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<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Sens.</journal-id>
<journal-title>Frontiers in Sensors</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Sens.</abbrev-journal-title>
<issn pub-type="epub">2673-5067</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
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<article-meta>
<article-id pub-id-type="publisher-id">1599365</article-id>
<article-id pub-id-type="doi">10.3389/fsens.2025.1599365</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Sensors</subject>
<subj-group>
<subject>Perspective</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>ASIX: Single-photon, energy resolved X-ray imaging with 50 <italic>&#x3bc;</italic>m hexagonal hybrid pixel</article-title>
<alt-title alt-title-type="left-running-head">Minuti et al.</alt-title>
<alt-title alt-title-type="right-running-head">
<ext-link ext-link-type="uri" xlink:href="https://doi.org/10.3389/fsens.2025.1599365">10.3389/fsens.2025.1599365</ext-link>
</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Minuti</surname>
<given-names>Massimo</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1792688/overview"/>
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<contrib contrib-type="author">
<name>
<surname>Baldini</surname>
<given-names>Luca</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Beccherle</surname>
<given-names>Roberto</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Bellazzini</surname>
<given-names>Ronaldo</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Bisht</surname>
<given-names>Ashish</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/2836466/overview"/>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Boscardin</surname>
<given-names>Maurizio</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1112165/overview"/>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Brez</surname>
<given-names>Alessandro</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Bruschi</surname>
<given-names>Paolo</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Ceccanti</surname>
<given-names>Marco</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Vignali</surname>
<given-names>Matteo Centis</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1796853/overview"/>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Frontini</surname>
<given-names>Luca</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Gaioni</surname>
<given-names>Luigi</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Ali</surname>
<given-names>Omar Hammad</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Latronico</surname>
<given-names>Luca</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Liberali</surname>
<given-names>Valentino</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Magazz&#xf9;</surname>
<given-names>Guido</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Manfreda</surname>
<given-names>Alberto</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Manghisoni</surname>
<given-names>Massimo</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1887831/overview"/>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Morsani</surname>
<given-names>Fabio</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Orsini</surname>
<given-names>Leonardo</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Palini</surname>
<given-names>Luca</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Rollins</surname>
<given-names>Melissa Pesce</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Pinchera</surname>
<given-names>Michele</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Piotto</surname>
<given-names>Massimo</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1991940/overview"/>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Profeti</surname>
<given-names>Alessandro</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Prosperi</surname>
<given-names>Paolo</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Ratti</surname>
<given-names>Lodovico</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff7">
<sup>7</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/692114/overview"/>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Ria</surname>
<given-names>Andrea</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Ronchin</surname>
<given-names>Sabina</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff8">
<sup>8</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1289772/overview"/>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Sgr&#xf2;</surname>
<given-names>Carmelo</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
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<contrib contrib-type="author">
<name>
<surname>Silvestri</surname>
<given-names>Stefano</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Spandre</surname>
<given-names>Gloria</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Stabile</surname>
<given-names>Alberto</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
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<contrib contrib-type="author">
<name>
<surname>Traversi</surname>
<given-names>Gianluca</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
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<contrib contrib-type="author">
<name>
<surname>Trucco</surname>
<given-names>Gabriella</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Vasquez</surname>
<given-names>Monica</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Zanardo</surname>
<given-names>Danny</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
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<aff id="aff1">
<sup>1</sup>
<institution>National Institute for Nuclear Physics (INFN)</institution>, <addr-line>Frascati</addr-line>, <country>Italy</country>
</aff>
<aff id="aff2">
<sup>2</sup>
<institution>Department of Physics, University of Pisa</institution>, <addr-line>Pisa</addr-line>, <country>Italy</country>
</aff>
<aff id="aff3">
<sup>3</sup>
<institution>Fondazione Bruno Kessler (FBK)</institution>, <addr-line>Trento</addr-line>, <country>Italy</country>
</aff>
<aff id="aff4">
<sup>4</sup>
<institution>Department of Information Engineering, University of Pisa, Pisa</institution>, <country>Italy</country>
</aff>
<aff id="aff5">
<sup>5</sup>
<institution>Department of Engineering and Applied Sciences, University of Bergamo, Bergamo</institution>, <country>Italy</country>
</aff>
<aff id="aff6">
<sup>6</sup>
<institution>Department of Physics, University of Milano, Milano</institution>, <country>Italy</country>
</aff>
<aff id="aff7">
<sup>7</sup>
<institution>Department of Electrical, Computer and Biomedical Engineering, University of Pavia, Pavia</institution>, <country>Italy</country>
</aff>
<aff id="aff8">
<sup>8</sup>
<institution>Trento Institute for Fundamental Physics and Applications</institution>, <addr-line>Trento</addr-line>, <country>Italy</country>
</aff>
<author-notes>
<fn fn-type="edited-by">
<p>
<bold>Edited by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/692341/overview">Alberto Quaranta</ext-link>, University of Trento, Italy</p>
</fn>
<fn fn-type="edited-by">
<p>
<bold>Reviewed by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1012682/overview">Simona Giordanengo</ext-link>, National Institute of Nuclear Physics of Turin, Italy</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/3114359/overview">Benedikt Ludwig Bergmann</ext-link>, Czech Technical University in Prague, Czechia</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Massimo Minuti, <email>massimo.minuti@pi.infn.it</email>
</corresp>
</author-notes>
<pub-date pub-type="epub">
