Polarisation studies of the prompt gamma-ray emission from GRB 041219a using the spectrometer aboard INTEGRAL

Abstract

Context. Linear polarisation in gamma-ray burst prompt emission is an important diagnostic with the potential to significantly constrain models. The spectrometer aboard INTEGRAL, SPI, has the capability to detect the signature of polarised emission from a bright γ-ray source. GRB 041219a is the most intense burst localised by INTEGRAL with a fluence of 5.7 ×10 −4 erg cm −2 over the energy range 20 keV-8 MeV and is an ideal candidate for such a study. Aims. Polarisation can be measured using multiple events scattered into adjacent detectors because the Compton scatter angle depends on the polarisation of the incoming photon. A search for linear polarisation in the most intense pulse of duration 66 seconds and in the brightest 12 seconds of GRB 041219a was performed in the 100-350 keV, 100-500 keV and 100 keV-1 MeV energy ranges. It was possible to divide the events into six directions in the energy ranges of 100-350 keV and 100-500 keV using the kinematics of the Compton scatter interactions. Methods. The multiple event data from the spectrometer was analysed and compared with the predicted instrument response obtained from Monte-Carlo simulations using the GEANT 4 INTEGRAL mass model. The χ 2 distribution between the real and simulated data as a function of the percentage polarisation and polarisation angle was calculated for all three energy ranges. The degree and angle of polarisation were obtained from the best-fit value of χ 2 . Results. A weak signal consistent with polarisation was found throughout the analyses. The degree of linear polarisation in the brightest pulse of duration 66 s was found to be 63 +31 −30 % at an angle of 70 +14 −11 degrees in the 100-350 keV energy range. The degree of polarisation was also constrained in the brightest 12 s of the GRB and a polarisation fraction of 96 +39 −40 % at an angle of 60 +12 −14 degrees was determined over the same energy range. However, despite extensive analysis and simulations, a systematic effect that could mimic the weak polarisation signal could not be definitively excluded. Conclusions. Our results over several energy ranges and time intervals are consistent with a polarisation signal of about 60% but at a low level of significance (∼2σ). The polarisation results are compared with predictions from the synchrotron and Compton drag processes. The spectrum of this GRB can also be well fit by a combined black body and power law model which could arise from a combination of the Compton and synchrotron processes, with different degrees of polarisation. We therefore conclude that the procedure described here demonstrates the effectiveness of using SPI as a polarimeter, and is a viable method of measuring polarisation levels in intense gamma-ray bursts.

High energy emission and polarisation limits for the INTEGRAL burst GRB 061122

“…The results of polarisation analysis using the SPI multiple event data of GRB 061122 are presented in Sect. 6, using the method described in McGlynn et al (2007). We also present afterglow results from Swift-XRT (Sect.…”

“…The simulation of the GRB multiple events was carried out as described in McGlynn et al (2007). The spectral parameters from the Band model of the T 90 spectrum were used to generate a set of simulated events arriving from the direction of the GRB.…”

“…The unpolarised simulation data were combined with the polarised simulation data, allowing the percentage of polarisation to be varied as a function of angle. The polarisation analysis procedure for GRB 061122 was carried out in the same manner as for GRB 041219a in McGlynn et al (2007). The SPI multiple event data were divided into six directions in the energy ranges of 100-350 keV and 100-500 keV using the kinematics of the Compton scatter interactions, and divided into 3 directions in the 100-1000 keV energy range.…”

Study of emission mechanism of Gamma-Ray Bursts by the gamma-ray polarization with IKAROS-GAP

“…[7] independently checked their analyses and found a polarization value of 41 +57 −44 % which is different from the previous two reports but consistent with all levels of polarization. The second reports showed also high degree of polarization for GRB 041219A with Π = 98 ± 33 % [8] and Π = 63 +31 −30 % [9] for the brightest pulse in the 100-350 keV energy band of INTEGRAL-SPI at 2 σ confidence level for 2 parameters of interest (Π and PA). [10] also reported the detection of polarization for time resolved analyses 1 , and suggested possible variable polarization properties for the same GRB 041219A in the 200-800 keV energy band observed with INTEGRAL-IBIS.…”

Integral Status Overview

“… Hard X-ray/soft γ-ray point source catalogues provide important new data on galactic and extragalactic source populations in the 15 keV -8 MeV band [6], [17], [18].  Detection of polarization in the high -energy emission of the Crab pulsar and in the prompt emission of gamma -ray burst GRB 041219A, both with SPI and IBIS [19], [20], [21], [22].  The detection of diffuse hard X-ray emission from the Ophiuchus cluster of galaxies [23].…”