IWORID 2025

Europe/Zurich
Bratislava, Slovakia

Bratislava, Slovakia

Andrea Sagatova (Slovak University of Technology in Bratislava)
Description

26th International Workshop on Radiation Imaging Detectors

Registration
Registration
Participants

Workshop topics

There are minutes attached to this event. Show them.
    • 17:00 22:00
      Social events: Conference Reception
    • 09:00 10:30
      Detector Systems: Opening, Session 1
    • 10:30 11:00
      Coffee Break 30m
    • 11:00 12:40
      Detector Systems: Session 2
      • 11:00
        Second-Generation Percival Sensor and System for upgraded soft X-ray imaging at FELs and Synchrotrons 20m

        PERCIVAL, "pixellated energy-resolving CMOS imager versatile and large," is a 2-megapixel soft X-ray imager developed for use at FELs and modern-day synchrotrons by a collaboration of light sources (DESY, Elettra, Diamond, Pohang Accelerator Lab, and Soleil) together with Rutherford Appleton Laboratories. To meet the science needs at these facilities, a combination of capabilities is necessary: a large, uninterrupted imaging area with small pixels, high dynamic range, high frame rate, and soft X-ray suitable entrance window to the sensor. PERCIVAL's stitched sensor offers over 4cm x 4cm uninterrupted imaging area (1408x1484 pixels of 27x27 um2). Three gains combine to deliver Percival's dynamic range: in the highest gain, noise levels below 13e- are achieved - suitable for single-photon discrimination down to ~250eV. In the lowest gain, up to 3.6Me- can be digitized per pixel per image. The imager is designed for 300Hz frame rate, operates essentially in a rolling-shutter mode, and can be run correspondingly faster in ROI mode utilizing a reduced number of its rows. BSI processing with thin entrance window makes the sensor suitable for soft X-ray use.

        The first generation of the sensor had some shortcomings - in particular, severe crosstalk in the sensor hampered parallel operation of ADC, streamout, and pixel switches. Circumventing these issues by separating the sensitive ADC operation in time from the aggressors resulted in significantly reduced maximum frame rate - and some non-linearities remained. Moreover, inadequate grounding of the pixel matrix resulted in current bias variation over the matrix ... and ultimately in significantly different baselines at center and edges of the detector. This limited the useable dynamic range in particularly in higher gains ... and rendered pixels at the edges of the sensor useable only in higher-noise, lower-amplification modes. The first-generation readout FPGA card and firmware added restrictions on data streamout speed, limiting the overall sensor operation to below 100Hz frame rate.

        Today, we are commissioning a 2nd-generation sensor and readout:
        The 2nd-generation "respin" sensor's design was modified to eliminate the crippling crosstalk to the ADC, and grounding of the pixel matrix was improved to enable use of the full sensor area also in highest gain modes. In parallel, completely new DAQ hard- and firmware now have the capability to handle data streams at the originally envisioned rates.
        To date, we have verified elimination of the crippling crosstalk and established our capability to use the full sensor - i.e. validated the chip design improvements. We are in the process of bringing the system to the original design speed of 300Hz frame rate - as this entails operating both the digital streamout and the ADCs at almost twice the previously-used clock speeds, debugging and commissioning fully will take some time. We will report on the state of the system, and the performances demonstrated with the upgraded sensor and system.

        Speaker: Cornelia Wunderer (DESY)
      • 11:20
        CYGNUS: Directional recoil detection for dark matter, particle physics and nuclear applications 20m

        The Australian National University (ANU) has been conducting studies in directional detector technology, with the aim of building a large detector called CYGNUS. Eventually, such a detector is likely to be located in Australia's new underground physics laboratory at Stawell in regional Victoria.

        The ANU group leads the experimental efforts of the Australian CYGNUS-Oz consortium through the prototype detectors. The most recent prototype called CYGNUS-n is based on gaseous Time Projection Chamber (TPC) technology. TPCs have an advantage in areas such as directional dark matter searches, as they allow for event-by-event reconstruction of three-dimensional particle tracks with excellent particle discrimination and a high degree of spatial and energy resolution. Recent studies suggest that a large-scale gaseous TPC would be sensitive enough to study solar neutrino fluxes and may offer other novel physics or industrial applications.

        This contribution presents the status and results of studies with CYGNUS-n with the future direction of the dark matter research and other applications like particle and nuclear physics. It focuses on R&D and development of optimal TPCs with specific research focus. This includes studies of gas impurities effect on TPC gain and negative ion drifts and the detachment of the electrons from the gain stage.

