All-sky angular power spectrum ā€“ I. Estimating brightness temperature fluctuations using the 150-MHz TGSS survey

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Date

2020

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Oxford University Press

Abstract

Measurements of the Galactic synchrotron emission are important for the 21-cm studies of the epoch of reionization. The study of synchrotron emission is also useful for quantifying the fluctuations in the magnetic field and the cosmic-ray electron density of the turbulent interstellar medium (ISM) of our Galaxy. Here, we present the all-sky angular power spectrum (Cā„“) measurements of the diffuse synchrotron emission obtained using the TIFR GMRT Sky Survey (TGSS) at 150 MHz.

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Methods: data analysis, Methods: statistical, Techniques: interferometric, Dark ages, Radio continuum: general

Citation

Ghosh, A. et al. (2020). All-sky angular power spectrum ā€“ I. Estimating brightness temperature fluctuations using the 150-MHz TGSS survey. Monthly Notices of the Royal Astronomical Society, 494(2), 1936ā€“1945

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https://doi.org/10.1093/mnras/staa762
 http://hdl.handle.net/10566/5882

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Research Articles (Physics)