Proceedings of XII Multifrequency Behaviour of High Energy Cosmic Sources Workshop — PoS(MULTIF2017) 2018
DOI: 10.22323/1.306.0068
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Polarimetry with POLAR

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Cited by 2 publications
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“…In addition, the photon flux induced by GeV DM has a plateau shape extending to sub-GeV energies, though the degree of polarization drops to 10%. This polarized low-energy γ-ray signal may be of interest to current X-ray telescopes such as the POLAR satellite, which is a X-ray polarimeter sensitive to an energy up to 0.5 MeV with a 10% MDP [33]. In addition, the Advanced Energetic Pair Telescope (AdEPT [34]) and the time projection chamber as a gamma-ray telescope and polarimeter (HARPO [35]) have been proposed to study the photon polarization at few percent level for the sub-GeV energy range.…”
Section: Discussionmentioning
confidence: 99%
“…In addition, the photon flux induced by GeV DM has a plateau shape extending to sub-GeV energies, though the degree of polarization drops to 10%. This polarized low-energy γ-ray signal may be of interest to current X-ray telescopes such as the POLAR satellite, which is a X-ray polarimeter sensitive to an energy up to 0.5 MeV with a 10% MDP [33]. In addition, the Advanced Energetic Pair Telescope (AdEPT [34]) and the time projection chamber as a gamma-ray telescope and polarimeter (HARPO [35]) have been proposed to study the photon polarization at few percent level for the sub-GeV energy range.…”
Section: Discussionmentioning
confidence: 99%
“…Additionally, we are currently working on a Bayesian approach to get posterior on PD and PA, this allows to give deviation and upper/lower limits more precisely. POLAR-2, as a following experiment of POALR, has already been selected to be launched on the China Space Station around 2024, and it is now being constructed [8,9]. Our previous work has estimated the detection of Crab pulsar with POLAR-2 [3].…”
Section: Figurementioning
confidence: 99%