Hunter, 2007) and GMT (Wessel et al., 2019).</p>
</sec>
<sec id="Ch1.S9">
  <label>9</label><title>Metadata</title>
<sec id="Ch1.S9.SS1">
  <label>9.1</label><title>DAS Metadata</title>
      <p id="d2e2359"><list list-type="bullet">
            <list-item>

      <p id="d2e2364"><bold>Interrogator:</bold> OptaSense QuantX</p>
            </list-item>
            <list-item>

      <p id="d2e2372"><bold>File Format:</bold> HDF5</p>
            </list-item>
            <list-item>

      <p id="d2e2380"><bold>Number of Channels:</bold> 7750</p>
            </list-item>
            <list-item>

      <p id="d2e2388"><bold>File Length:</bold> 30 s</p>
            </list-item>
            <list-item>

      <p id="d2e2396"><bold>Ping Rate:</bold> 5000 Hz</p>
            </list-item>
            <list-item>

      <p id="d2e2405"><bold>Sampling Rate:</bold> 250 Hz</p>
            </list-item>
            <list-item>

      <p id="d2e2413"><bold>Gauge Length:</bold> 10.2 m</p>
            </list-item>
            <list-item>

      <p id="d2e2421"><bold>Channel Spacing:</bold> 2.04 m</p>
            </list-item>
            <list-item>

      <p id="d2e2429"><bold>Data Unit:</bold> Optical phase shift<fn id="Ch1.Footn1"><p id="d2e2434">Note: The raw data can be converted to strain using the script provided in the accompanying repository (see Data and Code Availability section), which also demonstrates the HDF5 file structure and includes functions for data reading and visualization.</p></fn></p>
            </list-item>
          </list></p>
</sec>
<sec id="Ch1.S9.SS2">
  <label>9.2</label><title>Cable Geometry</title>
      <p id="d2e2447">The cable geometry is provided as a CSV file that defines the spatial coordinates of the DAS array after the removal of looped or otherwise non-usable cable sections. Consequently, the number of unique channels in this geometry file is lower than in the raw HDF5 waveform files; only channels explicitly listed in this file are considered valid for analysis. The CSV file contains the following columns: <list list-type="bullet"><list-item>
      <p id="d2e2452">channel_number_recorded: The channel number directly matching the channel numbers in the HDF5 files.</p></list-item><list-item>
      <p id="d2e2456">latitude/longitude: Geographic coordinates in decimal degrees.</p></list-item><list-item>
      <p id="d2e2460">elevation_m: Elevation in meters (negative values indicate channels below sea level).</p></list-item><list-item>
      <p id="d2e2464">comment: Label indicating whether the channel is located on Kefalonia, offshore, or on Ithaki.</p></list-item><list-item>
      <p id="d2e2468">final_section_id: Identifier for the specific cable sections used for earthquake locations.</p></list-item></list></p>
</sec>
<sec id="Ch1.S9.SS3">
  <label>9.3</label><title>Seismic Station Waveforms</title>
      <p id="d2e2479"><list list-type="bullet">
            <list-item>

      <p id="d2e2484"><bold>Seismic Stations:</bold> HP.FSK, HA.ATHR, HL.VLS, HT.EVGI, HT.DLMN, HT.ITHC, HT.DRAG</p>
            </list-item>
            <list-item>

      <p id="d2e2492"><bold>Sampling Rate:</bold> 100 Hz</p>
            </list-item>
            <list-item>

