Benjamin Schneider, Gregory Prigozhin, Richard F. Foster, Marshall W. Bautz, Hope Fu, Catherine E. Grant, Sarah Heine, Jill Juneau, Beverly LaMarr, Olivier Limousin, Nathan Lourie, Andrew Malonis, Eric D. Miller
{"title":"X-ray spectral performance of the Sony IMX290 CMOS sensor near Fano limit after a per-pixel gain calibration","authors":"Benjamin Schneider, Gregory Prigozhin, Richard F. Foster, Marshall W. Bautz, Hope Fu, Catherine E. Grant, Sarah Heine, Jill Juneau, Beverly LaMarr, Olivier Limousin, Nathan Lourie, Andrew Malonis, Eric D. Miller","doi":"arxiv-2409.05954","DOIUrl":null,"url":null,"abstract":"The advent of back-illuminated complementary metal-oxide-semiconductor (CMOS)\nsensors and their well-known advantages over charge-coupled devices (CCDs) make\nthem an attractive technology for future X-ray missions. However, numerous\nchallenges remain, including improving their depletion depth and identifying\neffective methods to calculate per-pixel gain conversion. We have tested a\ncommercial Sony IMX290LLR CMOS sensor under X-ray light using an $^{55}$Fe\nradioactive source and collected X-ray photons for $\\sim$15 consecutive days\nunder stable conditions at regulated temperatures of 21{\\deg}C and 26{\\deg}C.\nAt each temperature, the data set contained enough X-ray photons to produce one\nspectrum per pixel consisting only of single-pixel events. We determined the\ngain dispersion of its 2.1 million pixels using the peak fitting and the Energy\nCalibration by Correlation (ECC) methods. We measured a gain dispersion of\n0.4\\% at both temperatures and demonstrated the advantage of the ECC method in\nthe case of spectra with low statistics. The energy resolution at 5.9 keV after\nthe per-pixel gain correction is improved by $\\gtrsim$10 eV for single-pixel\nand all event spectra, with single-pixel event energy resolution reaching\n$123.6\\pm 0.2$ eV, close to the Fano limit of silicon sensors at room\ntemperature. Finally, our long data acquisition demonstrated the excellent\nstability of the detector over more than 30 days under a flux of $10^4$ photons\nper second.","PeriodicalId":501374,"journal":{"name":"arXiv - PHYS - Instrumentation and Detectors","volume":"109 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Instrumentation and Detectors","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.05954","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
The advent of back-illuminated complementary metal-oxide-semiconductor (CMOS)
sensors and their well-known advantages over charge-coupled devices (CCDs) make
them an attractive technology for future X-ray missions. However, numerous
challenges remain, including improving their depletion depth and identifying
effective methods to calculate per-pixel gain conversion. We have tested a
commercial Sony IMX290LLR CMOS sensor under X-ray light using an $^{55}$Fe
radioactive source and collected X-ray photons for $\sim$15 consecutive days
under stable conditions at regulated temperatures of 21{\deg}C and 26{\deg}C.
At each temperature, the data set contained enough X-ray photons to produce one
spectrum per pixel consisting only of single-pixel events. We determined the
gain dispersion of its 2.1 million pixels using the peak fitting and the Energy
Calibration by Correlation (ECC) methods. We measured a gain dispersion of
0.4\% at both temperatures and demonstrated the advantage of the ECC method in
the case of spectra with low statistics. The energy resolution at 5.9 keV after
the per-pixel gain correction is improved by $\gtrsim$10 eV for single-pixel
and all event spectra, with single-pixel event energy resolution reaching
$123.6\pm 0.2$ eV, close to the Fano limit of silicon sensors at room
temperature. Finally, our long data acquisition demonstrated the excellent
stability of the detector over more than 30 days under a flux of $10^4$ photons
per second.