TY - JOUR
T1 - Measurement of 1.7–74 MeV polarised γ rays with the HARPO TPC
AU - Geerebaert, Y.
AU - Gros, Ph
AU - Amano, S.
AU - Attié, D.
AU - Bernard, D.
AU - Bruel, P.
AU - Calvet, D.
AU - Colas, P.
AU - Daté, S.
AU - Delbart, A.
AU - Frotin, M.
AU - Giebels, B.
AU - Götz, D.
AU - Hashimoto, S.
AU - Horan, D.
AU - Kotaka, T.
AU - Louzir, M.
AU - Minamiyama, Y.
AU - Miyamoto, S.
AU - Ohkuma, H.
AU - Poilleux, P.
AU - Semeniouk, I.
AU - Sizun, P.
AU - Takemoto, A.
AU - Yamaguchi, M.
AU - Wang, S.
N1 - Publisher Copyright:
© 2016 Elsevier B.V.
PY - 2017/2/11
Y1 - 2017/2/11
N2 - Current γ-ray telescopes based on photon conversions to electron-positron pairs, such as Fermi, use tungsten converters. They suffer of limited angular resolution at low energies, and their sensitivity drops below 1 GeV. The low multiple scattering in a gaseous detector gives access to higher angular resolution in the MeV–GeV range, and to the linear polarisation of the photons through the azimuthal angle of the electron-positron pair. HARPO is an R&D programme to characterise the operation of a TPC (Time Projection Chamber) as a high angular-resolution and sensitivity telescope and polarimeter for γ rays from cosmic sources. It represents a first step towards a future space instrument. A 30 cm cubic TPC demonstrator was built, and filled with 2 bar argon-based gas. It was put in a polarised γ-ray beam at the NewSUBARU accelerator in Japan in November 2014. Data were taken at different photon energies from 1.7 MeV to 74 MeV, and with different polarisation configurations. The electronics setup is described, with an emphasis on the trigger system. The event reconstruction algorithm is quickly described, and preliminary measurements of the polarisation of 11 MeV photons are shown.
AB - Current γ-ray telescopes based on photon conversions to electron-positron pairs, such as Fermi, use tungsten converters. They suffer of limited angular resolution at low energies, and their sensitivity drops below 1 GeV. The low multiple scattering in a gaseous detector gives access to higher angular resolution in the MeV–GeV range, and to the linear polarisation of the photons through the azimuthal angle of the electron-positron pair. HARPO is an R&D programme to characterise the operation of a TPC (Time Projection Chamber) as a high angular-resolution and sensitivity telescope and polarimeter for γ rays from cosmic sources. It represents a first step towards a future space instrument. A 30 cm cubic TPC demonstrator was built, and filled with 2 bar argon-based gas. It was put in a polarised γ-ray beam at the NewSUBARU accelerator in Japan in November 2014. Data were taken at different photon energies from 1.7 MeV to 74 MeV, and with different polarisation configurations. The electronics setup is described, with an emphasis on the trigger system. The event reconstruction algorithm is quickly described, and preliminary measurements of the polarisation of 11 MeV photons are shown.
KW - Gamma-ray
KW - Gaseous detector
KW - Polarimetry
KW - TPC
UR - https://www.scopus.com/pages/publications/85003634578
U2 - 10.1016/j.nima.2016.06.031
DO - 10.1016/j.nima.2016.06.031
M3 - Article
AN - SCOPUS:85003634578
SN - 0168-9002
VL - 845
SP - 228
EP - 232
JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
ER -