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The first cut is the cheapest: optimizing Athena/X-IFU-like TES detectors resolution by filter truncation

dc.contributor.authorCeballos, M. Teresa
dc.contributor.authorCardiel López, Nicolás
dc.contributor.authorCobo, Beatriz
dc.contributor.authorSmith, Stephen J.
dc.contributor.authorWitthoeft, Michael C.
dc.contributor.authorPeille, Philippe
dc.contributor.authorDurkin, Malcolm S.
dc.date.accessioned2024-04-09T08:38:26Z
dc.date.available2024-04-09T08:38:26Z
dc.date.issued2024-03-21
dc.description.abstractThe X-ray Integral Field Unit (X-IFU) instrument on the future ESA mission Athena X-ray Observatory is a cryogenic micro-calorimeter array of Transition Edge Sensor (TES) detectors designed to provide spatially-resolved high-resolution spectroscopy. The onboard reconstruction software provides energy, spatial location and arrival time of incoming X-ray photons hitting the detector. A new processing algorithm based on a truncation of the classical optimal filter and called 0-padding, has been recently proposed aiming to reduce the computational cost without compromising energy resolution. Initial tests with simple synthetic data displayed promising results. This study explores the slightly better performance of the 0-padding filter and assess its final application to real data. The goal is to examine the larger sensitivity to instrumental conditions that was previously observed during the analysis of the simulations. This 0-padding technique is thoroughly tested using more realistic simulations and real data acquired from NASA and NIST laboratories employing X-IFU-like TES detectors. Different fitting methods are applied to the data, and a comparative analysis is performed to assess the energy resolution values obtained from these fittings. The 0-padding filter achieves energy resolutions as good as those obtained with standard filters, even with those of larger lengths, across different line complexes and instrumental conditions. This method proves to be useful for energy reconstruction of X-ray photons detected by the TES detectors provided proper corrections for baseline drift and jitter effects are applied. The finding is highly promising especially for onboard processing, offering efficiency in computational resources and facilitating the análisis of sources with higher count rates at high resolution.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipFondo Europeo de Desarrollo Regional (FEDER)
dc.description.sponsorshipMinisterio de Ciencia e Innovación (España)
dc.description.statuspub
dc.identifier.citationCeballos, M.T., Cardiel, N., Cobo, B. et al. The first cut is the cheapest: optimizing Athena/X-IFU-like TES detectors resolution by filter truncation. Exp Astron 57, 14 (2024). https://doi.org/10.1007/s10686-024-09930-2
dc.identifier.doi10.1007/s10686-024-09930-2
dc.identifier.essn1572-9508
dc.identifier.issn0922-6435
dc.identifier.officialurlhttps://link.springer.com/article/10.1007/s10686-024-09930-2
dc.identifier.urihttps://hdl.handle.net/20.500.14352/102852
dc.journal.titleExperimental Astronomy
dc.language.isoeng
dc.page.final14-46
dc.page.initial14-1
dc.publisherSpringer Nature
dc.relation.projectIDinfo:eu-repo/grantAgreement/MICINN//PID2021-122955OB-C41
dc.rightsAttribution 4.0 Internationalen
dc.rights.accessRightsopen access
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subject.cdu52-33
dc.subject.keywordAthena: the advanced telescope for high energy astrophysics
dc.subject.keywordX-IFU: the X-ray Integral Field Unit
dc.subject.keywordSpace instrumentation
dc.subject.keywordX-rays
dc.subject.keywordObservatory
dc.subject.keywordAstrophysics
dc.subject.keywordInstrumentation and methods for astrophysics
dc.subject.ucmAstrofísica
dc.subject.unesco2199 Otras Especialidades Astronómicas
dc.titleThe first cut is the cheapest: optimizing Athena/X-IFU-like TES detectors resolution by filter truncation
dc.typejournal article
dc.type.hasVersionVoR
dc.volume.number57
dspace.entity.typePublication
relation.isAuthorOfPublication2b15a442-d308-49d5-beda-1a98bb9db11e
relation.isAuthorOfPublication.latestForDiscovery2b15a442-d308-49d5-beda-1a98bb9db11e

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