Spectral index of synchrotron emission: insights from the diffuse and magnetised interstellar medium

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Table A.1

Medians of the brightness temperature spectral index for the three POSs and the two cases of weak and strong field at a resolution of 6.7′.

	POS


Weak field (B₀ = 4 μG)	xy	− 2.83 ± 0.01	− 2.92 ± 0.01
	yz	− 2.89 ± 0.02	− 2.98 ± 0.02
	zx	− 2.83 ± 0.01	− 2.92 ± 0.01

Strong field (B₀ = 20 μG)	xy	− 2.65	− 2.72
	yz	− 3.02 ± 0.03	− 3.08 ± 0.02
	zx	− 2.65	− 2.72

Notes. Labels and identify the frequency intervals 467−672 MHz and 833−1200 MHz, respectively.Errors have been estimated using the first and third quartiles. Errors smaller than 0.01 are not shown.

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