Radio properties of green pea galaxies | Astronomy & Astrophysics (A&A)

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Table 3.

Summary of the archival radio surveys used for flux measurements of the targeted and archival sources.

Survey	Observatory	Freq.	Resolution	Sensitivity
		[GHz]	[arcsec]	[mJy beam⁻¹]
FIRST	VLA	1.4	5.4	0.15 ^(a)
NVSS	VLA	1.4	45	0.45 ^(a)
VLASS	VLA	3.0	2.5	0.145
TGSS	GMRT	0.15	25	5
LoTSS	LOFAR	0.15	6	0.083
RACS	ASKAP	0.888	15–25	0.2

Notes.

^(a)

Although the median RMS noise is lower, the source-detection limit is 5 × rms and the catalogues contain sources above this limit.

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