        Speaker: Prof. Gregory Lane (Australian National University)
    • 12:40 14:00
      Lunch break Lunch 13.00 1h 20m Brartslava, Slovakia

      Brartslava, Slovakia

      Slovenská technická univerzita v Bratislave Fakulta informatiky a informačných technológií Ilkovičova 6276/2 842 16 Bratislava 4
    • 14:00 15:50
      Space Applications: Session 3
    • 15:50 16:20
      Coffee Break 30m
    • 16:20 18:00
      Poster: Session 1
      • 16:20
        Development and evaluation of linear array type ring detector for patient dose delivery monitoring system in high dose-rate brachytherapy 20m

        High dose-rate brachytherapy (HDR-BT) is a treatment technique in which a radioisotope (RI) is directly inserted into the human body. This allows for minimizing the dose to surrounding critical organs while concentrating the radiation dose on the tumor tissue, resulting in high therapeutic efficacy. Treatment planning for HDR-BT is performed based on anatomical images including the clinical applicator, and the prescribed dose is delivered to the clinical target volume. The dose distribution is determined by adjusting the dwell positions and dwell times of the source within the applicator, necessitating verification of dose accuracy under specific dwell conditions. In external beam radiotherapy, patient-specific quality assurance (PSQA) is routinely performed prior to treatment to verify the patient dose, typically using a flat panel detector mounted on the treatment machine. Similarly, research has been conducted to implement a PSQA system for HDR-BT using flat panel detectors. However, such systems are subject to limitations due to the dependency on irradiation distance and angle of the RI. Therefore, a new approach is required that allows for consistent control of source distance and angle while accommodating the curved geometry of clinical applicators.
        In this study, a ring detector with a fixed radius was developed to evaluate the feasibility of measuring dose distributions under specific RI dwell conditions. Monte Carlo (MC) simulation results using GATE v9.1 were also compared to validate the experimental results. A flexible material based on polydimethylsiloxane (PDMS) polymer was fabricated to allow bending to the irradiation radius of the Iridium-192 (Ir-192) source. Polycrystalline mercury (II) iodide, a material with high radiation conversion efficiency, was used as the sensing material, and mixed with PDMS to create a flexible detector. A flexible printed circuit board (fPCB) with 25 pixel electrodes was configured as a linear array, with each electrode measuring 2 cm × 0.1 cm and spaced at 0.3 cm intervals. The ring detector was constructed by fixing the fPCB into a semicircular shape, resulting in a radius of 3.85 cm.
        The repeatability of the detector was evaluated using the median value of the 25 pixels (57.0 nC), with a relative standard deviation of 0.87% over 10 repeated measurements. The linearity of dose with respect to dwell time showed a coefficient of determination of 0.9997. Dose measurements were conducted at positions spaced 0.5 cm apart from the pixel center point up to a distance of 2.5 cm. The experimental results were compared with MC simulations. The dose distribution decreased linearly as the Ir-192 source moved further from the detector. The slope of the linear function was 0.0051 for the measurement and 0.0137 for the simulation, indicating a difference of 0.0086 and a more gradual decrease in the measured data. Ir-192 follows the inverse square law, resulting in a power function for dose fall-off with distance.
        This study fixed the detector radius at 3.85 cm based on the detector size, resulting in a source-to-surface distance (SSD) of over 1 cm. In the future, by configuring an SSD of less than 1 cm to monitor the rapid intensity changes near the source, a PSQA system capable of verifying the calculated dose of HDR-BT applicators could be established.

        Speaker: Dr Moo-Jae Han (Seoul National University Bundang Hospital)
      • 16:40
        Performance Assessment of PbI₂ and PbO-Based Semiconductor Dosimeters in Ir-192 HDR Brachytherapy: Measurement and Simulation 20m

