A measurement of Galactic synchrotron emission using MWA drift scan observations

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dc.contributor.authorChatterjee, Suman
dc.contributor.authorSarkar, Shouvik
dc.contributor.authorChoudhuri, Samir
dc.date.accessioned2025-11-03T08:16:20Z
dc.date.available2025-11-03T08:16:20Z
dc.date.issued2025
dc.description.abstractStudying the diffuse Galactic synchrotron emission (hereafter, DGSE) at arc-minute angular scale is important to remove the foregrounds for the cosmological 21-cm observations. Statistical measurements of the large-scale DGSE can also be used to constrain the magnetic field and the cosmic ray electron density of our Galaxy's interstellar medium (ISM). Here, we have used the Murchison Widefield Array (MWA) drift scan observations at$154.2 \, {\rm MHz}$to measure the angular power spectrum$({\cal C}_{\ell})$of the DGSE of a region of the sky from right ascension (RA)$349^{\circ}$to$70.3^{\circ}$at the fixed declination$-26.7^{\circ}$ . In this RA range, we have chosen 24 pointing centers (PCs), for which we have removed all the bright point sources above$\sim430 \, {\rm mJy}\,(3σ)$ , and applied the Tapered Gridded Estimator (TGE) on residual data to estimate the${\cal C}_{\ell}$ . We use the angular multipole range$65 \le \ell \le 650$to fit the data with a model,${\cal C}^M_{\ell}=A\times \left(\frac{1000}{\ell}\right)^β+C$ , where we interpret the model as the combination of a power law$(\propto \ell^{-β})$nature of the DGSE and a constant part due to the Poisson fluctuations of the residual point sources. We are able to fit the model${\cal C}^M_{\ell}$for six PCs centered at$α=352.5^{\circ}, 353^{\circ}, 357^{\circ}, 4.5^{\circ}, 4^{\circ}$and$1^{\circ}$ . We run the Markov Chain Monte Carlo (MCMC) ensemble sampler to get the best-fit values of the parameters$A, β$and$C$for these PCs. We see that the values of$A$vary in the range$155$to$400$mK $^{2}$ , whereas the$β$varies in the range$0.9$to$1.7$ . We find that the value of$β$is consistent at$2-σ$level with the earlier measurement of the DGSE at similar frequency and angular scales
dc.identifier.citationChatterjee, S. et al. (2025) A measurement of Galactic synchrotron emission using MWA drift scan observations. [Online]
dc.identifier.urihttps://doi.org/10.48550/arxiv.2506.14310
dc.identifier.urihttps://hdl.handle.net/10566/21360
dc.language.isoen
dc.publisherCambridge University Press
dc.subjectLarge-scale structure of universe
dc.subjectfirst stars
dc.subjectcosmology
dc.subjectreionisation
dc.subjectdiffuse radiation
dc.titleA measurement of Galactic synchrotron emission using MWA drift scan observations
dc.typeArticle

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