Test and characterization of finely segmented pixel CZT detectors for future hard X-ray missions

  • G. Pinaroli
  • , G. A. Carini
  • , G. W. Deptuch
  • , D. S. Gorni
  • , P. Maj
  • , H. Krawczynski

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

The NuSTAR (Nuclear Spectroscopic Telescope Array) mission was launched in 2012, and it has successfully deployed the first orbiting telescopes to focus high energy X-ray (3-79 keV) light, providing a wealth of new information on high-energy X-rays sources. Follow-up missions, such as the proposed HEX-P, BEST, and FORCE, could perform a deeper black hole census providing a more refined measurement of black hole spins, allowing for greater knowledge about supermassive black holes. These missions are motivated by the recent breakthroughs in the hard X-ray mirror technologies, where mirrors, either made of monolithic silicon segments, or made directly or via replication of shells, demonstrate the feasibility of making hard X-ray mirrors with angular resolutions of 5-10 arc-seconds Half Power Diameter (HPD) compared to the NuSTAR's 1 arc-minute HPD. Such a high angular resolution requires matched detectors with higher degree of segmentation to fully benefit from the achievable improved spatial resolution. In the above framework, the HEXID ASIC, a novel pixelated front-end suitable for reading out a finely segmented CZT sensor with 150 µm pixel pitch in a hexagonal arrangement has been developed. This readout pixelated chip is capable of processing photon-generated charge packets over a large dynamic range (from 2 keV up to 180 keV), while keeping a low input noise (ENC <20 e-). In this work, the initial characterization of the ASIC prototype will be presented.

Original languageEnglish
Title of host publicationSpace Telescopes and Instrumentation 2024
Subtitle of host publicationUltraviolet to Gamma Ray
EditorsJan-Willem A. den Herder, Shouleh Nikzad, Kazuhiro Nakazawa
PublisherSPIE
ISBN (Electronic)9781510675094
DOIs
StatePublished - 2024
EventSpace Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray - Yokohama, Japan
Duration: Jun 16 2024Jun 21 2024

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume13093
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Conference

ConferenceSpace Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray
Country/TerritoryJapan
CityYokohama
Period06/16/2406/21/24

Keywords

  • CZT
  • Event Driven readout
  • low-noise front-end
  • Readout ASIC
  • Space Telescope
  • Spectroscopy
  • X-rays

Fingerprint

Dive into the research topics of 'Test and characterization of finely segmented pixel CZT detectors for future hard X-ray missions'. Together they form a unique fingerprint.

Cite this