        High-dose-rate (HDR) brachytherapy using Iridium-192 (Ir-192) sources is widely adopted in the treatment of various cancers due to its ability to deliver concentrated radiation doses with high spatial precision. Accurate dose verification is essential in this modality to ensure both treatment efficacy and patient safety. In this study, we investigate the feasibility and performance of polycrystalline semiconductor dosimeters (PSDs) fabricated with lead (Ⅱ) iodide (PbI₂) and lead oxide (PbO) materials for use in HDR brachytherapy dosimetry. Specifically, we evaluated the distance and angular dependence of these PSDs when exposed to an Ir-192 source, and validated the results through comprehensive Monte Carlo (MC) simulations using the GATE v9.1 toolkit.
        The PbI₂ and PbO materials were fabricated with dimensions of 0.2 cm x 0.2 cm through a polymer mixture, and gold electrodes were formed to construct the detector. Experimental measurements were performed to assess the PSDs’ responses at source-to-surface distances (SSD) ranging from 1 cm to 8 cm and at incident angles from 0° to 60°. In parallel, MC simulations replicated these conditions to model radiation interactions and validate the experimental results.
        For distance dependence, both PSD types showed signal attenuation consistent with the inverse-square law, with power-law exponents of approximately -1.9 for PbI₂ and -1.8 for PbO, in both measurements and simulations. High coefficients of determination (R² > 0.98) confirmed the strong correlation between distance and signal intensity. Additionally, the D50 values, representing the distance at which the normalized signal dropped by 50%, were closely matched between measurement and simulation, with discrepancies less than 0.01 cm for both PSD types. In evaluating angular dependence, both PSDs demonstrated a gradual decline in normalized signal intensity as the irradiation angle increased. The maximum signal reduction at 60° was approximately 25%, indicating significant angular sensitivity. The difference between experimental and simulation data remained within 5% for all angles, with the PbI₂-based PSD exhibiting slightly better agreement than the PbO counterpart. These findings highlight the reproducibility and reliability of the fabricated PSDs and their potential for accurate dosimetry. The use of PbI₂ and PbO as photoconductive materials is particularly promising due to their high atomic numbers and favorable charge transport properties, contributing to efficient photon absorption and stable signal generation. This study is among the first to report on the fabrication of PbI₂ and PbO-based PSDs and their comprehensive characterization under HDR Ir-192 irradiation through both experimental and simulated approaches. Compared to prior works that utilized TlBr or CsPbBr₃ without simulation validation, our dual-method approach enhances confidence in the clinical applicability of these PSDs.
        In conclusion, PbI₂ and PbO-based PSDs demonstrated reliable and predictable responses to Ir-192 irradiation in both distance and angular dependence measurements. The consistency with MC simulations supports the robustness of the fabrication and evaluation methodology. However, the observed angular sensitivity suggests that implementing angular correction factors would be necessary for clinical dosimetry applications. Future studies should focus on optimizing the PSD design for real-time monitoring and incorporating correction algorithms to enhance accuracy in complex treatment geometries.

        Speaker: Dr MOO JAE HAN (Seoul National University Bundang Hospital)
    • 19:20 21:20
      Social events: Boat trip on Danube river
    • 09:00 10:30
      Sensor Materials: Session 4
      • 09:00
        The influence of temperature changes on the spectrometric behavior of Timepix3 detectors with different sensors 20m

        Timepix3 is an advanced hybrid pixel detector designed for precise particle tracking and energy measurement over a wide range of ionizing radiation [1]. Currently, Timepix3 detectors are equipped with a variety of semiconductor sensors, including silicon (Si), silicon carbide (4H-SiC), gallium arsenide (GaAs), and cadmium telluride (CdTe), each offering specific advantages depending on application requirements. Si is known for its excellent energy resolution, although its efficiency declines at higher photon energies. CdTe and GaAs offer higher absorption coefficient, making them more suitable for high-energy γ-ray detection, while SiC stands out for its robustness in demanding radiation and high temperature environments.
        The ability to record individual interactions with precise timing and energy information, combined with a compact design, low power consumption and overall versatility, has led to its adoption in a wide range of applications. Timepix3 detectors have found applications in areas such as medicine [2], high energy and nuclear physics [3], neutron detection [4, 5] and space instrumentation [6], where robust performance and accurate radiation measurement are key requirements. In applications situated in harsh environments, detectors are expected to operate reliably under varying temperature conditions and prolonged exposure to different types of ionizing radiation. Temperature fluctuations are considered a possible factor that could influence detector performance and the accuracy of the acquired spectrometric data. Consequently, it is important to investigate the temperature dependence of such detectors, particularly with regard to their energy resolution and photopeak position.
        To determine this, Timepix3-based detectors equipped with all four available sensor types - Si, 4H-SiC, GaAs and CdTe - were systematically studied. The detectors were thermally stabilized and irradiated using characteristic X-rays and a Am-241 source across an energy range of approximately 8 to 60 keV. Measurements were performed over a temperature interval from 10 ℃ to 80 ℃, with calibration set at 40 ℃. The objective of the present study was to assess the impact of temperature fluctuations on the spectrometric characteristics of the sensors, in terms of energy resolution and photopeak position.
        The results obtained demonstrated a consistent trend across all sensor types. As the temperature increased, the photopeak position gradually shifted to lower energies, causing a reduction in measurement accuracy. This shift became more noticeable at temperatures above 60 °C and was more pronounced at higher photon energies. While the deviation from the calibrated peak position remained within 0-5% at lower temperatures for all detectors regardless of the sensor type, it increased to 3-10% for the detector with a silicon sensor, 5-14% for the 4H-SiC sensor, and reached approximately 6% for the GaAs-based detector at 60 °C. However, at temperatures above 60 °C, the electronic noise in GaAs and CdTe detectors became too high to enable reliable spectrometric analysis. These findings indicate that the temperature dependence of the spectrometric response is primarily influenced by the Timepix3 readout chip, with some contribution from the sensor material itself. In order to ensure accurate measurements across a broader temperature range without the need for active cooling or repeated calibrations at each operating condition, it is beneficial to implement a compensation method that corrects temperature-induced shifts in the spectral data.