<day>30</day>
<month>10</month>
<year>2025</year>
</pub-date>
<pub-date pub-type="collection">
<year>2025</year>
</pub-date>
<volume>6</volume>
<elocation-id>1599365</elocation-id>
<history>
<date date-type="received">
<day>24</day>
<month>03</month>
<year>2025</year>
</date>
<date date-type="accepted">
<day>03</day>
<month>09</month>
<year>2025</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2025 Minuti, Baldini, Beccherle, Bellazzini, Bisht, Boscardin, Brez, Bruschi, Ceccanti, Vignali, Frontini, Gaioni, Ali, Latronico, Liberali, Magazz&#xf9;, Manfreda, Manghisoni, Morsani, Orsini, Palini, Rollins, Pinchera, Piotto, Profeti, Prosperi, Ratti, Ria, Ronchin, Sgr&#xf2;, Silvestri, Spandre, Stabile, Traversi, Trucco, Vasquez and Zanardo.</copyright-statement>
<copyright-year>2025</copyright-year>
<copyright-holder>Minuti, Baldini, Beccherle, Bellazzini, Bisht, Boscardin, Brez, Bruschi, Ceccanti, Vignali, Frontini, Gaioni, Ali, Latronico, Liberali, Magazz&#xf9;, Manfreda, Manghisoni, Morsani, Orsini, Palini, Rollins, Pinchera, Piotto, Profeti, Prosperi, Ratti, Ria, Ronchin, Sgr&#xf2;, Silvestri, Spandre, Stabile, Traversi, Trucco, Vasquez and Zanardo</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/">
<p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</p>
</license>
</permissions>
<abstract>
<p>The Analog Spectral Imager for X-rays is a technology demonstrator of a small-pixel Hybrid Pixel Detector (HPD) designed for applications such as X-ray diffraction, synchrotron-based material science, and soft X-ray astrophysics requiring energy-resolved imaging. The ASIX architecture aims at mitigating the adverse effects of charge sharing, typical of small-pixel devices. In contrast to other frame-based photon counters or multi-threshold devices, ASIX employs, along with a <inline-formula id="inf2">
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</inline-formula>. While the baseline for the ASIX R&#x26;D sensor is silicon for <inline-formula id="inf10">
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</inline-formula>20&#xa0;keV operation, the design of the readout ASIC is compatible with High-Z materials sensors, such as cadmium-telluride or gallium-arsenide, for higher energies X-rays imaging, enabling potential extension to biomedical and preclinical research. This paper describes the ASIX imager architecture and reports on the development and testing of two Minimum Viable Products (MVPs), developed by coupling XPOL-III, a readily available 180-nm CMOS readout ASIC, to a <inline-formula id="inf11">
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</inline-formula> (silicon). These results confirm our preliminary models predicting the feasibility of simultaneous high energy and spatial resolution in such a small-pixel devices, thus securing the ASIX specifications. Finally, the paper highlights the technology gaps that ASIX would potentially fill in both terrestrial and space applications.</p>
</abstract>
<kwd-group>
<kwd>hybrid pixel detectors</kwd>
<kwd>X-ray spectral imaging</kwd>
<kwd>sub-pixel resolution</kwd>
<kwd>charge sharing</kwd>
<kwd>ASIC</kwd>
</kwd-group>
<counts>
<page-count count="8"/>
</counts>
<custom-meta-wrap>
<custom-meta>
<meta-name>section-at-acceptance</meta-name>
<meta-value>Sensor Devices</meta-value>
</custom-meta>
</custom-meta-wrap>
</article-meta>
</front>
<body>
<sec id="s1">
<title>1 Introduction</title>
<p>X-ray radiation is widely used for digital imaging in medical, industrial, scientific, cultural heritage, and security applications. The advent of highly integrated electronics has enabled the development of digital imaging devices that combine high-density pixel matrices with in-pixel intelligence, enabling precise energy discrimination during image acquisition. In X-ray imaging, energy discrimination not only enhances image quality by rejecting background noise but also supports advanced measurement techniques, such as those used to identify specific materials within a sample (<xref ref-type="bibr" rid="B20">Taguchi, 2013</xref>; <xref ref-type="bibr" rid="B19">Stein et al., 2023</xref>; <xref ref-type="bibr" rid="B21">Tortora et al., 2022</xref>). Achieving superior image quality requires balancing different detector capabilities, in particular spatial and energy resolution. Improvements in the spatial resolution of the detector, typically achieved by designing ever smaller pixels, are counterbalanced by charge-sharing issues that affect the performance of the detector for pixel size below <inline-formula id="inf20">
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</inline-formula> (<xref ref-type="bibr" rid="B14">Mathieson et al., 2002</xref>). Since their first implementations in the late 1970s, Hybrid-Pixel-Detectors (HPDs) based on VLSI readout ASICs have attracted the interest of researchers thanks to Moore&#x2019;s Law-driven increases in pixel capacity. A continuous increase in the number of functions integrated in the pixel cell was possible and particle sensing techniques gained a strong advantage in terms of signal-to-noise ratio, mainly due to the reduced capacitance at the front-end input node. This promising scenario motivated researchers to strive for detectors with higher spatial resolution and sensitivity. Significant efforts have led to the development of several sensor modules, some of which exhibit exceptional performance metrics. In particular, sensor modules such as the Medipix/Timepix (CERN, <xref ref-type="bibr" rid="B13">Llopart et al. (2022)</xref>; <xref ref-type="bibr" rid="B18">Sriskaran et al. (2024)</xref>), EIGER (Dectris Inc., <xref ref-type="bibr" rid="B16">Radicci et al. (2012)</xref>), and PIXIE (Pixirad Imaging Counters Srl, INFN Spin-off, <xref ref-type="bibr" rid="B2">Bellazzini et al. (2013)</xref>; <xref ref-type="bibr" rid="B3">Bellazzini et al. (2015)</xref>) have demonstrated outstanding capabilities. However, their energy and spatial resolution still limit the sensitivity of many of the measurement setups or equipment in which they are involved. In these devices, the output signal of the pixel amplifier is continuously compared with a global threshold, and the content of a dedicated counter is incremented whenever the signal crosses it, or alternatively, the amplitude of the signal is sampled by means of time-over-threshold techniques. In these architectures, imaging performance is inherently limited by electronic noise, threshold uniformity, and charge sharing issues. While these challenges can be mitigated to some extent by design-for-matching techniques and intelligent in-pixel charge summing schemes (<xref ref-type="bibr" rid="B3">Bellazzini et al., 2015</xref>; <xref ref-type="bibr" rid="B18">Sriskaran et al., 2024</xref>), they cannot be completely eliminated. For small-pixel devices, charge sharing remains the primary limiting factor for both energy and spatial resolution (<xref ref-type="bibr" rid="B1">Ballabriga et al., 2020</xref>). The ASIX (Analog Spectral Imager for X-rays) R&#x26;D project is focused on developing a small-scale <inline-formula id="inf21">
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</inline-formula> technology demonstrator aimed at overcoming fundamental limitations in HPDs used for X-ray spectral imaging. ASIX will incorporate 50 <inline-formula id="inf22">
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</inline-formula>m pixels in a hexagonal array with single-photon, ultra-low-noise analog readout (<inline-formula id="inf23">
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</inline-formula> ENC), capable of precisely sampling the full charge distribution generated by the X-ray photon absorption, thus enabling high spatial (10 <inline-formula id="inf24">
