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Pulse processing in TES detectors: comparative of different short filter methods based on optimal filtering. Case study for Athena X-IFU

dc.book.titleSPIE Astronomical Telescopes and Instrumentation, 2020
dc.contributor.authorCoboa, Beatriz
dc.contributor.authorCardiel López, Nicolás
dc.contributor.authorCeballosa, María Teresa
dc.contributor.authorPeillec, Philippe
dc.date.accessioned2023-06-16T13:03:23Z
dc.date.available2023-06-16T13:03:23Z
dc.date.issued2021-12-28
dc.description© 2020 SPIE. Conference on Space Telescopes and Instrumentation - Ultraviolet to Gamma Ray / SPIE Astronomical Telescopes + Instrumentation Conference (DEC 14-18, 2020, On-line). This work has been funded by the Spanish Ministry of Science, Innovation and Universities (MICINN) under project RTI2018-096686-B-C21 (co-funded by FEDER funds) and by the Spanish State Research Agency (AEI), Excellency Unit María de Maeztu, MDM-2017-0765.
dc.description.abstractIn the framework of the ESA Athena mission, the X-ray Integral Field Unit (X-IFU) instrument to be on board the X-ray Athena Observatory is a cryogenic micro-calorimeter array of Transition Edge Sensor (TES) detectors aimed at providing spatially resolved high-resolution spectroscopy. As a part of the on-board Event Processor (EP), the reconstruction software will provide the energy, spatial location and arrival time of the incoming X-ray photons hitting the detector and inducing current pulses on it. Being the standard optimal filtering technique the chosen baseline reconstruction algorithm, different modifications have been analyzed to process pulses shorter than those considered of high resolution (those where the full length is not available due to a close pulse after them) in order to select the best option based on energy resolution and computing performance results. It can be concluded that the best approach to optimize the energy resolution for short filters is the 0-padding filtering technique, benefiting also from a reduction in the computational resources. However, it’s high sensitivity to offset fluctuations currently prevents its use as the baseline treatment for the X-IFU application for lack of consolidated information on the actual stability it will get in flight.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Ciencia e Innovación (MICINN)/FEDER
dc.description.sponsorshipUnidad de Excelencia María de Maeztu
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/67986
dc.identifier.doi10.1117/12.2562733
dc.identifier.isbn978-1-5106-3676-7
dc.identifier.officialurlhttps://doi.org/10.1117/12.2562733
dc.identifier.relatedurlhttps://www.spiedigitallibrary.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/2448
dc.language.isoeng
dc.publisherSPI-Int Soc. Optical Engineering
dc.relation.ispartofseriesProceedings of the SPIE
dc.relation.projectIDRTI2018-096686-B-C21
dc.relation.projectIDMDM-2017-0765
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordAthena
dc.subject.keywordX-ray integral field unit
dc.subject.keywordX-ray spectroscopy
dc.subject.keywordSpace telescopes
dc.subject.keywordiIstrumentation
dc.subject.keywordReconstruction methods
dc.subject.keywordPerformance analysis
dc.subject.ucmFísica atmosférica
dc.subject.unesco2501 Ciencias de la Atmósfera
dc.titlePulse processing in TES detectors: comparative of different short filter methods based on optimal filtering. Case study for Athena X-IFU
dc.typebook part
dc.volume.number11444
dspace.entity.typePublication
relation.isAuthorOfPublication2b15a442-d308-49d5-beda-1a98bb9db11e
relation.isAuthorOfPublication.latestForDiscovery2b15a442-d308-49d5-beda-1a98bb9db11e

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