TY - JOUR
T1 - Observation of polarized hard X-ray emission from the Crab by the PoGOLite Pathfinder
AU - Chauvin, M.
AU - Florén, H. G.
AU - Jackson, M.
AU - Kamae, T.
AU - Kawano, T.
AU - Kiss, M.
AU - Kole, M.
AU - Mikhalev, V.
AU - Moretti, E.
AU - Olofsson, G.
AU - Rydström, S.
AU - Takahashi, H.
AU - Iyudin, A.
AU - Arimoto, M.
AU - Fukazawa, Y.
AU - Kataoka, J.
AU - Kawai, N.
AU - Mizuno, T.
AU - Ryde, F.
AU - Tajima, H.
AU - Takahashi, T.
AU - Pearce, M.
N1 - Publisher Copyright:
© 2015 The Authors.
PY - 2016/2/11
Y1 - 2016/2/11
N2 - We have measured the linear polarization of hard X-ray emission from the Crab in a previously unexplored energy interval, 20-120 keV. The introduction of two new observational parameters, the polarization fraction and angle stands to disentangle geometrical and physical effects, thereby providing information on the pulsar wind geometry and magnetic field environment. Measurements are conducted using the PoGOLite Pathfinder - a balloon-borne polarimeter. Polarization is determined by measuring the azimuthal Compton scattering angle of incident X-rays in an array of plastic scintillators housed in an anticoincidence well. The polarimetric response has been characterized prior to flight using both polarized and unpolarized calibration sources. We address possible systematic effects through observations of a background field. The measured polarization fraction for the integrated Crab light curve is 18.4+9.8 -10.6 per cent, corresponding to an upper limit (99 per cent credibility) of 42.4 per cent, for a polarization angle of (149.2 ± 16.0)°.
AB - We have measured the linear polarization of hard X-ray emission from the Crab in a previously unexplored energy interval, 20-120 keV. The introduction of two new observational parameters, the polarization fraction and angle stands to disentangle geometrical and physical effects, thereby providing information on the pulsar wind geometry and magnetic field environment. Measurements are conducted using the PoGOLite Pathfinder - a balloon-borne polarimeter. Polarization is determined by measuring the azimuthal Compton scattering angle of incident X-rays in an array of plastic scintillators housed in an anticoincidence well. The polarimetric response has been characterized prior to flight using both polarized and unpolarized calibration sources. We address possible systematic effects through observations of a background field. The measured polarization fraction for the integrated Crab light curve is 18.4+9.8 -10.6 per cent, corresponding to an upper limit (99 per cent credibility) of 42.4 per cent, for a polarization angle of (149.2 ± 16.0)°.
KW - Instrumentation: polarimeters
KW - Pulsars: individual: the crab pulsar
KW - Stars: neutron
KW - Techniques: polarimetric
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U2 - 10.1093/mnrasl/slv177
DO - 10.1093/mnrasl/slv177
M3 - Article
AN - SCOPUS:84959175886
SN - 1745-3933
VL - 456
SP - L84-L88
JO - Monthly Notices of the Royal Astronomical Society: Letters
JF - Monthly Notices of the Royal Astronomical Society: Letters
IS - 1
ER -