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</inline-formula>m) and energy resolution (350&#xa0;eV FWHM at 8&#xa0;keV) in a single measurement. Thanks to its targeted performance, ASIX has the potential to improve sensitivity in applications requiring precise determination of both the energy and position of detected X-ray photons. The following sections outline our approach and report initial results from the ASIX Minimum Viable Product (ASIX-MVP), a CNTT-funded project to develop an intermediate HPD prototype designed to validate preliminary models predicting the resolution performance envisioned for the ASIX demonstrator.</p>
</sec>
<sec id="s2">
<title>2 Hybrid pixel architecture for precise charge cluster reconstruction</title>
<p>In pixel detectors, charge sharing occurs when an incoming X-ray photon deposits charge that spreads across multiple adjacent pixels, making it difficult to assign the event to a single pixel. Traditionally, in photon counting detectors, charge sharing is considered a drawback because it degrades both energy resolution and positional accuracy by splitting charge among neighboring pixels (<xref ref-type="bibr" rid="B6">Delogu et al., 2023</xref>). In systems with analog readout, charge sharing is a key factor enabling sub-pixel resolution imaging, delivering higher precision as the average size of the charge cluster increases. Unfortunately, while the sensor&#x2019;s spatial resolution benefits from charge sharing, the energy resolution does not. Indeed, electronic noise comes into play, limiting the best achievable energy resolution. As the average cluster size increases, so does the uncertainty in the sum of the individual pixel signals (<xref ref-type="bibr" rid="B8">Dinapoli et al. (2014)</xref>; <xref ref-type="bibr" rid="B4">Cartier et al. (2016)</xref>). It must be noted that it is always possible to filter data to limit the average cluster size, thus improving the final energy resolution. However, this filtering negatively affects the spatial resolution and the sensor&#x2019;s data production rate. As a matter of fact, pixel detector systems do not perform equally well in all this metrics, and a trade-off must be set by tuning the sensor specifications in terms of pixel size, electronic noise, and sensor thickness. In our design we combine a fine-pitch <inline-formula id="inf25">
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</inline-formula>m pixel and an ultra-low-noise, fully analog readout with a self-triggering logic capable of identifying the pixel with the maximum charge and selecting it for readout along with its six neighbors (hexagonal matrix). With such detailed information available offline for every single photon, we shape the charge cluster by comparing the seven-pixel charge content against a digital threshold set at the pixel&#x2019;s noise level, after which we reconstruct:<list list-type="simple">
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<p>
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<p>Given the ASIX&#x2019;s baseline specifications, namely, the <inline-formula id="inf28">
<mml:math id="m28">
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</inline-formula> thick silicon sensor, this approach is expected to deliver simultaneous moderate sub-pixel resolution (<inline-formula id="inf30">
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</inline-formula>, FWHM at 8&#xa0;keV) X-ray imaging. A drawback of this charge-cluster reconstruction is the increased processing time per event. However, ASIX will counteract this side-effect by employing a highly parallelized architecture, distributing workload across multiple Analog-to-Digital-Converters (ADCs) integrated on chip with a density of <inline-formula id="inf32">
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</inline-formula>. This will allow simultaneous digitization of multiple clusters. The 65-nm CMOS technology, selected for the ASIX demonstrator, enables the implementation of a highly packed digital electronics in the output data path, leading to high-speed serialization and supporting a rate capability of up to <inline-formula id="inf33">
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</sec>
<sec id="s3">
<title>3 Minimum-viable-product implementation and early results</title>
<p>INFN and Fondazione Bruno Kessler, supported the ASIX-MVP project, which aimed to develop a Minimum-Viable-Product (MVP) for the ASIX demonstrator. The goal was to demonstrate the effectiveness of our preliminary models in predicting the performance of our sensor given the configuration in terms of pixel size, sensor material and thickness, and readout noise. The MVP builds upon XPOL-III, a large scale <inline-formula id="inf34">
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<mml:msup>
<mml:mrow>
<mml:mi>m</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>, poses a significant limitation for the use cases targeted by ASIX. However, its pixel geometry and readout principle, namely, 50 <inline-formula id="inf43">
<mml:math id="m43">
<mml:mrow>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m hexagonal arrangement and analog readout, are fully compatible with ASIX. Combined with its good noise performance and response uniformity, these features made XPOL-III a suitable candidate for the MVP development.</p>
<p>Although our baseline sensor is a <inline-formula id="inf44">
<mml:math id="m44">
<mml:mrow>
<mml:mo>&#x223c;</mml:mo>
<mml:mn>300</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m silicon, coupling the ASIX readout to sensors made of different materials and thicknesses would broaden the range of potential applications for the new device. With this in mind, ASIX-MVP was designed to exploit the versatility that is typical of hybrid pixel detectors.</p>
<p>In December 2024, we delivered two HPD variants:<list list-type="simple">
<list-item>
<p>
<inline-formula id="inf45">
<mml:math id="m45">
<mml:mrow>
<mml:mo>&#x2022;</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> a <inline-formula id="inf46">
<mml:math id="m46">
<mml:mrow>
<mml:mn>750</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m thick Cadmium-Telluride (CdTe) Schottky-type sensor with <inline-formula id="inf47">
<mml:math id="m47">
<mml:mrow>
<mml:mn>100</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m pixels</p>
</list-item>
<list-item>
<p>
<inline-formula id="inf48">
<mml:math id="m48">
<mml:mrow>
<mml:mo>&#x2022;</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> a <inline-formula id="inf49">
<mml:math id="m49">
<mml:mrow>
<mml:mn>300</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m thick n-on-p Silicon (Si) sensor with <inline-formula id="inf50">
<mml:math id="m50">
<mml:mrow>
<mml:mn>50</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m pixels</p>
</list-item>
</list>
</p>
<p>Both coupled to the same XPOL-III readout ASIC.</p>
<p>In the following subsections, we synthesize the ASIX MVPs basic properties evaluation process and its outcomes. The basic characteristics of the Si and CdTe hybrids are summarized in <xref ref-type="table" rid="T1">Table 1</xref>.</p>
<table-wrap id="T1" position="float">
<label>TABLE 1</label>
<caption>
<p>Summary of the basic properties of the ASIX-MVP HPDs.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th align="left">Parameter</th>
<th align="left">CdTe</th>
<th align="left">Si</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">Number of pixels</td>
<td align="left">
<inline-formula id="inf51">
<mml:math id="m51">
<mml:mrow>
