The Growth of Interest in Astronomical X-Ray Polarimetry

Astronomical X-ray polarimetry was first explored in the end of the 1960s by pioneering rocket instruments. The craze arising from the first discoveries of stellar and supernova remnant X-ray polarization led to the addition of X-ray polarimeters to early satellites. Unfortunately, the inadequacy of...

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Main Author: Frédéric Marin
Format: Article
Language:English
Published: MDPI AG 2018-03-01
Series:Galaxies
Subjects:
Online Access:http://www.mdpi.com/2075-4434/6/1/38
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author Frédéric Marin
author_facet Frédéric Marin
author_sort Frédéric Marin
collection DOAJ
description Astronomical X-ray polarimetry was first explored in the end of the 1960s by pioneering rocket instruments. The craze arising from the first discoveries of stellar and supernova remnant X-ray polarization led to the addition of X-ray polarimeters to early satellites. Unfortunately, the inadequacy of the diffraction and scattering technologies required to measure polarization with respect to the constraints driven by X-ray mirrors and detectors, coupled with long integration times, slowed down the field for almost 40 years. Thanks to the development of new, highly sensitive, compact X-ray polarimeters in the beginning of the 2000s, observing astronomical X-ray polarization has become feasible, and scientists are now ready to explore our high-energy sky thanks to modern X-ray polarimeters. In the forthcoming years, several X-ray missions (rockets, balloons, and satellites) will create new observational opportunities. Interest in astronomical X-ray polarimetry field has thus been renewed, and this paper presents for the first time a quantitative assessment, all based on scientific literature, of the growth of this interest.
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spelling doaj.art-610ae968a6f543268d740109aac8d5242022-12-22T00:14:33ZengMDPI AGGalaxies2075-44342018-03-01613810.3390/galaxies6010038galaxies6010038The Growth of Interest in Astronomical X-Ray PolarimetryFrédéric Marin0Observatoire Astronomique de Strasbourg, Université de Strasbourg, CNRS, UMR 7550, 11 rue de l'Université, F-67000 Strasbourg, FranceAstronomical X-ray polarimetry was first explored in the end of the 1960s by pioneering rocket instruments. The craze arising from the first discoveries of stellar and supernova remnant X-ray polarization led to the addition of X-ray polarimeters to early satellites. Unfortunately, the inadequacy of the diffraction and scattering technologies required to measure polarization with respect to the constraints driven by X-ray mirrors and detectors, coupled with long integration times, slowed down the field for almost 40 years. Thanks to the development of new, highly sensitive, compact X-ray polarimeters in the beginning of the 2000s, observing astronomical X-ray polarization has become feasible, and scientists are now ready to explore our high-energy sky thanks to modern X-ray polarimeters. In the forthcoming years, several X-ray missions (rockets, balloons, and satellites) will create new observational opportunities. Interest in astronomical X-ray polarimetry field has thus been renewed, and this paper presents for the first time a quantitative assessment, all based on scientific literature, of the growth of this interest.http://www.mdpi.com/2075-4434/6/1/38X-rayspolarimetrygeneralhistory of astronomy
spellingShingle Frédéric Marin
The Growth of Interest in Astronomical X-Ray Polarimetry
Galaxies
X-rays
polarimetry
general
history of astronomy
title The Growth of Interest in Astronomical X-Ray Polarimetry
title_full The Growth of Interest in Astronomical X-Ray Polarimetry
title_fullStr The Growth of Interest in Astronomical X-Ray Polarimetry
title_full_unstemmed The Growth of Interest in Astronomical X-Ray Polarimetry
title_short The Growth of Interest in Astronomical X-Ray Polarimetry
title_sort growth of interest in astronomical x ray polarimetry
topic X-rays
polarimetry
general
history of astronomy
url http://www.mdpi.com/2075-4434/6/1/38
work_keys_str_mv AT fredericmarin thegrowthofinterestinastronomicalxraypolarimetry
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