4.6 Article

Analysis of Polarimetry Data with Angular Uncertainties

Journal

ASTRONOMICAL JOURNAL
Volume 162, Issue 4, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.3847/1538-3881/ac173d

Keywords

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Funding

  1. Marshall Space Flight Center (MSFC) [80MSFC17C0012]
  2. National Aeronautics and Space Administration (NASA) through the Smithsonian Astrophysical Observatory (SAO) [SV3-73016]
  3. NASA [NAS8-03060]

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This study utilizes the maximum likelihood method to estimate the minimum detectable polarization, taking into account uncertainties in event track position angles. By deriving a simple relationship between track angle uncertainties and the energy-dependent modulation function, the process is made more straightforward.
For a track based polarimeter, such as the Imaging X-ray Polarimetry Explorer (IXPE), the sensitivity to polarization depends on the modulation factor, which is a strong function of energy. In previous work, a likelihood method was developed that would account for this variation in order to estimate the minimum detectable polarization (MDP). That method essentially required that the position angles of individual events should be known precisely. In a separate work, however, it was shown that using a machine-learning method for measuring event tracks can generate track angle uncertainties, which can be used in the analysis. Here, the maximum likelihood method is used as a basis for revising the estimate of the MDP in a general way that can include uncertainties in event track position angles. The resultant MDP depends solely upon the distribution of track angle uncertainties present in the input data. Due to the physics of the IXPE detectors, it is possible to derive a simple relationship between these angular uncertainties and the energy-dependent modulation function as a step in the process.

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