<mml:mn>26</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mn>752</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mn>152</mml:mn>
<mml:mo>&#xd7;</mml:mo>
<mml:mn>176</mml:mn>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
</inline-formula>
</td>
<td align="left">
<inline-formula id="inf52">
<mml:math id="m52">
<mml:mrow>
<mml:mn>107</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mn>008</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mn>304</mml:mn>
<mml:mo>&#xd7;</mml:mo>
<mml:mn>352</mml:mn>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
</inline-formula>
</td>
</tr>
<tr>
<td align="left">Pixel pitch</td>
<td align="left">100&#xa0;<inline-formula id="inf53">
<mml:math id="m53">
<mml:mrow>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m</td>
<td align="left">50&#xa0;<inline-formula id="inf54">
<mml:math id="m54">
<mml:mrow>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m</td>
</tr>
<tr>
<td align="left">Thickness</td>
<td align="left">750&#xa0;<inline-formula id="inf55">
<mml:math id="m55">
<mml:mrow>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m</td>
<td align="left">275&#xa0;<inline-formula id="inf56">
<mml:math id="m56">
<mml:mrow>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m</td>
</tr>
<tr>
<td align="left">Shaping time</td>
<td align="left">1&#xa0;<inline-formula id="inf57">
<mml:math id="m57">
<mml:mrow>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>s</td>
<td align="left">1&#xa0;<inline-formula id="inf58">
<mml:math id="m58">
<mml:mrow>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>s</td>
</tr>
<tr>
<td align="left">Pixel Noise (ENC)</td>
<td align="left">60&#xa0;<inline-formula id="inf59">
<mml:math id="m59">
<mml:mrow>
<mml:msup>
<mml:mrow>
<mml:mi>e</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
</mml:mrow>
</mml:msup>
</mml:mrow>
</mml:math>
</inline-formula>
</td>
<td align="left">70&#xa0;<inline-formula id="inf60">
<mml:math id="m60">
<mml:mrow>
<mml:msup>
<mml:mrow>
<mml:mi>e</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
</mml:mrow>
</mml:msup>
</mml:mrow>
</mml:math>
</inline-formula>
</td>
</tr>
<tr>
<td align="left">Energy resolution (FWHM)<xref ref-type="table-fn" rid="Tfn1">
<sup>1</sup>
</xref>
</td>
<td align="left">780&#xa0;eV&#xa0;(at <inline-formula id="inf61">
<mml:math id="m61">
<mml:mrow>
<mml:mn>17.5</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula>)</td>
<td align="left">620&#xa0;eV (at <inline-formula id="inf62">
<mml:math id="m62">
<mml:mrow>
<mml:mn>9.7</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula>)</td>
</tr>
<tr>
<td align="left">Spatial resolution<xref ref-type="table-fn" rid="Tfn2">
<sup>2</sup>
</xref>
</td>
<td align="left">
<inline-formula id="inf63">
<mml:math id="m63">
<mml:mrow>
<mml:mn>20</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m</td>
<td align="left">
<inline-formula id="inf64">
<mml:math id="m64">
<mml:mrow>
<mml:mn>7</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m</td>
</tr>
<tr>
<td align="left">Full scale linear range (FSLR)</td>
<td align="left">
<inline-formula id="inf65">
<mml:math id="m65">
<mml:mrow>
<mml:mn>130</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi mathvariant="normal">k</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>eV</td>
<td align="left">
<inline-formula id="inf66">
<mml:math id="m66">
<mml:mrow>
<mml:mn>110</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi mathvariant="normal">k</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>eV</td>
</tr>
<tr>
<td align="left">Minimum trigger threshold</td>
<td align="left">
<inline-formula id="inf67">
<mml:math id="m67">
<mml:mrow>
<mml:mo>&#x223c;</mml:mo>
<mml:mn>1.5</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>&#xa0;<inline-formula id="inf68">
<mml:math id="m68">
<mml:mrow>
<mml:mi mathvariant="normal">k</mml:mi>
<mml:mi>e</mml:mi>
<mml:mi>V</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> (1% of FSLR)</td>
<td align="left">
<inline-formula id="inf69">
<mml:math id="m69">
<mml:mrow>
<mml:mo>&#x223c;</mml:mo>
<mml:mn>1.0</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>&#xa0;<inline-formula id="inf70">
<mml:math id="m70">
<mml:mrow>
<mml:mi mathvariant="normal">k</mml:mi>
<mml:mi>e</mml:mi>
<mml:mi>V</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> (1% of FSLR)</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn id="Tfn1">
<label>1</label>
<p>FWHM measurements at Mo-<inline-formula id="inf71">
<mml:math id="m71">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> <inline-formula id="inf72">
<mml:math id="m72">
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mn>17.4</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> and Au-<inline-formula id="inf73">
<mml:math id="m73">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>(<inline-formula id="inf74">
<mml:math id="m74">
<mml:mrow>
<mml:mn>9.7</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula>) as shown in <xref ref-type="fig" rid="F2">Figure 2</xref> and corrected for the excess noise contribution due to the online pedestal subtraction.</p>
</fn>
<fn id="Tfn2">
<label>2</label>
<p>X-ray source: X-ray, Ag (25&#xa0;kV) for CdTe, Au (10&#xa0;kV) for Si.</p>
</fn>
</table-wrap-foot>
</table-wrap>
<sec id="s3-1">
<title>3.1 Detector assembly and initial test</title>
<p>Upon completion of assembly in late 2024, we installed the hybrids in a custom designed detector housing which provides light shielding and dry-air environment enabling the cooling down to <inline-formula id="inf75">
<mml:math id="m75">
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>30</mml:mn>
<mml:mo>&#xb0;</mml:mo>
<mml:mi>C</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>. This temperature control is particularly beneficial for long-exposure operations of these detectors. We then performed preliminary tests to evaluate sensors performance.</p>
<p>Our initial tests focused on evaluating the pixel noise. Pixel noise was estimated by analyzing the pedestal residuals of 100 pixels located at the sensor center; for each pixel, the standard deviation of the residuals was computed, and the mean of these values was taken as the representative noise level. This analysis revealed a slight difference between the CdTe and Si hybrids pixel&#x2019;s noise, yielding <inline-formula id="inf76">
<mml:math id="m76">
<mml:mrow>
<mml:mn>60</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:msup>
<mml:mrow>
<mml:mi>e</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
</mml:mrow>
</mml:msup>
</mml:mrow>
</mml:math>
</inline-formula> and <inline-formula id="inf77">
<mml:math id="m77">
<mml:mrow>
<mml:mn>70</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:msup>
<mml:mrow>
<mml:mi>e</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
</mml:mrow>
</mml:msup>
</mml:mrow>
</mml:math>
</inline-formula> ENC respectively. Although sensor leakage current typically impacts noise performance, in our case it appears negligible. We observed no significant change in noise across a <inline-formula id="inf78">
<mml:math id="m78">
<mml:mrow>
<mml:mn>50</mml:mn>
<mml:mo>&#xb0;</mml:mo>
<mml:mi>C</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> operating temperature range, despite leakage current varying by several orders of magnitude. Since the overall noise performance remained within <inline-formula id="inf79">
<mml:math id="m79">
<mml:mrow>
<mml:mo>&#xb1;</mml:mo>
<mml:mn>10</mml:mn>
<mml:mi>%</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> of our original expectations, we decided to postpone further investigations on this matter.</p>
</sec>
<sec id="s3-2">
<title>3.2 Spatial resolution</title>
