Discovery of the supernova remnant G351.0-5.4 | Astronomy & Astrophysics (A&A)

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Table 2

Radio observations.

Telescope	Frequency	Resolution	Largest scale	Flux density		Rms
	(MHz)		(arcmin)	(mJy)		(mJy beam^-1)
				East	West

GMRT	325	141′′× 89′′	≃32	151	280	1.5
VLA (NVSS)	1400	45′′× 45′′	≃16	48	67	0.5
Parkes 64 m	2417	10′.23 × 10′.62	–	~3000^b		11
Parkes 64 m (PMN)	4850	4′.9 × 4′.9	≃57^a	367	162	11

Notes..

^(a)

Although the PMN is a single dish survey, a limit on the largest scale is given by the filtering procedure applied during data reduction (Griffith & Wright 1993)

^(b)

The target emission is blended with the surrounding Galactic extended emission.

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