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High count rate effects in event processing for XRISM/Resolve x-ray microcalorimeter: I. Ground test

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arxiv 2501.03283 v1 pith:JMDCHFQV submitted 2025-01-06 astro-ph.IM

classification astro-ph.IM
keywords countx-raydataeffectshighperformancemicrocalorimeterrates
verification ladder T0 review T1 audit T2 compute T3 formal
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The spectroscopic performance of an X-ray microcalorimeter is compromised at high count rates. In this study, we utilize the Resolve X-ray microcalorimeter onboard the XRISM satellite to examine the effects observed during high count rate measurements and propose modeling approaches to mitigate them. We specifically address the following instrumental effects that impact performance: CPU limit, pile-up, and untriggered electrical cross talk. Experimental data at high count rates were acquired during ground testing using the flight model instrument and a calibration X-ray source. In the experiment, data processing not limited by the performance of the onboard CPU was run in parallel, which cannot be done in orbit. This makes it possible to access the data degradation caused by limited CPU performance. We use these data to develop models that allow for a more accurate estimation of the aforementioned effects. To illustrate the application of these models in observation planning, we present a simulated observation of GX 13+1. Understanding and addressing these issues is crucial to enhancing the reliability and precision of X-ray spectroscopy in situations characterized by elevated count rates.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. XRISM insights for interstellar Sulfur

    astro-ph.GA 2025-06 conditional novelty 8.0 of 10

    The paper reports the first high-signal detection of interstellar SII K-beta absorption and a direct measurement of sulfur depletion (40% ± 15%) from combined gas and dust absorption in the GX 340+0 sightline.

  2. The Structure of the Relativistic Fe Line in GX 340+0 as Viewed with XRISM/Resolve, NICER, and NuSTAR

    astro-ph.HE 2025-07 conditional novelty 6.0 of 10

    The Fe K line of GX 340+0 shows a dual-peaked structure with residual narrow emission features at the ~5% level that RELXILLNS reflection modeling alone does not reproduce.

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