<p>As a first check of the imaging performance of our devices, we performed a basic analysis of the Huttner 18-lead test pattern image response. The Huttner test pattern is a standard phantom used for estimation of the resolving power of a detection system for X-ray imaging. It consists of a <inline-formula id="inf80">
<mml:math id="m80">
<mml:mrow>
<mml:mn>50</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m thick lead foil with slits at ever increasing density. The resolving power of the imaging system can be roughly assessed by analyzing the transmission image acquired through the phantom. We complemented the Huttner test with the Edge-Spread-Function (ESF) analysis based on the slanted-edge technique (<xref ref-type="bibr" rid="B17">Samei et al., 1998</xref>). In this imaging setup, the CdTe and Si hybrids were illuminated using a silver (Ag) target X-ray tube operated at 25&#xa0;kV and one with gold (Au) target operated at 10&#xa0;kV, respectively. Specifically for the CdTe setup, the X-ray source configuration was chosen to avoid resolution degradation due to cadmium (Cd) fluorescence.</p>
<p>During the imaging performance evaluation test campaign, we formed the images binning the estimated photon absorption point onto a two-dimensional reticle with <inline-formula id="inf81">
<mml:math id="m81">
<mml:mrow>
<mml:mn>15</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
<mml:mtext>m</mml:mtext>
<mml:mo>&#xd7;</mml:mo>
<mml:mn>15</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
<mml:mtext>m</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> for the CdTe and <inline-formula id="inf82">
<mml:math id="m82">
<mml:mrow>
<mml:mn>10</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
<mml:mtext>m</mml:mtext>
<mml:mo>&#xd7;</mml:mo>
<mml:mn>10</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
<mml:mtext>m</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> virtual pixel for the silicon sensor module. We filtered data selecting events with up-to four pixels, which represents more than <inline-formula id="inf83">
<mml:math id="m83">
<mml:mrow>
<mml:mn>90</mml:mn>
<mml:mi>%</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> of the total. We computed the absorption point by applying basic center-of-gravity calculation. This technique is very simple and suitable for ease integration into hardware. However, more advanced techniques, aiming at reconstructing the centroid of the charge distribution, have the potential to provide more accurate results thus delivering even higher resolution images. We plan to explore the impact of such techniques in the near future. For the purpose of this paper, results obtained with the center-of-gravity calculation are already satisfactory. For the CdTe sensor, we estimated the spatial resolution, by means of the slanted-edge technique, acquiring an image of the edge of a <inline-formula id="inf84">
<mml:math id="m84">
<mml:mrow>
<mml:mn>500</mml:mn>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>m thick tungsten (W) tile with <inline-formula id="inf85">
<mml:math id="m85">
<mml:mrow>
<mml:mo>&#x223c;</mml:mo>
<mml:mn>0.06</mml:mn>
<mml:mtext>&#x2009;rad</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> inclination with respect to the pixel rows orientation. We analyzed the edge profile in a <inline-formula id="inf86">
<mml:math id="m86">
<mml:mrow>
<mml:mn>100</mml:mn>
<mml:mo>&#xd7;</mml:mo>
<mml:mn>40</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> pixels roi. We finally estimated a spatial resolution of approximately <inline-formula id="inf87">
<mml:math id="m87">
<mml:mrow>
<mml:mn>20</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
<mml:mtext>m</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula>, which was consistent with the <inline-formula id="inf88">
<mml:math id="m88">
<mml:mrow>
<mml:mn>40</mml:mn>
<mml:mi>%</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> modulation at <inline-formula id="inf89">
<mml:math id="m89">
<mml:mrow>
<mml:mn>10</mml:mn>
<mml:mtext>&#x2009;lp/mm</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> estimation performed by analyzing the intensity profile on the Huttner test image. Thanks to the much smaller pixel size, the Si sensor modules exhibit higher spatial resolution making our Huttner test pattern ineffective, showing nearly full modulation at the densest pattern <inline-formula id="inf90">
<mml:math id="m90">
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mn>10</mml:mn>
<mml:mtext>&#x2009;lp/mm</mml:mtext>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>. We analyzed the intensity profile of the <inline-formula id="inf91">
<mml:math id="m91">
<mml:mrow>
<mml:mo>&#x223c;</mml:mo>
<mml:mn>0.02</mml:mn>
<mml:mtext>&#x2009;rad</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> inclination edge in a <inline-formula id="inf92">
<mml:math id="m92">
<mml:mrow>
<mml:mn>100</mml:mn>
<mml:mo>&#xd7;</mml:mo>
<mml:mn>40</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> pixels roi in a portion of the Huttner test pattern image as shown in <xref ref-type="fig" rid="F1">Figure 1</xref>. We estimated a spatial resolution of <inline-formula id="inf93">
<mml:math id="m93">
<mml:mrow>
<mml:mn>7</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
<mml:mtext>m</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula>, corresponding to <inline-formula id="inf94">
<mml:math id="m94">
<mml:mrow>
<mml:mo>&#x223c;</mml:mo>
<mml:mn>50</mml:mn>
<mml:mi>%</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> modulation at <inline-formula id="inf95">
<mml:math id="m95">
<mml:mrow>
<mml:mn>30</mml:mn>
<mml:mtext>&#x2009;lp/mm</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> or up to <inline-formula id="inf96">
<mml:math id="m96">
<mml:mrow>
<mml:mn>50</mml:mn>
<mml:mtext>&#x2009;lp/mm</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> at <inline-formula id="inf97">
<mml:math id="m97">
<mml:mrow>
<mml:mn>10</mml:mn>
<mml:mi>%</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> modulation (<xref ref-type="fig" rid="F1">Figure 1</xref>). We confirmed such measurement by analyzing the same W-tile edge as we have done evaluating the CdTe spatial resolution.</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>MVPs image data acquired for the evaluation of the spatial resolution (top), together with the MTF plots (bottom). For the silicon sensor (left), we analyzed the profile of a <inline-formula id="inf98">
<mml:math id="m98">
<mml:mrow>
<mml:mo>&#x223c;</mml:mo>
<mml:mn>0.02</mml:mn>
<mml:mtext>&#x2009;rad</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> inclined edge in a <inline-formula id="inf99">
<mml:math id="m99">
<mml:mrow>
<mml:mn>100</mml:mn>
<mml:mo>&#xd7;</mml:mo>
<mml:mn>40</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> pixels ROI from the Huttner test pattern image acquired with <inline-formula id="inf100">
<mml:math id="m100">
<mml:mrow>
<mml:mn>10</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
<mml:mtext>m</mml:mtext>
<mml:mo>&#xd7;</mml:mo>
<mml:mn>10</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
<mml:mtext>m</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> binning. For the CdTe sensor (right), we analyzed the profile of a <inline-formula id="inf101">
<mml:math id="m101">
<mml:mrow>
<mml:mo>&#x223c;</mml:mo>
<mml:mn>0.06</mml:mn>
<mml:mtext>&#x2009;rad</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> inclined edge in a <inline-formula id="inf102">
<mml:math id="m102">
<mml:mrow>
<mml:mn>100</mml:mn>
<mml:mo>&#xd7;</mml:mo>
<mml:mn>40</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> pixels ROI from the Huttner test pattern image acquired with <inline-formula id="inf103">