        [1] T. Poikela, et al., JINST 9 (2014), C05013
        [2] D. Turecek, et al., Nucl. Instrum. Methods Phys. Res. A 895 (2018), 84-89
        [3] B. Bergmann, et al., Nucl. Instrum. Methods Phys. Res. A 978 (2020) 164401
        [4] C. Granja, et al., JINST 18 (2023) P01003
        [5] C. Oancea, et al., Phys. Med. Biol. 68 (2023) 185017
        [6] C. Granja, et al., JINST 17 (2022) C03019

        The authors acknowledge funding from the Slovak Research and Development Agency (Research Projects APVV-18-0273 and APVV-18-0243).

        Speaker: Nikola Kurucová (Institute of Nuclear and Physical Engineering, Faculty of Electrical Engineering and Information Technology, Slovak University of Technology in Bratislava)
    • 10:30 11:00
      Coffee Break 30m
    • 11:00 12:40
      Sensor Materials: Session 5
    • 12:40 14:00
      Lunch break Lunch 13.00 1h 20m
    • 14:00 15:50
      Detector Systems: Session 6
      • 14:00
        The SABRE South Experiment at the Stawell Underground Physics Laboratory 20m

        SABRE is an international collaboration that will operate similar particle de-
        tectors in the Northern (SABRE North) and Southern Hemispheres (SABRE
        South). This innovative approach distinguishes possible dark matter signals
        from seasonal backgrounds, a pioneering strategy only possible with a southern
        hemisphere experiment. SABRE South is located at the Stawell Underground
        Physics Laboratory (SUPL), in regional Victoria, Australia.
        SUPL is a newly built facility located 1024 m underground (∼2900 m water
        equivalent) within the Stawell Gold Mine and its construction has been com-
        pleted in 2023.
        SABRE South employs ultra-high purity NaI(Tl) crystals immersed in a Linear
        Alkyl Benzene (LAB) based liquid scintillator veto, enveloped by passive steel
        and polyethylene shielding alongside a plastic scintillator muon veto. Signifi-
        cant progress has been made in the procurement, testing, and preparation of
        equipment for installation of SABRE South. The SABRE South muon detector
        and the data acquisition systems are actively collecting data at SUPL and the
        SABRE South’s commissioning is planned to be completed by the end of 2025.
        This presentation will provide an update on the overall progress of the SABRE
        South construction, its anticipated performance, and its potential physics reach.

        Speaker: Zuzana Slavkovská (The Australian National University)
      • 14:20
        Development of Accurate Dosimetry SiPM-based Detectors for FLASH RT 20m

        Radiotherapy (RT) using X-rays is the main treatment strategy employed to treat human tumors with ~50% of all cancer patients receiving RT. The major drawback of RT treatment is that in order to deliver a lethal dose to cancerous cells, short- and long-term adverse side-effects are evident due to the irradiation of the surrounding normal healthy tissues that can severely impact the health and quality of life of the cancer patient.
        One way to circumvent the irradiation of the surrounding tissue is through Proton Beam Therapy (PBT) where instead of photons, protons are used to deliver the radiation with higher precision, thanks to their favorable ratio of Relative dose to Depth (Bragg Peak).
        Another way is through FLASH radiotherapy and particle therapy. Both are performed with the delivery of ultra-high dose rate radiation (UHDR), specifically a dose rate higher than 40 Gy/sec. The advantage of FLASH compared to conventional therapy (CONV) is based on the “FLASH effect”: improved normal tissue sparing while still maintaining tumor control. Accurate dosimetry and real-time beam monitoring are critical for its clinical translation, but current detectors suffer from saturation effects in the signal production and signal read-out when dealing with fast and intense beams.
        We report on our development and preliminary tests of a novel dosimeter for Ultra high-dose rate particle therapy, based on advanced Silicon Photomultiplier (SiPM) detectors coupled with scintillating fibers (SciFi). The SciFi detector aims towards an improved time and space resolution, with respect to the present commercial readout system. It will be suitable for both CONV and UHDR irradiations.
        We will describe the present status of the devices and facilities used for FLASH RT. We will show the preliminary design of the detector that is expected to be tested using a proton UHDR beam with the beam's energy ranging from 70 MeV (CONV) to 228 MeV (FLASH RT). The ultimate goal is a detector suited both for FLASH PBT and for Conventional RT, with good sensitivity, as well as spatial and energy resolution.

