Detection of polarized gamma-ray emission from the Crab nebula with the Hitomi Soft Gamma-ray Detector
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F18%3A00106529" target="_blank" >RIV/00216224:14310/18:00106529 - isvavai.cz</a>
Result on the web
<a href="https://arxiv.org/pdf/1810.00704.pdf" target="_blank" >https://arxiv.org/pdf/1810.00704.pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/pasj/psy118" target="_blank" >10.1093/pasj/psy118</a>
Alternative languages
Result language
angličtina
Original language name
Detection of polarized gamma-ray emission from the Crab nebula with the Hitomi Soft Gamma-ray Detector
Original language description
We present the results from the Hitomi Soft Gamma-ray Detector (SGD) observation of the Crab nebula. The main part of SGD is a Compton camera, which in addition to being a spectrometer, is capable of measuring polarization of gamma-ray photons. The Crab nebula is one of the brightest X-ray / gamma-ray sources on the sky, and, the only source from which polarized X-ray photons have been detected. SGD observed the Crab nebula during the initial test observation phase of Hitomi. We performed the data analysis of the SGD observation, the SGD background estimation and the SGD Monte Carlo simulations, and, successfully detected polarized gamma-ray emission from the Crab nebula with only about 5 ks exposure time. The obtained polarization fraction of the phase-integrated Crab emission (sum of pulsar and nebula emissions) is (22.1% +/- 10.6%), and, the polarization angle is 110.degrees 7 + 13.degrees 2 /-13.degrees 0 in the energy range of 60-160 keV (The errors correspond to the 1 sigma deviation). The confidence level of the polarization detection was 99.3%. The polarization angle measured by SGD is about one sigma deviation with the projected spin axis of the pulsar, 124.degrees 0 +/- 0.degrees 1.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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Continuities
S - Specificky vyzkum na vysokych skolach
Others
Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
ISSN
0004-6264
e-ISSN
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Volume of the periodical
70
Issue of the periodical within the volume
6
Country of publishing house
JP - JAPAN
Number of pages
19
Pages from-to
„113-1“-„113-19“
UT code for WoS article
000456072300015
EID of the result in the Scopus database
2-s2.0-85069453486