<mml:math id="m103">
<mml:mrow>
<mml:mn>15</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
<mml:mtext>m</mml:mtext>
<mml:mo>&#xd7;</mml:mo>
<mml:mn>15</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>&#x3bc;</mml:mi>
<mml:mtext>m</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> binning. Images were formed by accumulating clusters up to four pixels in size.</p>
</caption>
<graphic xlink:href="fsens-06-1599365-g001.tif">
<alt-text content-type="machine-generated">Two images are shown. The left image displays horizontal line patterns with varying frequencies labeled from ten to two point five line pairs per millimeter, used for modulation transfer function (MTF) analysis. Below it is a graph of MTF versus line pairs per millimeter, showing a downward trend. The right image contains an edge spread function (ESF) area marked for analysis. Below it is another MTF graph, similarly showing a downward trend.</alt-text>
</graphic>
</fig>
</sec>
<sec id="s3-3">
<title>3.3 Energy resolution</title>
<p>We evaluated energy resolution FWHM by analyzing the characteristic fluorescence radiation emitted by high-purity samples. For the CdTe sensor, we collected Molybdenum <inline-formula id="inf104">
<mml:math id="m104">
<mml:mrow>
<mml:mi>k</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>-lines fluorescence by illuminating a <inline-formula id="inf105">
<mml:math id="m105">
<mml:mrow>
<mml:mn>99.9</mml:mn>
<mml:mi>%</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> pure Mo sample with a silver target X-ray tube operated at 25&#xa0;kV. For the silicon sensor, we acquired the gold <inline-formula id="inf106">
<mml:math id="m106">
<mml:mrow>
<mml:mi>L</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>-lines fluorescence spectrum emitted by a <inline-formula id="inf107">
<mml:math id="m107">
<mml:mrow>
<mml:mn>99.9</mml:mn>
<mml:mi>%</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> pure Au sample. In both test cases, we obtained pulse-height distributions using data collected from a group of 100 pixels located at the center of each detector. We filtered data selecting only those events with only one pixel exceeding the 1-sigma noise-level threshold. It limits the analysis to roughly <inline-formula id="inf108">
<mml:math id="m108">
<mml:mrow>
<mml:mn>10</mml:mn>
<mml:mi>%</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> of the collected photons. <xref ref-type="fig" rid="F2">Figure 2</xref> shows the spectra acquired after minimal equalization of the pixels&#x2019; response function. We fitted data with independent Gaussian functions. The limited number of counts, registered in the low intensity peaks, determines the poor fitting accuracy. The latter, in conjunction with background effects which are related to the measurement setup, prevent us from focusing on those peak statistics for estimating the detector energy resolution. We postpone conducting deeper analysis on this topic to future measurements. Moreover, the presence of the <inline-formula id="inf109">
<mml:math id="m109">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
<mml:mn>1,2</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> doublet in the gold spectrum <inline-formula id="inf110">
<mml:math id="m110">
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mn>11.4</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>, makes it not an ideal reference peak to estimate the detector performance. Energy resolution was then estimated at the Mo-<inline-formula id="inf111">
<mml:math id="m111">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> <inline-formula id="inf112">
<mml:math id="m112">
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mn>17.4</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> for the CdTe module and at the Au-<inline-formula id="inf113">
<mml:math id="m113">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> <inline-formula id="inf114">
<mml:math id="m114">
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mn>9.7</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> peak for the Si module. We emphasize that, in this measurement, due to the online pedestal subtraction, we are artificially introducing an excess noise contribution which we estimate to be half of the original electronic noise <inline-formula id="inf115">
<mml:math id="m115">
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mi>E</mml:mi>
<mml:mi>N</mml:mi>
<mml:mi>C</mml:mi>
<mml:mo>/</mml:mo>
<mml:msqrt>
<mml:mrow>
<mml:mi>n</mml:mi>
</mml:mrow>
</mml:msqrt>
<mml:mo>,</mml:mo>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>n</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>4</mml:mn>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>, yielding roughly <inline-formula id="inf116">
<mml:math id="m116">
<mml:mrow>
<mml:mn>300</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>e</mml:mi>
<mml:mi>V</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>. The online pedestal subtraction is constrained by the DAQ electronics and is not mandatory for proper sensor operation. It could be replaced by a standard offline pedestal subtraction with negligible excess noise. Therefore, we estimate the sensors&#x2019; intrinsic energy resolution by removing this excess noise from the FWHM measured at the main peaks of the spectra shown in <xref ref-type="fig" rid="F2">Figure 2</xref>. With this in mind, we estimate an energy resolution of <inline-formula id="inf117">
<mml:math id="m117">
<mml:mrow>
<mml:mn>780</mml:mn>
<mml:mo>&#xb1;</mml:mo>
<mml:mn>30</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>e</mml:mi>
<mml:mi>V</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> (5% FWHM at <inline-formula id="inf118">
<mml:math id="m118">
<mml:mrow>
<mml:mn>17.5</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula>) and <inline-formula id="inf119">
<mml:math id="m119">
<mml:mrow>
<mml:mn>620</mml:mn>
<mml:mo>&#xb1;</mml:mo>
<mml:mn>30</mml:mn>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi>e</mml:mi>
<mml:mi>V</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> (7% FWHM at <inline-formula id="inf120">
<mml:math id="m120">
<mml:mrow>
<mml:mn>9.7</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula>), for the CdTe and the silicon sensor respectively. The CdTe sensor shows a degradation beyond the electronic noise limit (<inline-formula id="inf121">
<mml:math id="m121">
<mml:mrow>
<mml:mo>&#x223c;</mml:mo>
<mml:mn>670</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> eV), which we believe may be due to factors such as a drift in charge collection efficiency over the course of the data acquisition. Further investigation is planned, aiming to improve the outcomes of this measurement. On the other hand, for the Si sensor, the spread in the energy measurement is primarily dominated by the electronic noise.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>MVPs spectral data. (left) shows the Gold <inline-formula id="inf122">
<mml:math id="m122">
<mml:mrow>
<mml:mi>L</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>-lines fluorescence spectrum (<inline-formula id="inf123">
<mml:math id="m123">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
<mml:mn>1,2</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mn>9.7</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula>, <inline-formula id="inf124">
<mml:math id="m124">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
<mml:mn>1,2</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mn>11.5</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula>, <inline-formula id="inf125">
