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Investigating Radio Source Population and Spatial Characteristics of Diffuse Galactic Synchrotron Emission in the GAMA-23 Field with uGMRT Band-3

  • Authors: Rashmi Sagar, Abhirup Datta, Aishrila Mazumder

Rashmi Sagar et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 9.

Angular power spectrum (C) with 1σ error bars (in red and purple) plotted as a function of angular multipole () for the visibility-based estimator (TGE; S. Choudhuri et al. 2014) at frequency 325 MHz for six target pointings at different latitudes of the GAMA-23 field. The vertical gray shadow indicates the range of values used to fit the power law, and the best-fitting model C = A(1000/)β is shown in magenta. The dashed dotted line (in green) represents the fitting prediction (i.e., Smin = 5σ; S. S. Ali et al. 2008). The values of magnitude A, power-law index β and range for APS are given in Table 5 for Band-3.

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