Improving HEXITEC gain calibration through charge-shared and fluorescent multi-pixel events

  • Jessie Duncan
  • , Albert Y. Shih

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Scopus citations

Abstract

We describe two techniques to verify and improve the energy calibration of pixelated solid-state X-ray detectors by specifically analyzing multiple-pixel events. There are two primary types of multiple-pixel events. In fluorescent events, some of the incident photon energy is re-emitted as a Cd or Te characteristic X-ray, with mean free path (∼80-200 μm) comparable to the pixel pitch. Deposition of the fluorescence photon commonly occurs in an adjacent pixel. Isolating fluorescent double-pixel events provides low-energy (<15 keV) escape lines not intrinsic to the source. These lines reveal that the non-linearity of the gain at low energies is larger than previously thought, and can now be corrected. In charge-shared events, the cloud of deposited charge from one incident photon spreads across pixel boundaries. This causes charge loss due to variation in applied field strength within inter-pixel regions. The charge loss is a smooth function of the ratio between component energies, with more loss seen when a photon hits closer to the boundary and its energy is more evenly split. Characterization of this energy-split-dependent loss lets us extrapolate †split event behavior below the signal threshold. We can then verify consistency of the non-linear gain calibration at the lowest energies.

Original languageEnglish (US)
Title of host publicationUV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXII
EditorsOswald H. Siegmund
PublisherSPIE
ISBN (Electronic)9781510644809
DOIs
StatePublished - 2021
EventUV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXII 2021 - San Diego, United States
Duration: Aug 1 2021Aug 5 2021

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume11821
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Conference

ConferenceUV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXII 2021
Country/TerritoryUnited States
CitySan Diego
Period8/1/218/5/21

Bibliographical note

Funding Information:
This work was supported under the 2019 NASA Fellowship Program (80NSSC19k1687). by NASA instrument-development grant 80NSSC18K1257.

Publisher Copyright:
© COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.

Keywords

  • calibration
  • CdTe
  • charge sharing
  • Hard X-rays
  • solar flares
  • solid-state pixelated detectors
  • the Sun
  • X-ray detectors

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