<mml:math id="m125">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b3;</mml:mi>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mn>13.4</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula>) as recorded by the silicon sensor module. In this measurement we restricted the analysis to events with a one-pixel cluster size from a group of <inline-formula id="inf126">
<mml:math id="m126">
<mml:mrow>
<mml:mo>&#x223c;</mml:mo>
<mml:mn>100</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula> pixels at the center of the sensor&#x2019;s active area. (right) shows the Molybdenum <inline-formula id="inf127">
<mml:math id="m127">
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>-lines fluorescence spectrum (<inline-formula id="inf128">
<mml:math id="m128">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
<mml:mn>1,2</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mn>17.4</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula>, <inline-formula id="inf129">
<mml:math id="m129">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
<mml:mn>1</mml:mn>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>3</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mn>19.6</mml:mn>
<mml:mtext>&#x2009;keV</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula>) as recorded by the CdTe sensor module. The measured FWHM incorporates the excess electronic noise due to online pedestal subtraction, which we estimated to be roughly <inline-formula id="inf130">
<mml:math id="m130">
<mml:mrow>
<mml:mn>300</mml:mn>
<mml:mtext>&#x2009;eV</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> FWHM for both sensor modules. The energy scale was calibrated by linear regression, incorporating Fe-55 calibration data (not shown) alongside the measured spectra.</p>
</caption>
<graphic xlink:href="fsens-06-1599365-g002.tif">
<alt-text content-type="machine-generated">Two side-by-side graphs display energy spectra, each with counts versus channel. The left graph shows peaks at 9.69 keV, 11.32 keV, and 13.15 keV, marked by full width at half maximum (FWHM) values of 687, 766, and 948 eV respectively. The right graph displays peaks at 17.47 keV and 19.73 keV, with FWHM values of 841 and 1029 eV. Both graphs include axes labeled with energies in keV and have a blue shaded area indicating data distribution.</alt-text>
</graphic>
</fig>
</sec>
</sec>
<sec id="s4">
<title>4 Application outlook</title>
<p>Thanks to the fine pitch pixels, fully-analog event-driven readout, and targeted energy and spatial resolution, the ASIX&#x2019;s expected performance, combined with the versatility of hybrid pixel detectors, would offer several advantages over similar state-of-the-art detectors, opening the door to a wide range of applications that benefit from high-resolution effective single-photon processing. These applications can be broadly grouped into three main areas which we list in the following sub-sections.</p>
<sec id="s4-1">
<title>4.1 Material science and analytical imaging</title>
<p>X-ray Diffraction analysis (XRD) is pivotal in material science, serving academia and industry. The market relies on XRD for detailed crystallographic, chemical, and physical material data. While typical 2-D XRD detectors provide good positional and angular resolution, they often lack energy resolution. In practice, most XRD equipment makes use of Copper (Cu) X-ray tubes which emit 8.048&#xa0;keV <inline-formula id="inf131">
<mml:math id="m131">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>, 8.029&#xa0;keV <inline-formula id="inf132">
<mml:math id="m132">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>, 8.905&#xa0;keV Cu-<inline-formula id="inf133">
<mml:math id="m133">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> radiation. Isolating the Cu-<inline-formula id="inf134">
<mml:math id="m134">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> radiation from the Cu-<inline-formula id="inf135">
<mml:math id="m135">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> line is essential for achieving the best measurement accuracy. Current state-of-the-art pixel detectors do not have sufficiently good energy resolution to accomplish this task. As a result, passive k-edge absorption filtering is typically used (e.g., Nickel, 8.333&#xa0;keV&#xa0;K-edge). However, passive filters introduce artifacts, due to the K-edge itself. They also attenuate the primary peak and still leave residual Cu-<inline-formula id="inf136">
<mml:math id="m136">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> radiation. The ASIX approach addresses these limitations by offering:<list list-type="simple">
<list-item>
<p>
<inline-formula id="inf137">
<mml:math id="m137">
<mml:mrow>
<mml:mo>&#x2022;</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> an efficient electronic &#x201c;<inline-formula id="inf138">
<mml:math id="m138">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> filter&#x201d;, eliminating the need for passive filtering;</p>
</list-item>
<list-item>
<p>
<inline-formula id="inf139">
<mml:math id="m139">
<mml:mrow>
<mml:mo>&#x2022;</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> the option to exploit the monochromatic nature of the Cu-<inline-formula id="inf140">
<mml:math id="m140">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> beam, electronically filtering out the Cu-<inline-formula id="inf141">
<mml:math id="m141">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>, enabling more accurate analysis of complex data;</p>
</list-item>
<list-item>
<p>
<inline-formula id="inf142">
<mml:math id="m142">
<mml:mrow>
<mml:mo>&#x2022;</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> improved rejection of fluorescence background.</p>
</list-item>
</list>
</p>
<p>Similarly, synchrotron-based material science experiments could benefit from the ASIX&#x2019;s performance, enhancing contrast in high-resolution imaging through improved background rejection.</p>
</sec>
<sec id="s4-2">
<title>4.2 Biomedical and preclinical research</title>
<p>ASIX would allow for more precise imaging of biological samples, revealing finer details and structures that lower resolution sensors cannot distinguish (<xref ref-type="bibr" rid="B7">Delogu et al., 2024</xref>; <xref ref-type="bibr" rid="B9">Feruglio et al., 2024</xref>; <xref ref-type="bibr" rid="B5">Christodoulou et al., 2024</xref>; <xref ref-type="bibr" rid="B1">Ballabriga et al., 2020</xref>). Specifically, it would enhance the sensitivity of equipment used in imaging techniques such as X-ray-Absorption-Spectroscopy (XAS) and K-edge Subtraction (KES), enabling better discrimination of different tissues based on their X-ray absorption characteristics. Moreover, ASIX would inherently provide a flexible platform for evaluating advanced data processing techniques, thereby contributing to the medical research community&#x2019;s efforts to improve the accuracy of diagnostic equipment.</p>
</sec>
<sec id="s4-3">
<title>4.3 Astrophysics and satellite remote sensing</title>
<p>X-ray telescopes typically employ focusing mirrors and a combination of CCD-based imaging and/or SDD-based spectroscopic detectors (e.g., Chandra, XMM, eRosita, eXTP/SFA) or, more recently, polarization sensitive gaseous detectors (e.g., PolarLight, IXPE, eXTP/PFA).</p>
