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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

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • 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

  • 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