      <p id="d2e2500"><bold>Data Source:</bold> Continuous seismic waveforms are publicly accessible via the NOA EIDA node (<uri>https://eida.gein.noa.gr/</uri>, last access: 26 May 2026).</p>
            </list-item>
          </list></p>
</sec>
<sec id="Ch1.S9.SS4">
  <label>9.4</label><title>Earthquake Catalogs</title>
<sec id="Ch1.S9.SS4.SSS1">
  <label>9.4.1</label><title>Catalog with Absolute Earthquake Locations</title>
      <p id="d2e2525">The catalog contains 356 earthquakes and is provided as a CSV file with the following columns: event_id (unique event identifier), origin_time (UTC origin time), longitude (decimal degrees), latitude (decimal degrees), depth (km), Nobs (number of observations), and gap (azimuthal gap). Uncertainties are reported in kilometers as H_err and h_err (the semi-major and semi-minor axes of the horizontal error ellipse, respectively) and z_err (depth uncertainty). The catalog also includes the local magnitude (ML) and its standard deviation (ML_std).</p>
</sec>
<sec id="Ch1.S9.SS4.SSS2">
  <label>9.4.2</label><title>Enhanced Earthquake Catalog</title>
      <p id="d2e2536">This catalog expands upon the absolute locations dataset by incorporating additional events identified via waveform cross-correlation, bringing the total to 2871 events. The data is provided as a CSV file containing the following columns: event_id (unique event identifier), amplitude (event amplitude in micrometers), ML (local magnitude), reference (the template event ID associated with the target event), CCC (cross-correlation coefficient), detection_time (UTC detection time returned by the detector), longitude (decimal degrees), latitude (decimal degrees), and depth (km).</p>
      <p id="d2e2539">Note: The CCC and reference columns are left blank for the original 356 template earthquakes containing absolute locations.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S10" sec-type="conclusions">
  <label>10</label><title>Conclusions</title>
      <p id="d2e2552">In this study, we combine DAS recordings with permanent seismic stations from the HUSN to investigate seismicity on Kefalonia Island between 2–15 August 2024. Applying a semblance-based detector enables identification of more than 5700 earthquakes within a <inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> km radius of the starting point of the fiber-optic cable. Combining DAS and seismic data analysis and waveform cross-correlation enables location and magnitude estimates of 2871 events, of which 2790 concentrate in an active cluster offshore northwest of Kefalonia. The catalog shows very high seismicity rates with peaks in earthquake rates that exceed 100 events per hour. Individual inter-event times are as short as 3 s, while average inter-event times calculated over moving 100-event windows decrease to <inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> s. The short inter-event times and a <inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.4</mml:mn></mml:mrow></mml:math></inline-formula> enable a detailed spatiotemporal analysis of seismicity.</p>
      <p id="d2e2596">A comparison of the catalog produced here and the revised earthquake catalog of NOA for the active cluster northwest of Kefalonia shows the same number of events down to <inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 2.4, and a factor of <inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">38</mml:mn></mml:mrow></mml:math></inline-formula> increase in smaller events for the DAS-seismic-data catalog. The detailed catalog underscores the benefit of using DAS to strengthen seismic monitoring in regions where station coverage is limited and seismicity is intense.</p>
      <p id="d2e2620">This work makes the following data products publicly available: the DAS-seismic station earthquake catalog, continuous DAS recordings, detection lists, and supporting metadata. The dataset provides a resource for future studies of DAS data processing, integration with seismic stations for earthquake monitoring, and analyses of seismicity, in large part because it targets a highly productive natural seismic sequence.</p>
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      </body>
    <back><app-group>
        <supplementary-material position="anchor"><p id="d2e2622">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/essd-18-4677-2026-supplement" xlink:title="pdf">https://doi.org/10.5194/essd-18-4677-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e2634">G.M.B. Conceptualization, Writing – original draft, Writing – review and editing, Methodology, Visualization, Formal analysis, Data curation, Investigation. E.B. Conceptualization, Writing – review and editing, Methodology, Formal Analysis. M.P.R. Formal analysis, Data curation, Investigation. S.G. Conceptualization, Formal Analysis. G.P. Conceptualization, Formal Analysis. F.G. Conceptualization, Methodology, Writing – review and editing. E.B. Writing – review and editing. E.S. Writing – review and editing. R.M.H. Funding acquisition, Conceptualization, Writing – review and editing, Investigation.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e2640">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d2e2646">The authors decline responsibility for any possible errors in the dataset that could lead to erroneous evaluations.  Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. The authors bear the ultimate responsibility for providing appropriate place names. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e2655">The authors would like to acknowledge the National Observatory of Athens for maintaining and publicly sharing a manually reviewed earthquake catalog. The authors would like to thank the student assistants D. Drier and M. Roßbach for helping with the location of the DAS channels and with manual picking of events at seismic stations. The authors also thank M. Bagagli for helping with manual inspection of the initial list of detections. The authors would like to thank Dionisis Alisandratos for his patience and help during the set-up of the DAS experiment, and OTE Greece for providing access to the fiber-optic cable. G.M.B., M.P.R., and R.M.H., would like to thank Roger Crickmore (Luna Innovations) for the helpful discussion on cycle skipping in DAS.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e2660">G.M.B. and the DAS data acquisition were supported by the Volkswagen Foundation through a Momentum grant awarded to R.M.H.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e2666">This paper was edited by Andrea Rovida and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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