<p>The ASIX technology is a natural, high-performance development of the focal plane detectors for future science missions. Next-generation X-ray observatories will require detectors with high quantum efficiency across the soft X-ray band to observe the faint objects that drive their mission science objectives. For example, Lynx, one of the four strategic mission concepts under study for the 2020 Astrophysics Decadal Survey, offers significant advances over previous and planned X-ray missions and provides synergistic observations in the 2030s to a multitude of space and ground-based observatories across all wavelengths (<xref ref-type="bibr" rid="B10">Gaskin et al., 2019</xref>). While purely speculative, it is worth noting the alignment between the envisaged performance of ASIX and the requirements of the Lynx-HDXI instrument (<xref ref-type="bibr" rid="B11">Hull et al., 2019</xref>), particularly in terms of resolving power in both the energy and spatial domains. Thanks to the inherently event-driven nature of its readout, ASIX offers a timing resolution of the order of <inline-formula id="inf143">
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</inline-formula>, enabling the simultaneous measurement of time, energy, and position for each detected photon. A boost in source sensitivity, which can potentially reduce observing times, can be envisaged thanks to the high throughput of the system and the possibility of tailoring the energy range to specific mission objectives.</p>
<p>Moreover, as the space business boasts new investments and opportunities, particularly pushed by cube-satellites and the growing interest in Earth Observations, new opportunities in the field of Space Weather and protection of infrastructures become available for the ASIX technology.</p>
</sec>
</sec>
<sec id="s5">
<title>5 Discussion and conclusion</title>
<p>With the measured <inline-formula id="inf144">
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</inline-formula> spatial resolution and energy resolution (660&#xa0;eV FWHM at 9.7&#xa0;keV) limited by electronic noise in the <inline-formula id="inf145">
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</inline-formula>m thick silicon sensor, the MVP data demonstrate the feasibility of achieving simultaneous high spatial and energy resolution using a small-pixel hybrid pixel detector, paving the way for the next phase of ASIX development. To fully qualify the technology, a new hybrid must be realized, one that integrates a redesigned readout ASIC tailored to the ASIX architecture. The upcoming ASIC will be engineered to meet stringent noise performance requirements (<inline-formula id="inf146">
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</inline-formula>, ENC) while introducing a novel, parallel readout architecture based on multiple on-chip Analog-to-Digital Converters. This enhancement will enable efficient cluster-based readout at high event rates (up to <inline-formula id="inf147">
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<p>In the long term, ASIX is envisioned as a scalable building block for large-area sensor matrices with minimal inactive regions. Its modular architecture ensures that expanded arrays can maintain high-resolution performance with manageable interconnect complexity, supporting deployment in advanced imaging systems across various domains. Over the next 2&#xa0;years (2025&#x2013;2026), the ASIX team will focus on developing this next-generation readout ASIC. In parallel, we will fabricate an edgeless silicon sensor using an innovative construction process built on top of that proposed by <xref ref-type="bibr" rid="B12">Koybasi et al. (2020)</xref>, aimed at preserving wafer integrity without the use of a support wafer. These advancements will be key to transitioning ASIX from a promising demonstrator to a mature, deployable platform for high-performance X-ray spectral imaging. The ASIX project offers a novel approach to overcoming the long-standing trade-off between spatial and energy resolution in hybrid pixel detectors. By leveraging fine-pitch pixels, ultra-low-noise analog readout, and cluster-based reconstruction, ASIX will turn charge-sharing into an asset, enabling sub-pixel localization along with spectral fidelity. With its potential to deliver high-resolution, energy-resolved imaging, ASIX is well positioned to impact a wide range of applications, from materials analysis and biomedical imaging to astrophysics and remote sensing.</p>
</sec>
</body>
<back>
<sec sec-type="data-availability" id="s6">
<title>Data availability statement</title>
<p>The datasets presented in this article are not readily available because the data is private. Requests to access the datasets should be directed to M. Minuti, <email>minuti@infn.it</email>.</p>
</sec>
<sec sec-type="author-contributions" id="s7">
<title>Author contributions</title>
<p>MMi: Writing &#x2013; review and editing, Writing &#x2013; original draft. LB: Writing &#x2013; review and editing. RbB: Writing &#x2013; review and editing. RnB: Writing &#x2013; review and editing. AsB: Writing &#x2013; review and editing. MB: Writing &#x2013; review and editing. AlB: Writing &#x2013; review and editing. PB: Writing &#x2013; review and editing. MC: Writing &#x2013; review and editing. MCV: Writing &#x2013; review and editing. LF: Writing &#x2013; review and editing. LG: Writing &#x2013; review and editing. OH: Writing &#x2013; review and editing. LL: Writing &#x2013; review and editing. VL: Writing &#x2013; review and editing. GM: Writing &#x2013; review and editing. AM: Writing &#x2013; review and editing. MMa: Writing &#x2013; review and editing. FM: Writing &#x2013; review and editing. LO: Writing &#x2013; review and editing. LP: Writing &#x2013; review and editing. MPR: Writing &#x2013; review and editing. MiP: Writing &#x2013; review and editing. MaP: Writing &#x2013; review and editing. AP: Writing &#x2013; review and editing. PP: Writing &#x2013; review and editing. LR: Writing &#x2013; review and editing. AR: Writing &#x2013; review and editing. SR: Writing &#x2013; review and editing. CS: Writing &#x2013; review and editing. SS: Writing &#x2013; review and editing. GS: Writing &#x2013; review and editing. AS: Writing &#x2013; review and editing. GiT: Writing &#x2013; review and editing. GaT: Writing &#x2013; review and editing. MV: Writing &#x2013; review and editing. DZ: Writing &#x2013; review and editing.</p>
</sec>
<sec sec-type="funding-information" id="s8">
<title>Funding</title>
<p>The author(s) declare that financial support was received for the research and/or publication of this article. This work is funded by INFN CSN5, CSN2 and CNTT, the latter by means of the Research for Innovation (R4I) 2023 grant, and Fondazione Bruno Kessler.</p>
</sec>
<ack>
<p>We would like to acknowledge our colleagues Raffaello D&#x2019;Alessandro, Mirko Massi, and Mirko Brianzi from the Physics Department at University of Firenze and INFN for their invaluable support in the ASIX MVP hybrid assembly.</p>
</ack>
<sec sec-type="COI-statement" id="s9">
<title>Conflict of interest</title>
<p>The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
<sec sec-type="ai-statement" id="s10">
<title>Generative AI statement</title>
<p>The author(s) declare that Generative AI was used in the creation of this manuscript to assist in refining the language of specific sections. All technical content, interpretation of data, and scientific conclusions were written and verified by the authors.</p>
<p>Any alternative text (alt text) provided alongside figures in this article has been generated by Frontiers with the support of artificial intelligence and reasonable efforts have been made to ensure accuracy, including review by the authors wherever possible. If you identify any issues, please contact us.</p>
</sec>
<sec sec-type="disclaimer" id="s11">
<title>Publisher&#x2019;s note</title>
<p>All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.</p>
</sec>
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