        Speaker: Georgios Mystridis (University of Foggia, Fondazione Bruno Kessler)
    • 15:50 16:20
      Coffee Break 30m
    • 16:20 18:00
      Detector Systems: Session 7
    • 18:00 19:30
      Social events: Committee Dinner
    • 09:00 10:30
      Medical Applications: Session 8
    • 10:30 11:00
      Coffee Break 30m
    • 11:00 12:40
      Medical Applications: Session 9
    • 12:40 14:00
      Lunch break Lunch 13.00 1h 20m
    • 14:00 15:50
      Industrial Applications: Session 10
    • 15:50 16:20
      Coffee Break 30m
    • 16:20 18:00
      Poster: Session 2
      • 16:20
        SPECTRUM 1k – Single Pixel Counting Readout Chip with In-Pixel Energy Histogramming 20m

        A new single photon-counting IC prototype called SPECTRUM1k with pixel matrix 40 × 24 and pixel pitch 75 µm is developed by the Microelectronics Group of the AGH University of Krakow as a solution for X-ray color imaging. The chip, produced in CMOS 40 nm technology, is made up of 960 individually configured pixels, each composed of an amplifier, an analog-to-digital converter, and 64 × 12-bit memory cells that allow one to perform in-pixel energy histogramming. Thanks to the proposed architecture working with the 200 MHz chip clock and 1 Gcps/mm2 multi energy photon intensities up-to about 23 ms exposition time is feasible (365 µs exposition time whenever monoenergetic photons are used only). In-pixel offset (Ϭ = 3.5%) and gain (Ϭ = 5.8%) spread, the amplifier performance (ENC = 95 e- rms) and the ADC resolution (ENOB = 5.4 b) allow to convert the incoming photons’ energy with FWHM = 3.7 ke @134.2 keV upon 45 µW (high-speed mode) or 12 µW (low-speed mode) per pixel power consumption.

        Speaker: Piotr Kmon (AGH UST Krakow)
      • 16:40
        Cosmic ray measurements with compact scintillator telescopes and SiPM readout 20m

        The Extreme Energy Events (EEE) Collaboration has built and operated so far a large set of cosmic ray telescopes, based on Multigap Resistive Plate Chambers, which are installed in high school buildings over the Italian territory for scientific and educational activities. To extend the potential of the EEE Project, a number of additional, scintillator-based, cosmic ray telescopes, were built and operated over the last years, as discussed in the present contribution.
        A first detection facility includes four telescopes with two planes of segmented scintillator tiles, and an overall detection area of 40 x 60 cm2, with Silicon Photomultipliers (SiPM) readout on each tile. These
        detectors, which are equipped with low power electronics and environmental sensors, have been used inseveral measurement campaigns over a wide range of geographical latitudes, on board of boats sailing in the Mediterranean and across the Arctic Sea, and have been also installed for long-term experiments at NyȦlesund (79° N), in the Svalbard archipelago. They were used for various analysis, also including the observation of Forbush decrease events in regions characterized by a low geomagnetic cutoff, and to investigate periodic components in the measured muon rate.
        A second facility, mainly used for educational activities within the EEE Collaboration, is represented by the Cosmic Box (CB) detectors, small-size scintillator-based telescopes with SiPM readout, which were designed and built with the help of student teams. Their use allows efficiency measurement of MRPC telescopes and complementary measurements of the cosmic ray flux under conditions where the MRPC telescopes could not be easily installed or by schools not hosting one of the MRPC telescopes. Such detectors have been used since several years in a number of on-site measurements, to investigate the altitude dependence of the cosmic ray flux, in underground sites with a strongly reduced muon flux, and to perform measurements according to the
        school proposals, during the yearly Cosmic Box Contest, where the best proposals are evaluated and awarded.

        Speaker: Dr Cristina Ripoli (University and INFN of Salerno)
    • 20:00 22:00
      Social events: Conference Dinner
    • 09:00 10:30
      Front-end Electronics: Session 11
    • 10:30 11:00
      Coffee Break 30m
    • 11:00 12:40
      Front-end Electronics: Imaging Theory, Session 12
    • 12:40 14:00
      Lunch break Lunch 13.00 1h 20m
    • 14:30 16:00
      Social events: Guided tour around Bratislava