How to Detect X-Rays and Gamma-Rays from Space: Optics and Detectors

BULGARELLI, ANDREA

doi:10.1007/978-981-15-6337-9_3

How to Detect X-Rays and Gamma-Rays from Space: Optics and Detectors

Date Issued

2020

Author(s)

FIORETTI, VALENTINA

•

BULGARELLI, ANDREA

DOI

10.1007/978-981-15-6337-9_3

Abstract

The measurable quantities of the sky’s light, for any wavelength, are energy, position, arrival time, and polarization. Each of them reveal different information about the science target (e.g. gas dynamics, state and distribution of the matter, temperature, luminosity) and require specific detecting solutions. In the study of X-rays and gamma-rays up to the TeV regime, their absorption by the atmosphere (by 50% at 30 km altitude for 1 MeV photon) requires the development of space applications. The science goals of the mission define which technological benchmark should be maximised (e.g. energy or spatial resolution), but the final design of high energy instruments is the result of a trade-off analysis among the detection specifications, the need for space-borne electronic systems and materials, and the limited resources in mass budget, electrical power, and telemetry rates.

Coverage

Tutorial Guide to X-ray and Gamma-ray Astronomy

Start page

55

Uri

http://hdl.handle.net/20.500.12386/31397

Url

https://link.springer.com/chapter/10.1007/978-981-15-6337-9_3

Ads BibCode

2020tgxg.book...55F

Rights

open.access

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Fioretti-Bulgarelli2020_Chapter.pdf

Description

[Administrators only]

Size

3.1 MB

Format

Adobe PDF

Checksum (MD5)

826d8efd7e85507878a92a668a0e470d

Name

front.pdf

Size

173.42 KB

Format

Adobe PDF

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How to Detect X-Rays and Gamma-Rays from Space: Optics and Detectors

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